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51. The LiteBIRD mission to explore cosmic inflation

Author

Ghigna, T., Adler, A., Aizawa, K., Akamatsu, H., Akizawa, R., Allys, E., Anand, A., Aumont, J., Austermann, J., Azzoni, S., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Basyrov, A., Beckman, S., Bersanelli, M., Bortolami, M., Bouchet, F., Brinckmann, T., Campeti, P., Carinos, E., Carones, A., Casas, F. J., Cheung, K., Chinone, Y., Clermont, L., Columbro, F., Coppolecchia, A., Curtis, D., de Bernardis, P., de Haan, T., de la Hoz, E., De Petris, M., Della Torre, S., Monache, G. Delle, Di Giorgi, E., Dickinson, C., Diego-Palazuelos, P., García, J. J. Díaz, Dobbs, M., Dotani, T., D'Alessandro, G., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Farias, N., Ferreira, E., Franceschet, C., Fuskeland, U., Galloni, G., Galloway, M., Ganga, K., Gerbino, M., Gervasi, M., Génova-Santos, R. T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., González, R. González, Grandsire, L., Gruppuso, A., Halverson, N. W., Hargrave, P., Harper, S. E., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Herranz, D., Hivon, E., Hlozek, R. A., Hoang, T. D., Hubmayr, J., Ichiki, K., Ikuma, K., Ishino, H., Jaehnig, G., Jost, B., Kohri, K., Konishi, K., Lamagna, L., Lattanzi, M., Leloup, C., Levrier, F., Lonappan, A. I., Luzzi, G., Macias-Perez, J., Maffei, B., Marchitelli, E., Martínez-González, E., Masi, S., Matarrese, S., Matsumura, T., Micheli, S., Migliaccio, M., Monelli, M., Montier, L., Morgante, G., Mousset, L., Nagano, Y., Nagata, R., Natoli, P., Novelli, A., Noviello, F., Obata, I., Occhiuzzi, A., Odagiri, K., Omae, R., Pagano, L., Paiella, A., Paoletti, D., Pascual-Cisneros, G., Patanchon, G., Pavlidou, V., Piacentini, F., Piat, M., Piccirilli, G., Pinchera, M., Pisano, G., Porcelli, L., Raffuzzi, N., Raum, C., Remazeilles, M., Ritacco, A., Rubino-Martin, J., Ruiz-Granda, M., Sakurai, Y., Savini, G., Scott, D., Sekimoto, Y., Shiraishi, M., Signorelli, G., Stever, S. L., Sullivan, R. M., Suzuki, A., Takaku, R., Takakura, H., Takakura, S., Tartari, Y. Takase. A., Tassis, K., Thompson, K. L., Tomasi, M., Tristram, M., Tucker, C., Vacher, L., van Tent, B., Vielva, P., Watanuki, K., Wehus, I. K., Westbrook, B., Weymann-Despres, G., Winter, B., Wollack, E. J., Zacchei, A., Zannoni, M., Zhou, Y., and Collaboration, the LiteBIRD

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Physics - Instrumentation and Detectors
Abstract

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangian point L2, this JAXA-led strategic L-class mission will conduct a comprehensive mapping of the CMB polarization across the entire sky. During its 3-year mission, LiteBIRD will employ three telescopes within 15 unique frequency bands (ranging from 34 through 448 GHz), targeting a sensitivity of 2.2\,$\mu$K-arcmin and a resolution of 0.5$^\circ$ at 100\,GHz. Its primary goal is to measure the tensor-to-scalar ratio $r$ with an uncertainty $\delta r = 0.001$, including systematic errors and margin. If $r \geq 0.01$, LiteBIRD expects to achieve a $>5\sigma$ detection in the $\ell=$2-10 and $\ell=$11-200 ranges separately, providing crucial insight into the early Universe. We describe LiteBIRD's scientific objectives, the application of systems engineering to mission requirements, the anticipated scientific impact, and the operations and scanning strategies vital to minimizing systematic effects. We will also highlight LiteBIRD's synergies with concurrent CMB projects., Comment: 23 pages, 9 figures, 1 table, SPIE Astronomical Telescopes + Instrumentation 2024

Published
2024

52. Cosmoglobe DR2. II. CIB monopole measurements from COBE-DIRBE through global Bayesian analysis

Author

Watts, D. J., Galloway, M., Gjerløw, E., San, M., Aurlien, R., Basyrov, A., Brilenkov, M., Eriksen, H. K., Fuskeland, U., Herman, D., Ihle, H. T., Lunde, J. G. S., Næss, S. K., Stutzer, N. -O., Thommesen, H., and Wehus, I. K.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We derive new constraints on the CIB monopole spectrum from a set of reprocessed COBE-DIRBE sky maps that have lower instrumental and astrophysical contamination than the legacy DIRBE maps. These maps have been generated through a global Bayesian analysis framework that simultaneously fits cosmological, astrophysical, and instrumental parameters, as described in a series of papers collectively referred to as Cosmoglobe DR2. We have applied this method to the DIRBE TODs, complemented by selected HFI and FIRAS sky maps to break key astrophysical degeneracies, as well as WISE and Gaia compact object catalogs. In this paper, we focus on the CIB monopole constraints that result from this work. We report positive detections of an isotropic signal in six out of the ten DIRBE bands (1.25, 2.2, 3.5, 100, 140, and 240 $\mathrm{\mu m}$). For the 2.2 $\mu$m channel, we find an amplitude of $10.2\pm1.2\,\mathrm{nW\,m^{-2}\,sr^{-1}}$, 74 % lower than that reported from the official DIRBE maps. For the 240 $\mu\mathrm{m}$ channel, we find $6\pm3\mathrm{nW\,m^{-2}\,sr^{-1}}$, 56 % lower than the official DIRBE release. We interpret these lower values as resulting from improved zodiacal light and Galactic foreground modeling. For the bands between 4.9 and 60 $\mu\mathrm{m}$, the presence of excess radiation in solar-centric coordinates precludes the definition of lower limits. However, the analysis still provides well-defined upper limits. For the 12 $\mu\mathrm{m}$ channel, we find an upper 95 % confidence limit of 55 $\mathrm{nW\,m^{-2}\,sr^{-1}}$, more than a factor of eight lower than the corresponding legacy result of 468 $\mathrm{nW\,m^{-2}\,sr^{-1}}$. The results presented in this paper redefine the state-of-the-art CIB monopole constraints from COBE-DIRBE, and provide a real-world illustration of the power of global end-to-end analysis of multiple complementary datasets., Comment: 17 pages, 9 figures, submitted to A&A. Comments welcome! Data products can be found at https://www.cosmoglobe.uio.no/products/cosmoglobe-dr2.html

Published
2024

53. Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling

Author

Kini, Yves, Salmi, Tuomo, Vinciguerra, Serena, Watts, Anna L., Bilous, Anna, Galloway, Duncan K., van der Wateren, Emma, Khalsa, Guru Partap, Bogdanov, Slavko, Buchner, Johannes, and Suleimanov, Valery

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Pulse profile modelling (PPM) is a comprehensive relativistic ray-tracing technique employed to determine the properties of neutron stars. In this study, we apply this technique to the Type I X-ray burster and accretion-powered millisecond pulsar XTE J1814-338, extracting its fundamental properties using PPM of its thermonuclear burst oscillations. Using data from its 2003 outburst, and a single uniform temperature hot spot model, we infer XTE J1814-338 to be located at a distance of $7.2^{+0.3}_{-0.4}$ kpc, with a mass of $1.21^{+0.05}_{-0.05}$ M$_\odot$ and an equatorial radius of $7.0^{+0.4}_{-0.4}$ km. Our results also offer insight into the time evolution of the hot spot but point to some potential shortcomings of the single uniform temperature hot spot model. We explore the implications of this result, including what we can learn about thermonuclear burst oscillation mechanisms and the importance of modelling the accretion contribution to the emission during the burst., Comment: Accepted for publication in MNRAS. The Zenodo link is public

Published
2024
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54. Aspects of the geometry and topology of expanding horizons

Author

Galloway, Gregory J. and Mendes, Abraão

Subjects
General Relativity and Quantum Cosmology, Mathematics - Differential Geometry
Abstract

The aim of this paper is to extend some basic results about marginally outer trapped surfaces to the context of surfaces having general null expansion. Motivated in part by recent work of Chai-Wan, we introduce the notion of $\mathfrak{g}$-stability for a general closed hypersurface $\Sigma$ in an ambient initial data set and prove that, under natural energy conditions, $\Sigma$ has positive Yamabe type, that is, $\Sigma$ admits a metric of positive scalar curvature, provided $\Sigma$ is $\mathfrak{g}$-stable. A similar result is obtained when $\Sigma$ is embedded in a null hypersurface of a spacetime satisfying the dominant energy condition. Area bounds under similar conditions are obtained in the case where $\Sigma$ is $2$-dimensional. Conditions implying $\mathfrak{g}$-stability are also discussed. Finally, we obtain a spacetime positive mass theorem for initial data sets with compact boundary $\Sigma$ of positive null expansion, assuming that the dominant energy condition is sufficiently strict near $\Sigma$. This extends recent results of Galloway-Lee and Lee-Lesourd-Unger., Comment: 13 pages. Comments welcome; v2: this is a substantial revision of the first version, including some corrections/clarifications and the addition of some new material. Accepted for publication in Proc. of AMS

Published
2024

55. Venous Thromboembolism

Author

Galloway, Olivia W., Kohli, Anirudh, Neff, Marc, editor, Beekley, Alec, editor, Yoon-Flannery, Kahyun, editor, and Ratnasekera, Asanthi, editor

Published
2025
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61. Sub-wavelength coherent imaging of periodic samples using a 13.5 nm tabletop high harmonic light source

Author

Gardner, Dennis F., Tanksalvala, Michael, Shanblatt, Elisabeth R., Zhang, Xiaoshi, Galloway, Benjamin R., Porter, Christina L., Karl Jr., Robert, Bevis, Charles, Adams, Daniel E., Kapteyn, Henry C., Murnane, Margaret M., and Mancini, Giulia F.

Subjects
Physics - Optics, Physics - Instrumentation and Detectors
Abstract

Coherent diffractive imaging is unique as the only route for achieving diffraction-limited spatial resolution in the extreme ultraviolet and X-ray regions, limited only by the wavelength of the light. Recently, advances in coherent short wavelength light sources, coupled with progress in algorithm development, have significantly enhanced the power of x-ray imaging. However, to date, high-fidelity diffraction imaging of periodic objects has been a challenge because the scattered light is concentrated in isolated peaks. Here, we use tabletop 13.5nm high harmonic beams to make two significant advances. First we demonstrate high-quality imaging of an extended, nearly-periodic sample for the first time. Second, we achieve sub-wavelength spatial resolution (12.6nm) imaging at short wavelengths, also for the first time. The key to both advances is a novel technique called modulus enforced probe, which enables robust, quantitative, reconstructions of periodic objects. This work is important for imaging next generation nano-engineered devices., Comment: 15 pages, 5 figures

Published
2024
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62. LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields

Author

Paoletti, D., Rubino-Martin, J., Shiraishi, M., Molinari, D., Chluba, J., Finelli, F., Baccigalupi, C., Errard, J., Gruppuso, A., Lonappan, A. I., Tartari, A., Allys, E., Anand, A., Aumont, J., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Bersanelli, M., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., Della Torre, S., Diego-Palazuelos, P., Eriksen, H. K., Fuskeland, U., Galloni, G., Galloway, M., Gerbino, M., Gervasi, M., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., Grupp, F., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Hivon, E., Ichiki, K., Ishino, H., Kohri, K., Komatsu, E., Krachmalnicoff, N., Lamagna, L., Lattanzi, M., Lembo, M., Levrier, F., López-Caniego, M., Luzzi, G., Martínez-González, E., Masi, S., Matarrese, S., Micheli, S., Migliaccio, M., Monelli, M., Montier, L., Morgante, G., Mousset, L., Nagata, R., Namikawa, T., Natoli, P., Novelli, A., Obata, I., Occhiuzzi, A., Odagiri, K., Pagano, L., Paiella, A., Pascual-Cisneros, G., Piacentini, F., Piccirilli, G., Remazeilles, M., Ritacco, A., Ruiz-Granda, M., Sakurai, Y., Scott, D., Stever, S. L., Sullivan, R. M., Takase, Y., Tassis, K., Terenzi, L., Tristram, M., Vacher, L., van Tent, B., Vielva, P., Wehus, I. K., Weymann-Despres, G., Zannoni, M., and Zhou, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present detailed forecasts for the constraints on primordial magnetic fields (PMFs) that will be obtained with the LiteBIRD satellite. The constraints are driven by the effects of PMFs on the CMB anisotropies: the gravitational effects of magnetically-induced perturbations; the effects on the thermal and ionization history of the Universe; the Faraday rotation imprint on the CMB polarization; and the non-Gaussianities induced in polarization anisotropies. LiteBIRD represents a sensitive probe for PMFs and by exploiting all the physical effects, it will be able to improve the current limit coming from Planck. In particular, thanks to its accurate $B$-mode polarization measurement, LiteBIRD will improve the constraints on infrared configurations for the gravitational effect, giving $B_{\rm 1\,Mpc}^{n_{\rm B} =-2.9} < 0.8$ nG at 95% C.L., potentially opening the possibility to detect nanogauss fields with high significance. We also observe a significant improvement in the limits when marginalized over the spectral index, $B_{1\,{\rm Mpc}}^{\rm marg}< 2.2$ nG at 95% C.L. From the thermal history effect, which relies mainly on $E$-mode polarization data, we obtain a significant improvement for all PMF configurations, with the marginalized case, $\sqrt{\langle B^2\rangle}^{\rm marg}<0.50$ nG at 95% C.L. Faraday rotation constraints will take advantage of the wide frequency coverage of LiteBIRD and the high sensitivity in $B$ modes, improving the limits by orders of magnitude with respect to current results, $B_{1\,{\rm Mpc}}^{n_{\rm B} =-2.9} < 3.2$ nG at 95% C.L. Finally, non-Gaussianities of the $B$-mode polarization can probe PMFs at the level of 1 nG, again significantly improving the current bounds from Planck. Altogether our forecasts represent a broad collection of complementary probes, providing conservative limits on PMF characteristics that will be achieved with LiteBIRD., Comment: 51 pages, 24 figures, abstract shortened

Published
2024
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63. Inferring system parameters from the bursts of the accretion-powered pulsar IGR J17498-2921

Author

Galloway, D. K., Goodwin, A. J., Hilder, T., Waterson, L., and Cupák, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Thermonuclear (type-I) bursts exhibit properties that depend both on the local surface conditions of the neutron stars on which they ignite, as well as the physical parameters of the host binary system. However, constraining the system parameters requires a comprehensive method to compare the observed bursts to simulations. We have further developed the beansp code for this purpose and analysed the bursts observed from IGR J17498-2921, a 401-Hz accretion-powered pulsar, discovered during it's 2011 outburst. We find good agreement with a model having H-deficient fuel with X = 0.15 +/- 0.4, and CNO metallicity Z=0.0014^{+0.0004}_{-0.0003}, about a tenth of the solar value. The model has the system at a distance of 5.7^{+0.6}_{-0.5} kpc, with a massive (approx. 2 M_sun) neutron star and a likely inclination of 60 deg. We also re-analysed the data from the 2002 outburst of the accretion-powered millisecond pulsar SAX J1808.4-3658. For that system we find a substantially closer distance than previously inferred, at 2.7 +/- 0.3 kpc, likely driven by a larger degree of burst emission anisotropy. The other system parameters are largely consistent with the previous analysis. We briefly discuss the implications for the evolution of these two systems., Comment: 10 pages, 7 figures, accompanying data at https://dx.doi.org/ 10.26180/24773367; accepted by MNRAS

Published
2024

64. Offline tagging of radon-induced backgrounds in XENON1T and applicability to other liquid xenon detectors

Author

Aprile, E., Aalbers, J., Abe, K., Maouloud, S. Ahmed, Althueser, L., Andrieu, B., Angelino, E., Angevaare, J. R., Martin, D. Antón, Arneodo, F., Baudis, L., Baxter, A. L., Bazyk, M., Bellagamba, L., Biondi, R., Bismark, A., Brookes, E. J., Brown, A., Bruno, G., Budnik, R., Bui, T. K., Cardoso, J. M. R., Chavez, A. P. Cimental, Colijn, A. P., Conrad, J., Cuenca-García, J. J., D'Andrea, V., Garcia, L. C. Daniel, Decowski, M. P., Di Donato, C., Di Gangi, P., Diglio, S., Eitel, K., Elykov, A., Ferella, A. D., Ferrari, C., Fischer, H., Flehmke, T., Flierman, M., Fulgione, W., Fuselli, C., Gaemers, P., Gaior, R., Galloway, M., Gao, F., Ghosh, S., Glade-Beucke, R., Grandi, L., Grigat, J., Guan, H., Guida, M., Hammann, R., Higuera, A., Hils, C., Hoetzsch, L., Hood, N. F., Iacovacci, M., Itow, Y., Jakob, J., Joerg, F., Joy, A., Kaminaga, Y., Kara, M., Kavrigin, P., Kazama, S., Kobayashi, M., Kopec, A., Kuger, F., Landsman, H., Lang, R. F., Levinson, L., Li, I., Li, S., Liang, S., Lin, Y. T., Lindemann, S., Lindner, M., Liu, K., Loizeau, J., Lombardi, F., Long, J., Lopes, J. A. M., Luce, T., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Manenti, L., Marignetti, F., Undagoitia, T. Marrodán, Martens, K., Masbou, J., Masson, E., Mastroianni, S., Melchiorre, A., Messina, M., Michael, A., Miuchi, K., Molinario, A., Moriyama, S., Morå, K., Mosbacher, Y., Murra, M., Müller, J., Ni, K., Oberlack, U., Paetsch, B., Palacio, J., Pan, Y., Pellegrini, Q., Peres, R., Peters, C., Pienaar, J., Pierre, M., Plante, G., Pollmann, T. R., Principe, L., Qi, J., Qin, J., García, D. Ramírez, Rajado, M., Shi, J., Singh, R., Sanchez, L., Santos, J. M. F. dos, Sarnoff, I., Sartorelli, G., Schreiner, J., Schulte, D., Schulte, P., Eißing, H. Schulze, Schumann, M., Lavina, L. Scotto, Selvi, M., Semeria, F., Shagin, P., Shi, S., Silva, M., Simgen, H., Takeda, A., Tan, P. -L., Terliuk, A., Thers, D., Toschi, F., Trinchero, G., Tunnell, C., Tönnies, F., Valerius, K., Vecchi, S., Vetter, S., Volta, G., Weinheimer, C., Weiss, M., Wenz, D., Wittweg, C., Wolf, T., Wu, V. H. S., Xing, Y., Xu, D., Xu, Z., Yamashita, M., Yang, L., Ye, J., Yuan, L., Zavattini, G., Zhong, M., and Zhu, T.

Subjects
High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

This paper details the first application of a software tagging algorithm to reduce radon-induced backgrounds in liquid noble element time projection chambers, such as XENON1T and XENONnT. The convection velocity field in XENON1T was mapped out using $^{222}\text{Rn}$ and $^{218}\text{Po}$ events, and the root-mean-square convection speed was measured to be $0.30 \pm 0.01$ cm/s. Given this velocity field, $^{214}\text{Pb}$ background events can be tagged when they are followed by $^{214}\text{Bi}$ and $^{214}\text{Po}$ decays, or preceded by $^{218}\text{Po}$ decays. This was achieved by evolving a point cloud in the direction of a measured convection velocity field, and searching for $^{214}\text{Bi}$ and $^{214}\text{Po}$ decays or $^{218}\text{Po}$ decays within a volume defined by the point cloud. In XENON1T, this tagging system achieved a $^{214}\text{Pb}$ background reduction of $6.2^{+0.4}_{-0.9}\%$ with an exposure loss of $1.8\pm 0.2 \%$, despite the timescales of convection being smaller than the relevant decay times. We show that the performance can be improved in XENONnT, and that the performance of such a software-tagging approach can be expected to be further improved in a diffusion-limited scenario. Finally, a similar method might be useful to tag the cosmogenic $^{137}\text{Xe}$ background, which is relevant to the search for neutrinoless double-beta decay., Comment: 17 pages, 19 figures

Published
2024
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65. A new launch pad failure mode: Analysis of fine particles from the launch of the first Starship orbital test flight

Author

Dotson, B., Metzger, P., Hafner, J., Shackelford, A., Birkenfeld, K., Britt, D., Ford, A., Truscott, R., Truscott, S., Zavaleta, J., Zemke, J., Purvis, K., Scudder, M., Johnson, C., Galloway, J., and DeShetler, J.

Subjects
Physics - Space Physics
Abstract

This study examines the characteristics, composition, and origin of fine particle debris samples collected following the launch of the first Starship orbital test flight, which suggests a new launch pad failure mode previously unknown. Particle shapes, sizes, bulk densities, and VIS/NIR/MIR spectra, of collected fine particle material from Port Isabel, TX, were analyzed and compared to pulverized concrete, Fondag (high temperature concrete), limestone, and sand recovered from the area near the Starship launch pad after this test flight. Raman spectroscopy was also used to determine mineral compositions of each sample. Results suggest that the fine particle material lofted by the Starship launch is consistent with sand derived from the launch site. These results imply that the destruction of the launch pad eroded and lofted material into the air from the underlying sandy, base-layer. From calculations, this lofted material likely remained suspended in the air for minutes following the launch from recirculation, allowing for transport over an extended range. Most of the recovered material was too coarse to be a respiration hazard, as a small mass fraction of the particles (<1%) had diameters of 10 um or less. Video analysis and ballistic models also provide insight into the failure mechanism associated with the launch pad, which was consistent with a high-pressure eruption from the region below the failed launch pad.

