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1. Astrometric detection of a Neptune-mass candidate planet in the nearest M-dwarf binary system GJ65 with VLTI/GRAVITY

Author: GRAVITY Collaboration, Abuter, R., Amorim, A., Benisty, M., Berger, J-P., Bonnet, H., Bourdarot, G., Bourget, P., Brandner, W., Clénet, Y., Davies, R., Delplancke-Ströbele, F., Dembet, R., Drescher, A., Eckart, A., Eisenhauer, F., Feuchtgruber, H., Finger, G., Förster-Schreiber, N. M., Garcia, P., Garcia-Lopez, R., Gao, F., Gendron, E., Genzel, R., Gillessen, S., Hartl, M., Haubois, X., Haussmann, F., Henning, T., Hippler, S., Horrobin, M., Jochum, L., Jocou, L., Kaufer, A., Kervella, P., Lacour, S., Lapeyrère, V., Bouquin, J. B. Le, Ledoux, C., Léna, P., Lutz, D., Mang, F., Mérand, A., More, N., Nowak, M., Ott, T., Paumard, T., Perraut, K., Perrin, G., Pfuhl, O., Rabien, S., Ribeiro, D. C., Bordoni, M. Sadun, Shangguan, J., Shimizu, T., Stadler, J., Straub, O., Straubmeier, C., Sturm, E., Tacconi, L. J., Tristram, K. R. W, Vincent, F., von Fellenberg, S., Widmann, F., Wieprecht, E., Woillez, J., Yazici, S., and Zins, G.
Subjects: Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: The detection of low-mass planets orbiting the nearest stars is a central stake of exoplanetary science, as they can be directly characterized much more easily than their distant counterparts. Here, we present the results of our long-term astrometric observations of the nearest binary M-dwarf Gliese 65 AB (GJ65), located at a distance of only 2.67 pc. We monitored the relative astrometry of the two components from 2016 to 2023 with the VLTI/GRAVITY interferometric instrument. We derived highly accurate orbital parameters for the stellar system, along with the dynamical masses of the two red dwarfs. The GRAVITY measurements exhibit a mean accuracy per epoch of 50-60 microarcseconds in 1.5h of observing time using the 1.8m Auxiliary Telescopes. The residuals of the two-body orbital fit enable us to search for the presence of companions orbiting one of the two stars (S-type orbit) through the reflex motion they imprint on the differential A-B astrometry. We detected a Neptune-mass candidate companion with an orbital period of p = 156 +/- 1 d and a mass of m = 36 +/- 7 Mearth. The best-fit orbit is within the dynamical stability region of the stellar pair. It has a low eccentricity, e = 0.1 - 0.3, and the planetary orbit plane has a moderate-to-high inclination of i > 30{\deg} with respect to the stellar pair, with further observations required to confirm these values. These observations demonstrate the capability of interferometric astrometry to reach microarcsecond accuracy in the narrow-angle regime for planet detection by reflex motion from the ground. This capability offers new perspectives and potential synergies with Gaia in the pursuit of low-mass exoplanets in the solar neighborhood., Comment: Corresponding authors: G.Bourdarot, P.Kervella, O.Pfuhl. Accepted in A&A Letters
Published: 2024

2. Near-Infrared Observations of Outflows and YSOs in the Massive Star-Forming Region AFGL 5180

Author: Crowe, S., Fedriani, R., Tan, J. C., Whittle, M., Zhang, Y., Garatti, A. Caratti o, Farias, J. P., Gautam, A., Telkamp, Z., Rothberg, B., Grudic, M., Andersen, M., Cosentino, G., Garcia-Lopez, R., Rosero, V., Tanaka, K., Pinna, E., Rossi, F., Miller, D., Agapito, G., Plantet, C., Ghose, E., Christou, J., Power, J., Puglisi, A., Briguglio, R., Brusa, G., Taylor, G., Zhang, X., Mazzoni, T., Bonaglia, M., Esposito, S., and Veillet, C.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Methods: Broad- and narrow-band imaging of AFGL 5180 was made in the NIR with the LBT, in both seeing-limited ($\sim0.5\arcsec$) and high angular resolution ($\sim0.09\arcsec$) Adaptive Optics (AO) modes, as well as with HST. Archival ALMA continuum data was also utilized. Results: At least 40 jet knots were identified via NIR emission from H$_2$ and [FeII] tracing shocked gas. Bright jet knots outflowing from the central most massive protostar, S4, are detected towards the east of the source and are resolved in fine detail with the AO imaging. Additional knots are distributed throughout the field, likely indicating the presence of multiple driving sources. Sub-millimeter sources detected by ALMA are shown to be grouped in two main complexes, AFGL 5180 M and a small cluster $\sim15\arcsec$ to the south, AFGL 5180 S. From our NIR continuum images we identify YSO candidates down to masses of $\sim 0.1\:M_\odot$. Combined with the sub-mm sources, this yields a surface number density of such YSOs of $N_* \sim 10^3 {\rm pc}^{-2}$ within a projected radius of about 0.1 pc. Such a value is similar to those predicted by models of both Core Accretion from a turbulent clump environment and Competitive Accretion. The radial profile of $N_*$ is relatively flat on scales out to 0.2~pc, with only modest enhancement around the massive protostar inside 0.05~pc. Conclusions: This study demonstrates the utility of high-resolution NIR imaging, in particular with AO, for detecting outflow activity and YSOs in distant regions. The presented images reveal the complex morphology of outflow-shocked gas within the large-scale bipolar flow of a massive protostar, as well as clear evidence for several other outflow driving sources in the region. Finally, this work presents a novel approach to compare the observed YSO surface number density from our study against different models of massive star formation., Comment: Accepted to Astronomy & Astrophysics (A&A)
Published: 2023
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3. A dynamical measure of the black hole mass in a quasar 11 billion years ago

Author: Abuter, R., Allouche, F., Amorim, A., Bailet, C., Berdeu, A., Berger, J.-P., Berio, P., Bigioli, A., Boebion, O., Bolzer, M.-L., Bonnet, H., Bourdarot, G., Bourget, P., Brandner, W., Cao, Y., Conzelmann, R., Comin, M., Clénet, Y., Courtney-Barrer, B., Davies, R., Defrère, D., Delboulbé, A., Delplancke-Ströbele, F., Dembet, R., Dexter, J., de Zeeuw, P. T., Drescher, A., Eckart, A., Édouard, C., Eisenhauer, F., Fabricius, M., Feuchtgruber, H., Finger, G., Förster Schreiber, N. M., Garcia, P., Garcia Lopez, R., Gao, F., Gendron, E., Genzel, R., Gil, J. P., Gillessen, S., Gomes, T., Gonté, F., Gouvret, C., Guajardo, P., Guieu, S., Hackenberg, W., Haddad, N., Hartl, M., Haubois, X., Haußmann, F., Heißel, G., Henning, Th., Hippler, S., Hönig, S. F., Horrobin, M., Hubin, N., Jacqmart, E., Jocou, L., Kaufer, A., Kervella, P., Kolb, J., Korhonen, H., Lacour, S., Lagarde, S., Lai, O., Lapeyrère, V., Laugier, R., Le Bouquin, J.-B., Leftley, J., Léna, P., Lewis, S., Liu, D., Lopez, B., Lutz, D., Magnard, Y., Mang, F., Marcotto, A., Maurel, D., Mérand, A., Millour, F., More, N., Netzer, H., Nowacki, H., Nowak, M., Oberti, S., Ott, T., Pallanca, L., Paumard, T., Perraut, K., Perrin, G., Petrov, R., Pfuhl, O., Pourré, N., Rabien, S., Rau, C., Riquelme, M., Robbe-Dubois, S., Rochat, S., Salman, M., Sanchez-Bermudez, J., Santos, D. J. D., Scheithauer, S., Schöller, M., Schubert, J., Schuhler, N., Shangguan, J., Shchekaturov, P., Shimizu, T. T., Sevin, A., Soulez, F., Spang, A., Stadler, E., Sternberg, A., Straubmeier, C., Sturm, E., Sykes, C., Tacconi, L. J., Tristram, K. R. W., Vincent, F., von Fellenberg, S., Uysal, S., Widmann, F., Wieprecht, E., Wiezorrek, E., Woillez, J., and Zins, G.
Published: 2024
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4. FU Orionis disk outburst: evidence for a gravitational instability scenario triggered in a magnetically dead zone

Author: Bourdarot, G., Berger, J-P., Lesur, G., Perraut, K., Malbet, F., Millan-Gabet, R., Bouquin, J-B. Le, Garcia-Lopez, R., Monnier, J. D., Labdon, A., Kraus, S., Labadie, L., and Aarnio, A.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract: Context: FUors outbursts are a crucial stage of accretion in young stars. However a complete mechanism at the origin of the outburst still remains missing. Aims: We aim at constraining the instability mechanism in FU Orionis star itself, by directly probing the size and the evolution in time of the outburst region with near-infrared interferometry, and to confront it to physical models of this region. Methods: FU Orionis has been a regular target of near-infrared interferometry. In this paper, we analyze more than 20 years of interferometric observations to perform a temporal monitoring of the region of the outburst, and compare it to the spatial structure deduced from 1D MHD simulations. Results: We measure from the interferometric observations that the size variation of the outburst region is compatible with a constant or slightly decreasing size over time in the H and K band. The temporal variation and the mean sizes are consistently reproduced by our 1D MHD simulations. We find that the most compatible scenario is a model of an outburst occurring in a magnetically layered disk, where a Magneto-Rotational Instability (MRI) is triggered by a Gravitational Instability (GI) at the outer edge of a dead-zone. The scenario of a pure Thermal Instability (TI) fails to reproduce our interferometric sizes since it can only be sustained in a very compact zone of the disk <0.1 AU. The scenario of MRI-GI could be compatible with an external perturbation enhancing the GI, such as tidal interactions with a stellar companion, or a planet at the outer edge of the dead-zone. Conclusions: The layered disk model driven by MRI turbulence is favored to interpret the spatial structure and temporal evolution of FU Orionis outburst region. Understanding this phase gives a crucial link between the early phase of disk evolution and the process of planet formation in the first inner AUs., Comment: Accepted for publication in A&A
Published: 2023
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5. ASTRI Mini-Array Core Science at the Observatorio del Teide

Author: Vercellone, S., Bigongiari, C., Burtovoi, A., Cardillo, M., Catalano, O., Franceschini, A., Lombardi, S., Nava, L., Pintore, F., Stamerra, A., Tavecchio, F., Zampieri, L., Batista, R. Alves, Amato, E., Antonelli, L. A., Arcaro, C., Gonzalez, J. Becerra, Bonnoli, G., Bottcher, M., Brunetti, G., Compagnino, A. A., Crestan, S., Ai, A. D, Fiori, M., Galanti, G., Giuliani, A., Pino, E. M. de Gouveia Dal, Green, J. G., Lamastra, A., Landoni, M., Lucarelli, F., Morlino, G., Olmi, B., Peretti, E., Piano, G., Ponti, G., Poretti, E., Romano, P., Saturni, F. G., Scuderi, S., Tutone, A., Umana, G., Acosta-Pulido, J. A., Barai, P., Bonanno, A., Bonanno, G., Bruno, P., Bulgarelli, A., Conforti, V., Costa, A., Cusumano, G., Del Santo, M., del Valle, M. V., Della Ceca, R., Falceta-Goncalves, D. A., Fioretti, V., Germani, S., Garcia-Lopez, R. J., Ghedina, A., Giordano, V., Kreter, M., Incardona, F., Iovenitti, S., La Barbera, A., La Palombara, N., La Parola, V., Leto, G., Longo, F., Lopez-Oramas, A., Maccarone, M. C., Mereghetti, S., Millul, R., Naletto, G., Pagliaro, A., Parmiggiani, N., Righi, C., Rodriguez-Ramirez, J. C., Romeo, G., Sangiorgi, P., de Lima, R. Santos, Tagliaferri, G., Testa, V., Tosti, G., Acosta, M. Vazquez, Zywucka, N., Caraveo, P. A., and Pareschi, G.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the Observatorio del Teide a mini-array (ASTRI Mini-Array) composed of nine telescopes similar to the small-size dual-mirror Schwarzschild-Couder telescope (ASTRI-Horn) currently operating on the slopes of Mt. Etna in Sicily. The ASTRI Mini-Array will surpass the current Cherenkov telescope array differential sensitivity above a few tera-electronvolt (TeV), extending the energy band well above hundreds of TeV. This will allow us to explore a new window of the electromagnetic spectrum, by convolving the sensitivity performance with excellent angular and energy resolution figures. In this paper we describe the Core Science that we will address during the first four years of operation, providing examples of the breakthrough results that we will obtain when dealing with current open questions, such as the acceleration of cosmic rays, cosmology and fundamental physics and the new window, for the TeV energy band, of the time-domain astrophysics., Comment: Published in Journal of High Energy Astrophysics. 46 Figures, 7 Tables
Published: 2022
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6. PENELLOPE III. The peculiar accretion variability of XX Cha and its impact on the observed spread of accretion rates

Author: Claes, R. A. B., Manara, C. F., Garcia-Lopez, R., Natta, A., Fang, M., Fockter, Z. P., Ábrahám, P., Alcalá, J. M., Campbell-White, J., Garatti, A. Caratti o, Covino, E., Fedele, D., Frasca, A., Gameiro, J. F., Herczeg, G. J., Kóspál, Á., Petr-Gotzens, M. G., Rosotti, G., Venuti, L., and Zsidi, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The processes regulating protoplanetary disk evolution are constrained by studying how mass accretion rates scale with stellar and disk properties. The spread in these relations can be used as a constraint to the models of disk evolution, but only if the impact of accretion variability is correctly accounted for. While the effect of variability might be substantial in the embedded phases of star formation, it is often considered limited at later stages. Here we report on the observed large variation in the accretion rate for one target, XX Cha, and we discuss the impact on population studies of classical T Tauri stars. The mass accretion rate determined by fitting the UV-to-near-infrared spectrum in recent X-Shooter observations is compared with the one measured with the same instrument 11 years before. XX Cha displays an accretion variability of almost 2 dex between 2010 and 2021. Although the timescales on which this variability happens are uncertain, XX Cha displays an extreme accretion variability for a classical T Tauri star. If such behavior is common among classical T Tauri stars, possibly on longer timescales than previously probed, it could be relevant for discussing the disk evolution models constrained by the observed spread in accretion rates. Finally, we remark that previous studies of accretion variability based on spectral lines may have underestimated the variability of some targets., Comment: Accepted for publication in A&A letters
Published: 2022
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7. Probing inner and outer disk misalignments in transition disks

Author: Bohn, A. J., Benisty, M., Perraut, K., van der Marel, N., Wölfer, L., van Dishoeck, E. F., Facchini, S., Manara, C. F., Teague, R., Francis, L., Berger, J-P., Garcia-Lopez, R., Ginski, C., Henning, T., Kenworthy, M., Kraus, S., Ménard, F., Mérand, A., and Pérez, L. M.
Subjects: Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: For several transition disks (TDs), dark regions interpreted as shadows have been observed in scattered light imaging and are hypothesized to originate from misalignments between distinct disk regions. We aim to investigate the presence of misalignments in TDs. We study the inner disk geometries of 20 well-known transition disks with VLTI/GRAVITY observations and use complementary $^{12}$CO and $^{13}$CO molecular line data from ALMA to derive the orientation of the outer disk regions. We fit simple models to the GRAVITY data to derive the inner disks inclination and position angles. The outer disk geometries were derived from Keplerian fits to the ALMA velocity maps and compared to the inner disk constraints. We also predicted the locations of shadows for significantly misaligned systems. Our analysis reveals six disks to exhibit significant misalignments between their inner and outer disks. The predicted shadow positions agree well with the scattered light images of HD100453 and HD142527, and we find supporting evidence for a shadow in the disk around CQ Tau. In the other three targets for which we infer significantly misaligned disks, V1247 Ori, V1366 Ori, and RY Lup, we do not see any evident sign of shadows in the scattered light images. The scattered light shadows observed in DoAr44, HD135344B, and HD139614 are consistent with our observations, yet the underlying morphology is likely too complex to be described by our models and the accuracy achieved by our observations. Whereas we can derive precise constraints on the potential shadow positions for well-resolved inner disks around HAeBe stars, the statistical uncertainties for the marginally resolved inner disks around the TTS of our sample make it difficult to extract conclusive constraints for the presence of shadows in these systems., Comment: Accepted for publication in Astronomy \& Astrophysics
Published: 2021
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8. The GRAVITY Young Stellar Object survey. VII. The inner dusty disks of T Tauri stars

Author: The GRAVITY Collaboration, Perraut, K., Labadie, L., Bouvier, J., Ménard, F., Klarmann, L., Dougados, C., Benisty, M., Berger, J. -P., Bouarour, Y. -I., Brandner, W., Garatti, A. Caratti o, Caselli, P., de Zeeuw, P. T., Garcia-Lopez, R., Henning, T., Sanchez-Bermudez, J., Sousa, A., van Dishoeck, E., Alécian, E., Amorim, A., Clénet, Y., Davies, R., Drescher, A., Duvert, G., Eckart, A., Eisenhauer, F., Förster-Schreiber, N. M., Garciaınst, P., Gendron, E., Genzel, R., Gillessen, S., Grellmann, R., Heissel, G., Hippler, S., Horrobin, M., Hubert, Z., Jocou, L., Kervella, P., Lacour, S., Lapeyrère, V., Bouquin, J. -B. Le, Léna, P., Lutz, D., Ott, T., Paumard, T., Perrin, G., Scheithauer, S., Shangguan, J., Shimizu, T., Stadler, J., Straub, O., Straubmeier, C., Sturm, E., Tacconi, L., Vincent, F., von Fellenberg, S., and Widmann, F.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: These protoplanetary disks in T Tauri stars play a central role in star and planet formation. We spatially resolve at sub-au scales the innermost regions of a sample of T Tauri's disks to better understand their morphology and composition. We extended our homogeneous data set of 27 Herbig stars and collected near-IR K-band observations of 17 T Tauri stars, spanning effective temperatures and luminosities in the ranges of ~4000-6000 K and ~0.4-10 Lsun. We focus on the continuum emission and develop semi-physical geometrical models to fit the interferometric data and search for trends between the properties of the disk and the central star. The best-fit models of the disk's inner rim correspond to wide rings. We extend the Radius-luminosity relation toward the smallest luminosities (0.4-10 Lsun) and find the R~L^(1/2) trend is no longer valid, since the K-band sizes measured with GRAVITY are larger than the predicted sizes from sublimation radius computation. No clear correlation between the K-band half-flux radius and the mass accretion rate is seen. Having magnetic truncation radii in agreement with the K-band GRAVITY sizes would require magnetic fields as strong as a few kG, which should have been detected, suggesting that accretion is not the main process governing the location of the half-flux radius of the inner dusty disk. Our measurements agree with models that take into account the scattered light. The N-to-K band size ratio may be a proxy for disentangling disks with silicate features in emission from disks with weak and/or in absorption silicate features. When comparing inclinations and PA of the inner disks to those of the outer disks (ALMA) in nine objects of our sample, we detect misalignments for four objects., Comment: Accepted for publication in A&A; 20 pages, 15 figures, 9 tables
Published: 2021
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9. Launching the asymmetric bipolar jet of DO Tau