Published
2024

66. Dark Matter Line Searches with the Cherenkov Telescope Array

Author

Abe, S., Abhir, J., Abhishek, A., Acero, F., Acharyya, A., Adam, R., Aguasca-Cabot, A., Agudo, I., Aguirre-Santaella, A., Alfaro, J., Alfaro, R., Alvarez-Crespo, N., Batista, R. Alves, Amans, J. -P., Amato, E., Ambrosi, G., Angel, L., Aramo, C., Arcaro, C., Arnesen, T. T. H., Arrabito, L., Asano, K., Ascasibar, Y., Aschersleben, J., Ashkar, H., Backes, M., Baktash, A., Balazs, C., Balbo, M., Larriva, A. Baquero, Martins, V. Barbosa, de Almeida, U. Barres, Barrio, J. A., Batković, I., Batzofin, R., Baxter, J., González, J. Becerra, Beck, G., Benbow, W., Berge, D., Bernardini, E., Bernete, J., Bernlöhr, K., Berti, A., Bertucci, B., Bhattacharjee, P., Bhattacharyya, S., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Bocchino, F., Boisson, C., Bolmont, J., Bonnoli, G., Bonollo, A., Bordas, P., Bosnjak, Z., Bottacini, E., Böttcher, M., Bringmann, T., Bronzini, E., Brose, R., Brown, A. M., Brunelli, G., Bulgarelli, A., Bulik, T., Burelli, I., Burmistrov, L., Burton, M., Buscemi, M., Bylund, T., Cailleux, J., Campoy-Ordaz, A., Cantlay, B. K., Capasso, G., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Caroff, S., Carosi, A., Carosi, R., Carquin, E., Carrasco, M. -S., Cassol, F., Castaldini, L., Castrejon, N., Castro-Tirado, A. J., Cerasole, D., Cerruti, M., Chadwick, P. M., Chaty, S., Chen, A. W., Chernyakova, M., Chiavassa, A., Chudoba, J., Chytka, L., Cicciari, G. M., Cifuentes, A., Araujo, C. H. Coimbra, Colapietro, M., Conforti, V., Conte, F., Contreras, J. L., Costa, A., Costantini, H., Cotter, G., Cristofari, P., Cuevas, O., Curtis-Ginsberg, Z., D'Amico, G., D'Ammando, F., Dai, S., Dalchenko, M., Dazzi, F., De Angelis, A., de Lavergne, M. de Bony, De Caprio, V., Pino, E. M. de Gouveia Dal, De Lotto, B., De Lucia, M., de Menezes, R., de Naurois, M., de Souza, V., del Peral, L., del Valle, M. V., Giler, A. G. Delgado, Mengual, J. Delgado, Delgado, C., Dell'aiera, M., della Volpe, D., Depaoli, D., Di Girolamo, T., Di Piano, A., Di Pierro, F., Di Tria, R., Di Venere, L., Díaz, C., Diebold, S., Dinesh, A., Djuvsland, J., Dominik, R. M., Prester, D. Dominis, Donini, A., Dorner, D., Dörner, J., Doro, M., Dournaux, J. -L., Duangchan, C., Dubos, C., Ducci, L., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Elsässer, D., Emery, G., Errando, M., Escanuela, C., Escarate, P., Godoy, M. Escobar, Escudero, J., Esposito, P., Ettori, S., Falceta-Goncalves, D., Fedorova, E., Fegan, S., Feng, Q., Ferrand, G., Ferrarotto, F., Fiandrini, E., Fiasson, A., Filipovic, M., Fioretti, V., Fiori, M., Foffano, L., Guiteras, L. Font, Fontaine, G., Fröse, S., Fukazawa, Y., Fukui, Y., Furniss, A., Galanti, G., Galaz, G., Galelli, C., Gallozzi, S., Gammaldi, V., Garczarczyk, M., Gasbarra, C., Gasparrini, D., Ghalumyan, A., Gianotti, F., Giarrusso, M., Paiva, J. G. Giesbrecht Formiga, Giglietto, N., Giordano, F., Giuffrida, R., Glicenstein, J. -F., Glombitza, J., Goldoni, P., González, J. M., González, M. M., Coelho, J. Goulart, Gradetzke, T., Granot, J., Grasso, D., Grau, R., Gréaux, L., Green, D., Green, J. G., Grolleron, G., Guedes, L. M. V., Gueta, O., Hackfeld, J., Hadasch, D., Hamal, P., Hanlon, W., Hara, S., Harvey, V. M., Hassan, T., Hayashi, K., Heß, B., Heckmann, L., Heller, M., Cadena, S. Hernández, Hervet, O., Hinton, J., Hiroshima, N., Hnatyk, B., Hnatyk, R., Hofmann, W., Holder, J., Horan, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Iarlori, M., Inada, T., Incardona, F., Inoue, S., Inoue, Y., Iocco, F., Iori, M., Ishio, K., Jamrozy, M., Janecek, P., Jankowsky, F., Jean, P., Quiles, J. Jimenez, Jin, W., Juramy-Gilles, C., Jurysek, J., Kagaya, M., Kalekin, O., Karas, V., Katagiri, H., Kataoka, J., Kaufmann, S., Kazanas, D., Kerszberg, D., Kieda, D. B., Kleiner, T., Kluge, G., Kobayashi, Y., Kohri, K., Komin, N., Kornecki, P., Kosack, K., Kowal, G., Kubo, H., Kushida, J., La Barbera, A., La Palombara, N., Láinez, M., Lamastra, A., Lapington, J., Laporte, P., Lazarević, S., Lazendic-Galloway, J., Lemoine-Goumard, M., Lenain, J. -P., Leone, F., Leonora, E., Leto, G., Lindfors, E., Linhoff, M., Liodakis, I., Lipniacka, A., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Bahilo, J. Lozano, Luque-Escamilla, P. L., Macias, O., Majumdar, P., Mallamaci, M., Malyshev, D., Mandat, D., Manicò, G., Mariotti, M., Márquez, I., Marquez, P., Marsella, G., Martí, J., Martínez, G. A., Martínez, M., Martinez, O., Marty, C., Mas-Aguilar, A., Mastropietro, M., Mazin, D., Menchiari, S., Mestre, E., Meunier, J. -L., Meyer, D. M. -A., Meyer, M., Miceli, D., Miceli, M., Michailidis, M., Michałowski, J., Miener, T., Miranda, J. M., Mitchell, A., Mizote, M., Mizuno, T., Moderski, R., Molero, M., Molfese, C., Molina, E., Montaruli, T., Moralejo, A., Morcuende, D., Morselli, A., Moulin, E., Zamanillo, V. Moya, Munari, K., Murach, T., Muraczewski, A., Muraishi, H., Nakamori, T., Nayak, A., Nemmen, R., Neto, J. P., Nickel, L., Niemiec, J., Nieto, D., Rosillo, M. Nievas, Nikołajuk, M., Nikolić, L., Nishijima, K., Noda, K., Nosek, D., Novotny, V., Nozaki, S., Ohishi, M., Ohtani, Y., Okumura, A., Olive, J. -F., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, E., Orlando, S., Ostrowski, M., Otero-Santos, J., Oya, I., Pagano, I., Pagliaro, A., Palatiello, M., Panebianco, G., Paneque, D., Pantaleo, F. R., Paredes, J. M., Parmiggiani, N., Patricelli, B., Pe'er, A., Pech, M., Pecimotika, M., Pensec, U., Peresano, M., Pérez-Romero, J., Persic, M., Peters, K. P., Petruk, O., Piano, G., Pierre, E., Pietropaolo, E., Pihet, M., Pinchbeck, L., Pirola, G., Pittori, C., Plard, C., Podobnik, F., Pohl, M., Pollet, V., Ponti, G., Prandini, E., Principe, G., Priyadarshi, C., Produit, N., Prouza, M., Pueschel, E., Pühlhofer, G., Pumo, M. L., Queiroz, F., Quirrenbach, A., Rainò, S., Rando, R., Razzaque, S., Regeard, M., Reimer, A., Reimer, O., Reisenegger, A., Rhode, W., Ribeiro, D., Ribó, M., Ricci, C., Richtler, T., Rico, J., Rieger, F., Riitano, L., Rizi, V., Roache, E., Fernandez, G. Rodriguez, Frías, M. D. Rodríguez, Rodríguez-Vázquez, J. J., Romano, P., Romeo, G., Rosado, J., de Leon, A. Rosales, Rowell, G., Rudak, B., Ruiter, A. J., Rulten, C. B., Sadeh, I., Saha, L., Saito, T., Salzmann, H., Sánchez-Conde, M., Sandaker, H., Sangiorgi, P., Sano, H., Santander, M., Santos-Lima, R., Sapienza, V., Šarić, T., Sarkar, A., Sarkar, S., Saturni, F. G., Savarese, S., Scherer, A., Schiavone, F., Schipani, P., Schleicher, B., Schovanek, P., Schubert, J. L., Schwanke, U., Arroyo, M. Seglar, Seitenzahl, I. R., Sergijenko, O., Servillat, M., Siegert, T., Siejkowski, H., Siqueira, C., Sliusar, V., Slowikowska, A., Sol, H., Spencer, S. T., Spiga, D., Stamerra, A., Stanič, S., Starecki, T., Starling, R., Stawarz, Ł., Steppa, C., Hatlen, E. Sæther, Stolarczyk, T., Strišković, J., Suda, Y., Świerk, P., Tajima, H., Tak, D., Takahashi, M., Takeishi, R., Tavernier, T., Tejedor, L. A., Terauchi, K., Teshima, M., Testa, V., Tian, W. W., Tibaldo, L., Tibolla, O., Peixoto, C. J. Todero, Torradeflot, F., Torres, D. F., Tosti, G., Tothill, N., Toussenel, F., Tramacere, A., Travnicek, P., Tripodo, G., Trois, A., Truzzi, S., Tutone, A., Vaclavek, L., Vacula, M., Vallania, P., Vallés, R., van Eldik, C., van Scherpenberg, J., Vandenbroucke, J., Vassiliev, V., Acosta, M. Vázquez, Vecchi, M., Ventura, S., Vercellone, S., Verna, G., Viana, A., Viaux, N., Vigliano, A., Vignatti, J., Vigorito, C. F., Villanueva, J., Visentin, E., Vitale, V., Vodeb, V., Voisin, V., Voitsekhovskyi, V., Vorobiov, S., Voutsinas, G., Vovk, I., Vuillaume, T., Wagner, S. J., Walter, R., White, M., White, R., Wierzcholska, A., Will, M., Williams, D. A., Wohlleben, F., Wolter, A., Yamamoto, T., Yang, L., Yoshida, T., Yoshikoshi, T., Zaharijas, G., Zampieri, L., Sanchez, R. Zanmar, Zavrtanik, D., Zavrtanik, M., Zdziarski, A. A., Zech, A., Zhang, W., Zhdanov, V. I., Ziętara, K., Živec, M., and Zuriaga-Puig, J.

Subjects
High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from astrophysical or instrumental backgrounds. We provide an updated assessment of the sensitivity of the Cherenkov Telescope Array (CTA) to such signals, based on observations of the Galactic centre region as well as of selected dwarf spheroidal galaxies. We find that current limits and detection prospects for dark matter masses above 300 GeV will be significantly improved, by up to an order of magnitude in the multi-TeV range. This demonstrates that CTA will set a new standard for gamma-ray astronomy also in this respect, as the world's largest and most sensitive high-energy gamma-ray observatory, in particular due to its exquisite energy resolution at TeV energies and the adopted observational strategy focussing on regions with large dark matter densities. Throughout our analysis, we use up-to-date instrument response functions, and we thoroughly model the effect of instrumental systematic uncertainties in our statistical treatment. We further present results for other potential signatures with sharp spectral features, e.g.~box-shaped spectra, that would likewise very clearly point to a particle dark matter origin., Comment: 44 pages JCAP style (excluding author list and references), 19 figures; minor changes to match published version

Published
2024
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67. Rigidity aspects of Penrose's singularity theorem

Author

Galloway, Gregory J. and Ling, Eric

Subjects
General Relativity and Quantum Cosmology, Mathematics - Differential Geometry
Abstract

In this paper, we study rigidity aspects of Penrose's singularity theorem. Specifically, we aim to answer the following question: if a spacetime satisfies the hypotheses of Penrose's singularity theorem except with weakly trapped surfaces instead of trapped surfaces, then what can be said about the global spacetime structure if the spacetime is null geodesically complete? In this setting, we show that we obtain a foliation of MOTS which generate totally geodesic null hypersurfaces. Depending on our starting assumptions, we obtain either local or global rigidity results. We apply our arguments to cosmological spacetimes (i.e., spacetimes with compact Cauchy surfaces) and scenarios involving topological censorship., Comment: 18 pages. v3 agrees with published version

Published
2024
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68. The XENONnT Dark Matter Experiment

Author

XENON Collaboration, Aprile, E., Aalbers, J., Abe, K., Maouloud, S. Ahmed, Althueser, L., Andrieu, B., Angelino, E., Angevaare, J. R., Antochi, V. C., Martin, D. Antón, Arneodo, F., Balata, M., Baudis, L., Baxter, A. L., Bazyk, M., Bellagamba, L., Biondi, R., Bismark, A., Brookes, E. J., Brown, A., Bruenner, S., Bruno, G., Budnik, R., Bui, T. K., Cai, C., Cardoso, J. M. R., Cassese, F., Chiarini, A., Cichon, D., Chavez, A. P. Cimental, Colijn, A. P., Conrad, J., Corrieri, R., Cuenca-García, J. J., Cussonneau, J. P., Dadoun, O., D'Andrea, V., Decowski, M. P., De Fazio, B., Di Gangi, P., Diglio, S., Disdier, J. M., Douillet, D., Eitel, K., Elykov, A., Farrell, S., Ferella, A. D., Ferrari, C., Fischer, H., Flierman, M., Form, S., Front, D., Fulgione, W., Fuselli, C., Gaemers, P., Gaior, R., Rosso, A. Gallo, Galloway, M., Gao, F., Gardner, R., Garroum, N., Glade-Beucke, R., Grandi, L., Grigat, J., Guan, H., Guerzoni, M., Guida, M., Hammann, R., Higuera, A., Hils, C., Hoetzsch, L., Hood, N. F., Howlett, J., Huhmann, C., Iacovacci, M., Iaquaniello, G., Iven, L., Itow, Y., Jakob, J., Joerg, F., Joy, A., Kara, M., Kavrigin, P., Kazama, S., Kobayashi, M., Koltman, G., Kopec, A., Kuger, F., Landsman, H., Lang, R. F., Levinson, L., Li, I., Li, S., Liang, S., Lindemann, S., Lindner, M., Liu, K., Loizeau, J., Lombardi, F., Long, J., Lopes, J. A. M., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Manenti, L., Marignetti, F., Undagoitia, T. Marrodán, Martella, P., Martens, K., Masbou, J., Masson, D., Masson, E., Mastroianni, S., Mele, E., Messina, M., Michinelli, R., Miuchi, K., Molinario, A., Moriyama, S., Morå, K., Mosbacher, Y., Murra, M., Müller, J., Ni, K., Nisi, S., Oberlack, U., Orlandi, D., Othegraven, R., Paetsch, B., Palacio, J., Parlati, S., Paschos, P., Pellegrini, Q., Peres, R., Peters, C., Pienaar, J., Pierre, M., Plante, G., Pollmann, T. R., Qi, J., Qin, J., García, D. Ramírez, Rynge, M., Shi, J., Singh, R., Sanchez, L., Santos, J. M. F. dos, Sarnoff, I., Sartorelli, G., Schreiner, J., Schulte, D., Schulte, P., Eißing, H. Schulze, Schumann, M., Lavina, L. Scotto, Selvi, M., Semeria, F., Shagin, P., Shi, S., Shockley, E., Silva, M., Simgen, H., Stephen, J., Stern, M., Stillwell, B. K., Takeda, A., Tan, P. -L., Tatananni, D., Terliuk, A., Thers, D., Toschi, F., Trinchero, G., Tunnell, C., Tönnies, F., Valerius, K., Volta, G., Weinheimer, C., Weiss, M., Wenz, D., Westermann, J., Wittweg, C., Wolf, T., Wu, V. H. S., Xing, Y., Xu, D., Xu, Z., Yamashita, M., Yang, L., Ye, J., Yuan, L., Zavattini, G., Zhong, M., and Zhu, T.