Author: Erkal, J., Dougados, C., Coffey, D., Cabrit, S., Bacciotti, F., Garcia-Lopez, R., Fedele, D., and Chrysostomou, A.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The role of bipolar jets in the formation of stars, and in particular how they are launched, is still not well understood. We probe the protostellar jet launching mechanism, via high resolution observations of the near-IR [FeII] 1.53,1.64 micron lines. We consider the bipolar jet from the Classical T Tauri star, DO Tau, & investigate jet morphology & kinematics close to the star, using AO-assisted IFU observations from GEMINI/NIFS. The brighter, blue-shifted jet is collimated quickly after launch. This early collimation requires the presence of magnetic fields. We confirm velocity asymmetries between the two jet lobes, & confirm no time variability in the asymmetry over a 20 year interval. This sustained asymmetry is in accordance with recent simulations of magnetised disk-winds. We examine the data for jet rotation. We report an upper limit on differences in radial velocity of 6.3 & 8.7 km/s for the blue & red-shifted jets, respectively. Interpreting this as an upper limit on jet rotation implies that any steady, axisymmetric magneto-centrifugal model of jet launching is constrained to a launch radius in the disk-plane of 0.5 & 0.3 au for the blue & red-shifted jets, respectively. This supports an X-wind or narrow disk-wind model. This pertains only to the observed high velocity [FeII] emission, & does not rule out a wider flow launched from a wider radius. We report detection of small amplitude jet axis wiggling in both lobes. We rule out orbital motion of the jet source as the cause. Precession can better account for the observations but requires double the precession angle, & a different phase for the counter-jet. Such non-solid body precession could arise from an inclined massive Jupiter companion, or a warping instability induced by launching a magnetic disk-wind. Overall, our observations are consistent with an origin of the DO Tau jets from the inner regions of the disk., Comment: Accepted for publication in A&A - 18 pages, 11 figures (incl. Appendix)
Published: 2021
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10. The GRAVITY young stellar object survey III. The dusty disk of RY Lup

Author: GRAVITY Collaboration, Bouarour, Y. -I., Perraut, K., Ménard, F., Brandner, W., Garatti, A. Caratti o, Caselli, P., van Dishoeck, E., Dougados, C., Garcia-Lopez, R., Grellmann, R., Henning, T., Klarmann, L., Labadie, L., Natta, A., Sanchez-Bermudez, J., Thi, W. -F., de Zeeuw, P. T., Amorim, A., Bauböck, M., Benisty, M., Berger, J. -P., Clenet, Y., Foresto, V. Coudé du, Duvert, G., Eckart, A., Eisenhauer, F., Eupen, F., Filho, M., Gao, F., Garcia, P., Gendron, E., Genzel, R., Gillessen, S., Jiménez-Rosales, A., Jocou, L., Hippler, S., Horrobin, M., Hubert, Z., Kervella, P., Lacour, S., Bouquin, J. -B. Le, Léna, P., Ott, T., Paumard, T., Perrin, G., Pfuhl, O., Rousset, G., Scheithauer, S., Shangguan, J., Stadler, J., Straub, O., Straubmeier, C., Sturm, E., Vincent, F. H., von Fellenberg, S. D., Widmann, F., and Wiest, M.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We use PIONIER data from the ESO archive and GRAVITY data that were obtained in June 2017 with the four 8m telescopes. We use a parametric disk model and the 3D radiative transfer code MCFOST to reproduce the Spectral Energy Distribution and match the interferometric observations. To match the SED , our model requires a stellar luminosity of 2.5 Lsun, higher than any previously determined values. Such a high value is needed to accommodate the circumstellar extinction caused by the highly inclined disk, which has been neglected in previous studies. While using an effective temperature of 4800 K determined through high-resolution spectroscopy, we derive a stellar radius of 2.29 Rsun. These revised fundamental parameters, when combined with the mass estimates available , lead to an age of 0.5-2.0 Ma for RY Lup, in better agreement with the age of the Lupus association than previous determinations. Our disk model nicely reproduces the interferometric GRAVITY data and is in good agreement with the PIONIER ones. We derive an inner rim location at 0.12~au from the central star. This model corresponds to an inclination of the inner disk of 50deg, which is in mild tension with previous determinations of a more inclined outer disk from SPHERE (70 deg in NIR) and ALMA(67 $\pm$5 deg) images, but consistent with the inclination determination from the ALMA CO spectra (55$\pm$5deg). Increasing the inclination of the inner disk to 70 deg leads to a higher line-of-sight extinction and therefore requires a higher stellar luminosity of 4.65 Lsun to match the observed flux levels. This luminosity would translate to a stellar radius of 3.13~Rsun, leading to an age of 2-3~Ma, and a stellar mass of about 2 Msun, in disagreement with the observed dynamical mass estimate of 1.3-1.5 Msun. Critically, this high-inclination inner disk model also fails to reproduce the visibilities observed with GRAVITY., Comment: Accepted for publication in A&A; 11 pages, 5 figures, 3 tables
Published: 2020
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11. Mirror, mirror on the outflow cavity wall. Near-infrared CO overtone disc emission of the high-mass YSO IRAS 11101-5829

Author: Fedriani, R., Garatti, A. Caratti o, Koutoulaki, M., Garcia-Lopez, R., Natta, A., Cesaroni, R., Oudmaijer, R., Coffey, D., Ray, T., and Stecklum, B.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Aims: The inner regions of high-mass protostars are often invisible in the near-infrared. We aim to investigate the inner gaseous disc of IRAS11101-5829 through scattered light from the outflow cavity walls. Methods: We observed the environment of the high-mass young stellar object IRAS11101-5829 and the closest knots of its jet, HH135-136, with the VLT/SINFONI. We also retrieved archival data from the high-resolution long-slit spectrograph VLT/X-shooter. Results: We detect the first three bandheads of the $\upsilon=2-0$ CO vibrational emission for the first time in this object. It is coincident with continuum and Br$\gamma$ emission and extends up to $\sim10000$ au to the north-east and $\sim10 000$ au to the south-west. The line profiles have been modelled as a Keplerian rotating disc assuming a single ring in LTE. The model output gives a temperature of $\sim3000$ K, a CO column density of $\sim1\times10^{22}\mathrm{ cm^{-2}}$, and a projected Keplerian velocity $v_\mathrm{K}\sin i_\mathrm{disc} \sim 25\mathrm{ km s^{-1}}$, which is consistent with previous modelling in other high-mass protostars. In particular, the low value of $v_\mathrm{K}\sin i_\mathrm{disc}$ suggests that the disc is observed almost face-on, whereas the well-constrained geometry of the jet imposes that the disc must be close to edge-on. This apparent discrepancy is interpreted as the CO seen reflected in the mirror of the outflow cavity wall. Conclusions: From both jet geometry and disc modelling, we conclude that all the CO emission is seen through reflection by the cavity walls and not directly. This result implies that in the case of highly embedded objects, as for many high-mass protostars, line profile modelling alone might be deceptive and the observed emission could affect the derived physical and geometrical properties; in particular the inclination of the system can be incorrectly interpreted., Comment: 11 pages, 10 figures
Published: 2020
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12. The GRAVITY Young Stellar Object survey -- I. Probing the disks of Herbig Ae/Be stars in terrestrial orbits

Author: Perraut, K., Labadie, L., Lazareff, B., Klarmann, L., Segura-Cox, D., Benisty, M., Bouvier, J., Brandner, W., Garatti, A. Caratti o, Caselli, P., Dougados, C., Garcia, P., Garcia-Lopez, R., Kendrew, S., Koutoulaki, M., Kervella, P., Lin, C. -C., Pineda, J., Sanchez-Bermudez, J., van Dishoeck, E., Abuter, R., Amorim, A., Berger, J. -P., Bonnet, H., Buron, A., Cantalloube, F., Clénet, Y., Foresto, V. Coudé du, Dexter, J., de Zeeuw, P. T., Duvert, G., Eckart, A., Eisenhauer, F., Eupen, F., Gao, F., Gendron, E., Genzel, R., Gillessen, S., Gordo, P., Grellmann, R., Haubois, X., Haussmann, F., Henning, T., Hippler, S., Horrobin, M., Hubert, Z., Jocou, L., Lacour, S., Bouquin, J. -B. Le, Léna, P., Mérand, A., Ott, T., Paumard, T., Perrin, G., Pfuhl, O., Rabien, S., Ray, T., Rau, C., Rousset, G., Scheithauer, S., Straub, O., Straubmeier, C., Sturm, E., Vincent, F., Waisberg, I., Wank, I., Widmann, F., Wieprecht, E., Wiest, M., Wiezorrek, E., Woillez, J., and Yazici, S.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: The formation and the evolution of protoplanetary disks are important stages in the lifetime of stars. The processes of disk evolution and planet formation are intrinsically linked. We spatially resolve with GRAVITY/VLTI in the K-band the sub au-scale region of 27 stars to gain statistical understanding of their properties. We look for correlations with stellar parameters, such as luminosity, mass, temperature and age. Our sample also cover a range of various properties in terms of reprocessed flux, flared or flat morphology, and gaps. We developed semi-physical geometrical models to fit our interferometric data. Our best models correspond to smooth and wide rings, implying that wedge-shaped rims at the dust sublimation edge are favored, as found in the H-band. The closure phases are generally non-null with a median value of ~10 deg, indicating spatial asymmetries of the intensity distributions. Multi-size grain populations could explain the closure phase ranges below 20-25 deg but other scenarios should be invoked to explain the largest ones. Our measurements extend the Radius-Luminosity relation to ~1e4 Lsun and confirm the significant spread around the mean relation observed in the H-band. Gapped sources exhibit a large N-to-K band size ratio and large values of this ratio are only observed for the members of our sample that would be older than 1 Ma, less massive, and with lower luminosity. In the 2 Ms mass range, we observe a correlation in the increase of the relative age with the transition from group II to group I, and an increase of the N-to-K size ratio. However, the size of the current sample does not yet permit us to invoke a clear universal evolution mechanism across the HAeBe mass range. The measured locations of the K-band emission suggest that these disks might be structured by forming young planets, rather than by depletion due to EUV, FUV, and X-ray photo-evaporation., Comment: Accepted for publication in A&A; 23 pages, 16 figures, 7 tables
Published: 2019
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13. Measuring the ionisation fraction in a jet from a massive protostar

Author: Fedriani, R., Garatti, A. Caratti o, Purser, S. J. D., Sanna, A., Tan, J. C., Garcia-Lopez, R., Ray, T. P., Coffey, D., Stecklum, B., and Hoare, M.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: It is important to determine if massive stars form via disc accretion, like their low-mass counterparts. Theory and observation indicate that protostellar jets are a natural consequence of accretion discs and are likely to be crucial for removing angular momentum during the collapse. However, massive protostars are typically rarer, more distant and more dust enshrouded, making observational studies of their jets more challenging. A fundamental question is whether the degree of ionisation in jets is similar across the mass spectrum. Here we determine an ionisation fraction of $\sim5-12\%$ in the jet from the massive protostar G35.20-0.74N, based on spatially coincident infrared and radio emission. This is similar to the values found in jets from lower-mass young stars, implying a unified mechanism of shock ionisation applies in jets across most of the protostellar mass spectrum, up to at least $\sim10$ solar masses., Comment: Published in Nature Communications. This is author's version. Full article is available here https://rdcu.be/bN6ps . 10 pages, 4 Figures, including methods and references
Published: 2019
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14. Parsec-scale jets driven by high-mass young stellar objects. Connecting the au- and the parsec-scale jet in IRAS 13481-6124

Author: Fedriani, R., Garatti, A. Caratti o, Coffey, D., Garcia-Lopez, R., Kraus, S., Weigelt, G., Stecklum, B., Ray, T. P., and Walmsley, C. M.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Context: Protostellar jets in high-mass young stellar objects (HMYSOs) play a key role in the understanding of star formation and provide us with an excellent tool to study fundamental properties of HMYSOs. Aims: We aim at studying the physical and kinematic properties of the near-IR (NIR) jet of IRAS\,13481-6124 from au to parsec scales. Methods: Our study includes NIR data from the Very Large Telescope instruments SINFONI, CRIRES, and ISAAC. Information about the source and its immediate environment is retrieved with SINFONI. The technique of spectro-astrometry is performed with CRIRES to study the jet on au scales. The parsec-scale jet and its kinematic and dynamic properties are investigated using ISAAC. Results: The SINFONI spectra in the $H$ and $K$ band are rich in emission lines that are mainly associated with ejection and accretion processes. Spectro-astrometry is applied to the Br$\gamma$ line, and for the first time, to the Br$\alpha$ line, revealing their jet origin with milliarcsecond-scale photocentre displacements ($11-15$\,au). This allows us to constrain the kinematics of the au-scale jet and to derive its position angle ($\sim216^{\circ}$). ISAAC spectroscopy reveals H$_2$ emission along the parsec-scale jet, which allows us to infer kinematic and dynamic properties of the NIR parsec-scale jet. The mass-loss rate inferred for the NIR jet is $\dot{M}_\mathrm{ejec}\sim10^{-4}\mathrm{\,M_\odot\,yr^{-1}}$ and the thrust is $\dot{P}\sim10^{-2}\mathrm{\,M_\odot\,yr^{-1}\,km\,s^{-1}}$ , which is roughly constant for the formation history of the young star. A tentative estimate of the ionisation fraction is derived for the massive jet by comparing the radio and NIR mass-loss rates. An ionisation fraction $\lesssim8\%$ is obtained, which means that the bulk of the ejecta is traced by the NIR jet and that the radio jet only delineates a small portion of it., Comment: Accepted for publication in A&A
Published: 2018
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15. The GRAVITY young stellar object survey: XIV. Investigating the magnetospheric accretion-ejection processes in S CrA N.

Author: Nowacki, H., Perraut, K., Labadie, L., Bouvier, J., Dougados, C., Benisty, M., Wojtczak, J. A., Soulain, A., Alecian, E., Brandner, W., Caratti o Garatti, A., Garcia Lopez, R., Ganci, V., Sánchez-Bermúdez, J., Berger, J.-P., Bourdarot, G., Caselli, P., Clénet, Y., Davies, R., and Drescher, A.
Subjects: ACCRETION disks, GAS distribution, STAR observations, ORIGIN of planets, RADIATIVE transfer
Abstract: Context. The dust- and gas-rich protoplanetary disks around young stellar systems play a key role in star and planet formation. While considerable progress has recently been made in probing these disks on large scales of a few tens of astronomical units (au), the central au requires further investigation. Aims.We aim to unveil the physical processes at play in the innermost regions of the strongly accreting T Tauri Star S CrA N by means of near-infrared interferometric observations. As recent spectropolarimetric observations suggest that S CrA N might undergo intense ejection processes, we focus on the accretion–ejection phenomena and on the star–disk interaction region. Methods. We obtained interferometric observations with VLTI/GRAVITY in the K-band during two consecutive nights in August 2022. The analysis of the continuum emission, coupled with the differential analysis across the Brγ line, allows us to constrain the morphology of the dust and the gas distribution in the innermost regions of S CrA N and to investigate their temporal variability. These observations are compared to magnetospheric accretion–ejection models of T Tauri stars and to previous observations in order to elucidate the physical processes operating in these regions. Results. The K-band continuum emission is well reproduced with an azimuthally modulated dusty ring with a half-light radius of 0.24 au (∼20 R*), an inclination of ∼30°, and a position angle of ∼150°. As the star alone cannot explain such a large sublimation front, we propose that magnetospheric accretion is an important dust-heating mechanism leading to this continuum emission. The Brγ-emitting region (0.05–0.06 au; 5–7 R*) is found to be more compact than the continuum, to be similar in size or larger than the magnetospheric truncation radius. The on-sky displacements across the Brγ spectral channels are aligned along a position angle offset by 45° from the disk, and extend up to 2 R*. This is in agreement with radiative transfer models combining magnetospheric accretion and disk winds. These on-sky displacements remain unchanged from one night to another, while the line flux decreases by 13%, suggesting a dominant contribution of wind to the origin of the Brγ line. Conclusions. Our observations support the scenario where the Brγ line originates from a combination of (variable) accretion–ejection processes in the inner disk region. [ABSTRACT FROM AUTHOR]
Published: 2024
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16. PENELLOPE. VI. Searching the PENELLOPE/UVES sample with spectro-astrometry: Two new microjets of Sz 103 and XXCha

Author: Sperling, T., primary, Eislöffel, J., additional, Manara, C. F., additional, Campbell-White, J., additional, Schneider, C., additional, Frasca, A., additional, Maucó, K., additional, Siwak, M., additional, Fuhrmeister, B., additional, and Garcia Lopez, R., additional
Published: 2024
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17. GIARPS/GRAVITY Survey: Broad-Band 0.44–2.4 Micron High-Resolution Spectra of T-Tauri and Herbig AeBe Stars – Combining High Spatial and High Spectral Resolution Data to Unveil the Inner Disc Physics

Author: Massi, F., Caratti o Garatti, A., Garcia Lopez, R., Benisty, M., Brand, J., Brandner, W., Casu, S., Coffey, D., Dougados, C., Giannetti, A., Labadie, L., Leurini, S., Moscadelli, L., Natta, A., Pedani, M., Perraut, K., Ray, T., Sanna, A., Sanna, N., and Sauty, Christophe, editor
Published: 2019
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18. Near-infrared observations of outflows and young stellar objects in the massive star-forming region AFGL 5180

Author: Crowe, S., primary, Fedriani, R., additional, Tan, J. C., additional, Whittle, M., additional, Zhang, Y., additional, Caratti o Garatti, A., additional, Farias, J. P., additional, Gautam, A., additional, Telkamp, Z., additional, Rothberg, B., additional, Grudić, M., additional, Andersen, M., additional, Cosentino, G., additional, Garcia-Lopez, R., additional, Rosero, V., additional, Tanaka, K., additional, Pinna, E., additional, Rossi, F., additional, Miller, D., additional, Agapito, G., additional, Plantet, C., additional, Ghose, E., additional, Christou, J., additional, Power, J., additional, Puglisi, A., additional, Briguglio, R., additional, Brusa, G., additional, Taylor, G., additional, Zhang, X., additional, Mazzoni, T., additional, Bonaglia, M., additional, Esposito, S., additional, and Veillet, C., additional
Published: 2024
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19. A measure of the size of the magnetospheric accretion region in TW Hydrae

Author: Garcia Lopez, R., Natta, A., Caratti o Garatti, A., Ray, T. P., Fedriani, R., Koutoulaki, M., and Klarmann, L.
Subjects: Stars, Variable -- Observations -- Spectra, Very long baseline interferometry -- Usage, Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract: Stars form by accreting material from their surrounding disks. There is a consensus that matter flowing through the disk is channelled onto the stellar surface by the stellar magnetic field. This is thought to be strong enough to truncate the disk close to the corotation radius, at which the disk rotates at the same rate as the star. Spectro-interferometric studies in young stellar objects show that hydrogen emission (a well known tracer of accretion activity) mostly comes from a region a few milliarcseconds across, usually located within the dust sublimation radius.sup.1-3. The origin of the hydrogen emission could be the stellar magnetosphere, a rotating wind or a disk. In the case of intermediate-mass Herbig AeBe stars, the fact that Brackett [gamma] (Br[gamma]) emission is spatially resolved rules out the possibility that most of the emission comes from the magnetosphere.sup.4-6 because the weak magnetic fields (some tenths of a gauss) detected in these sources.sup.7,8 result in very compact magnetospheres. In the case of T Tauri sources, their larger magnetospheres should make them easier to resolve. The small angular size of the magnetosphere (a few tenths of a milliarcsecond), however, along with the presence of winds.sup.9,10 make the interpretation of the observations challenging. Here we report optical long-baseline interferometric observations that spatially resolve the inner disk of the T Tauri star TW Hydrae. We find that the near-infrared hydrogen emission comes from a region approximately 3.5 stellar radii across. This region is within the continuum dusty disk emitting region (7 stellar radii across) and also within the corotation radius, which is twice as big. This indicates that the hydrogen emission originates in the accretion columns (funnel flows of matter accreting onto the star), as expected in magnetospheric accretion models, rather than in a wind emitted at much larger distance (more than one astronomical unit). The size of the inner disk of the T Tauri star TW Hydrae is determined using optical long-baseline interferometric observations, indicating that hydrogen emission comes from a region approximately 3.5 stellar radii across., Author(s): R. Garcia Lopez [sup.1] [sup.1] [sup.2] [sup.3] , A. Natta [sup.2] , A. Caratti o Garatti [sup.1] [sup.2] [sup.3] , T. P. Ray [sup.2] , R. Fedriani [sup.2] [sup.4] [...]
Published: 2020
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20. Rivaroxaban or aspirin for patent foramen ovale and embolic stroke of undetermined source: a prespecified subgroup analysis from the NAVIGATE ESUS trial

Author: Abdelhamid, N, Abdul Rahman, D, Abdul-Saheb, M, Abreu, P, Abroskina, M, Abu Ahmad, F, Accassat, S, Acciaresi, M, Adami, A, Ahmad, N, Ahmed, F, Alberto Hawkes, M, Alemseged, F, Ali, A, Altavilla, R, Alwis, L, Amarenco, P, Amaro, S, Amaya Sanchez, LE, Amelia Pinto, A, Ameriso, SF, Amin, H, Amino, T, Amjad, AK, Anagnostou, E, Andersen, G, Anderson, C, Anderson, DC, Andrea Falco, M, Andres Mackinnon, F, Andreu, D, Androulakis, M, Angel Gamero, M, Angel Saredo, G, Angeles Diaz, R, Angels Font, M, Anticoli, S, Arauz, A, Arauz Gongora, AA, Araya, P, Arenillas Lara, JF, Arias Rivas, S, Arnold, M, Augustin, S, Avelar, W, Azevedo, E, Babikian, V, Bacellar, A, Badalyan, K, Bae, HJ, Baez Martinez, EM, Bagelmann, H, Bailey, P, Bak, Z, Baker, M, Balazs, A, Baldaranov, D, Balogun, I, Balueva, T, Bankuti, Z, Bar, M, Baranowska, A, Bardutzky, J, Barker Trejo, S, Barlinn, J, Baronnet, F, Barroso, C, Barteys, M, Bartolottiova, T, Barulin, A, Bas, M, Bashir, S, Basile, V, Bathe-Peters, R, Bathula, R, Batista, C, Batur Caglayan, H, Baumgartner, P, Bazan, R, Bazhenova, O, Beaudry, M, Beer, J, Behnam, Y, Beilei, C, Beinlich, A, Bejot, Y, Belkin, A, Benavente, OR, Benjamin, A, Berardi, V, Bereczki, D, Berkowitz, SD, Berlingieri, J, Berrios, W, Berrouschot, J, Bhandari, M, Bhargavah, M, Bicker, H, Bicsak, T, Bilik, M, Bindila, D, Birchenall, J, Birnbaum, L, Black, T, Blacker, D, Blacquiere, D, Blanc-Labarre, C, Blank, C, Blazejewska-Hyzorek, B, Bloch, S, Bodiguel, E, Bogdanov, E, Boos, L, Borcsik, L, Bornstein, N, Bouly, S, Braga, G, Bragado, I, Bravi, MC, Brokalaki, C, Brola, W, Brouns, R, Bruce, D, Brzoska-Mizgalska, J, Buck, B, Buksinska-Lisik, M, Burke, J, Burn, M, Bustamante, G, Cabrejo, L, Cai, K, Cajaraville, S, Calejo, M, Calvet, D, Campillo, J, Campos Costa, E, Camps, P, Can Alaydin, H, Candeloro, E, Canepa, C, Cantu Brito, CG, Cappellari, M, Carcel, C, Cardona Portela, P, Cardoso, F, Carek, M, Carletti, M, Carlos Portilla, J, Caruso, P, Casado-Naranjo, I, Castellini, P, Castro, D, Castro Meira, F, Cavallini, A, Cayuela Caudevilla, N, Cenciarelli, S, Cereda, C, Cerrone, P, Chakrabarti, A, Chaloulos-Iakovidis, P, Chamorro, A, Chandrasena, D, Chang, DI, Che, C, Chembala, J, Chen, J, Chen, Z, Chen, T, Chen, H, Chen, X, Chen, G, Chen, L, Chen, S, Cheripelli, B, Chin, M, Chiquete Anaya, E, Chorazy, M, Christensen, H, Christensen, T, Christian, L, Chu, F, Chung, CS, Clark, W, Clarke, R, Claverie, S, Clemente Agostoni, E, Clissold, B, Coelho, J, Cohen, D, Colakoglu, S, Collas, D, Condurso, R, Connolly, SJ, Consoli, D, Constantin, C, Constantino Silva, AB, Contardo, L, Corlobe, A, Correia, M, Correia, C, Cortijo Garcia, E, Coull, B, Coutts, S, Coveney, S, Cras, P, Crols, R, Crozier, S, Csanyi, A, Csiba, L, Csontos, K, Csuha, R, Cui, L, Cunha, L, Curtze, S, Czerska, M, Czlonkowska, A, Czurko, M, Czuryszkiewicz, M, Dagnino, M, Dai, C, Daineko, A, Dalek, G, Damgaard, D, Danese, A, Dani, K, Danku, V, Dario Toledo, W, Dávalos, A, De Havenon, A, De Keyser, J, De Klippel, N, De La Torre, J, De Pauw, A, De Smedt, A, De Torres, R, De Vries Basson, MM, Dearborn, J, Deganutto, R, Degeorgia, M, Deguchi, I, Del Giudice, A, Delcourt, C, Delgado-Mederos, R, Della Marca, G, Delpont, B, Deltour, S, Demets, DL, Dennis, M, Desai, J, Devine, J, Dhollander, I, Di Mascio, MT, Diaconu, M, Diaz Otero, F, Dietzel, J, Diez-Tejedor, E, Ding, N, Ding, J, Diomedi, M, Dioszeghy, P, Distefano, M, Domigo, V, Dorodnicov, E, Dossi, D, Doubal, F, Druzenko, I, Du, P, Du, J, Duman, T, Duodu, Y, Dutta, D, Dylewicz, L, Eckstein, J, Ehrensperger, E, Ehrlich, S, Einer Allende, G, Elena Halac, B, Elyas, S, Endres, M, Engelbrecht, JM, Engelter, S, Epinat, M, Eren, F, Esbjornsson, M, Escribano, B, Escudero, I, Esisi, B, Essa, B, Esterbauer, M, Evans, N, Eveson, D, Fabio, S, Fang, L, Fanta, S, Fares, M, Fatar, M, Faust, K, Favate, A, Fazekas, F, Federica Denaro, M, Fedin, A, Felipe Amaya, P, Feng, J, Ferencova, K, Fernanda Gilli, M, Fernandez, MD, Fernandez Pirrone, PN, Fernandez Vera, J, Ferrari, J, Ferreira, A, Ferreira Junior, G, Fidler, M, Field, D, Field, T, Figueroa, C, Fiksa, J, Filipov, A, Firstenfeld, A, Fisch, L, Fischer, U, Fisselier, M, Fiszer, U, Fluri, F, Fortea, G, Fotherby, K, Fraczek, A, France, E, Freitas, G, Frey, S, Frick, M, Friedman, A, Friedrich, M, Frisullo, G, Fryze, W, Fuentes Gimeno, B, Fujigasaki, H, Fukuyama, K, Furlan, A, Furlanis, G, Furnace, J, Gabriel, M, Gabriel Reich, E, Gagliardi, RJ, Galati, F, Galli Giqueauk, E, Gallina, A, Gallinella, E, Gallo, J, Gangadharan, S, Gao, Y, Garcia Lopez, R, Garcia Pastor, A, Garcia Sanchez, SM, Garnauf, M, Garnier, P, Gasecki, D, Gasic, K, Gasiorek, K, Gasser, S, Gaugg, M, Gebreyohanns, M, Gebura, K, Geng, J, Geniz Clavijo, M, Georg Haeusler, K, Geran, R, Geremek, M, Gerocs, Z, Ghia, D, Giannandrea, D, Giatsidis, F, Gien Lopez, JA, Gil Nunez, A, Gimenez, L, Giralt, E, Glabinski, A, Gladstone, D, Gliem, M, Gluszkiewicz, M, Goddeau, R, Gogoleva, E, Gokce, M, Goldemund, D, Golikov, K, Gomes Neto, A, Gomez Schneider, M, Gomez-Choco, M, Gomis, M, Gongora-Rivera, JF, Gonysheva, Y, Gonzalez, L, Gonzalez Toledo, ME, Gottschal, M, Gozdzik, I, Grabowski, S, Graf, S, Green, D, Greer, D, Gregorio, T, Greisenegger, S, Greshnova, I, Griebe, M, Grzesik, M, Guan, J, Guarda, S, Gueguen, A, Guidoux, C, Guillermo Povedano, P, Guillon, B, Guiraudg, V, Gunathilagan, G, Guryanova, N, Gusev, V, Gustavo Persi, G, Gutiérrez, R, Guyler, P, Gyuker, N, Hachinski, V, Hajas, A, Hallevi, H, Hankey, G, Hankey, GJ, Hanouskova, L, Hao, L, Haraguchi, K, Haralur Sreekantaiah, Y, Haratz, S, Hargroves, D, Harkness, K, Harmel, P, Harrasser, M, Hart, RG, Harvey, M, Hasan, R, Hasegawa, Y, Hassan, A, Hattori, M, Hatzitolios, A, Hauk, M, Hayashi, T, Hayhoe, H, Hedna, VS, Heine, M, Held, V, Hellwig, S, Henkner, J, Henninger, N, Hermans, S, Hernandez, J, Herrero, D, Hervieu-Begue, M, Herzig, R, Hicken, L, Hieber, M, Hill, M, Hirose, M, Hobeanu, MC, Hobson, B, Hochstetter, M, Hoe Heo, J, Hoffmann, M, Holmstedt, C, Hon, P, Hong, KS, Honma, Y, Horev, A, Horgan, G, Horvath, L, Horvath, M, Hoyer, C, Huang, D, Huang, H, Huber, B, Huhtakangas, J, Hussain, M, Igarashi, S, Iglesias Mohedano, AM, Ignacio Tembl, J, Impellizzeri, M, Inanc, Y, Ioli, P, Irina Aniculaesei, A, Ishida, K, Itabashi, R, Iversen, H, Jagolino, A, Jakab, K, Jander, S, Janka, H, Jankovych, J, Jansen, J, Jasek, L, Javier Alet, M, Javor, L, Jin, X, Jing, P, Joachim, B, Joan Macleod, M, Johnson, M, Jose Martin, J, Joyner, C, Judit Szabo, K, Jun-Oconnell, A, Jura, R, Kaczorowska, B, Kadlcikova, J, Kahles, T, Kakaletsis, N, Kakuk, I, Kalinowska, K, Kaminska, K, Kaneko, C, Kanellos, I, Kapeller, P, Kapica-Topczewska, K, Karasz, O, Karlinski, M, Karlsson, JE, Kasa, K, Kashaeva, E, Kasner, SE, Kaste, M, Kasza, J, Katalin Iljicsov, A, Katsurayama, M, Kaur, S, Kawanishi, M, Kaygorodtseva, S, Ke, K, Kei, A, Keilitz, J, Kellner, J, Kelly, P, Kelly, S, Kemlink, D, Kerekgyarto, M, Keskinarkaus, I, Khairutdinova, D, Khanna, A, Khaw, A, Kholopov, M, Khoumri, C, Kirpicheva, S, Kirshner, H, Kitagawa, K, Kittner, S, Kivioja, R, Klein, F, Kleindorfer, D, Kleinig, T, Klivenyi, P, Knecht, S, Kobayashi, Y, Kobayashi, A, Koch, M, Koehler, L, Koivu, M, Kolianov, V, Koltsov, I, Kondo, T, Konkov, I, Kopecky, S, Korompoki, E, Korpela, J, Kosarz-Lanczek, K, Koutroubi, A, Kovacs, K, Kovacs, T, Kovacs, H, Kowalczyk, K, Kowalska, M, Krajickova, D, Kral, M, Krarup Hansen, C, Kraska, J, Krebs, S, Krejci, V, Kremer, C, Kreuzpointer, R, Krzyzanowska, M, Kucken, D, Kulakowska, A, Kunzmann, J, Kurenkova, N, Kuris, A, Kurkowska-Jastrzebska, I, Kurtenkova, N, Kurushina, O, Kusnick, G, Kustova, M, Kuwashiro, T, Kwan Cha, J, Lago, A, Lagutenko, M, Lajos, B, Lambeck, J, Lamy, C, Landolfi, A, Lanfranconi, S, Lang, W, Lara Lezama, LB, Lara Rodriguez, B, Largo, T, Lasek-Bal, A, Latte, L, Lauer, V, Lavados, P, Le Bouc, R, Leal Cantu, R, Lechner, H, Lecouturier, K, Leder, S, Lee, J, Lee, BC, Leger, A, Leira, E, Leisse, I, Leker, R, Lembo, G, Lenskaya, L, Leyden, J, Li, G, Li, M, Li, S, Li, J, Liamis, G, Liang, H, Liang, Z, Ligot, N, Lin, H, Lindert, R, Lindgren, A, Linna, M, Litwin, T, Liu, K, Liu, X, Llull, L, Lohninger, B, Longoni, M, Loomis, C, Lopes, D, Lopez Fernandez, M, Lopez Garza, N, Lord, A, Louw, S, Lovasz, R, Lowenkopf, T, Lu, Z, Lubke-Detring, SC, Luder, R, Lujan, S, Luo, B, Lupinogina, L, Luschin, G, Lutsep, H, Lvova, A, Ly, J, Grosse, G.M., Ma, H, Ma, C, Machado, M, Machado, C, Macher, S, Machetanz, J, Macian-Montoro, F, Mackey, E, Mackey, A, Maclean, G, Maestre-Moreno, J, Magadan, A, Magyar, T, Mahagney, A, Majid, A, Majjhoo, A, Makaritsis, K, Mandzia, J, Mangas Guijarro, M, Mangion, D, Manios, E, Mann, S, Manning, L, Manno, C, Manuel Garcia, J, Maqueda, V, Mar Castellanos, M, Mar Freijo, M, Marando, C, Marcela Lepera, S, Marcos Couto, J, Maria Bruera, G, Maria Greco, L, Maria Lorenzo, A, Maria Obmann, S, Maria Roa, A, Marini, C, Marinkovic, I, Mario Sumay, G, Mario Torres, C, Marko, M, Markova, S, Markus, H, Marsh, R, Marsili, 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Windt, J, Winkler, A, Winska-Tereszkiewicz, A, Wisniewska, A, Wittayer, M, Wlodek, A, Wojnarowska-Arendt, A, Wolf, M, Wolff, V, Wolter, C, Wong, A, Wook Nah, H, Worthmann, H, Wu, W, Wu, S, Wunderlich, S, Wurzinger, H, Wyse, DG, Xiao, B, Xiaopeng, W, Ximenez-Carrillo, A, Xiong, L, Xiong, Y, Xiong, W, Xu, Y, Xu, J, Xu, Z, Yalo, B, Yamada, T, Yamasaki, M, Yang, L, Yang, Y, Yang, X, Yang, Q, Yang, B, Yang, J, Yasuhiro, I, Yee Lam, M, Yegappan, C, Yip, S, Ylikallio, E, Ylikotila, P, Yongwon Jin, A, Yoon, BW, Yoshida, Y, Yperzeele, L, Yuan, H, Yuasa, H, Zalewska, J, Zanferrari, C, Zapata, E, Zboznovits, D, Zelenka, I, Zhang, C, Zhang, B, Zhang, S, Zhang, M, Zhang, X, Zhang, J, Zhao, L, Zhirnova, O, Zhou, L, Zielinska-Turek, J, Zinchenko, I, Ziomek, M, Zitzmann, A, Zweifler, R, Zwiernik, J, Kasner, Scott E, Swaminathan, Balakumar, Lavados, Pablo, Sharma, Mukul, Muir, Keith, Veltkamp, Roland, Ameriso, Sebastian F, Endres, Matthias, Lutsep, Helmi, Messé, Steven R, Spence, J David, Nedeltechev, Krassen, Perera, Kanjana, Santo, Gustavo, Olavarria, Veronica, Lindgren, Arne, Bangdiwala, Shrikant, Shoamanesh, Ashkan, Berkowitz, Scott D, Mundl, Hardi, Connolly, Stuart J, and Hart, Robert G
Published: 2018
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21. From Espresso to Codex

Author: Liske, J., Pasquini, L., Bonifacio, P., Bouchy, F., Carswell, R. F., Cristiani, S., Dessauges, M., D'Odorico, S., D'Odorico, V., Grazian, A., Garcia-Lopez, R., Haehnelt, M., Israelian, G., Lovis, C., Martin, E., Mayor, M., Molaro, P., Murphy, M. T., Pepe, F., Queloz, D., Rebolo, R., Udry, S., Vanzella, E., Viel, M., Wiklind, T., Zapatero, M., and Zucker, S.
Subjects: Astrophysics
Abstract: CODEX and ESPRESSO are concepts for ultra-stable, high-resolution spectrographs at the E-ELT and VLT, respectively. Both instruments are well motivated by distinct sets of science drivers. However, ESPRESSO will also be a stepping stone towards CODEX both in a scientific as well as in a technical sense. Here we discuss this role of ESPRESSO with respect to one of the most exciting CODEX science cases, i.e. the dynamical determination of the cosmic expansion history., Comment: To appear in the Proceedings of the Workshop "Science with the VLT in the ELT era", 8-12 October 2007, Garching, A. Moorwood, ed
Published: 2008
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22. The RICH detector of the AMS-02 experiment: status and physics prospects

Author: Pereira, Rui, Aguilar-Benitez, M., Arruda, L., Barao, F., Baret, B., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Borges, J., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Costado, M., Crespo, D., Delgado, C., Diaz, C., Derome, L., Goncalves, P., Garcia-Lopez, R., de la Guia, C., Herrero, A., Lanciotti, E., Laurenti, G., Malinin, A., Mana, C., Marin, J., Mangin-Brinet, M., Martinez, G., Menchaca-Rocha, A., Palomares, C., Pimenta, M., Putze, A., Sallaz-Damaz, Y., Seo, E. S., Sevilla, I., Torrento, A., Vargas-Trevino, M., and Veziant, O.
Subjects: Astrophysics
Abstract: The Alpha Magnetic Spectrometer (AMS), whose final version AMS-02 is to be installed on the International Space Station (ISS) for at least 3 years, is a detector designed to measure charged cosmic ray spectra with energies up to the TeV region and with high energy photon detection capability up to a few hundred GeV. It is equipped with several subsystems, one of which is a proximity focusing RICH detector with a dual radiator (aerogel+NaF) that provides reliable measurements for particle velocity and charge. The assembly and testing of the AMS RICH is currently being finished and the full AMS detector is expected to be ready by the end of 2008. The RICH detector of AMS-02 is presented. Physics prospects are briefly discussed., Comment: 5 pages. Contribution to the 10th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications (Como 2007). Presenter: Rui Pereira
Published: 2008
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23. The CODEX-ESPRESSO experiment: cosmic dynamics, fundamental physics, planets and much more..