Subjects
Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract

The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (8.5 tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run., Comment: 32 pages, 19 figures

Published
2024

71. Detection of Leptospira kirschneri in a short-beaked common dolphin (Delphinus delphis delphis) stranded off the coast of southern California, USA.

Author

Prager, Katherine, Danil, Kerri, Wurster, Elyse, Colegrove, Kathleen, Galloway, Renee, Kettler, Niesa, Mani, Rinosh, McDonough, Ryelan, Sahl, Jason, Stone, Nathan, Wagner, David, and Lloyd-Smith, James

Subjects
Delphinus delphis, Leptospira, Cetacean, Common dolphin, Marine mammal, Northeastern Pacific, Animals, Leptospira, Leptospirosis, California, Female, Phylogeny, Common Dolphins
Abstract

BACKGROUND: Pathogenic Leptospira species are globally important zoonotic pathogens capable of infecting a wide range of host species. In marine mammals, reports of Leptospira have predominantly been in pinnipeds, with isolated reports of infections in cetaceans. CASE PRESENTATION: On 28 June 2021, a 150.5 cm long female, short-beaked common dolphin (Delphinus delphis delphis) stranded alive on the coast of southern California and subsequently died. Gross necropsy revealed multifocal cortical pallor within the reniculi of the kidney, and lymphoplasmacytic tubulointerstitial nephritis was observed histologically. Immunohistochemistry confirmed Leptospira infection, and PCR followed by lfb1 gene amplicon sequencing suggested that the infecting organism was L.kirschneri. Leptospira DNA capture and enrichment allowed for whole-genome sequencing to be conducted. Phylogenetic analyses confirmed the causative agent was a previously undescribed, divergent lineage of L.kirschneri. CONCLUSIONS: We report the first detection of pathogenic Leptospira in a short-beaked common dolphin, and the first detection in any cetacean in the northeastern Pacific Ocean. Renal lesions were consistent with leptospirosis in other host species, including marine mammals, and were the most significant lesions detected overall, suggesting leptospirosis as the likely cause of death. We identified the cause of the infection as L.kirschneri, a species detected only once before in a marine mammal - a northern elephant seal (Mirounga angustirostris) of the northeastern Pacific. These findings raise questions about the mechanism of transmission, given the obligate marine lifestyle of cetaceans (in contrast to pinnipeds, which spend time on land) and the commonly accepted view that Leptospira are quickly killed by salt water. They also raise important questions regarding the source of infection, and whether it arose from transmission among marine mammals or from terrestrial-to-marine spillover. Moving forward, surveillance and sampling must be expanded to better understand the extent to which Leptospira infections occur in the marine ecosystem and possible epidemiological linkages between and among marine and terrestrial host species. Generating Leptospira genomes from different host species will yield crucial information about possible transmission links, and our study highlights the power of new techniques such as DNA enrichment to illuminate the complex ecology of this important zoonotic pathogen.

Published
2024

72. Ecology and Chronic Wasting Disease Epidemiology Shape Prion Protein Gene Variation in Rocky Mountain Elk (Cervus elaphus nelsoni)

Author

Hoar, Bruce R, Ernest, Holly B, Johnson, Laura NL, LaCava, Melanie EF, Sandidge, Douglas J, Gerow, Ken, Mousel, Michelle R, Galloway, Nathan L, Swain, William, and Malmberg, Jennifer L

Subjects
Veterinary Sciences, Agricultural, Veterinary and Food Sciences, Genetics, Brain Disorders, 2.1 Biological and endogenous factors, Aetiology, Animals, Wasting Disease, Chronic, Prion Proteins, Leucine, Prions, Codon, Deer, Cervus elaphus nelsoni, chronic wasting disease, disease ecology, evolution, Rocky Mountain elk, prion, PRNP, transmissible spongiform encephalopathy, Zoology, Veterinary sciences
Abstract

As chronic wasting disease (CWD) continues to spread across North America, the relationship between CWD and host genetics has become of interest. In Rocky Mountain elk (Cervus elaphus nelsoni), one or two copies of a leucine allele at codon 132 of the prion protein gene (132L*) has been shown to prolong the incubation period of CWD. Our study examined the relationship between CWD epidemiology and codon 132 evolution in elk from Wyoming, USA, from 2011 to 2018. Using PCR and Sanger sequencing, we genotyped 997 elk and assessed the relationship between genotype and CWD prevalence estimated from surveillance data. Using logistic regression, we showed that each 1% increase in CWD prevalence is associated with a 9.6% increase in the odds that an elk would have at least one copy of leucine at codon 132. In some regions, however, 132L* variants were found in the absence of CWD, indicating that evolutionary and epidemiologic patterns can be heterogeneous across space and time. We also provide evidence that naturally occurring CWD is not rare in 132L* elk, which merits the study of shedding kinetics in 132L* elk and the influence of genotype on CWD strain diversity. The management implications of cervid adaptations to CWD are difficult to predict. Studies that investigate the degree to which evolutionary outcomes are shaped by host spatial structure can provide useful epidemiologic insight, which can in turn aid management by informing scale and extent of mitigation actions.

Published
2024

73. Bridging Theory to Practice: Exploring the Role of an Educative Translingual Curriculum to Support Linguistically Diverse Classroom Practices

Author

Holland White, Emily Phillips Galloway, and Robert T. Jiménez

Abstract

This study investigates how five teachers of multilingual learners (MLLs), working in an officially English-centric school district, make sense of a reading curriculum based in translingual pedagogies, or instruction that builds on language and languaging practices (e.g., language brokering, translation, and codemeshing) familiar to multilingual youth. Participating teachers, describing themselves as mostly monolingual educators, utilized the curriculum during a support class for their MLLs. We show how this curriculum, containing what we classify as educative curriculum materials (Davis & Krajcik, 2005), operated to support, and extend linguistically supportive instructional practices occurring within participating teachers' classroom figured worlds (Holland et al., 1998). Using data from classroom observations and teacher interviews, we show how the curriculum operated as a mediating artifact to support teachers' development of more linguistically diverse practices within their classrooms. Findings indicate that curriculum materials bridged theory to practice by supporting teacher development of these practices, which, in turn, bolstered their beliefs in the importance of students' home languages, and led to a shift in how teachers understood, interpreted, and resisted English-centric policies at their schools.

Published
2024
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74. THE ULTIMATE MEN'S HEALTH GUY

Author

Galloway, Noah, Vercher, John, Gonzalez, Daniel, and Smith, Bryan

Subjects
Psychological aspects, Social aspects, Health aspects, Men -- Psychological aspects -- Health aspects -- Social aspects
Abstract

For a decade, we've SEARCHED THE NATION FOR MEN WE ADMIRE--men who are PHYSICALLY STRONG, yes, but also MENTALLY RESILIENT, SOCIALLY CONNECTED, and ALL-AROUND GOOD GUYS. This year's finalists embody [...]

Published
2024

76. Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD

Author

Leloup, C., Patanchon, G., Errard, J., Franceschet, C., Gudmundsson, J. E., Henrot-Versillé, S., Imada, H., Ishino, H., Matsumura, T., Puglisi, G., Wang, W., Adler, A., Aumont, J., Aurlien, R., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basyrov, A., Bersanelli, M., Blinov, D., Bortolami, M., Brinckmann, T., Campeti, P., Carones, A., Carralot, F., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., de Haan, T., De Petris, M., Della Torre, S., Diego-Palazuelos, P., Eriksen, H. K., Finelli, F., Fuskeland, U., Galloni, G., Galloway, M., Georges, M., Gerbino, M., Gervasi, M., Génova-Santos, R. T., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., Gruppuso, A., Hazumi, M., Hergt, L. T., Herranz, D., Hivon, E., Hoang, T. D., Jost, B., Kohri, K., Krachmalnicoff, N., Lee, A. T., Lembo, M., Levrier, F., Lonappan, A. I., López-Caniego, M., Macias-Perez, J., Martínez-González, E., Masi, S., Matarrese, S., Micheli, S., Monelli, M., Montier, L., Morgante, G., Mot, B., Mousset, L., Namikawa, T., Natoli, P., Novelli, A., Noviello, F., Obata, I., Odagiri, K., Pagano, L., Paiella, A., Paoletti, D., Pascual-Cisneros, G., Pavlidou, V., Piacentini, F., Piccirilli, G., Pisano, G., Polenta, G., Raffuzzi, N., Remazeilles, M., Ritacco, A., Rizzieri, A., Ruiz-Granda, M., Sakurai, Y., Shiraishi, M., Stever, S. L., Takase, Y., Tassis, K., Terenzi, L., Thompson, K. L., Tristram, M., Vacher, L., Vielva, P., Wehus, I. K., Weymann-Despres, G., Zannoni, M., and Zhou, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present a study of the impact of an uncertainty in the beam far side-lobe knowledge on the measurement of the Cosmic Microwave Background $B$-mode signal at large scale. It is expected to be one of the main source of systematic effects in future CMB observations. Because it is crucial for all-sky survey missions to take into account the interplays between beam systematic effects and all the data analysis steps, the primary goal of this paper is to provide the methodology to carry out the end-to-end study of their effect for a space-borne CMB polarization experiment, up to the cosmological results in the form of a bias $\delta r$ on the tensor-to-scalar ratio $r$. LiteBIRD is dedicated to target the measurement of CMB primordial $B$ modes by reaching a sensitivity of $\sigma \left( r \right) \leq 10^{-3}$ assuming $r=0$. As a demonstration of our framework, we derive the relationship between the knowledge of the beam far side-lobes and the tentatively allocated error budget under given assumptions on design, simulation and component separation method. We assume no mitigation of the far side-lobes effect at any stage of the analysis pipeline. We show that $\delta r$ is mostly due to the integrated fractional power difference between the estimated beams and the true beams in the far side-lobes region, with little dependence on the actual shape of the beams, for low enough $\delta r$. Under our set of assumptions, in particular considering the specific foreground cleaning method we used, we find that the integrated fractional power in the far side-lobes should be known at a level as tight as $\sim 10^{-4}$, to achieve the required limit on the bias $\delta r < 1.9 \times 10^{-5}$. The framework and tools developed for this study can be easily adapted to provide requirements under different design, data analysis frameworks and for other future space-borne experiments beyond LiteBIRD.