Author: Cristiani, S., Avila, G., Bonifacio, P., Bouchy, F., Carswell, B., D'Odorico, S., D'Odorico, V., Delabre, B., Dekker, H., Dessauges, M., Dimarcantonio, P., Garcia-Lopez, R., Grazian, A., Haehnelt, M., Herreros, J. M., Israelian, G., Levshakov, S., Liske, J., Lovis, C., Manescau, A., Martin, E., Mayor, M., Megevand, D., Molaro, P., Murphy, M., Pasquini, L., Pepe, F., Perez, J., Queloz, D., Rebolo, R., Santin, P., Shaver, P., Span, P., Udry, S., Vanzella, E., Viel, M., Zapatero, M. R., Zerbi, F., and Zucker, S.
Subjects: Astrophysics
Abstract: CODEX, a high resolution, super-stable spectrograph to be fed by the E-ELT, the most powerful telescope ever conceived, will for the first time provide the possibility of directly measuring the change of the expansion rate of the Universe with time and much more, from the variability of fundamental constants to the search for other earths. A study for the implementation at the VLT of a precursor of CODEX, dubbed ESPRESSO, is presently carried out by a collaboration including ESO, IAC, INAF, IoA Cambridge and Observatoire de Geneve. The present talk is focused on the cosmological aspects of the experiment., Comment: 6 pages Latex, to appear in the proceedings of `A Century of Cosmology', S. Servolo, August 2007, to be published in Il Nuovo Cimento
Published: 2007
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24. The MAGIC Project: Contributions to ICRC 2007

Author: Albert, J., Aliu, E., Anderhub, H., Antoranz, P., Armada, A., Baixeras, C., Barrio, J. A., Bartko, H., Bastieri, D., Becker, J. K., Bednarek, W., Berger, K., Bigongiari, C., Biland, A., Bock, R. K., Bordas, P., Bosch-Ramon, V., Bretz, T., Britvitch, I., Cabras, G., Camara, M., Carmona, E., Chilingarian, A., Coarasa, J. A., Commichau, S., Contreras, J. L., Cortina, J., Costado, M. T., Curtef, V., Danielyan, V., Dazzi, F., De Angelis, A., Delgado, C., Reyes, R. de los, De Lotto, B., De Maria, M., De Sabata, F., Dorner, D., Doro, M., Errando, M., Fagiolini, M., Ferenc, D., Fernández, E., Firpo, R., Flix, J., Fonseca, M. V., Font, L., Fuchs, M., Galante, N., García-López, R. J., Garczarczyk, M., Gaug, M., Giller, M., Goebel, F., Hakobyan, D., Hayashida, M., Hengstebeck, T., Herrero, A., Höhne, D., Hose, J., Hsu, C. C., Jacon, P., Jogler, T., Kosyra, R., Kranich, D., Kritzer, R., Laille, A., Lindfors, E., Lombardi, S., Longo, F., López, J., López, M., Lorenz, E., Majumdar, P., Maneva, G., Mannheim, K., Mansutti, O., Mariotti, M., Martínez, M., Mazin, D., Merck, C., Meucci, M., Meyer, M., Miranda, J. M., Mirzoyan, R., Mizobuchi, S., Moralejo, A., Nieto, D., Nilsson, K., Ninkovic, J., na-Wilhelmi, E. O, Otte, N., Oya, I., Paneque, D., Paoletti, R., Paredes, J. M., Pasanen, M., Pascoli, D., Pauss, F., Pegna, R., Persic, M., Peruzzo, L., Piccioli, A., Prandini, E., Puchades, N., Raymers, A., Rhode, W., Ribó, M., Rico, J., Rissi, M., Robert, A., Rügamer, S., Saggion, A., Saito, T. Y., Sánchez, A., Sartori, P., Scalzotto, V., Scapin, V., Schmitt, R., Schweizer, T., Shayduk, M., Shinozaki, K., Shore, S. N., Sidro, N., Sillanpää, A., Sobczynska, D., Spanier, F., Stamerra, A., Stark, L. S., Takalo, L., Temnikov, P., Tescaro, D., Teshima, M., Torres, D. F., Turini, N., Vankov, H., Venturini, A., Vitale, V., Wagner, R. M., Wibig, T., Wittek, W., Zandanel, F., Zanin, R., and Zapatero, J.
Subjects: Astrophysics
Abstract: The MAGIC Project: Contributions to ICRC 2007, Merida, Mexico. Contents pages for the Contribution on behalf of the MAGIC Collaboration to the 30th ICRC that took place in July 2007 in Merida, Mexico. The contents are in html form with clickable links to the papers that exist on the Astrophysics archive. We hope that this will make it easier to access the output of the conference in a systematic way. Comments on how useful this is/ how it could be improved should be sent to michela.demaria@iuav.it., Comment: HTML file with clickable links to papers
Published: 2007

25. The AMS-RICH velocity and charge reconstruction

Author: Barao, F., Aguilar-Benitez, M., Arruda, L., Baret, B., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Borges, J., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Costado, M., Crespo, D., Delgado, C., Diaz, C., Derome, L., Goncalves, P., Garcia-Lopez, R., de la Guia, C., Herrero, A., Lanciotti, E., Laurenti, G., Malinin, A., Mana, C., Marin, J., Mangin-Brinet, M., Martinez, G., Menchaca-Rocha, A., Palomares, C., Pereira, R., Pimenta, M., Putze, A., Sallaz-Damaz, Y., Seo, E. S., Sevilla, I., Torrento, A., Vargas-Trevino, M., and Veziant, O.
Subjects: Astrophysics
Abstract: The AMS detector, to be installed on the International Space Station, includes a Ring Imaging Cerenkov detector with two different radiators, silica aerogel (n=1.05) and sodium fluoride (n=1.334). This detector is designed to provide very precise measurements of velocity and electric charge in a wide range of cosmic nuclei energies and atomic numbers. The detector geometry, in particular the presence of a reflector for acceptance purposes, leads to complex Cerenkov patterns detected in a pixelized photomultiplier matrix. The results of different reconstruction methods applied to test beam data as well as to simulated samples are presented. To ensure nominal performances throughout the flight, several detector parameters have to be carefully monitored. The algorithms developed to fulfill these requirements are presented. The velocity and charge measurements provided by the RICH detector endow the AMS spectrometer with precise particle identification capabilities in a wide energy range. The expected performances on light isotope separation are discussed., Comment: Contribution to the ICRC07, Merida, Mexico (2007); Presenter: F. Barao
Published: 2007

26. MAGIC upper limits on the very high energy emission from GRBs

Author: Albert, J., Aliu, E., Anderhub, H., Antoranz, P., Armada, A., Baixeras, C., Barrio, J. A., Bartko, H., Bastieri, D., Becker, J., Bednarek, W., Berger, K., Bigongiari, C., Biland, A., Bock, R. K., Bordas, P., Bosch-Ramon, V., Bretz, T., Britvitch, I., Camara, M., Carmona, E., Chilingarian, A., Ciprini, S., Coarasa, J. A., Commichau, S., Contreras, J. L., Cortina, J., Costado, M. T., Curtef, V., Danielyan, V., Dazzi, F., De Angelis, A., Delgado, C., Reyes, R. de los, De Lotto, B., Domingo-Santamaria, E., Dorner, D., Doro, M., Errando, M., Fagiolini, M., Ferenc, D., Fernandez, E., Firpo, R., Flix, J., Fonseca, M. V., Font, L., Fuchs, M., Galante, N., Garcia-Lopez, R., Garczarczyk, M., Gaug, M., Giller, M., Goebel, F., Hakobyan, D., Hayashida, M., Hengstebeck, T., Herrero, A., Hohne, D., Hose, J., and Hsu, C. C.
Subjects: Astrophysics
Abstract: The fast repositioning system of the MAGIC Telescope has allowed during its first data cycle, between 2005 and the beginning of year 2006, observing nine different GRBs as possible sources of very high energy gammas. These observations were triggered by alerts from Swift, HETE-II, and Integral; they started as fast as possible after the alerts and lasted for several minutes, with an energy threshold varying between 80 and 200 GeV, depending upon the zenith angle of the burst. No evidence for gamma signals was found, and upper limits for the flux were derived for all events, using the standard analysis chain of MAGIC. For the bursts with measured redshift, the upper limits are compatible with a power law extrapolation, when the intrinsic fluxes are evaluated taking into account the attenuation due to the scattering in the Metagalactic Radiation Field (MRF)., Comment: 25 pages, 9 figures, final version accepted by ApJ. Changet title to "MAGIC upped limits on the VERY high energy emission from GRBs", re-organized chapter with description of observation, removed non necessaries figures, added plot of effective area depending on zenith angle, added an appendix explaining the upper limit calculation, added some references
Published: 2006
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27. The Ring Imaging Cherenkov detector (RICH) of the AMS experiment

Author: Barao, F., Benitez, M. Aguilar, Alcaraz, J., Arruda, L., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Brinet, M., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Delgado, C., Diaz, C., Derome, L., Eraud, L., Garcia-Lopez, R. J., Gallin-Martel, L., Giovacchini, F., Goncalves, P., Lanciotti, E., Laurenti, G., Malinine, A., Mana, C., Marin, J., Martinez, G., Menchaca-Rocha, A., Molla, M., Palomares, C., Panniello, M., Pereira, R., Pimenta, M., Protasov, K., Sanchez, E., Seo, E-S., Sevilla, N., Torrento, A., Vargas-Trevino, M., and Veziant, O.
Subjects: Astrophysics
Abstract: The Alpha Magnetic Spectrometer (AMS) experiment to be installed on the International Space Station (ISS) will be equipped with a proximity focusing Ring Imaging Cherenkov (RICH) detector for measuring the electric charge and velocity of the charged cosmic particles. A RICH prototype consisting of 96 photomultiplier units, including a piece of the conical reflector, was built and its performance evaluated with ion beam data. Preliminary results of the in-beam tests performed with ion fragments resulting from collisions of a 158 GeV/c/nuc primary beam of Indium ions (CERN SPS) on a Pb target are reported. The collected data included tests to the final front-end electronics and to different aerogel radiators. Cherenkov rings for a large range of charged nuclei and with reflected photons were observed. The data analysis confirms the design goals. Charge separation up to Fe and velocity resolution of the order of 0.1% for singly charged particles are obtained., Comment: 29th International Conference on Cosmic Rays (Pune, India)
Published: 2006

28. FU Orionis disk outburst: Evidence for a gravitational instability scenario triggered in a magnetically dead zone

Author: Bourdarot, G., primary, Berger, J.-P., additional, Lesur, G., additional, Perraut, K., additional, Malbet, F., additional, Millan-Gabet, R., additional, Le Bouquin, J.-B., additional, Garcia-Lopez, R., additional, Monnier, J. D., additional, Labdon, A., additional, Kraus, S., additional, Labadie, L., additional, and Aarnio, A., additional
Published: 2023
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29. The GRAVITY young stellar object survey: XI. Imaging the hot gas emission around the Herbig Ae star HD58647.

Author: Bouarour, Y.-I., Garcia Lopez, R., Sanchez-Bermudez, J., Caratti o Garatti, A., Perraut, K., Aimar, N., Amorim, A., Berger, J.-P., Bourdarot, G., Brandner, W., Clénet, Y., de Zeeuw, P. T., Dougados, C., Drescher, A., Eckart, A., Eisenhauer, F., Flock, M., Garcia, P., Gendron, E., and Genzel, R.
Subjects: *STARS, *STELLAR radiation, *CIRCUMSTELLAR matter, *GRAVITY, *DUST
Abstract: Aims. We aim to investigate the origin of the HI Brγ emission in young stars by using GRAVITY to image the innermost region of circumstellar disks, where important physical processes such as accretion and winds occur. With high spectral and angular resolution, we focus on studying the continuum and the HI Brγ-emitting area of the Herbig star HD 58647. Methods. Using VLTI-GRAVITY, we conducted observations of HD 58647 with both high spectral and high angular resolution. Thanks to the extensive uv coverage, we were able to obtain detailed images of the circumstellar environment at a sub-au scale, specifically capturing the continuum and the Brγ-emitting region. Through the analysis of velocity-dispersed images and photocentre shifts, we were able to investigate the kinematics of the HI Brγ-emitting region. Results. The recovered continuum images show extended emission where the disk major axis is oriented along a position angle of 14°. The size of the continuum emission at 5-σ levels is ~1.5 times more extended than the sizes reported from geometrical fitting (3.69 mas ± 0.02 mas). This result supports the existence of dust particles close to the stellar surface, screened from the stellar radiation by an optically thick gaseous disk. Moreover, for the first time with GRAVITY, the hot gas component of HD 58647 traced by the Brγ has been imaged. This allowed us to constrain the size of the Brγ-emitting region and study the kinematics of the hot gas; we find its velocity field to be roughly consistent with gas that obeys Keplerian motion. The velocity-dispersed images show that the size of the hot gas emission is from a more compact region than the continuum (2.3 mas ± 0.2 mas). Finally, the line phases show that the emission is not entirely consistent with Keplerian rotation, hinting at a more complex structure in the hot gaseous disk. [ABSTRACT FROM AUTHOR]
Published: 2024
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30. Properties of Cosmic Aluminum Nuclei: Results from the Alpha Magnetic Spectrometer

Author: Liu, Z, Paniccia, M, Zhang, C, Aguilar, M, Ali Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Liu Z., Paniccia M., Zhang C., Aguilar M., Ali Cavasonza L., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Acosta M. V., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Liu, Z, Paniccia, M, Zhang, C, Aguilar, M, Ali Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Liu Z., Paniccia M., Zhang C., Aguilar M., Ali Cavasonza L., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Acosta M. V., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., and Zuccon P.
Abstract: We report the properties of aluminum (Al) nuclei in cosmic rays measured in the rigidity range 2.15 GV to 3.0 TV with 0.51 million nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We observed that above 6 GV the Al spectrum is well described by the weighted sum of the silicon spectrum (primary cosmic rays) and the fluorine spectrum (secondary cosmic rays). The fraction of the primary component increases with rigidity and becomes dominant at highest rigidities. Al/Si abundance ratio at the source is determined independent of cosmic ray propagation.
Published: 2022

31. Observation of Z>2 trapped nuclei by AMS on ISS

Author: Giovacchini, F, Oliva, A, Valencia-Otero, M, Aguilar, M, Ali Cavasonza, L, Allen, M, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Galaktionov, Y, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Kanishev, K, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Lyu, S, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Mo, D, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Piandani, R, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Schulz von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Giovacchini F., Oliva A., Valencia-Otero M., Aguilar M., Ali Cavasonza L., Allen M. S., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Galaktionov Y., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Kanishev K., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Lyu S. S., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Mo D. C., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Piandani R., Plyaskin V., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Schulz von Dratzig A., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Giovacchini, F, Oliva, A, Valencia-Otero, M, Aguilar, M, Ali Cavasonza, L, Allen, M, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Galaktionov, Y, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Kanishev, K, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Lyu, S, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Mo, D, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Piandani, R, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Schulz von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Giovacchini F., Oliva A., Valencia-Otero M., Aguilar M., Ali Cavasonza L., Allen M. S., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Galaktionov Y., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Kanishev K., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Lyu S. S., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Mo D. C., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Piandani R., Plyaskin V., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Schulz von Dratzig A., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., and Zuccon P.
Abstract: The Alpha Magnetic Spectrometer (AMS-02) is a high energy particle physics experiment operating continuously aboard the International Space Station (ISS) since the 19th of May of 2011. A component of trapped Z>2 ions located in the South Atlantic Anomaly (SAA) has been detected traversing the instrument both in down-going and up-going directions.
Published: 2022

32. Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer

Author: Chen, Y, Paniccia, M, Aguilar, M, Ali Cavasonza, L, Allen, M, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beischer, B, Berdugo, J, Bertucci, B, Bindi, V, de Boer, W, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Galaktionov, Y, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Kanishev, K, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Lyu, S, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Mo, D, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Piandani, R, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zimmermann, N, Zuccon, P, Chen Y., Paniccia M., Aguilar M., Ali Cavasonza L., Allen M. S., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beischer B., Berdugo J., Bertucci B., Bindi V., de Boer W., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Galaktionov Y., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Kanishev K., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Lyu S. S., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Mo D. C., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Piandani R., Plyaskin V., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zimmermann N., Zuccon P., Chen, Y, Paniccia, M, Aguilar, M, Ali Cavasonza, L, Allen, M, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beischer, B, Berdugo, J, Bertucci, B, Bindi, V, de Boer, W, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Galaktionov, Y, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Kanishev, K, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Lyu, S, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Mo, D, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Piandani, R, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zimmermann, N, Zuccon, P, Chen Y., Paniccia M., Aguilar M., Ali Cavasonza L., Allen M. S., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beischer B., Berdugo J., Bertucci B., Bindi V., de Boer W., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Galaktionov Y., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Kanishev K., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Lyu S. S., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Mo D. C., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Piandani R., Plyaskin V., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zimmermann N., and Zuccon P.
Abstract: We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62 million iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.
Published: 2022

33. Study of the bipolar jet of the YSO Th 28 with VLT/SINFONI: Jet morphology and H2 emission

Author: Melnikov, S., primary, Boley, P. A., additional, Dmitrienko, N. S., additional, Caratti o Garatti, A., additional, Garcia Lopez, R., additional, Stecklum, B., additional, Eisloeffel, J., additional, and Weigelt, G., additional
Published: 2023
Full Text: View/download PDF

34. Direct discovery of the inner exoplanet in the HD 206893 system

Author: Hinkley, S., primary, Lacour, S., additional, Marleau, G.-D., additional, Lagrange, A.-M., additional, Wang, J. J., additional, Kammerer, J., additional, Cumming, A., additional, Nowak, M., additional, Rodet, L., additional, Stolker, T., additional, Balmer, W.-O., additional, Ray, S., additional, Bonnefoy, M., additional, Mollière, P., additional, Lazzoni, C., additional, Kennedy, G., additional, Mordasini, C., additional, Abuter, R., additional, Aigrain, S., additional, Amorim, A., additional, Asensio-Torres, R., additional, Babusiaux, C., additional, Benisty, M., additional, Berger, J.-P., additional, Beust, H., additional, Blunt, S., additional, Boccaletti, A., additional, Bohn, A., additional, Bonnet, H., additional, Bourdarot, G., additional, Brandner, W., additional, Cantalloube, F., additional, Caselli, P., additional, Charnay, B., additional, Chauvin, G., additional, Chomez, A., additional, Choquet, E., additional, Christiaens, V., additional, Clénet, Y., additional, Coudé du Foresto, V., additional, Cridland, A., additional, Delorme, P., additional, Dembet, R., additional, Drescher, A., additional, Duvert, G., additional, Eckart, A., additional, Eisenhauer, F., additional, Feuchtgruber, H., additional, Galland, F., additional, Garcia, P., additional, Garcia Lopez, R., additional, Gardner, T., additional, Gendron, E., additional, Genzel, R., additional, Gillessen, S., additional, Girard, J. H., additional, Grandjean, A., additional, Haubois, X., additional, Heißel, G., additional, Henning, Th., additional, Hippler, S., additional, Horrobin, M., additional, Houllé, M., additional, Hubert, Z., additional, Jocou, L., additional, Keppler, M., additional, Kervella, P., additional, Kreidberg, L., additional, Lapeyrère, V., additional, Le Bouquin, J.-B., additional, Léna, P., additional, Lutz, D., additional, Maire, A.-L., additional, Mang, F., additional, Mérand, A., additional, Meunier, N., additional, Monnier, J. D., additional, Mouillet, D., additional, Nasedkin, E., additional, Ott, T., additional, Otten, G. P. P. L., additional, Paladini, C., additional, Paumard, T., additional, Perraut, K., additional, Perrin, G., additional, Philipot, F., additional, Pfuhl, O., additional, Pourré, N., additional, Pueyo, L., additional, Rameau, J., additional, Rickman, E., additional, Rubini, P., additional, Rustamkulov, Z., additional, Samland, M., additional, Shangguan, J., additional, Shimizu, T., additional, Sing, D., additional, Straubmeier, C., additional, Sturm, E., additional, Tacconi, L. J., additional, van Dishoeck, E. F., additional, Vigan, A., additional, Vincent, F., additional, Ward-Duong, K., additional, Widmann, F., additional, Wieprecht, E., additional, Wiezorrek, E., additional, Woillez, J., additional, Yazici, S., additional, Young, A., additional, and Zicher, N., additional
Published: 2023
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35. Temporal structures in electron spectra and charge sign effects in galactic cosmic rays

Author: Aguilar, M. (M.), Cavasonza, L. A. (L. Ali), Ambrosi, G. (G.), Arruda, L. (L.), Attig, N. (N.), Bagwell, C. (C.), Barao, F. (F.), Barrin, L. (L.), Bartoloni, A. (A.), Basegmez-du Pree, S. (S.), Battiston, R. (R.), Behlmann, M. (M.), Belyaev, N. (N.), Berdugo, J. (J.), Bertucci, B. (B.), Bindi, V. (V.), Bollweg, K. (K.), Bolster, J. (J.), Borgia, B. (B.), Boschini, M. J. (M. J.), Bourquin, M. (M.), Bueno, E. F. (E. F.), Burger, J. (J.), Burger, W. J. (W. J.), Burmeister, S. (S.), Cai, X. D. (X. D.), Capell, M. (M.), Casaus, J. (J.), Castellini, G. (G.), Cervelli, F. (F.), Chang, Y. H. (Y. H.), Chen, G. M. (G. M.), Chen, G. R. (G. R.), Chen, H. S. (H. S.), Chen, Y. (Y.), Cheng, L. (L.), Chou, H. Y. (H. Y.), Chouridou, S. (S.), Choutko, V. (V.), Chung, C. H. (C. H.), Clark, C. (C.), Coignet, G. (G.), Consolandi, C. (C.), Contin, A. (A.), Corti, C. (C.), Cui, Z. (Z.), Dadzie, K. (K.), Dass, A. (A.), Delgado, C. (C.), Della Torre, S. (S.), Demirkoez, M. B. (M. B.), Derome, L. (L.), Di Falco, S. (S.), Di Felice, V. (V.), Diaz, C. (C.), Dimiccoli, F. (F.), von Doetinchem, P. (P.), Dong, F. (F.), Donnini, F. (F.), Duranti, M. (M.), Egorov, A. (A.), Eline, A. (A.), Faldi, F. (F.), Feng, J. (J.), Fiandrini, E. (E.), Fisher, P. (P.), Formato, V. (V.), Freeman, C. (C.), Gamez, C. (C.), Garcia-Lopez, R. J. (R. J.), Gargiulo, C. (C.), Gast, H. (H.), Gervasi, M. (M.), Giovacchini, F. (F.), Gomez-Coral, D. M. (D. M.), Gong, J. (J.), Goy, C. (C.), Grabski, V. (V.), Grandi, D. (D.), Graziani, M. (M.), Guracho, A. N. (A. N.), Haino, S. (S.), Han, K. C. (K. C.), Hashmani, R. K. (R. K.), He, Z. H. (Z. H.), Heber, B. (B.), Hsieh, T. H. (T. H.), Hu, J. Y. (J. Y.), Incagli, M. (M.), Jang, W. Y. (W. Y.), Jia, Y. (Yi), Jinchi, H. (H.), Karagoez, G. (G.), Khiali, B. (B.), Kim, G. N. (G. N.), Kirn, T. (Th.), Kounina, O. (O.), Kounine, A. (A.), Koutsenko, V. (V.), Krasnopevtsev, D. (D.), Kuhlman, A. (A.), Kulemzin, A. (A.), La Vacca, G. (G.), Laudi, E. (E.), Laurenti, G. (G.), LaVecchia, G. (G.), Lazzizzera, I. (I.), Lee, H. T. (H. T.), Lee, S. C. (S. C.), Li, H. L. (H. L.), Li, J. Q. (J. Q.), Li, M. (M.), Li, Q. (Q.), Li, Q. Y. (Q. Y.), Li, S. (S.), Li, S. L. (S. L.), Li, J. H. (J. H.), Li, Z. H. (Z. H.), Liang, J. (J.), Liang, M. J. (M. J.), Light, C. (C.), Lin, C. H. (C. H.), Lippert, T. (T.), Liu, J. H. (J. H.), Lu, S. Q. (S. Q.), Lu, Y. S. (Y. S.), Luebelsmeyer, K. (K.), Luo, J. Z. (J. Z.), Luo, X. (Xi), Machate, F. (F.), Mana, C. (C.), Marin, J. (J.), Marquardt, J. (J.), Martin, T. (T.), Martinez, G. (G.), Masi, N. (N.), Maurin, D. (D.), Medvedeva, T. (T.), Menchaca-Rocha, A. (A.), Meng, Q. (Q.), Mikhailov, V. V. (V. V.), Molero, M. (M.), Mott, P. (P.), Mussolin, L. (L.), Negrete, J. (J.), Nikonov, N. (N.), Nozzoli, F. (F.), Ocampo-Peleteiro, J. (J.), Oliva, A. (A.), Orcinha, M. (M.), Palermo, M. (M.), Palmonari, F. (F.), Paniccia, M. (M.), Pashnin, A. (A.), Pauluzzi, M. (M.), Pensotti, S. (S.), Plyaskin, V. (V.), Pohl, M. (M.), Poluianov, S. (S.), Qin, X. (X.), Qu, Z. Y. (Z. Y.), Quadrani, L. (L.), Rancoita, P. G. (P. G.), Rapin, D. (D.), Conde, A. R. (A. Reina), Robyn, E. (E.), Rosier-Lees, S. (S.), Rozhkov, A. (A.), Rozza, D. (D.), Sagdeev, R. (R.), Schael, S. (S.), von Dratzig, A. S. (A. Schultz), Schwering, G. (G.), Seo, E. S. (E. S.), Shan, B. S. (B. S.), Siedenburg, T. (T.), Song, J. W. (J. W.), Song, X. J. (X. J.), Sonnabend, R. (R.), Strigari, L. (L.), Su, T. (T.), Sun, Q. (Q.), Sun, Z. T. (Z. T.), Tacconi, M. (M.), Tang, X. W. (X. W.), Tang, Z. C. (Z. C.), Tian, J. (J.), Ting, S. C. (Samuel C. C.), Ting, S. M. (S. M.), Tomassetti, N. (N.), Torsti, J. (J.), Urban, T. (T.), Usoskin, I. (I.), Vagelli, V. (V.), Vainio, R. (R.), Valencia-Otero, M. (M.), Valente, E. (E.), Valtonen, E. (E.), Acosta, M. V. (M. Vazquez), Vecchi, M. (M.), Velasco, M. (M.), Vialle, J. P. (J. P.), Wang, C. X. (C. X.), Wang, L. (L.), Wang, L. Q. (L. Q.), Wang, N. H. (N. H.), Wang, Q. L. (Q. L.), Wang, S. (S.), Wang, X. (X.), Wang, Y. (Yu), Wang, Z. M. (Z. M.), Wei, J. (J.), Weng, Z. L. (Z. L.), Wu, H. (H.), Xiong, R. Q. (R. Q.), Xu, W. (W.), Yan, Q. (Q.), Yang, Y. (Y.), Yashin, I. I. (I. I.), Yelland, A. (A.), Yi, H. (H.), Yu, Y. M. (Y. M.), Yu, Z. Q. (Z. Q.), Zannoni, M. (M.), Zhang, C. (C.), Zhang, F. (F.), Zhang, F. Z. (F. Z.), Zhang, J. H. (J. H.), Zhang, Z. (Z.), Zhao, F. (F.), Zheng, C. (C.), Zheng, Z. M. (Z. M.), Zhuang, H. L. (H. L.), Zhukov, V. (V.), Zichichi, A. (A.), Zuccon, P. (P.), Aguilar, M. (M.), Cavasonza, L. A. (L. Ali), Ambrosi, G. (G.), Arruda, L. (L.), Attig, N. (N.), Bagwell, C. (C.), Barao, F. (F.), Barrin, L. (L.), Bartoloni, A. (A.), Basegmez-du Pree, S. (S.), Battiston, R. (R.), Behlmann, M. (M.), Belyaev, N. (N.), Berdugo, J. (J.), Bertucci, B. (B.), Bindi, V. (V.), Bollweg, K. (K.), Bolster, J. (J.), Borgia, B. (B.), Boschini, M. J. (M. J.), Bourquin, M. (M.), Bueno, E. F. (E. F.), Burger, J. (J.), Burger, W. J. (W. J.), Burmeister, S. (S.), Cai, X. D. (X. D.), Capell, M. (M.), Casaus, J. (J.), Castellini, G. (G.), Cervelli, F. (F.), Chang, Y. H. (Y. H.), Chen, G. M. (G. M.), Chen, G. R. (G. R.), Chen, H. S. (H. S.), Chen, Y. (Y.), Cheng, L. (L.), Chou, H. Y. (H. Y.), Chouridou, S. (S.), Choutko, V. (V.), Chung, C. H. (C. H.), Clark, C. (C.), Coignet, G. (G.), Consolandi, C. (C.), Contin, A. (A.), Corti, C. (C.), Cui, Z. (Z.), Dadzie, K. (K.), Dass, A. (A.), Delgado, C. (C.), Della Torre, S. (S.), Demirkoez, M. B. (M. B.), Derome, L. (L.), Di Falco, S. (S.), Di Felice, V. (V.), Diaz, C. (C.), Dimiccoli, F. (F.), von Doetinchem, P. (P.), Dong, F. (F.), Donnini, F. (F.), Duranti, M. (M.), Egorov, A. (A.), Eline, A. (A.), Faldi, F. (F.), Feng, J. (J.), Fiandrini, E. (E.), Fisher, P. (P.), Formato, V. (V.), Freeman, C. (C.), Gamez, C. (C.), Garcia-Lopez, R. J. (R. J.), Gargiulo, C. (C.), Gast, H. (H.), Gervasi, M. (M.), Giovacchini, F. (F.), Gomez-Coral, D. M. (D. M.), Gong, J. (J.), Goy, C. (C.), Grabski, V. (V.), Grandi, D. (D.), Graziani, M. (M.), Guracho, A. N. (A. N.), Haino, S. (S.), Han, K. C. (K. C.), Hashmani, R. K. (R. K.), He, Z. H. (Z. H.), Heber, B. (B.), Hsieh, T. H. (T. H.), Hu, J. Y. (J. Y.), Incagli, M. (M.), Jang, W. Y. (W. Y.), Jia, Y. (Yi), Jinchi, H. (H.), Karagoez, G. (G.), Khiali, B. (B.), Kim, G. N. (G. N.), Kirn, T. (Th.), Kounina, O. (O.), Kounine, A. (A.), Koutsenko, V. (V.), Krasnopevtsev, D. (D.), Kuhlman, A. (A.), Kulemzin, A. (A.), La Vacca, G. (G.), Laudi, E. (E.), Laurenti, G. (G.), LaVecchia, G. (G.), Lazzizzera, I. (I.), Lee, H. T. (H. T.), Lee, S. C. (S. C.), Li, H. L. (H. L.), Li, J. Q. (J. Q.), Li, M. (M.), Li, Q. (Q.), Li, Q. Y. (Q. Y.), Li, S. (S.), Li, S. L. (S. L.), Li, J. H. (J. H.), Li, Z. H. (Z. H.), Liang, J. (J.), Liang, M. J. (M. J.), Light, C. (C.), Lin, C. H. (C. H.), Lippert, T. (T.), Liu, J. H. (J. H.), Lu, S. Q. (S. Q.), Lu, Y. S. (Y. S.), Luebelsmeyer, K. (K.), Luo, J. Z. (J. Z.), Luo, X. (Xi), Machate, F. (F.), Mana, C. (C.), Marin, J. (J.), Marquardt, J. (J.), Martin, T. (T.), Martinez, G. (G.), Masi, N. (N.), Maurin, D. (D.), Medvedeva, T. (T.), Menchaca-Rocha, A. (A.), Meng, Q. (Q.), Mikhailov, V. V. (V. V.), Molero, M. (M.), Mott, P. (P.), Mussolin, L. (L.), Negrete, J. (J.), Nikonov, N. (N.), Nozzoli, F. (F.), Ocampo-Peleteiro, J. (J.), Oliva, A. (A.), Orcinha, M. (M.), Palermo, M. (M.), Palmonari, F. (F.), Paniccia, M. (M.), Pashnin, A. (A.), Pauluzzi, M. (M.), Pensotti, S. (S.), Plyaskin, V. (V.), Pohl, M. (M.), Poluianov, S. (S.), Qin, X. (X.), Qu, Z. Y. (Z. Y.), Quadrani, L. (L.), Rancoita, P. G. (P. G.), Rapin, D. (D.), Conde, A. R. (A. Reina), Robyn, E. (E.), Rosier-Lees, S. (S.), Rozhkov, A. (A.), Rozza, D. (D.), Sagdeev, R. (R.), Schael, S. (S.), von Dratzig, A. S. (A. Schultz), Schwering, G. (G.), Seo, E. S. (E. S.), Shan, B. S. (B. S.), Siedenburg, T. (T.), Song, J. W. (J. W.), Song, X. J. (X. J.), Sonnabend, R. (R.), Strigari, L. (L.), Su, T. (T.), Sun, Q. (Q.), Sun, Z. T. (Z. T.), Tacconi, M. (M.), Tang, X. W. (X. W.), Tang, Z. C. (Z. C.), Tian, J. (J.), Ting, S. C. (Samuel C. C.), Ting, S. M. (S. M.), Tomassetti, N. (N.), Torsti, J. (J.), Urban, T. (T.), Usoskin, I. (I.), Vagelli, V. (V.), Vainio, R. (R.), Valencia-Otero, M. (M.), Valente, E. (E.), Valtonen, E. (E.), Acosta, M. V. (M. Vazquez), Vecchi, M. (M.), Velasco, M. (M.), Vialle, J. P. (J. P.), Wang, C. X. (C. X.), Wang, L. (L.), Wang, L. Q. (L. Q.), Wang, N. H. (N. H.), Wang, Q. L. (Q. L.), Wang, S. (S.), Wang, X. (X.), Wang, Y. (Yu), Wang, Z. M. (Z. M.), Wei, J. (J.), Weng, Z. L. (Z. L.), Wu, H. (H.), Xiong, R. Q. (R. Q.), Xu, W. (W.), Yan, Q. (Q.), Yang, Y. (Y.), Yashin, I. I. (I. I.), Yelland, A. (A.), Yi, H. (H.), Yu, Y. M. (Y. M.), Yu, Z. Q. (Z. Q.), Zannoni, M. (M.), Zhang, C. (C.), Zhang, F. (F.), Zhang, F. Z. (F. Z.), Zhang, J. H. (J. H.), Zhang, Z. (Z.), Zhao, F. (F.), Zheng, C. (C.), Zheng, Z. M. (Z. M.), Zhuang, H. L. (H. L.), Zhukov, V. (V.), Zichichi, A. (A.), and Zuccon, P. (P.)
Abstract: We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0 x 10⁸ electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6 sigma at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.
Published: 2023

36. Properties of cosmic-ray sulfur and determination of the composition of primary cosmic-ray carbon, neon, magnesium, and sulfur:ten-year results from the Alpha Magnetic Spectrometer