Published
2023

77. LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing

Author

Namikawa, T., Lonappan, A. I., Baccigalupi, C., Bartolo, N., Beck, D., Benabed, K., Challinor, A., Diego-Palazuelos, P., Errard, J., Farrens, S., Gruppuso, A., Krachmalnicoff, N., Migliaccio, M., Martínez-González, E., Pettorino, V., Piccirilli, G., Ruiz-Granda, M., Sherwin, B., Starck, J., Vielva, P., Akizawa, R., Anand, A., Aumont, J., Aurlien, R., Azzoni, S., Ballardini, M., Banday, A. J., Barreiro, R. B., Bersanelli, M., Blinov, D., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carones, A., Carralot, F., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., de Haan, T., De Petris, M., Della Torre, S., Di Giorgi, E., Eriksen, H. K., Finelli, F., Franceschet, C., Fuskeland, U., Galloni, G., Galloway, M., Georges, M., Gerbino, M., Gervasi, M., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Hivon, E., Kohri, K., Komatsu, E., Lamagna, L., Lattanzi, M., Leloup, C., Lembo, M., López-Caniego, M., Luzzi, G., Maffei, B., Masi, S., Massa, M., Matarrese, S., Matsumura, T., Micheli, S., Moggi, A., Monelli, M., Montier, L., Morgante, G., Mot, B., Mousset, L., Nagata, R., Natoli, P., Novelli, A., Obata, I., Occhiuzzi, A., Pagano, L., Paiella, A., Paoletti, D., Pascual-Cisneros, G., Pavlidou, V., Piacentini, F., Pinchera, M., Pisano, G., Polenta, G., Puglisi, G., Remazeilles, M., Ritacco, A., Rizzieri, A., Rubino-Martin, J., Sakurai, Y., Scott, D., Shiraishi, M., Signorelli, G., Stever, S. L., Takase, Y., Tanimura, H., Tartari, A., Tassis, K., Terenzi, L., Tristram, M., Vacher, L., van Tent, B., Wehus, I. K., Weymann-Despres, G., Zannoni, M., and Zhou, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We estimate the efficiency of mitigating the lensing $B$-mode polarization, the so-called delensing, for the $LiteBIRD$ experiment with multiple external data sets of lensing-mass tracers. The current best bound on the tensor-to-scalar ratio, $r$, is limited by lensing rather than Galactic foregrounds. Delensing will be a critical step to improve sensitivity to $r$ as measurements of $r$ become more and more limited by lensing. In this paper, we extend the analysis of the recent $LiteBIRD$ forecast paper to include multiple mass tracers, i.e., the CMB lensing maps from $LiteBIRD$ and CMB-S4-like experiment, cosmic infrared background, and galaxy number density from $Euclid$- and LSST-like survey. We find that multi-tracer delensing will further improve the constraint on $r$ by about $20\%$. In $LiteBIRD$, the residual Galactic foregrounds also significantly contribute to uncertainties of the $B$-modes, and delensing becomes more important if the residual foregrounds are further reduced by an improved component separation method., Comment: 21 pages, 7 figures

Published
2023
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78. LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB

Author

Lonappan, A. I., Namikawa, T., Piccirilli, G., Diego-Palazuelos, P., Ruiz-Granda, M., Migliaccio, M., Baccigalupi, C., Bartolo, N., Beck, D., Benabed, K., Challinor, A., Errard, J., Farrens, S., Gruppuso, A., Krachmalnicoff, N., Martínez-González, E., Pettorino, V., Sherwin, B., Starck, J., Vielva, P., Akizawa, R., Anand, A., Aumont, J., Aurlien, R., Azzoni, S., Ballardini, M., Banday, A. J., Barreiro, R. B., Bersanelli, M., Blinov, D., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carones, A., Carralot, F., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., De Petris, M., Della Torre, S., Di Giorgi, E., Eriksen, H. K., Finelli, F., Franceschet, C., Fuskeland, U., Galloni, G., Galloway, M., Georges, M., Gerbino, M., Gervasi, M., Génova-Santos, R. T., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Hivon, E., Kohri, K., Komatsu, E., Lamagna, L., Lattanzi, M., Leloup, C., Lembo, M., López-Caniego, M., Luzzi, G., Macias-Perez, J., Maffei, B., Masi, S., Massa, M., Matarrese, S., Matsumura, T., Micheli, S., Moggi, A., Monelli, M., Montier, L., Morgante, G., Mot, B., Mousset, L., Nagata, R., Natoli, P., Novelli, A., Obata, I., Occhiuzzi, A., Pagano, L., Paiella, A., Paoletti, D., Pascual-Cisneros, G., Pavlidou, V., Piacentini, F., Pinchera, M., Pisano, G., Polenta, G., Puglisi, G., Remazeilles, M., Ritacco, A., Rizzieri, A., Sakurai, Y., Scott, D., Shiraishi, M., Signorelli, G., Stever, S. L., Takase, Y., Tanimura, H., Tartari, A., Tassis, K., Terenzi, L., Tristram, M., Vacher, L., van Tent, B., Wehus, I. K., Weymann-Despres, G., Zannoni, M., and Zhou, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We explore the capability of measuring lensing signals in $LiteBIRD$ full-sky polarization maps. With a $30$ arcmin beam width and an impressively low polarization noise of $2.16\,\mu$K-arcmin, $LiteBIRD$ will be able to measure the full-sky polarization of the cosmic microwave background (CMB) very precisely. This unique sensitivity also enables the reconstruction of a nearly full-sky lensing map using only polarization data, even considering its limited capability to capture small-scale CMB anisotropies. In this paper, we investigate the ability to construct a full-sky lensing measurement in the presence of Galactic foregrounds, finding that several possible biases from Galactic foregrounds should be negligible after component separation by harmonic-space internal linear combination. We find that the signal-to-noise ratio of the lensing is approximately $40$ using only polarization data measured over $90\%$ of the sky. This achievement is comparable to $Planck$'s recent lensing measurement with both temperature and polarization and represents a four-fold improvement over $Planck$'s polarization-only lensing measurement. The $LiteBIRD$ lensing map will complement the $Planck$ lensing map and provide several opportunities for cross-correlation science, especially in the northern hemisphere.

Published
2023
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79. LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization

Author

Campeti, P., Komatsu, E., Baccigalupi, C., Ballardini, M., Bartolo, N., Carones, A., Errard, J., Finelli, F., Flauger, R., Galli, S., Galloni, G., Giardiello, S., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Kohri, K., Leloup, C., Lesgourgues, J., Macias-Perez, J., Martínez-González, E., Matarrese, S., Matsumura, T., Montier, L., Namikawa, T., Paoletti, D., Poletti, D., Remazeilles, M., Shiraishi, M., van Tent, B., Tristram, M., Vacher, L., Vittorio, N., Weymann-Despres, G., Anand, A., Aumont, J., Aurlien, R., Banday, A. J., Barreiro, R. B., Basyrov, A., Bersanelli, M., Blinov, D., Bortolami, M., Brinckmann, T., Calabrese, E., Carralot, F., Casas, F. J., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., De Petris, M., Della Torre, S., Di Giorgi, E., Diego-Palazuelos, P., Eriksen, H. K., Franceschet, C., Fuskeland, U., Galloway, M., Georges, M., Gerbino, M., Gervasi, M., Ghigna, T., Gimeno-Amo, C., Gjerløw, E., Gruppuso, A., Gudmundsson, J., Krachmalnicoff, N., Lamagna, L., Lattanzi, M., Lembo, M., Lonappan, A. I., Masi, S., Massa, M., Micheli, S., Moggi, A., Monelli, M., Morgante, G., Mot, B., Mousset, L., Nagata, R., Natoli, P., Novelli, A., Obata, I., Pagano, L., Paiella, A., Pavlidou, V., Piacentini, F., Pinchera, M., Pisano, G., Puglisi, G., Raffuzzi, N., Ritacco, A., Rizzieri, A., Ruiz-Granda, M., Savini, G., Scott, D., Signorelli, G., Stever, S. L., Stutzer, N., Sullivan, R. M., Tartari, A., Tassis, K., Terenzi, L., Thompson, K. L., Vielva, P., Wehus, I. K., and Zhou, Y.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology
Abstract

We study the possibility of using the $LiteBIRD$ satellite $B$-mode survey to constrain models of inflation producing specific features in CMB angular power spectra. We explore a particular model example, i.e. spectator axion-SU(2) gauge field inflation. This model can source parity-violating gravitational waves from the amplification of gauge field fluctuations driven by a pseudoscalar "axionlike" field, rolling for a few e-folds during inflation. The sourced gravitational waves can exceed the vacuum contribution at reionization bump scales by about an order of magnitude and can be comparable to the vacuum contribution at recombination bump scales. We argue that a satellite mission with full sky coverage and access to the reionization bump scales is necessary to understand the origin of the primordial gravitational wave signal and distinguish among two production mechanisms: quantum vacuum fluctuations of spacetime and matter sources during inflation. We present the expected constraints on model parameters from $LiteBIRD$ satellite simulations, which complement and expand previous studies in the literature. We find that $LiteBIRD$ will be able to exclude with high significance standard single-field slow-roll models, such as the Starobinsky model, if the true model is the axion-SU(2) model with a feature at CMB scales. We further investigate the possibility of using the parity-violating signature of the model, such as the $TB$ and $EB$ angular power spectra, to disentangle it from the standard single-field slow-roll scenario. We find that most of the discriminating power of $LiteBIRD$ will reside in $BB$ angular power spectra rather than in $TB$ and $EB$ correlations., Comment: 22 pages, 13 figures. Submitted to JCAP

Published
2023

80. Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data

Author

Watts, D. J., Fuskeland, U., Aurlien, R., Basyrov, A., Bianchi, L. A., Brilenkov, M., Eriksen, H. K., Fornazier, K. S. F., Galloway, M., Gjerløw, E., Hensley, B., Hergt, L. T., Herman, D., Ihle, H., Lee, K., Lunde, J. G. S., Nerval, S. K., San, M., Stutzer, N. O., Thommesen, H., and Wehus, I. K.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present the first model of full-sky polarized synchrotron emission that is derived from all WMAP and Planck LFI frequency maps. The basis of this analysis is the set of end-to-end reprocessed Cosmoglobe Data Release 1 sky maps presented in a companion paper, which have significantly lower instrumental systematics than the legacy products from each experiment. We find that the resulting polarized synchrotron amplitude map has an average noise rms of $3.2\,\mathrm{\mu K}$ at 30 GHz and $2^{\circ}$ FWHM, which is 30% lower than the recently released BeyondPlanck model that included only LFI+WMAP Ka-V data, and 29% lower than the WMAP K-band map alone. The mean $B$-to-$E$ power spectrum ratio is $0.40\pm0.02$, with amplitudes consistent with those measured previously by Planck and QUIJOTE. Assuming a power law model for the synchrotron spectral energy distribution, and using the $T$--$T$ plot method, we find a full-sky inverse noise-variance weighted mean of $\beta_{\mathrm{s}}=-3.07\pm0.07$ between Cosmoglobe DR1 K-band and 30 GHz, in good agreement with previous estimates. In summary, the novel Cosmoglobe DR1 synchrotron model is both more sensitive and systematically cleaner than similar previous models, and it has a more complete error description that is defined by a set of Monte Carlo posterior samples. We believe that these products are preferable over previous Planck and WMAP products for all synchrotron-related scientific applications, including simulation, forecasting and component separation., Comment: 15 pages, 15 figures, submitted to A&A

Published
2023
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81. Chasing Gravitational Waves with the Cherenkov Telescope Array