Author: Aguilar, M. (M.), Cavasonza, L. A. (L. Ali), Alpat, B. (B.), Ambrosi, G. (G.), Arruda, L. (L.), Attig, N. (N.), Bagwell, C. (C.), Barao, F. (F.), Barrin, L. (L.), Bartoloni, A. (A.), Basegmez-du Pree, S. (S.), Battiston, R. (R.), Belyaev, N. (N.), Berdugo, J. (J.), Bertucci, B. (B.), Bindi, V. (V.), Bollweg, K. (K.), Bolster, J. (J.), Borchiellini, M. (M.), Borgia, B. (B.), Boschini, M. J. (M. J.), Bourquin, M. (M.), Bueno, E. F. (E. F.), Burger, J. (J.), Burger, W. J. (W. J.), Cai, X. D. (X. D.), Capell, M. (M.), Casaus, J. (J.), Castellini, G. (G.), Cervelli, F. (F.), Chang, Y. H. (Y. H.), Chen, G. M. (G. M.), Chen, G. R. (G. R.), Chen, H. (H.), Chen, H. S. (H. S.), Chen, Y. (Y.), Cheng, L. (L.), Chou, H. Y. (H. Y.), Chouridou, S. (S.), Choutko, V. (V.), Chung, C. H. (C. H.), Clark, C. (C.), Coignet, G. (G.), Consolandi, C. (C.), Contin, A. (A.), Corti, C. (C.), Cui, Z. (Z.), Dadzie, K. (K.), Dass, A. (A.), Delgado, C. (C.), Della Torre, S. (S.), Demirkoz, M. B. (M. B.), Derome, L. (L.), Di Falco, S. (S.), Di Felice, V. (V.), Diaz, C. (C.), Dimiccoli, F. (F.), von Doetinchem, P. (P.), Dong, F. (F.), Donnini, F. (F.), Duranti, M. (M.), Egorov, A. (A.), Eline, A. (A.), Faldi, F. (F.), Feng, J. (J.), Fiandrini, E. (E.), Fisher, P. (P.), Formato, V. (V.), Gamez, C. (C.), Garcia-Lopez, R. J. (R. J.), Gargiulo, C. (C.), Gast, H. (H.), Gervasi, M. (M.), Giovacchini, F. (F.), Gomez-Coral, D. M. (D. M.), Gong, J. (J.), Goy, C. (C.), Grabski, V. (V.), Grandi, D. (D.), Graziani, M. (M.), Guracho, A. N. (A. N.), Haino, S. (S.), Han, K. C. (K. C.), Hashmani, R. K. (R. K.), He, Z. H. (Z. H.), Heber, B. (B.), Hsieh, T. H. (T. H.), Hu, J. Y. (J. Y.), Huang, B. W. (B. W.), Incagli, M. (M.), Jang, W. Y. (W. Y.), Jia, Y. (Yi), Jinchi, H. (H.), Karagoz, G. (G.), Khiali, B. (B.), Kim, G. N. (G. N.), Kirn, T. (Th.), Kounina, O. (O.), Kounine, A. (A.), Koutsenko, V. (V.), Krasnopevtsev, D. (D.), Kuhlman, A. (A.), Kulemzin, A. (A.), La Vacca, G. (G.), Laudi, E. (E.), Laurenti, G. (G.), LaVecchia, G. (G.), Lazzizzera, I. (I.), Lee, H. T. (H. T.), Lee, S. C. (S. C.), Li, H. L. (H. L.), Li, J. Q. (J. Q.), Li, M. (M.), Li, Q. (Q.), Li, Q. Y. (Q. Y.), Li, S. (S.), Li, S. L. (S. L.), Li, J. H. (J. H.), Li, Z. H. (Z. H.), Liang, J. (J.), Liang, M. J. (M. J.), Lin, C. H. (C. H.), Lippert, T. (T.), Liu, J. H. (J. H.), Lu, S. Q. (S. Q.), Lu, Y. S. (Y. S.), Luebelsmeyer, K. (K.), Luo, J. Z. (J. Z.), Luo, S. D. (S. D.), Luo, X. (Xi), Machate, F. (F.), Mana, C. (C.), Marin, J. (J.), Marquardt, J. (J.), Martin, T. (T.), Martinez, G. (G.), Masi, N. (N.), Maurin, D. (D.), Medvedeva, T. (T.), Menchaca-Rocha, A. (A.), Meng, Q. (Q.), Mikhailov, V. V. (V. V.), Molero, M. (M.), Mott, P. (P.), Mussolin, L. (L.), Negrete, J. (J.), Nikonov, N. (N.), Nozzoli, F. (F.), Ocampo-Peleteiro, J. (J.), Oliva, A. (A.), Orcinha, M. (M.), Ottupara, M. A. (M. A.), Palermo, M. (M.), Palmonari, F. (F.), Paniccia, M. (M.), Pashnin, A. (A.), Pauluzzi, M. (M.), Pensotti, S. (S.), Plyaskin, V. (V.), Poluianov, S. (Stepan), Qin, X. (X.), Qu, Z. Y. (Z. Y.), Quadrani, L. (L.), Rancoita, P. G. (P. G.), Rapin, D. (D.), Conde, A. R. (A. Reina), Robyn, E. (E.), Romaneehsen, L. (L.), Rozhkov, A. (A.), Rozza, D. (D.), Sagdeev, R. (R.), Schael, S. (S.), von Dratzig, A. S. (A. Schultz), Schwering, G. (G.), Seo, E. S. (E. S.), Shan, B. S. (B. S.), Siedenburg, T. (T.), Song, J. W. (J. W.), Song, X. J. (X. J.), Sonnabend, R. (R.), Strigari, L. (L.), Su, T. (T.), Sun, Q. (Q.), Sun, Z. T. (Z. T.), Tacconi, M. (M.), Tang, X. W. (X. W.), Tang, Z. C. (Z. C.), Tian, J. (J.), Tian, Y. (Y.), Ting, S. C. (Samuel C. C.), Urban, T. (T.), Usoskin, I. (Ilya), Vagelli, V. (V.), Vainio, R. (R.), Valencia-Otero, M. (M.), Valente, E. (E.), Valtonen, E. (E.), Acosta, M. V. (M. Vazquez), Vecchi, M. (M.), Velasco, M. (M.), Vialle, J. P. (J. P.), Wang, C. X. (C. X.), Wang, L. (L.), Wang, L. Q. (L. Q.), Wang, N. H. (N. H.), Wang, Q. L. (Q. L.), Wang, S. (S.), Wang, X. (X.), Wang, Y. (Yu), Wang, Z. M. (Z. M.), Wei, J. (J.), Weng, Z. L. (Z. L.), Wu, H. (H.), Wu, Y. (Y.), Xiao, J. N. (J. N.), Xiong, R. Q. (R. Q.), Xiong, X. Z. (X. Z.), Xu, W. (W.), Yan, Q. (Q.), Yang, H. T. (H. T.), Yang, Y. (Y.), Yashin, I. I. (I. I.), Yelland, A. (A.), Yi, H. (H.), You, Y. H. (Y. H.), Yu, Y. M. (Y. M.), Yu, Z. Q. (Z. Q.), Zannoni, M. (M.), Zhang, C. (C.), Zhang, F. (F.), Zhang, F. Z. (F. Z.), Zhang, J. (J.), Zhang, J. H. (J. H.), Zhang, Z. (Z.), Zhao, F. (F.), Zheng, C. (C.), Zheng, Z. M. (Z. M.), Zhuang, H. L. (H. L.), Zhukov, V. (V.), Zichichi, A. (A.), Zuccon, P. (P.), Aguilar, M. (M.), Cavasonza, L. A. (L. Ali), Alpat, B. (B.), Ambrosi, G. (G.), Arruda, L. (L.), Attig, N. (N.), Bagwell, C. (C.), Barao, F. (F.), Barrin, L. (L.), Bartoloni, A. (A.), Basegmez-du Pree, S. (S.), Battiston, R. (R.), Belyaev, N. (N.), Berdugo, J. (J.), Bertucci, B. (B.), Bindi, V. (V.), Bollweg, K. (K.), Bolster, J. (J.), Borchiellini, M. (M.), Borgia, B. (B.), Boschini, M. J. (M. J.), Bourquin, M. (M.), Bueno, E. F. (E. F.), Burger, J. (J.), Burger, W. J. (W. J.), Cai, X. D. (X. D.), Capell, M. (M.), Casaus, J. (J.), Castellini, G. (G.), Cervelli, F. (F.), Chang, Y. H. (Y. H.), Chen, G. M. (G. M.), Chen, G. R. (G. R.), Chen, H. (H.), Chen, H. S. (H. S.), Chen, Y. (Y.), Cheng, L. (L.), Chou, H. Y. (H. Y.), Chouridou, S. (S.), Choutko, V. (V.), Chung, C. H. (C. H.), Clark, C. (C.), Coignet, G. (G.), Consolandi, C. (C.), Contin, A. (A.), Corti, C. (C.), Cui, Z. (Z.), Dadzie, K. (K.), Dass, A. (A.), Delgado, C. (C.), Della Torre, S. (S.), Demirkoz, M. B. (M. B.), Derome, L. (L.), Di Falco, S. (S.), Di Felice, V. (V.), Diaz, C. (C.), Dimiccoli, F. (F.), von Doetinchem, P. (P.), Dong, F. (F.), Donnini, F. (F.), Duranti, M. (M.), Egorov, A. (A.), Eline, A. (A.), Faldi, F. (F.), Feng, J. (J.), Fiandrini, E. (E.), Fisher, P. (P.), Formato, V. (V.), Gamez, C. (C.), Garcia-Lopez, R. J. (R. J.), Gargiulo, C. (C.), Gast, H. (H.), Gervasi, M. (M.), Giovacchini, F. (F.), Gomez-Coral, D. M. (D. M.), Gong, J. (J.), Goy, C. (C.), Grabski, V. (V.), Grandi, D. (D.), Graziani, M. (M.), Guracho, A. N. (A. N.), Haino, S. (S.), Han, K. C. (K. C.), Hashmani, R. K. (R. K.), He, Z. H. (Z. H.), Heber, B. (B.), Hsieh, T. H. (T. H.), Hu, J. Y. (J. Y.), Huang, B. W. (B. W.), Incagli, M. (M.), Jang, W. Y. (W. Y.), Jia, Y. (Yi), Jinchi, H. (H.), Karagoz, G. (G.), Khiali, B. (B.), Kim, G. N. (G. N.), Kirn, T. (Th.), Kounina, O. (O.), Kounine, A. (A.), Koutsenko, V. (V.), Krasnopevtsev, D. (D.), Kuhlman, A. (A.), Kulemzin, A. (A.), La Vacca, G. (G.), Laudi, E. (E.), Laurenti, G. (G.), LaVecchia, G. (G.), Lazzizzera, I. (I.), Lee, H. T. (H. T.), Lee, S. C. (S. C.), Li, H. L. (H. L.), Li, J. Q. (J. Q.), Li, M. (M.), Li, Q. (Q.), Li, Q. Y. (Q. Y.), Li, S. (S.), Li, S. L. (S. L.), Li, J. H. (J. H.), Li, Z. H. (Z. H.), Liang, J. (J.), Liang, M. J. (M. J.), Lin, C. H. (C. H.), Lippert, T. (T.), Liu, J. H. (J. H.), Lu, S. Q. (S. Q.), Lu, Y. S. (Y. S.), Luebelsmeyer, K. (K.), Luo, J. Z. (J. Z.), Luo, S. D. (S. D.), Luo, X. (Xi), Machate, F. (F.), Mana, C. (C.), Marin, J. (J.), Marquardt, J. (J.), Martin, T. (T.), Martinez, G. (G.), Masi, N. (N.), Maurin, D. (D.), Medvedeva, T. (T.), Menchaca-Rocha, A. (A.), Meng, Q. (Q.), Mikhailov, V. V. (V. V.), Molero, M. (M.), Mott, P. (P.), Mussolin, L. (L.), Negrete, J. (J.), Nikonov, N. (N.), Nozzoli, F. (F.), Ocampo-Peleteiro, J. (J.), Oliva, A. (A.), Orcinha, M. (M.), Ottupara, M. A. (M. A.), Palermo, M. (M.), Palmonari, F. (F.), Paniccia, M. (M.), Pashnin, A. (A.), Pauluzzi, M. (M.), Pensotti, S. (S.), Plyaskin, V. (V.), Poluianov, S. (Stepan), Qin, X. (X.), Qu, Z. Y. (Z. Y.), Quadrani, L. (L.), Rancoita, P. G. (P. G.), Rapin, D. (D.), Conde, A. R. (A. Reina), Robyn, E. (E.), Romaneehsen, L. (L.), Rozhkov, A. (A.), Rozza, D. (D.), Sagdeev, R. (R.), Schael, S. (S.), von Dratzig, A. S. (A. Schultz), Schwering, G. (G.), Seo, E. S. (E. S.), Shan, B. S. (B. S.), Siedenburg, T. (T.), Song, J. W. (J. W.), Song, X. J. (X. J.), Sonnabend, R. (R.), Strigari, L. (L.), Su, T. (T.), Sun, Q. (Q.), Sun, Z. T. (Z. T.), Tacconi, M. (M.), Tang, X. W. (X. W.), Tang, Z. C. (Z. C.), Tian, J. (J.), Tian, Y. (Y.), Ting, S. C. (Samuel C. C.), Urban, T. (T.), Usoskin, I. (Ilya), Vagelli, V. (V.), Vainio, R. (R.), Valencia-Otero, M. (M.), Valente, E. (E.), Valtonen, E. (E.), Acosta, M. V. (M. Vazquez), Vecchi, M. (M.), Velasco, M. (M.), Vialle, J. P. (J. P.), Wang, C. X. (C. X.), Wang, L. (L.), Wang, L. Q. (L. Q.), Wang, N. H. (N. H.), Wang, Q. L. (Q. L.), Wang, S. (S.), Wang, X. (X.), Wang, Y. (Yu), Wang, Z. M. (Z. M.), Wei, J. (J.), Weng, Z. L. (Z. L.), Wu, H. (H.), Wu, Y. (Y.), Xiao, J. N. (J. N.), Xiong, R. Q. (R. Q.), Xiong, X. Z. (X. Z.), Xu, W. (W.), Yan, Q. (Q.), Yang, H. T. (H. T.), Yang, Y. (Y.), Yashin, I. I. (I. I.), Yelland, A. (A.), Yi, H. (H.), You, Y. H. (Y. H.), Yu, Y. M. (Y. M.), Yu, Z. Q. (Z. Q.), Zannoni, M. (M.), Zhang, C. (C.), Zhang, F. (F.), Zhang, F. Z. (F. Z.), Zhang, J. (J.), Zhang, J. H. (J. H.), Zhang, Z. (Z.), Zhao, F. (F.), Zheng, C. (C.), Zheng, Z. M. (Z. M.), Zhuang, H. L. (H. L.), Zhukov, V. (V.), Zichichi, A. (A.), and Zuccon, P. (P.)
Abstract: We report the properties of primary cosmic-ray sulfur (S) in the rigidity range 2.15 GV to 3.0 TV based on 0.38 x 10⁶ sulfur nuclei collected by the Alpha Magnetic Spectrometer experiment (AMS). We observed that above 90 GV the rigidity dependence of the S flux is identical to the rigidity dependence of Ne-Mg-Si fluxes, which is different from the rigidity dependence of the He-C-O-Fe fluxes. We found that, similar to N, Na, and Al cosmic rays, over the entire rigidity range, the traditional primary cosmic rays S, Ne, Mg, and C all have sizeable secondary components, and the S, Ne, and Mg fluxes are well described by the weighted sum of the primary silicon flux and the secondary fluorine flux, and the C flux is well described by the weighted sum of the primary oxygen flux and the secondary boron flux. The primary and secondary contributions of the traditional primary cosmic-ray fluxes of C, Ne, Mg, and S (even Z elements) are distinctly different from the primary and secondary contributions of the N, Na, and Al (odd Z elements) fluxes. The abundance ratio at the source for S/Si is 0.167 ± 0.006, for Ne/Si is 0.833 ± 0.025, for Mg/Si is 0.994 ± 0.029, and for C/O is 0.836 ± 0.025. These values are determined independent of cosmic-ray propagation.
Published: 2023

37. Publisher Correction: Measuring the ionisation fraction in a jet from a massive protostar

Author: Fedriani, R., Caratti o Garatti, A., Purser, S. J. D., Sanna, A., Tan, J. C., Garcia-Lopez, R., Ray, T. P., Coffey, D., Stecklum, B., and Hoare, M.
Published: 2019
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38. The Cherenkov Telescope Array potential for the study of young supernova remnants

Author: Acharya, B.S., Aramo, C., Babic, A., Barrio, J.A., Baushev, A., Becker Tjus, J., Berge, D., Bohacova, M., Bonardi, A., Brown, A., Bugaev, V., Bulik, T., Burton, M., Busetto, G., Caraveo, P., Carosi, R., Carr, J., Chadwick, P., Chudoba, J., Conforti, V., Connaughton, V., Contreras, J.L., Cotter, G., Dazzi, F., De Franco, A., de la Calle, I., de los Reyes Lopez, R., De Lotto, B., De Palma, F., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Dournaux, J.-L., Dwarkadas, V., Ebr, J., Egberts, K., Fesquet, M., Fleischhack, H., Font, L., Fontaine, G., Förster, A., Fuessling, M., Garcia, B., Garcia López, R., Garczarczyk, M., Gargano, F., Garrido, D., Gaug, M., Giglietto, N., Giordano, F., Giuliani, A., Godinovic, N., Gonzalez, M.M., Grabarczyk, T., Hassan, T., Hörandel, J., Hrabovsky, M., Hrupec, D., Humensky, T.B., Huovelin, J., Jamrozy, M., Janecek, P., Kaaret, P.E., Katz, U., Kaufmann, S., Khélifi, B., Kluźniak, W., Kocot, J., Komin, N., Kubo, H., Kushida, J., Lamanna, G., Lee, W.H., Lenain, J.-P., Lohse, T., Lombardi, S., López-Coto, R., López-Oramas, A., Lucarelli, F., Maccarone, M.C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Mazziotta, M.N., Meagher, K., Mirabal, N., Morselli, A., Moulin, E., Niemiec, J., Nievas, M., Nishijima, K., Nosek, D., Nunio, F., Ohishi, M., Ohm, S., Ong, R.A., Orito, R., Otte, N., Palatka, M., Pareschi, G., Pech, M., Persic, M., Pohl, M., Prouza, M., Quirrenbach, A., Rainó, S., Rodriguez Fernandez, G., Romano, P., Rovero, A.C., Rudak, B., Schovanek, P., Shayduk, M., Siejkowski, H., Sillanpää, A., Stefanik, S., Stolarczyk, T., Szanecki, M., Szepieniec, T., Tejedor, L.A., Telezhinsky, I., Teshima, M., Tibaldo, L., Tibolla, O., Tovmassian, G., Travnicek, P., Trzeciak, M., Vallania, P., van Eldik, C., Vercellone, S., Vigorito, C., Wagner, S.J., Wakely, S.P., Weinstein, A., Wierzcholska, A., Wilhelm, A., Wojcik, P., and Yoshikoshi, T.
Published: 2015
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39. ESPRESSO: A High Resolution Spectrograph for the Combined Coudé Focus of the VLT

Author: Pasquini, Luca, Manescau, A., Avila, G., Delabre, B., Dekker, H., Liske, J., D’Odorico, S., Pepe, F., Dessauges, M., Lovis, C., Megevand, D., Queloz, D., Udry, S., Cristiani, S., Bonifacio, P., Dimarcantonio, P., D’Odorico, V., Molaro, P., Vanzella, E., Viel, M., Haehnelt, M., Carswell, B., Murphy, M., Garcia-Lopez, R., Herreros, J. M., Perez, J., Zapatero, M. R., Rebolo, R., Israelian, G., Martin, E., Zerbi, F., Spanò, P., Levshakov, S., Santos, N., Zucker, S., Burton, W. B., editor, Christensen, Lars Lindberg, editor, and Moorwood, Alan, editor
Published: 2009
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40. From ESPRESSO to CODEX

Author: Liske, J., Pasquini, L., Bonifacio, P., Bouchy, F., Carswell, R. F., Cristiani, S., Dessauges, M., D’Odorico, S., D’Odorico, V., Grazian, A., Garcia-Lopez, R., Haehnelt, M., Israelian, G., Lovis, C., Martin, E., Mayor, M., Molaro, P., Murphy, M. T., Pepe, F., Queloz, D., Rebolo, R., Udry, S., Vanzella, E., Viel, M., Wiklind, T., Zapatero, M., Zucker, S., Burton, W. B., editor, Christensen, Lars Lindberg, editor, and Moorwood, Alan, editor
Published: 2009
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41. Constraining the nature of the PDS 70 protoplanets with VLTI/GRAVITY

Author: Wang, JJ, Vigan, A, Lacour, S, Nowak, M, Stolker, T, De Rosa, RJ, Ginzburg, S, Gao, P, Abuter, R, Amorim, A, Asensio-Torres, R, Bauböck, M, Benisty, M, Berger, JP, Beust, H, Beuzit, JL, Blunt, S, Boccaletti, A, Bohn, A, Bonnefoy, M, Bonnet, H, Brandner, W, Cantalloube, F, Caselli, P, Charnay, B, Chauvin, G, Choquet, E, Christiaens, V, Clénet, Y, Coudé Du Foresto, V, Cridland, A, De Zeeuw, PT, Dembet, R, Dexter, J, Drescher, A, Duvert, G, Eckart, A, Eisenhauer, F, Facchini, S, Gao, F, Garcia, P, Garcia Lopez, R, Gardner, T, Gendron, E, Genzel, R, Gillessen, S, Girard, J, Haubois, X, Heißel, G, Henning, T, Hinkley, S, Hippler, S, Horrobin, M, Houllé, M, Hubert, Z, Jiménez-Rosales, A, Jocou, L, Kammerer, J, Keppler, M, Kervella, P, Meyer, M, Kreidberg, L, Lagrange, AM, Lapeyrère, V, Le Bouquin, JB, Léna, P, Lutz, D, Maire, AL, Ménard, F, Mérand, A, Mollière, P, Monnier, JD, Mouillet, D, Müller, A, Nasedkin, E, Ott, T, Otten, GPPL, Paladini, C, Paumard, T, Perraut, K, Perrin, G, Pfuhl, O, Pueyo, L, Rameau, J, Rodet, L, Rodríguez-Coira, G, Rousset, G, Scheithauer, S, Shangguan, J, Shimizu, T, Stadler, J, Straub, O, Straubmeier, C, Sturm, E, Tacconi, LJ, Van Dishoeck, EF, Vincent, F, Von Fellenberg, SD, Ward-Duong, K, Widmann, F, Wang, JJ [0000-0003-0774-6502], Vigan, A [0000-0002-5902-7828], Lacour, S [0000-0002-6948-0263], Stolker, T [0000-0002-5823-3072], De Rosa, RJ [0000-0002-4918-0247], Gao, P [0000-0002-8518-9601], Asensio-Torres, R [0000-0003-2990-0726], Benisty, M [0000-0002-7695-7605], Beuzit, JL [0000-0002-7391-479X], Blunt, S [0000-0002-3199-2888], Bohn, A [0000-0003-1401-9952], Bonnefoy, M [0000-0001-5579-5339], Brandner, W [0000-0003-1939-6351], Caselli, P [0000-0003-1481-7911], Charnay, B [0000-0003-0977-6545], Choquet, E [0000-0002-9173-0740], Christiaens, V [0000-0002-0101-8814], Clénet, Y [0000-0002-8382-2020], De Zeeuw, PT [0000-0003-4175-3474], Dexter, J [0000-0003-3903-0373], Eckart, A [0000-0001-6049-3132], Facchini, S [0000-0003-4689-2684], Gao, F [0000-0002-2581-9114], Garcia Lopez, R [0000-0002-2144-0991], Gardner, T [0000-0002-3003-3183], Genzel, R [0000-0002-2767-9653], Gillessen, S [0000-0002-5708-0481], Girard, J [0000-0001-8627-0404], Henning, T [0000-0002-1493-300X], Hinkley, S [0000-0001-8074-2562], Hippler, S [0000-0002-3912-6108], Horrobin, M [0000-0001-5451-7847], Kervella, P [0000-0003-0626-1749], Meyer, M [0000-0003-1227-3084], Kreidberg, L [0000-0003-0514-1147], Le Bouquin, JB [0000-0002-0493-4674], Lutz, D [0000-0003-0291-9582], Maire, AL [0000-0002-2591-4138], Mérand, A [0000-0002-1637-7393], Monnier, JD [0000-0002-3380-3307], Ott, T [0000-0003-1572-0396], Paumard, T [0000-0003-0655-0452], Perrin, G [0000-0003-0680-0167], Rameau, J [0000-0003-0029-0258], Rodríguez-Coira, G [0000-0002-4177-6433], Shangguan, J [0000-0002-4569-9009], Shimizu, T [0000-0002-2125-4670], Straub, O [0000-0001-5755-0677], Straubmeier, C [0000-0002-0671-9302], Sturm, E [0000-0002-0018-3666], Tacconi, LJ [0000-0002-1485-9401], Van Dishoeck, EF [0000-0001-7591-1907], Vincent, F [0000-0002-3855-0708], Von Fellenberg, SD [0000-0002-9156-2249], Ward-Duong, K [0000-0002-4479-8291], and Apollo - University of Cambridge Repository
Subjects: Orbit determination, Exoplanet formation, Long baseline interferometry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics, Exoplanet atmospheres
Abstract: We present K-band interferometric observations of the PDS 70 protoplanets along with their host star using VLTI/GRAVITY. We obtained K-band spectra and 100 $\mu$as precision astrometry of both PDS 70 b and c in two epochs, as well as spatially resolving the hot inner disk around the star. Rejecting unstable orbits, we found a nonzero eccentricity for PDS 70 b of $0.17 \pm 0.06$, a near-circular orbit for PDS 70 c, and an orbital configuration that is consistent with the planets migrating into a 2:1 mean motion resonance. Enforcing dynamical stability, we obtained a 95% upper limit on the mass of PDS 70 b of 10 $M_\textrm{Jup}$, while the mass of PDS 70 c was unconstrained. The GRAVITY K-band spectra rules out pure blackbody models for the photospheres of both planets. Instead, the models with the most support from the data are planetary atmospheres that are dusty, but the nature of the dust is unclear. Any circumplanetary dust around these planets is not well constrained by the planets' 1-5 $\mu$m spectral energy distributions (SEDs) and requires longer wavelength data to probe with SED analysis. However with VLTI/GRAVITY, we made the first observations of a circumplanetary environment with sub-au spatial resolution, placing an upper limit of 0.3~au on the size of a bright disk around PDS 70 b.
Published: 2022
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42. Observation of Z>2 trapped nuclei by AMS on ISS

Author: Giovacchini, F., Oliva, A., Valencia-Otero, M., Aguilar, M., Ali Cavasonza, L., Allen, M. S., Alpat, B., Ambrosi, G., Arruda, L., Attig, N., Barao, F., Barrin, L., Bartoloni, A., Basegmez-Du Pree, S., Battiston, R., Behlmann, M., Beranek, B., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Borgia, B., Boschini, M. J., Bourquin, M., Bueno, E. F., Burger, J., Burger, W. J., Burmeister, S., Cai, X. D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y. H., Chen, G. M., Chen, G. R., Chen, H. S., Chen, Y., Cheng, L., Chou, H. Y., Chouridou, S., Choutko, V., Chung, C. H., Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., Delgado, C., Della Torre, S., Demirkoz, M. B., Derome, L., Di Falco, S., Di Felice, V., Diaz, C., Dimiccoli, F., von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Freeman, C., Galaktionov, Y., Gamez, C., Garcia-Lopez, R. J., Gargiulo, C., Gast, H., Gervasi, M., Gomez-Coral, D. M., Gong, J., Goy, C., Grabski, V., Grandi, D., Graziani, M., Haino, S., Han, K. C., Hashmani, R. K., Z. H., He, Heber, B., Hsieh, T. H., J. Y., Hu, Incagli, M., Jang, W. Y., Jia, Y., Jinchi, H., Kanishev, K., Khiali, B., Kim, G. N., Kirn, Th., Konyushikhin, M., Kounina, O., Kounine, A., Koutsenko, V., Kuhlman, A., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., Lazzizzera, I., Lebedev, A., Lee, H. T., Lee, S. C., J. Q., Li, Li, M., Li, Q., Li, S., J. H., Li, Z. H., Li, Liang, J., Light, C., Lin, C. H., Lippert, T., Liu, J. H., Liu, Z., S. Q., Lu, Y. S., Lu, Luebelsmeyer, K., Luo, J. Z., Luo, X., Lyu, S. S., Machate, F., Mana, C., Marin, J., Marquardt, J., Martin, T., Martinez, G., Masi, N., Maurin, D., Menchaca-Rocha, A., Meng, Q., Mikhailov, V. V., D. C., Mo, Molero, M., Mott, P., Mussolin, L., Negrete, J., Nikonov, N., Nozzoli, F., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Phan, H. D., Piandani, R., Plyaskin, V., Poluianov, S., Qin, X., Z. Y., Qu, Quadrani, L., Rancoita, P. G., Rapin, D., Reina Conde, A., Robyn, E., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, S., Schulz von Dratzig, A., Schwering, G., Seo, E. S., Shakfa, Z., Shan, B. S., Siedenburg, T., Song, J. W., Song, X. J., Sonnabend, R., Strigari, L., Su, T., Sun, Q., Sun, Z. T., Tacconi, M., Tang, X. W., Tang, Z. C., Tian, J., Ting, S. C. C., Ting, S. M., Tomassetti, N., Torsti, J., Tuysuz, C., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valente, E., Valtonen, E., Vazquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J. P., Wang, C. X., Wang, L., Wang, L. Q., Wang, N. H., Wang, Q. L., Wang, S., Wang, X., Wang, Y., Wang, Z. M., Wei, J., Weng, Z. L., Wu, H., Xiong, R. Q., Xu, W., Yan, Q., Yang, Y., Yashin, I. I., Yi, H., Y. M., Yu, Z. Q., Yu, Zannoni, M., Zhang, C., Zhang, F., Zhang, F. Z., Zhang, J. H., Zhang, Z., Zhao, F., Zheng, C., Zheng, Z. M., Zhuang, H. L., Zhukov, V., Zichichi, A., Zuccon, P., Giovacchini, F, Oliva, A, Valencia-Otero, M, Aguilar, M, Ali Cavasonza, L, Allen, M, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Galaktionov, Y, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Kanishev, K, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Lyu, S, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Mo, D, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Piandani, R, Plyaskin, V, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Schulz von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, and Zuccon, P
Subjects: FIS/05 - ASTRONOMIA E ASTROFISICA, Alpha magnetic spectrometer, South atlantic anomalies, International Space station, High-energy particle physic, Particle physics experiment
Abstract: The Alpha Magnetic Spectrometer (AMS-02) is a high energy particle physics experiment operating continuously aboard the International Space Station (ISS) since the 19th of May of 2011. A component of trapped Z>2 ions located in the South Atlantic Anomaly (SAA) has been detected traversing the instrument both in down-going and up-going directions.
Published: 2022

43. Properties of Cosmic Aluminum Nuclei: Results from the Alpha Magnetic Spectrometer

Author: Liu Z., Paniccia M., Zhang C., Aguilar M., Ali Cavasonza L., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn Th., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Reina Conde A., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Acosta M. V., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Liu, Z, Paniccia, M, Zhang, C, Aguilar, M, Ali Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Reina Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, and Zuccon, P
Subjects: FIS/05 - ASTRONOMIA E ASTROFISICA, Rigidity, Space stations, Cosmic ray, Particle spectrometer, Cosmology
Abstract: We report the properties of aluminum (Al) nuclei in cosmic rays measured in the rigidity range 2.15 GV to 3.0 TV with 0.51 million nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We observed that above 6 GV the Al spectrum is well described by the weighted sum of the silicon spectrum (primary cosmic rays) and the fluorine spectrum (secondary cosmic rays). The fraction of the primary component increases with rigidity and becomes dominant at highest rigidities. Al/Si abundance ratio at the source is determined independent of cosmic ray propagation.
Published: 2022

44. Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV

Author: Aguilar, M, Cavasonza, L, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Dass, A, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Karagoz, G, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Dass A., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Karagoz G., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Aguilar, M, Cavasonza, L, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Dass, A, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Karagoz, G, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Dass A., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Karagoz G., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., Machate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., and Zuccon P.
Abstract: We present the precision measurement of the daily proton fluxes in cosmic rays from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV based on 5.5×109 protons collected with the Alpha Magnetic Spectrometer aboard the International Space Station. The proton fluxes exhibit variations on multiple timescales. From 2014 to 2018, we observed recurrent flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. The rigidity dependence of the 27-day periodicity is different from the rigidity dependences of 9-day and 13.5-day periods. Unexpectedly, the strength of 9-day and 13.5-day periodicities increases with increasing rigidities up to ~10 GV and ~20 GV, respectively. Then the strength of the periodicities decreases with increasing rigidity up to 100 GV.
Published: 2021

45. Erratum: Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen [Phys. Rev. Lett. 127, 021101 (2021)]

Author: Aguilar, M, Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., MacHate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Aguilar, M, Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., MacHate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., and Zuccon P.
Abstract: This corrects the article DOI: 10.1103/PhysRevLett.127.021101.
Published: 2021

46. Erratum: Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen [Phys. Rev. Lett. 127, 021101 (2021)]

Author: Aguilar M., Aguilar, M, Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., MacHate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., Zuccon P., Aguilar M., Aguilar, M, Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Basegmez-Du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M, Bourquin, M, Bueno, E, Burger, J, Burger, W, Burmeister, S, Cai, X, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y, Chen, G, Chen, H, Chen, Y, Cheng, L, Chou, H, Chouridou, S, Choutko, V, Chung, C, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirkoz, M, Derome, L, Di Falco, S, Di Felice, V, Diaz, C, Dimiccoli, F, Von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gamez, C, Garcia-Lopez, R, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gomez-Coral, D, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K, Hashmani, R, He, Z, Heber, B, Hsieh, T, Hu, J, Incagli, M, Jang, W, Jia, Y, Jinchi, H, Khiali, B, Kim, G, Kirn, T, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H, Lee, S, Li, J, Li, M, Li, Q, Li, S, Li, Z, Liang, J, Light, C, Lin, C, Lippert, T, Liu, J, Liu, Z, Lu, S, Lu, Y, Luebelsmeyer, K, Luo, J, Luo, X, Machate, F, Mana, C, Marin, J, Marquardt, J, Martin, T, Martinez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z, Quadrani, L, Rancoita, P, Rapin, D, Conde, A, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, Von Dratzig, A, Schwering, G, Seo, E, Shakfa, Z, Shan, B, Siedenburg, T, Solano, C, Song, J, Song, X, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z, Tacconi, M, Tang, X, Tang, Z, Tian, J, Ting, S, Tomassetti, N, Torsti, J, Tuysuz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vazquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J, Wang, C, Wang, L, Wang, N, Wang, Q, Wang, S, Wang, X, Wang, Y, Wang, Z, Wei, J, Weng, Z, Wu, H, Xiong, R, Xu, W, Yan, Q, Yang, Y, Yashin, I, Yi, H, Yu, Y, Yu, Z, Zannoni, M, Zhang, C, Zhang, F, Zhang, J, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z, Zhuang, H, Zhukov, V, Zichichi, A, Zuccon, P, Aguilar M., Cavasonza L. A., Alpat B., Ambrosi G., Arruda L., Attig N., Barao F., Barrin L., Bartoloni A., Basegmez-Du Pree S., Battiston R., Behlmann M., Beranek B., Berdugo J., Bertucci B., Bindi V., Bollweg K., Borgia B., Boschini M. J., Bourquin M., Bueno E. F., Burger J., Burger W. J., Burmeister S., Cai X. D., Capell M., Casaus J., Castellini G., Cervelli F., Chang Y. H., Chen G. M., Chen G. R., Chen H. S., Chen Y., Cheng L., Chou H. Y., Chouridou S., Choutko V., Chung C. H., Clark C., Coignet G., Consolandi C., Contin A., Corti C., Cui Z., Dadzie K., Delgado C., Della Torre S., Demirkoz M. B., Derome L., Di Falco S., Di Felice V., Diaz C., Dimiccoli F., Von Doetinchem P., Dong F., Donnini F., Duranti M., Egorov A., Eline A., Feng J., Fiandrini E., Fisher P., Formato V., Freeman C., Gamez C., Garcia-Lopez R. J., Gargiulo C., Gast H., Gervasi M., Giovacchini F., Gomez-Coral D. M., Gong J., Goy C., Grabski V., Grandi D., Graziani M., Haino S., Han K. C., Hashmani R. K., He Z. H., Heber B., Hsieh T. H., Hu J. Y., Incagli M., Jang W. Y., Jia Y., Jinchi H., Khiali B., Kim G. N., Kirn T., Konyushikhin M., Kounina O., Kounine A., Koutsenko V., Krasnopevtsev D., Kuhlman A., Kulemzin A., La Vacca G., Laudi E., Laurenti G., Lazzizzera I., Lebedev A., Lee H. T., Lee S. C., Li J. Q., Li M., Li Q., Li S., Li J. H., Li Z. H., Liang J., Light C., Lin C. H., Lippert T., Liu J. H., Liu Z., Lu S. Q., Lu Y. S., Luebelsmeyer K., Luo J. Z., Luo X., MacHate F., Mana C., Marin J., Marquardt J., Martin T., Martinez G., Masi N., Maurin D., Medvedeva T., Menchaca-Rocha A., Meng Q., Mikhailov V. V., Molero M., Mott P., Mussolin L., Negrete J., Nikonov N., Nozzoli F., Oliva A., Orcinha M., Palermo M., Palmonari F., Paniccia M., Pashnin A., Pauluzzi M., Pensotti S., Phan H. D., Plyaskin V., Pohl M., Poluianov S., Qin X., Qu Z. Y., Quadrani L., Rancoita P. G., Rapin D., Conde A. R., Robyn E., Rosier-Lees S., Rozhkov A., Rozza D., Sagdeev R., Schael S., Von Dratzig A. S., Schwering G., Seo E. S., Shakfa Z., Shan B. S., Siedenburg T., Solano C., Song J. W., Song X. J., Sonnabend R., Strigari L., Su T., Sun Q., Sun Z. T., Tacconi M., Tang X. W., Tang Z. C., Tian J., Ting S. C. C., Ting S. M., Tomassetti N., Torsti J., Tuysuz C., Urban T., Usoskin I., Vagelli V., Vainio R., Valencia-Otero M., Valente E., Valtonen E., Vazquez Acosta M., Vecchi M., Velasco M., Vialle J. P., Wang C. X., Wang L., Wang L. Q., Wang N. H., Wang Q. L., Wang S., Wang X., Wang Y., Wang Z. M., Wei J., Weng Z. L., Wu H., Xiong R. Q., Xu W., Yan Q., Yang Y., Yashin I. I., Yi H., Yu Y. M., Yu Z. Q., Zannoni M., Zhang C., Zhang F., Zhang F. Z., Zhang J. H., Zhang Z., Zhao F., Zheng C., Zheng Z. M., Zhuang H. L., Zhukov V., Zichichi A., and Zuccon P.
Abstract: This corrects the article DOI: 10.1103/PhysRevLett.127.021101.
Published: 2021

47. Codex

Author: Pasquini, Luca, Avila, G., Délabre, B., Dekker, H., D’Odorico, S., Liske, J., Manescau, A., Bonifacio, P., Cristiani, S., D’Odorico, V., Molaro, P., Vanzella, E., Santin, P., Viel, M., Dessauges-Zavadsky, M., Lovis, C., Mayor, M., Pepe, F., Queloz, D., Udry, S., Haehnelt, M., Murphy, M., Garcia-Lopez, R., Bouchy, F., Levshakov, S., Zucker, S., Leibundgut, Bruno, editor, Santos, Nuno C., editor, Pasquini, Luca, editor, Correia, Alexandre C. M., editor, and Romaniello, Martino, editor
Published: 2008
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48. PENELLOPE