Author

Green, Jarred Gershon, Carosi, Alessandro, Nava, Lara, Patricelli, Barbara, Schüssler, Fabian, Seglar-Arroyo, Monica, Consortium, Cta, Abe, Kazuki, Abe, Shotaro, Acharyya, Atreya, Adam, Remi, Aguasca-Cabot, Arnau, Agudo, Ivan, Alfaro, Jorge, Alvarez-Crespo, Nuria, Batista, Rafael Alves, Amans, Jean-Philippe, Amato, Elena, Ambrosino, Filippo, Angüner, Ekrem Oguzhan, Antonelli, Lucio Angelo, Aramo, Carla, Arcaro, Cornelia, Arrabito, Luisa, Asano, Katsuaki, Aschersleben, Jann, Ashkar, Halim, Stuani, Luiz Augusto, Baack, Dominik, Backes, Michael, Balazs, Csaba, Balbo, Matteo, Larriva, Andres Baquero, Martins, Victor Barbosa, de Almeida, Ulisses Barres, Barrio, Juan Abel, Bastieri, Denis, Batista, Pedro Ivo, Batković, Ivana, Batzofin, Rowan William, Baxter, Joshua Ryo, Beck, Geoffrey, Tjus, Julia Becker, Beiske, Lukas, Belardinelli, Daniele, Benbow, Wystan, Bernardini, Elisa, Medrano, Juan Bernete, Bernlöhr, Konrad, Berti, Alessio, Beshley, Vasyl, Bhattacharjee, Pooja, Bhattacharyya, Saptashwa, Bi, Baiyang, Biederbeck, Noah, Biland, Adrian, Bissaldi, Elisabetta, Blanch, Oscar, Blazek, Jiri, Boisson, Catherine, Bolmont, Julien, Bonnoli, Giacomo, Bordas, Pol, Bošnjak, Željka, Bradascio, Federica, Braiding, Catherine, Bronzini, Ettore, Brose, Robert, Brown, Anthony M., Brun, Francois, Brunelli, Giulia, Bulgarelli, Andrea, Burelli, Irene, Burmistrov, Leonid, Burton, Michael, Bylund, Tomas, Calisse, Paolo Gherardo, Campoy-Ordaz, Anna, Cantlay, Brandon Khan, Capalbi, Milvia, Caproni, Anderson, Capuzzo-Dolcetta, Roberto, Carlile, Colin, Caroff, Sami, Carosi, Roberto, Carrasco, Marie-Sophie, Cascone, Enrico, Cassol, Franca, Castrejon, Noelia, Catalani, Fernando, Cerasole, Davide, Cerruti, Matteo, Chaty, Sylvain, Chen, Andrew W, Chernyakova, Maria, Chiavassa, Andrea, Chudoba, Jiří, Araujo, Carlos Henrique Coimbra, Conforti, Vito, Conte, Francesco, Contreras, Jose Luis, Cossou, Christophe, Costa, Alessandro, Costantini, Heide, Cristofari, Pierre, Cuevas, Omar, Curtis-Ginsberg, Zachary, D'Amico, Giacomo, D'Ammando, Filippo, Dadina, Mauro, Dalchenko, Mykhailo, David, Ludovic, Davids, Isak Delberth, Dazzi, Francesco, De Angelis, Alessandro, de Lavergne, Mathieu de Bony, De Caprio, Vincenzo, De Cesare, Giovanni, Pino, Elisabete M. de Gouveia Dal, De Lotto, Barbara, de Lucia, Mario, de Menezes, Raniere, de Naurois, Mathieu, Wilhelmi, Emma de Oña, De Simone, Nicola, de Souza, Vitor, Del Peral, Luis, del Valle, Maria Victoria, Delagnes, Eric, Giler, Andres Gabriel Delgado, Delgado, Carlos, Dell'aiera, Michael, Della Ceca, Roberto, Della Valle, Massimo, Della Volpe, Domenico, Depaoli, Davide, Dettlaff, Antonios, Di Girolamo, Tristano, Di Piano, Ambra, Di Pierro, Federico, Di Tria, Riccardo, Di Venere, Leonardo, Díaz-Bahamondes, Christian, Dib, Claudio, Diebold, Sebastian, Dima, Razvan, Dinesh, Adithiya, Djannati-Ataï, Arache, Djuvsland, Julia Isabel, Dominguez, Alberto, Dominik, Rune Michael, Donini, Alice, Dorner, Daniela, Dörner, Julien, Doro, Michele, Anjos, Rita de Cassia dos, Dournaux, Jean-Laurent, Dravins, Dainis, Duangchan, Chaimongkol, Dubos, Coline, Ducci, Lozenzo, Dwarkadas, Vikram V., Ebr, Jan, Eckner, Christopher, Egberts, Kathrin, Einecke, Sabrina, Elsässer, Dominik, Emery, Gabriel, Godoy, Miguel Escobar, Escudero, Juan, Esposito, Paolo, Falceta-Gonçalves, Diego, Ramazani, Vandad Fallah, Faure, Alice, Fedorova, Elena, Fegan, Stephen, Feijen, Kirsty, Feng, Qi, Ferrand, Gilles, Ferrarotto, Fabio, Fiandrini, Emanuele, Fiasson, Armand, Fioretti, Valentina, Foffano, Luca, Guiteras, Lluis Font, Fontaine, Gerard, Fröse, Stefan, Fukami, Satoshi, Fukui, Yasuo, Funk, Stefan, Gaggero, Daniele, Galanti, Giorgio, Galaz, Gaspar, Gallant, Yves A., Gallozzi, Stefano, Gammaldi, Viviana, Gasbarra, Claudio, Gaug, Markus, Ghalumyan, Arsen, Gianotti, Fulvio, Giarrusso, Marina, Giglietto, Nicola, Giordano, Francesco, Giuliani, Andrea, Glicenstein, Jean-Francois, Glombitza, Jonas, Goldoni, Paolo, González, José Mauricio, González, Maria Magdalena, Coelho, Jaziel Goulart, Granot, Jonathan, Grasso, Dario, Haro, Roger Grau, Green, David, Greenshaw, Tim, Grolleron, Guillaume, Grube, Jeff, Gueta, Orel, Gunji, Shuichi, Hadasch, Daniela, Hamal, Petr, Hanlon, William, Hara, Satoshi, Harvey, Violet M., Hashiyama, Kazuaki, Hassan, Tarek, Heller, Matthieu, Cadena, Sergio Hernández, Hie, Jonathan, Hiroshima, Nagisa, Hnatyk, Bohdan, Hnatyk, Roman, Hoffmann, Dirk, Hofmann, Werner, Holler, Markus, Horan, Deirdre, Horvath, Pavel, Hovatta, Talvikki, Hrupec, Dario, Hussain, Saqib, Iarlori, Marco, Inada, Tomohiro, Incardona, Federico, Inome, Yusuke, Inoue, Susumu, Iocco, Fabio, Ishio, Kazuma, Jamrozy, Marek, Janecek, Petr, Jankowsky, Felix, Jarnot, Christian, Jean, Pierre, Martínez, Irene Jiménez, Jin, Weidong, Jocou, Laurent, Juramy-Gilles, Claire, Jurysek, Jakub, KALEKIN, Oleg, Kantzas, Dimitrios, Karas, Vladimir, Kaufmann, Sarah, Kerszberg, Daniel, Khelifi, Bruno, Kieda, David B, Kleiner, Tobias Kai, Kluźniak, Włodzimierz, Kobayashi, Yukiho, Kohri, Kazunori, Komin, Nukri, Kornecki, Paula, Kosack, Karl, Kubo, Hidetoshi, Kushida, Junko, La Barbera, Antonino, La Palombara, Nicola, Lainez, Maria, Lamastra, Alessandra, Lapington, Jon S, Lazarevic, Sanja, Lazendic-Galloway, Jasmina, Leach, Steven, Lemoine-Goumard, Marianne, Lenain, Jean-Philippe, Leto, Giuseppe, Leuschner, Fabian, Lindfors, Elina, Linhoff, Maximilian, Liodakis, Ioannis, Loïc, Lozach, Lombardi, Saverio, Longo, Francesco, López-Coto, Rubén, López-Moya, Marcos, López-Oramas, Alicia, Loporchio, Serena, Bahilo, Julio Lozano, Luque-Escamilla, Pedro L., Macias, Oscar, Maier, Gernot, Majumdar, Pratik, Malyshev, Denys, Malyshev, Dmitry, Mandat, Dusan, Manicò, Giulio, Marinos, Peter David, Markoff, Sera, Márquez, Isabel, Marquez, Patricia, Marsella, Giovanni, Martí, Josep, Martin, Pierrick, Martínez, Gustavo Augusto, Martínez, Manel, Martinez, Oibar, Marty, Christophe, Mas-Aguilar, Alvaro, Mastropietro, Michele, Maurin, Gilles, Max-Moerbeck, Walter, Mazin, Daniel, Melkumyan, David, Menchiari, Stefano, Mestre, Enrique, Meunier, Jean-Luc, Meyer, Dominique M. -A., Miceli, Davide, Michailidis, Miltiadis, Michałowski, Jerzy, Miener, Tjark, Miranda, Jose Miguel, Mitchell, Alison, Mizote, Masaya, Mizuno, Tsunefumi, Moderski, Rafal, Mohrmann, Lars, Molero, Miguel, Molfese, Cesare, Molina, Edgar, Montaruli, Teresa, Moralejo, Abelardo, Morcuende, Daniel, Morik, Katharina, Morselli, Aldo, Moulin, Emmanuel, Zamanillo, Victor Moya, Mukherjee, Reshmi, Munari, Kevin, Muraczewski, Adam, Muraishi, Hiroshi, Nakamori, Takeshi, Nayak, Amrit, Nemmen, Rodrigo, Nickel, Lukas, Niemiec, Jacek, Nieto, Daniel, Rosillo, Mireia Nievas, Nikołajuk, Marek, Nishijima, Kyoshi, Noda, Koji, Nosek, Dalibor, Novosyadlyj, Bohdan, Novotný, Vladimír, Nozaki, Seiya, O'Brien, Paul, Ohishi, Michiko, Ohtani, Yoshiki, Okumura, Akira, Olive, Jean-François, Olmi, Barbara, Ong, Rene A., Orienti, Monica, Orito, Reiko, Orlandini, Mauro, Orlando, Elena, Ostrowski, Michal, Otte, Nepomuk, Oya, Igor, Pagano, Isabella, Pagliaro, Antonio, Palatiello, Michele, Panebianco, Gabriele, Paredes, Josep M., Parmiggiani, Nicolò, Patel, Sonal Ramesh, Pavlović, Dijana, Pe'er, Asaf, Pech, Miroslav, Pecimotika, Mario, Peresano, Michele, Pérez-Romero, Judit, Peron, Giada, Persic, Massimo, Petrucci, Pierre-Olivier, Petruk, Oleh, Pfeifle, Felix, Pintore, Fabio, Pirola, Giorgio, Pittori, Carlotta, Plard, Cyann, Podobnik, Franjo, Pohl, Martin, Pons, Estelle, Prandini, Elisa, Prast, Julie, Principe, Giacomo, Priyadarshi, Chaitanya, Produit, Nicolas, Prokhorov, Dmitry, Pueschel, Elisa, Pühlhofer, Gerd, Pumo, Maria Letizia, Punch, Michael, Quirrenbach, Andreas, Raino, Silvia, Randazzo, Nunzio, Rando, Riccardo, Ravel, Thierry, Razzaque, Soebur, Regeard, Maxime, Reichherzer, Patrick, Reimer, Anita, Reimer, Olaf, Reisenegger, Andreas, Reposeur, Thierry, Reville, Brian, Rhode, Wolfgang, Ribó, Marc, Richtler, Tom, Rieger, Frank, Roache, Emmet, Fernandez, Gonzalo Rodriguez, Frías, Maria Dolores Rodríguez, Rodríguez-Vázquez, Juan José, Romano, Patrizia, Romeo, Giuseppe, Rosado, Jaime, Rowell, Gavin P, Rudak, Bronislaw, Ruiter, Ashley J., Rulten, Cameron Boyd, Russo, Federico, Sadeh, Iftach, Saha, Lab, Saito, Takayuki, Sakurai, Shunsuke, Salzmann, Heiko, Sanchez, David, Sanchez-Conde, Miguel, Sangiorgi, Pierluca, Sano, Hidetoshi, Santander, Marcos, Santangelo, Andrea, Santos-Lima, Reinaldo, Sanuy, Andreu, Šarić, Toni, Sarkar, Arkadipta, Sarkar, Subir, Saturni, Francesco Gabriele, Savchenko, Volodymyr, Scherer, Andres, Schipani, Pietro, Schleicher, Bernd, Schovanek, Petr, Schubert, Jan Lukas, Schwanke, Ullrich, Schwefer, Georg, Scuderi, Salvatore, Arroyo, Monica Seglar, Seitenzahl, Ivo, Sergijenko, Olga, Sguera, Vito, Shang, Ruo-Yu, Sharma, Pooja, Sidibe, Guereguin Der Sylvestre, Sidoli, Lara, Siejkowski, Hubert, Siqueira, Clarissa, Sizun, Patrick, Sliusar, Vitalii, Slowikowska, Agnieszka, Sol, Helene, Specovius, Andreas, Spencer, Samuel Timothy, Spiga, Daniele, Stamerra, Antonio, Stanič, Samo, Starecki, Tomasz, Starling, Rhaana, Steppa, Constantin, Stolarczyk, Thierry, Strišković, Jelena, Strzys, Marcel C., Suda, Yusuke, Suomijarvi, Tiina, Tak, Donggeun, Takahashi, Mitsunari, Takeishi, Ryuji, Tam, Pak-Hin Thomas, Tanaka, Shuta J, Tanaka, Takaaki, Terauchi, Kenta, Testa, Vincenzo, Tibaldo, Luigi, Tibolla, Omar, Torradeflot, Francesc, Torres, Diego F., Torresi, Eleonora, Tothill, Nick, Toussenel, Francois, Touzard, Victoria, Tramacere, Andrea, Travnicek, Petr, Tripodo, Giovanni, Truzzi, Stefano, Tsiahina, Adellain, Tutone, Antonio, Vacula, Martin, Vallage, Bertrand, Vallania, Piero, Vallés, Ramon, van Eldik, Christopher, van Scherpenberg, Juliane, Vandenbroucke, Justin, Vassiliev, Vladimir, Venault, Philippe, Ventura, Sofia, Vercellone, Stefano, Verna, Gaia, Viana, Aion, Viaux, Nicolás, Vigliano, Alessandro, Vignatti, Jonatan, Vigorito, Carlo francesco, Vitale, Vincenzo, Vodeb, Veronika, Voisin, Vincent, Vorobiov, Serguei, Voutsinas, Georgios Gerasimos, Vovk, Ievgen, Waegebaert, Vincent, Wagner, Stefan Joachim, Walter, Roland, Ward, Martin, Wechakama, Maneenate, White, Richard, Wierzcholska, Alicja, Will, Martin, Williams, David A., Wohlleben, Frederik, Wolter, Anna, Yamamoto, Tokonatsu, Yamazaki, Ryo, Yang, Lili, Yoshida, Tatsuo, Yoshikoshi, Takanori, Zacharias, Michael, Sanchez, Ricardo Zanmar, Zavrtanik, Danilo, Zavrtanik, Marko, Zdziarski, Andrzej A., Zech, Andreas, Zhdanov, Valery I., Ziȩtara, Krzysztof, Živec, Miha, and Zuriaga-Puig, Jaume