Author: Claes, R. A. B., primary, Manara, C. F., additional, Garcia-Lopez, R., additional, Natta, A., additional, Fang, M., additional, Fockter, Z. P., additional, Ábrahám, P., additional, Alcalá, J. M., additional, Campbell-White, J., additional, Caratti o Garatti, A., additional, Covino, E., additional, Fedele, D., additional, Frasca, A., additional, Gameiro, J. F., additional, Herczeg, G. J., additional, Kóspál, Á., additional, Petr-Gotzens, M. G., additional, Rosotti, G., additional, Venuti, L., additional, and Zsidi, G., additional
Published: 2022
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49. Introducing the CTA concept

Author: Acharya, B.S., Actis, M., Aghajani, T., Agnetta, G., Aguilar, J., Aharonian, F., Ajello, M., Akhperjanian, A., Alcubierre, M., Aleksić, J., Alfaro, R., Aliu, E., Allafort, A.J., Allan, D., Allekotte, I., Amato, E., Anderson, J., Angüner, E.O., Antonelli, L.A., Antoranz, P., Aravantinos, A., Arlen, T., Armstrong, T., Arnaldi, H., Arrabito, L., Asano, K., Ashton, T., Asorey, H.G., Awane, Y., Baba, H., Babic, A., Baby, N., Bähr, J., Bais, A., Baixeras, C., Bajtlik, S., Balbo, M., Balis, D., Balkowski, C., Bamba, A., Bandiera, R., Barber, A., Barbier, C., Barceló, M., Barnacka, A., Barnstedt, J., Barres de Almeida, U., Barrio, J.A., Basili, A., Basso, S., Bastieri, D., Bauer, C., Baushev, A., Becerra, J., Becherini, Y., Bechtol, K.C., Becker Tjus, J., Beckmann, V., Bednarek, W., Behera, B., Belluso, M., Benbow, W., Berdugo, J., Berger, K., Bernard, F., Bernardino, T., Bernlöhr, K., Bhat, N., Bhattacharyya, S., Bigongiari, C., Biland, A., Billotta, S., Bird, T., Birsin, E., Bissaldi, E., Biteau, J., Bitossi, M., Blake, S., Blanch Bigas, O., Blasi, P., Bobkov, A., Boccone, V., Boettcher, M., Bogacz, L., Bogart, J., Bogdan, M., Boisson, C., Boix Gargallo, J., Bolmont, J., Bonanno, G., Bonardi, A., Bonev, T., Bonifacio, P., Bonnoli, G., Bordas, P., Borgland, A., Borkowski, J., Bose, R., Botner, O., Bottani, A., Bouchet, L., Bourgeat, M., Boutonnet, C., Bouvier, A., Brau-Nogué, S., Braun, I., Bretz, T., Briggs, M., Bringmann, T., Brook, P., Brun, P., Brunetti, L., Buanes, T., Buckley, J., Buehler, R., Bugaev, V., Bulgarelli, A., Bulik, T., Busetto, G., Buson, S., Byrum, K., Cailles, M., Cameron, R., Camprecios, J., Canestrari, R., Cantu, S., Capalbi, M., Caraveo, P., Carmona, E., Carosi, A., Carr, J., Carton, P.-H., Casanova, S., Casiraghi, M., Catalano, O., Cavazzani, S., Cazaux, S., Cerruti, M., Chabanne, E., Chadwick, P., Champion, C., Chen, A., Chiang, J., Chiappetti, L., Chikawa, M., Chitnis, V.R., Chollet, F., Chudoba, J., Cieślar, M., Cillis, A., Cohen-Tanugi, J., Colafrancesco, S., Colin, P., Colome, J., Colonges, S., Compin, M., Conconi, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J.L., Coppi, P., Corona, P., Corti, D., Cortina, J., Cossio, L., Costantini, H., Cotter, G., Courty, B., Couturier, S., Covino, S., Crimi, G., Criswell, S.J., Croston, J., Cusumano, G., Dafonseca, M., Dale, O., Daniel, M., Darling, J., Davids, I., Dazzi, F., De Angelis, A., De Caprio, V., De Frondat, F., de Gouveia Dal Pino, E.M., de la Calle, I., De La Vega, G.A., de los Reyes Lopez, R., De Lotto, B., De Luca, A., de Mello Neto, J.R.T., de Naurois, M., de Oliveira, Y., de Oña Wilhelmi, E., de Souza, V., Decerprit, G., Decock, G., Deil, C., Delagnes, E., Deleglise, G., Delgado, C., Della Volpe, D., Demange, P., Depaola, G., Dettlaff, A., Di Paola, A., Di Pierro, F., Díaz, C., Dick, J., Dickherber, R., Dickinson, H., Diez-Blanco, V., Digel, S., Dimitrov, D., Disset, G., Djannati-Ataï, A., Doert, M., Dohmke, M., Domainko, W., Dominis Prester, D., Donat, A., Dorner, D., Doro, M., Dournaux, J.-L., Drake, G., Dravins, D., Drury, L., Dubois, F., Dubois, R., Dubus, G., Dufour, C., Dumas, D., Dumm, J., Durand, D., Dyks, J., Dyrda, M., Ebr, J., Edy, E., Egberts, K., Eger, P., Einecke, S., Eleftheriadis, C., Elles, S., Emmanoulopoulos, D., Engelhaupt, D., Enomoto, R., Ernenwein, J.-P., Errando, M., Etchegoyen, A., Evans, P., Falcone, A., Fantinel, D., Farakos, K., Farnier, C., Fasola, G., Favill, B., Fede, E., Federici, S., Fegan, S., Feinstein, F., Ferenc, D., Ferrando, P., Fesquet, M., Fiasson, A., Fillin-Martino, E., Fink, D., Finley, C., Finley, J.P., Fiorini, M., Firpo Curcoll, R., Flores, H., Florin, D., Focke, W., Föhr, C., Fokitis, E., Font, L., Fontaine, G., Fornasa, M., Förster, A., Fortson, L., Fouque, N., Franckowiak, A., Fransson, C., Fraser, G., Frei, R., Albuquerque, I.F.M., Fresnillo, L., Fruck, C., Fujita, Y., Fukazawa, Y., Fukui, Y., Funk, S., Gäbele, W., Gabici, S., Gabriele, R., Gadola, A., Galante, N., Gall, D., Gallant, Y., Gámez-García, J., García, B., Garcia López, R., Gardiol, D., Garrido, D., Garrido, L., Gascon, D., Gaug, M., Gaweda, J., Gebremedhin, L., Geffroy, N., Gerard, L., Ghedina, A., Ghigo, M., Giannakaki, E., Gianotti, F., Giarrusso, S., Giavitto, G., Giebels, B., Gika, V., Giommi, P., Girard, N., Giro, E., Giuliani, A., Glanzman, T., Glicenstein, J.-F., Godinovic, N., Golev, V., Gomez Berisso, M., Gómez-Ortega, J., Gonzalez, M.M., González, A., González, F., González Muñoz, A., Gothe, K.S., Gougerot, M., Graciani, R., Grandi, P., Grañena, F., Granot, J., Grasseau, G., Gredig, R., Green, A., Greenshaw, T., Grégoire, T., Grimm, O., Grube, J., Grudzinska, M., Gruev, V., Grünewald, S., Grygorczuk, J., Guarino, V., Gunji, S., Gyuk, G., Hadasch, D., Hagiwara, R., Hahn, J., Hakansson, N., Hallgren, A., Hamer Heras, N., Hara, S., Hardcastle, M.J., Harris, J., Hassan, T., Hatanaka, K., Haubold, T., Haupt, A., Hayakawa, T., Hayashida, M., Heller, R., Henault, F., Henri, G., Hermann, G., Hermel, R., Herrero, A., Hidaka, N., Hinton, J., Hoffmann, D., Hofmann, W., Hofverberg, P., Holder, J., Horns, D., Horville, D., Houles, J., Hrabovsky, M., Hrupec, D., Huan, H., Huber, B., Huet, J.-M., Hughes, G., Humensky, T.B., Huovelin, J., Ibarra, A., Illa, J.M., Impiombato, D., Incorvaia, S., Inoue, S., Inoue, Y., Ioka, K., Ismailova, E., Jablonski, C., Jacholkowska, A., Jamrozy, M., Janiak, M., Jean, P., Jeanney, C., Jimenez, J.J., Jogler, T., Johnson, T., Journet, L., Juffroy, C., Jung, I., Kaaret, P., Kabuki, S., Kagaya, M., Kakuwa, J., Kalkuhl, C., Kankanyan, R., Karastergiou, A., Kärcher, K., Karczewski, M., Karkar, S., Kasperek, J., Kastana, D., Katagiri, H., Kataoka, J., Katarzyński, K., Katz, U., Kawanaka, N., Kellner-Leidel, B., Kelly, H., Kendziorra, E., Khélifi, B., Kieda, D.B., Kifune, T., Kihm, T., Kishimoto, T., Kitamoto, K., Kluźniak, W., Knapic, C., Knapp, J., Knödlseder, J., Köck, F., Kocot, J., Kodani, K., Köhne, J.-H., Kohri, K., Kokkotas, K., Kolitzus, D., Komin, N., Kominis, I., Konno, Y., Köppel, H., Korohoda, P., Kosack, K., Koss, G., Kossakowski, R., Kostka, P., Koul, R., Kowal, G., Koyama, S., Kozioł, J., Krähenbühl, T., Krause, J., Krawzcynski, H., Krennrich, F., Krepps, A., Kretzschmann, A., Krobot, R., Krueger, P., Kubo, H., Kudryavtsev, V.A., Kushida, J., Kuznetsov, A., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lacombe, K., Lamanna, G., Lande, J., Languignon, D., Lapington, J., Laporte, P., Lavalley, C., Le Flour, T., Le Padellec, A., Lee, S.-H., Lee, W.H., Leigui de Oliveira, M.A., Lelas, D., Lenain, J.-P., Leopold, D.J., Lerch, T., Lessio, L., Lieunard, B., Lindfors, E., Liolios, A., Lipniacka, A., Lockart, H., Lohse, T., Lombardi, S., Lopatin, A., Lopez, M., López-Coto, R., López-Oramas, A., Lorca, A., Lorenz, E., Lubinski, P., Lucarelli, F., Lüdecke, H., Ludwin, J., Luque-Escamilla, P.L., Lustermann, W., Luz, O., Lyard, E., Maccarone, M.C., Maccarone, T.J., Madejski, G.M., Madhavan, A., Mahabir, M., Maier, G., Majumdar, P., Malaguti, G., Maltezos, S., Manalaysay, A., Mancilla, A., Mandat, D., Maneva, G., Mangano, A., Manigot, P., Mannheim, K., Manthos, I., Maragos, N., Marcowith, A., Mariotti, M., Marisaldi, M., Markoff, S., Marszałek, A., Martens, C., Martí, J., Martin, J.-M., Martin, P., Martínez, G., Martínez, F., Martínez, M., Masserot, A., Mastichiadis, A., Mathieu, A., Matsumoto, H., Mattana, F., Mattiazzo, S., Maurin, G., Maxfield, S., Maya, J., Mazin, D., Mc Comb, L., McCubbin, N., McHardy, I., McKay, R., Medina, C., Melioli, C., Melkumyan, D., Mereghetti, S., Mertsch, P., Meucci, M., Michałowski, J., Micolon, P., Mihailidis, A., Mineo, T., Minuti, M., Mirabal, N., Mirabel, F., Miranda, J.M., Mirzoyan, R., Mizuno, T., Moal, B., Moderski, R., Mognet, I., Molinari, E., Molinaro, M., Montaruli, T., Monteiro, I., Moore, P., Moralejo Olaizola, A., Mordalska, M., Morello, C., Mori, K., Mottez, F., Moudden, Y., Moulin, E., Mrusek, I., Mukherjee, R., Munar-Adrover, P., Muraishi, H., Murase, K., Murphy, A., Nagataki, S., Naito, T., Nakajima, D., Nakamori, T., Nakayama, K., Naumann, C., Naumann, D., Naumann-Godo, M., Nayman, P., Nedbal, D., Neise, D., Nellen, L., Neustroev, V., Neyroud, N., Nicastro, L., Nicolau-Kukliński, J., Niedźwiecki, A., Niemiec, J., Nieto, D., Nikolaidis, A., Nishijima, K., Nolan, S., Northrop, R., Nosek, D., Nowak, N., Nozato, A., O’Brien, P., Ohira, Y., Ohishi, M., Ohm, S., Ohoka, H., Okuda, T., Okumura, A., Olive, J.-F., Ong, R.A., Orito, R., Orr, M., Osborne, J., Ostrowski, M., Otero, L.A., Otte, N., Ovcharov, E., Oya, I., Ozieblo, A., Padilla, L., Paiano, S., Paillot, D., Paizis, A., Palanque, S., Palatka, M., Pallota, J., Panagiotidis, K., Panazol, J.-L., Paneque, D., Panter, M., Paoletti, R., Papayannis, A., Papyan, G., Paredes, J.M., Pareschi, G., Parks, G., Parraud, J.-M., Parsons, D., Paz Arribas, M., Pech, M., Pedaletti, G., Pelassa, V., Pelat, D., Perez, M.d.C., Persic, M., Petrucci, P.-O., Peyaud, B., Pichel, A., Pita, S., Pizzolato, F., Platos, Ł., Platzer, R., Pogosyan, L., Pohl, M., Pojmanski, G., Ponz, J.D., Potter, W., Poutanen, J., Prandini, E., Prast, J., Preece, R., Profeti, F., Prokoph, H., Prouza, M., Proyetti, M., Puerto-Gimenez, I., Pühlhofer, G., Puljak, I., Punch, M., Pyzioł, R., Quel, E.J., Quinn, J., Quirrenbach, A., Racero, E., Rajda, P.J., Ramon, P., Rando, R., Rannot, R.C., Rataj, M., Raue, M., Reardon, P., Reimann, O., Reimer, A., Reimer, O., Reitberger, K., Renaud, M., Renner, S., Reville, B., Rhode, W., Ribó, M., Ribordy, M., Richer, M.G., Rico, J., Ridky, J., Rieger, F., Ringegni, P., Ripken, J., Ristori, P.R., Riviére, A., Rivoire, S., Rob, L., Roeser, U., Rohlfs, R., Rojas, G., Romano, P., Romaszkan, W., Romero, G.E., Rosen, S., Rosier Lees, S., Ross, D., Rouaix, G., Rousselle, J., Rousselle, S., Rovero, A.C., Roy, F., Royer, S., Rudak, B., Rulten, C., Rupiński, M., Russo, F., Ryde, F., Sacco, B., Saemann, E.O., Saggion, A., Sahakian, V., Saito, K., Saito, T., Saito, Y., Sakaki, N., Sakonaka, R., Salini, A., Sanchez, F., Sanchez-Conde, M., Sandoval, A., Sandaker, H., Sant’Ambrogio, E., Santangelo, A., Santos, E.M., Sanuy, A., Sapozhnikov, L., Sarkar, S., Sartore, N., Sasaki, H., Satalecka, K., Sawada, M., Scalzotto, V., Scapin, V., Scarcioffolo, M., Schafer, J., Schanz, T., Schlenstedt, S., Schlickeiser, R., Schmidt, T., Schmoll, J., Schovanek, P., Schroedter, M., Schultz, C., Schultze, J., Schulz, A., Schure, K., Schwab, T., Schwanke, U., Schwarz, J., Schwarzburg, S., Schweizer, T., Schwemmer, S., Segreto, A., Seiradakis, J.-H., Sembroski, G.H., Seweryn, K., Sharma, M., Shayduk, M., Shellard, R.C., Shi, J., Shibata, T., Shibuya, A., Shum, E., Sidoli, L., Sidz, M., Sieiro, J., Sikora, M., Silk, J., Sillanpää, A., Singh, B.B., Sitarek, J., Skole, C., Smareglia, R., Smith, A., Smith, D., Smith, J., Smith, N., Sobczyńska, D., Sol, H., Sottile, G., Sowiński, M., Spanier, F., Spiga, D., Spyrou, S., Stamatescu, V., Stamerra, A., Starling, R., Stawarz, Ł., Steenkamp, R., Stegmann, C., Steiner, S., Stergioulas, N., Sternberger, R., Sterzel, M., Stinzing, F., Stodulski, M., Straumann, U., Strazzeri, E., Stringhetti, L., Suarez, A., Suchenek, M., Sugawara, R., Sulanke, K.-H., Sun, S., Supanitsky, A.D., Suric, T., Sutcliffe, P., Sykes, J., Szanecki, M., Szepieniec, T., Szostek, A., Tagliaferri, G., Tajima, H., Takahashi, H., Takahashi, K., Takalo, L., Takami, H., Talbot, G., Tammi, J., Tanaka, M., Tanaka, S., Tasan, J., Tavani, M., Tavernet, J.-P., Tejedor, L.A., Telezhinsky, I., Temnikov, P., Tenzer, C., Terada, Y., Terrier, R., Teshima, M., Testa, V., Tezier, D., Thuermann, D., Tibaldo, L., Tibolla, O., Tiengo, A., Tluczykont, M., Todero Peixoto, C.J., Tokanai, F., Tokarz, M., Toma, K., Torii, K., Tornikoski, M., Torres, D.F., Torres, M., Tosti, G., Totani, T., Toussenel, F., Tovmassian, G., Travnicek, P., Trifoglio, M., Troyano, I., Tsinganos, K., Ueno, H., Umehara, K., Upadhya, S.S., Usher, T., Uslenghi, M., Valdes-Galicia, J.F., Vallania, P., Vallejo, G., van Driel, W., van Eldik, C., Vandenbrouke, J., Vanderwalt, J., Vankov, H., Vasileiadis, G., Vassiliev, V., Veberic, D., Vegas, I., Vercellone, S., Vergani, S., Veyssiére, C., Vialle, J.P., Viana, A., Videla, M., Vincent, P., Vincent, S., Vink, J., Vlahakis, N., Vlahos, L., Vogler, P., Vollhardt, A., von Gunten, H.-P., Vorobiov, S., Vuerli, C., Waegebaert, V., Wagner, R., Wagner, R.G., Wagner, S., Wakely, S.P., Walter, R., Walther, T., Warda, K., Warwick, R., Wawer, P., Wawrzaszek, R., Webb, N., Wegner, P., Weinstein, A., Weitzel, Q., Welsing, R., Werner, M., Wetteskind, H., White, R., Wierzcholska, A., Wiesand, S., Wilkinson, M., Williams, D.A., Willingale, R., Winiarski, K., Wischnewski, R., Wiśniewski, Ł., Wood, M., Wörnlein, A., Xiong, Q., Yadav, K.K., Yamamoto, H., Yamamoto, T., Yamazaki, R., Yanagita, S., Yebras, J.M., Yelos, D., Yoshida, A., Yoshida, T., Yoshikoshi, T., Zabalza, V., Zacharias, M., Zajczyk, A., Zanin, R., Zdziarski, A., Zech, A., Zhao, A., Zhou, X., Ziętara, K., Ziolkowski, J., Ziółkowski, P., Zitelli, V., Zurbach, C., and Żychowski, P.
Published: 2013
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50. Early Galactic Evolution of Carbon, Nitrogen and Oxygen

Author: Israelian, G., Garcia Lopez, R. J., Rebolo, R., Matteucci, Francesca, editor, and Giovannelli, Franco, editor
Published: 2000
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