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this gravitational wave event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100GeV) photons which have yet to be detected in coincidence with a gravitational wave signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. New observing modes and follow-up strategies are being developed for CTA to rapidly cover localization areas of gravitational wave events that are typically larger than the CTA field of view. This work will evaluate and provide estimations on the expected number of of gravitational wave events that will be observable with CTA, considering both on- and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA., Comment: Presented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219)

Published
2023

82. The dementia care study (D‐CARE): Recruitment strategies and demographic characteristics of participants in a pragmatic randomized trial of dementia care

Author

Yang, Mia, Samper‐Ternent, Rafael, Volpi, Elena, Green, Aval‐Na'Ree, Lichtenstein, Maya, Araujo, Katy, Borek, Pamela, Charpentier, Peter, Dziura, James, Gill, Thomas M, Galloway, Rebecca, Greene, Erich J, Lenoir, Kristin, Peduzzi, Peter, Meng, Can, Reese, Jordan, Shelton, Amy, Skokos, Eleni A, Summapund, Jenny, Unger, Erin, Reuben, David B, Williamson, Jeff D, and Stevens, Alan B

Subjects
Biomedical and Clinical Sciences, Biological Psychology, Clinical Sciences, Neurosciences, Psychology, Clinical Research, Brain Disorders, Patient Safety, Alzheimer's Disease including Alzheimer's Disease Related Dementias (AD/ADRD), Clinical Trials and Supportive Activities, Aging, Alzheimer's Disease, Dementia, Behavioral and Social Science, Acquired Cognitive Impairment, Neurodegenerative, Neurological, Good Health and Well Being, caregivers, dementia care, pragmatic clinical trials, recruitment, Geriatrics, Clinical sciences, Biological psychology
Abstract

IntroductionPragmatic research studies that include diverse dyads of persons living with dementia (PLWD) and their family caregivers are rare.MethodsCommunity-dwelling dyads were recruited for a pragmatic clinical trial evaluating three approaches to dementia care. Four clinical trial sites used shared and site-specific recruitment strategies to enroll health system patients.ResultsElectronic health record (EHR) queries of patients with a diagnosis of dementia and engagement of their clinicians were the main recruitment strategies. A total of 2176 dyads were enrolled, with 80% recruited after the onset of the pandemic. PLWD had a mean age of 80.6 years (SD 8.5), 58.4% were women, and 8.8% were Hispanic/Latino, and 11.9% were Black/African American. Caregivers were mostly children of the PLWD (46.5%) or spouses/partners (45.2%), 75.8% were women, 9.4% were Hispanic/Latino, and 11.6% were Black/African American.DiscussionHealth systems can successfully enroll diverse dyads in a pragmatic clinical trial.

Published
2024

83. Virology—the path forward

Author

Rasmussen, Angela L, Gronvall, Gigi K, Lowen, Anice C, Goodrum, Felicia, Alwine, James, Andersen, Kristian G, Anthony, Simon J, Baines, Joel, Banerjee, Arinjay, Broadbent, Andrew J, Brooke, Christopher B, Campos, Samuel K, Caposio, Patrizia, Casadevall, Arturo, Chan, Gary C, Cliffe, Anna R, Collins-McMillen, Donna, Connell, Nancy, Damania, Blossom, Daugherty, Matthew D, Debbink, Kari, Dermody, Terence S, DiMaio, Daniel, Duprex, W Paul, Emerman, Michael, Galloway, Denise A, Garry, Robert F, Goldstein, Stephen A, Greninger, Alexander L, Hartman, Amy L, Hogue, Brenda G, Horner, Stacy M, Hotez, Peter J, Jung, Jae U, Kamil, Jeremy P, Karst, Stephanie M, Laimins, Lou, Lakdawala, Seema S, Landais, Igor, Letko, Michael, Lindenbach, Brett, Liu, Shan-Lu, Luftig, Micah, McFadden, Grant, Mehle, Andrew, Morrison, Juliet, Moscona, Anne, Mühlberger, Elke, Munger, Joshua, Münger, Karl, Murphy, Eain, Neufeldt, Christopher J, Nikolich, Janko Z, O'Connor, Christine M, Pekosz, Andrew, Permar, Sallie R, Pfeiffer, Julie K, Popescu, Saskia V, Purdy, John G, Racaniello, Vincent R, Rice, Charles M, Runstadler, Jonathan A, Sapp, Martin J, Scott, Rona S, Smith, Gregory A, Sorrell, Erin M, Speranza, Emily, Streblow, Daniel, Tibbetts, Scott A, Toth, Zsolt, Van Doorslaer, Koenraad, Weiss, Susan R, White, Elizabeth A, White, Timothy M, Wobus, Christiane E, Worobey, Michael, Yamaoka, Satoko, and Yurochko, Andrew

Subjects
Agricultural, Veterinary and Food Sciences, Biological Sciences, Biomedical and Clinical Sciences, Coronaviruses, Prevention, Emerging Infectious Diseases, Infectious Diseases, Good Health and Well Being, Humans, Containment of Biohazards, COVID-19, United States, Viruses, Virology, Biomedical Research, virology, SARS-CoV-2, oversight, biosafety, emergence, Agricultural and Veterinary Sciences, Medical and Health Sciences, Agricultural, veterinary and food sciences, Biological sciences, Biomedical and clinical sciences
Abstract

In the United States (US), biosafety and biosecurity oversight of research on viruses is being reappraised. Safety in virology research is paramount and oversight frameworks should be reviewed periodically. Changes should be made with care, however, to avoid impeding science that is essential for rapidly reducing and responding to pandemic threats as well as addressing more common challenges caused by infectious diseases. Decades of research uniquely positioned the US to be able to respond to the COVID-19 crisis with astounding speed, delivering life-saving vaccines within a year of identifying the virus. We should embolden and empower this strength, which is a vital part of protecting the health, economy, and security of US citizens. Herein, we offer our perspectives on priorities for revised rules governing virology research in the US.

Published
2024

84. The XENONnT dark matter experiment.

Author

Aprile, E, Aalbers, J, Abe, K, Ahmed Maouloud, S, Althueser, L, Andrieu, B, Angelino, E, Angevaare, J, Antochi, V, Antón Martin, D, Arneodo, F, Balata, M, Baudis, L, Baxter, A, Bazyk, M, Bellagamba, L, Biondi, R, Bismark, A, Brookes, E, Brown, A, Bruenner, S, Bruno, G, Budnik, R, Bui, T, Cai, C, Cardoso, J, Cassese, F, Chiarini, A, Cichon, D, Cimental Chavez, A, Colijn, A, Conrad, J, Corrieri, R, Cuenca-García, J, Cussonneau, J, Dadoun, O, DAndrea, V, Decowski, M, De Fazio, B, Gangi, P, Diglio, S, Disdier, J, Douillet, D, Eitel, K, Elykov, A, Farrell, S, Ferella, A, Ferrari, C, Fischer, H, Flierman, M, Form, S, Front, D, Fulgione, W, Fuselli, C, Gaemers, P, Gaior, R, Rosso, A, Galloway, M, Gao, F, Gardner, R, Garroum, N, Glade-Beucke, R, Grandi, L, Grigat, J, Guan, H, Guerzoni, M, Guida, M, Hammann, R, Higuera, A, Hils, C, Hoetzsch, L, Hood, N, Howlett, J, Huhmann, C, Iacovacci, M, Iaquaniello, G, Iven, L, Itow, Y, Jakob, J, Joerg, F, Joy, A, Kara, M, Kavrigin, P, Kazama, S, Kobayashi, M, Koltman, G, Kopec, A, Kuger, F, Landsman, H, Lang, R, Levinson, L, Li, I, Li, S, Liang, S, Lindemann, S, Lindner, M, Liu, K, Loizeau, J, Lombardi, F, and Long, J

Abstract

The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (8.5 tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run.

Published
2024

85. Metagenomic Detection of Bacterial Zoonotic Pathogens among Febrile Patients, Tanzania, 2007-2009

Author

Rolfe, Robert J., Sheldon, Sarah W., Kingry, Luke C., Petersen, Jeannine M., Maro, Venance P., Kinabo, Grace D., Saganda, Wilbrod, Maze, Michael J., Halliday, Jo E.B., Nicholson, William L., Galloway, Renee L., Rubach, Matthew P., and Crump, John A.

Subjects
Diagnosis, Identification and classification, Genetic aspects, Methods, Causes of, Bacterial infections -- Diagnosis -- Causes of, DNA sequencing -- Methods, Pathogenic bacteria -- Identification and classification -- Genetic aspects, RNA sequencing -- Methods, Fever -- Diagnosis -- Causes of, Genomics -- Methods, Zoonoses -- Diagnosis -- Causes of, Nucleotide sequencing -- Methods, Bacteria, Pathogenic -- Identification and classification -- Genetic aspects, Hyperthermia -- Diagnosis -- Causes of
Abstract

Bacterial zoonoses cause severe febrile illness in East Africa (2). Patients with bacterial zoonotic diseases can have nonspecific febrile illnesses that are difficult to diagnose clinically or in the laboratory [...]

Published
2024
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86. Higher dose corticosteroids in hospitalised COVID-19 patients requiring ventilatory support (RECOVERY): a randomised, controlled, open-label, platform trial

Author

Abani, O., Abbas, A., Abbas, F., Abbas, J., Abbas, K., Abbas, M., Abbasi, S., Abbass, H., Abbott, A., Abdallah, N., Abdelaziz, A., Abdelfattah, M., Abdelqader, B., Abdul, A., Abdul, B., Abdul, S., Abdul Rasheed, A., Abdulakeem, A., Abdul-Kadir, R., Abdullah, A., Abdulmumeen, A., Abdul-Raheem, R., Abdulshukkoor, N., Abdusamad, K., Abed El Khaleq, Y., Abedalla, M., Abeer Ul Amna, A., Abel, L., Abernethy, K., Abeywickrema, M., Abhinaya, C., Abidin, A., Aboaba, A., Aboagye-Odei, A., Aboah, C., Aboelela, H., Abo-Leyah, H., Abouelela, K., Abou-Haggar, A., Abouibrahim, M., Abousamra, A., Abouzaid, M., Abraham, M., Abraham, T., Abraheem, A., Abrams, J., Abrams, R., Abu, H.J., Abu-Arafeh, A., Abubacker, S.M., Abung, A., Abusamra, Y., Aceampong, Y., Achara, A., Acharya, D., Acheampong, F., Acheampong, P., Acheampong, S., Acheson, J., Achieng, S., Acosta, A., Acquah, R., Acton, C., Adabie-Ankrah, J., Adair, P., Adam, A.S., Adam, F., Adam, M., Adamali, H., Adamczyk, M., Adams, C., Adams, D., Adams, K., Adams, L., Adams, N., Adams, R., Adams, T., Adamu-Ikeme, L., Adatia, K., Adcock, K., Addai-Boampong, L., Addo, A., Adeagbo, O., Adebiyi, A., Adedeji, O., Adegeye, Y., Adegoke, K., Adell, V., Adenwalla, S., Adeoye, F.W., Adesemoye, O.A., Adewunmi, E.O., Adeyanju, A., Adeyemi, J., Adeyemo, T., Adhikari, B., Adhikari, S.A., Adhikary, R., Aditya, A., Adjepong, P., Adkins, G., Adnan, A., Adriaanse, M., Aeron-Thomas, J., Affleck, D., Afnan, C., Afridi, M., Afrim, P., Afriyie, F.A., Aftab, Z.A., Afum-Adjei Awuah, A., Agarwal, M., Agasiya, P.N., Agbeko, R., Agbo, C., Aggarwal, S., Aghababaie, A., Aguilar Jimenez, L., Agyekum, J.A., Agyen, K., Ahadome, E.K., Ahamed Sadiq, S., Ahammed Nazeer, M.H., Ahmad, M., Ahmad, S., Ahmed, A., Ahmed, B.A.R., Ahmed, B., Ahmed, F., Ahmed, H., Ahmed, I., Ahmed, K., Ahmed, L., Ahmed, M., Ahmed, M.C., Ahmed, M.S., Ahmed, N., Ahmed, O., Ahmed, R.A., Ahmed, R., Ahmed, S., Ahmed, S.G., Ahmed, S.H., Ahmed Ali, R., Ahmed Mohamud, B., Ahmer, S., Ahonia, A., Aidoo, C., Aiken, C., Ail, D., Ainsworth, M., Aissa, M., Aitken, L., Ajay, B., Ajibode, A., Ajmi, A., Akhtar, N., Akili, S., Akinbiyi, B., Akindolie, O., Akinfenwa, Y., Akinkugbe, O., Akinpelu, I., Akram, M., Aktinade, O., Akudi, U., Al Aaraj, A.S.A.R., Al Balushi, A., Al Dakhola, M., Al Swaifi, A., Al-Abadi, E., Alabi, A., Aladangady, N., Alafifi, M., Alam, A., Alam, S., Al-Asadi, A., Alatzoglou, K., Albert, P., Albertus, A., Albon, L., Alcala, A., Alcorn, G., Alcorn, S., Aldana, A., Alderdice, D., Aldesouki, A., Aldouri, R., Aldridge, J., Aldridge, N., Ale, R., Ale, R.M., Alegria, A., Alexander, A., Alexander, C., Alexander, J., Alexander, P.D.G., Al-fori, J., Alghazawi, L., Alhabsha, O., Al-Hakim, B., Alhameed, R., Al-Hayali, M., Al-Hity, S., Ali, A., Ali, F.R., Ali, J., Ali, M., Ali, M.S., Ali, N., Ali, O., Ali, R., Ali, S., Aliberti, E., Alin, J., Alina, A., Alipustain, A., Alisjahbana, B., Aliyuda, F., Alizadeh, K., Al-Jibury, M., Al-Juboori, S., Al-Khalil, M., Alkhudhayri, A., Alkhusheh, M., Allan, F., Allan, N., Allanson, A., Allcock, R., Allen, E., Allen, J., Allen, K., Allen, L., Allen, P., Allen, R., Allen, S., Allen, T., Alli, A., Allison, K., Allman, B., Allsop, H.K., Allsop, L., Allsup, D., Almahroos, A.F.T., Al-Moasseb, H., Al-Obaidi, M., Alomari, L., Al-Rabahi, A., Al-Ramadhani, B., Al-Saadi, Z., Al-Sammarraie, R., Alshaer, I., Al-Shahi Salman, R., Al-Shamkhani, W., Alsheikh, F., Al-Sheklly, B., Altaf, S., Alty, A., Alvarez, M., Alvarez Corral, M., Alveyn, E., Alzetani, M., Amamou, S., Amar, N., Ambalavanan, S., Ambrogetti, R., Ambrose, C., Ameen, A., Amelia Ganefianty, A., Ames, K., Amezaga, M.R., Amin, A., Amin, K., Amin, S., Amin, T., Amit, B., Amjad, A., Amjad, N., Amoah-Dankwa, J., Amoako-Adusei, A., Amosun, V., Amsal, M., Amsha, K., Amuasi, J., Amutio Martin, N., Amy, P., Anada, A., Anand, A., Anandappa, S., Anantapatnaikuni, S.D., Andari, N.K.N., Anderson, E., Anderson, J., Anderson, L., Anderson, M., Anderson, N., Anderson, R., Anderson, S., Anderson, W., Andreou, P., Andrews, A., Andrews, J., Aneke, K., Ang, A., Ang, W.W., Angel, T., Angela, A., Angelini, P., Anguvaa, L., Anichtchik, O., Anim-Somuah, M., Aniruddhan, K., Annett, J., Anning, L., Ansah, M., Anstey, P.J., Anstey, R., Anthony, A., Anthony-Pillai, A., Antill, P., Antonina, Z., Anu, V., Anwar, M., Anwar, S., Apetri, E., Apostolopoulos, A., Appleby, S., Appleyard, D., Aquino, M.F., Araba, B., Aransiola, S., Araujo, M., Archer, A., Archer, D., Archer, S., Arcoria, D., Ardley, C., Arhin-Sam, G., Arias, A.-M., Aribike, O., Arimoto, R., Arisanti, N.L.P.E., Arkley, C., Armah, C., Armata, I., Armistead, J., Armitage, A., Armstrong, C., Armstrong, M., Armstrong, S., Armstrong, W., Armtrong, P., Arndt, H., Arnison-Newgass, C., Arnold, D., Arnold, R., Arnott, A., Arora, D., Arora, K., Arora, P., Arora, R., Arter, A., Arthur, A., Artini, N.M., Arumaithurai, A., Arya, A., Arya, R., Aryal, D., Asandei, D., Asare, G.A., Asghar, A., Asghar, M., Ashab, A., Ashbrook-Raby, C., Ashby, H., Ashcroft, J., Ashcroft, S., Asher, G., Ashfak, Z., Ashfaq, A., Asiamah, H.A., Ashish, A., Ashley, D., Ashman-Flavell, S., Ashok, S., Ashour, A.-E.-A., Ashraf, M.Z., Ashraf, S., Ashraq, M.B., Ashton, D., Ashton, S., Ashworth, A., Ashworth, F.J., Ashworth, R., Aslam, A., Aslam, I., Aslam, S., Aslett, L., Asogan, H., Asrar, A., Assaf, O., Astin-Chamberlain, R., Atabudzi, Y.E., Athavale, P., Athorne, D., Atkins, B., Atkins, C., Atkins, S., Atkinson, J., Atkinson, V., Atomode, A., Atraskiewicz, B., Attia, A.A., Attubato, E., Attwood, M., Aubrey, P., Auer, Z., Aujayeb, A., Aung, A.T., Aung, H., Aung, H.W.W., Aung, K.K., Aung, K.T., Aung, N., Aung, Y., Aung, Z.M., Austin, E., Austin, K., Auwal, A., Avari, M., Avery, M., Aveyard, N., Avis, J., Aviss, G., Avram, C., Avram, P., Awadelkareem, A., Awadzi, G., Awaly, M., Awan, A., Awisi, S., Aya, A., Ayaz, E., Ayerh, J.M., Ayers, A., Azam, J., Azeem, A., Azharuddin, M., Aziz, A., Aziz, G., Aziz, I., Aziz, N., Azkoul, A., Azman Shah, A., Azzopardi, G., Azzoug, H., Babatunde, F., Babi, M., Babiker, B., Babington, G., Babirecki, M., Babores, M., Babs-Osibodu, A.O., Bac, T., Bacciarelli, S., Bachar, R., Bachour, M.-E., Bachti, A., Bacon, G., Bacon, J., Badal, B., Badat, A., Bader, M., Badhan, G.R., Badhrinarayanan, S., Bae, J.P., Baggaley, A., Baggott, A., Bagley, G., Bagmane, D., Bagshaw, L., Bahadori, K., Bahurupi, Y., Bailey, A., Bailey, J., Bailey, K., Bailey, L., Bailey, M.A., Bailey, M., Bailey, P., Bailey, S., Baillie, H., Baillie, J.K., Bain, J., Bains, V., Baird, D., Baird, E., Baird, K., Baird, S., Baird, T., Baird, Y., Bajandouh, A., Bajracharya, M., Baker, D.C., Baker, E., Baker, J., Baker, K., Baker, M., Baker, R., Baker, T.-A., Baker, V., Bakere, H., Bakerly, N., Baker-Moffatt, M., Bakhai, A., Bakhtiar, N., Bakoulas, P., Bakthavatsalam, D., Balachandran, N., Balan, A., Balasingam, P., Balaskas, T., Balasubramaniam, M., Balatoni, N., Balcombe, A., Baldwin, A., Baldwin, C., Baldwin, D., Baldwin, F., Baldwin-Jones, R., Bale, N., Balfour, J., Ball, M., Ball, Ro, Ballard, K., Balluz, I., Balmforth, C., Balogh, E., Baltmr, A., Baluwala, A., Bambridge, G., Bamford, A., Bamford, P., Bamgboye, A., Bancroft, E., Bancroft, H., Banda, J., Bandaru, K., Bandi, S., Bandla, N., Bandyopadhyam, S., Banerjee, A., Banerjee, R., Bang, P., Baniya, S., Bani-Saad, O., Banks, H., Banks, L., Banks, P., Bann, C., Bannister, H., Bannister, O., Banton, L., Bao, D.G., Bao, T., Baptist, M., Baqai, T., Baral, A.M., Baral, S.C., Baramova, D., Barber, R., Barbon, E., Barbosa, M., Barbour, J., Barclay, A., Barclay, C., Bardsley, G., Bareford, S., Bari, S., Barimbing, M., Barker, A., Barker, D., Barker, E., Barker, H., Barker, J., Barker, L., Barker, O., Barker-Williams, K., Barkha, S., Barla, J., Barlow, G., Barlow, R., Barlow, V., Barnacle, J., Barnard, A., Barnes, D., Barnes, N., Barnes, R., Barnes, T., Barnetson, C., Barnett, A., Barnett-Vanes, A., Barning, P.G., Barnsley, W., Barr, A., Barr, D., Barr, J., Barr, C., Barratt, N., Barratt, S., Barrera, M., Barrett, A., Barrett, Fi, Barrett, J., Barrett, S., Barrow, E., Bartholomew, J., Barthwal, M.S., Bartlett, C., Bartlett, G., Bartlett, J., Bartlett, L., Bartley, S., Bartolmeu-Pires, S., Barton, A., Barton, G., Barton, J., Barton, L., Barton, R., Baruah, R., Baryschpolec, S., Bashir, H., Bashyal, A., Basker, B., Basnet, S., Basnyat, B., Basoglu, A., Basran, A., Bassett, J., Bassett, G., Bassford, C., Bassoy, B., Bastion, V., Bastola, A., Basumatary, A., Basvi, P., Batac, J.A., Bataduwaarachchi, V.R., Bate, T., Bateman, H.J., Bateman, K., Bateman, V., Bates, E., Bates, H., Bates, M., Bates, S., Batham, S., Batista, A., Batla, A., Batra, D., Batty, H., Batty, T., Batty, A., Baum, M., Baumber, R., Bautista, C., Bawa, F., Bawa, T., Bawani, F.S., Bax, S., Baxter, M., Baxter, N., Baxter, Z., Bayes, H., Bayo, L.-A., Bazari, F., Bazaz, R., Bazli, A., Beacham, L., Beadles, W., Beadon, K., Beak, P., Beale, A., Beard, K., Bearpark, J., Beasley, A., Beattie, S., Beaumont, K., Beaumont-Jewell, D., Beaver, T., Beavis, S., Beazley, C., Beck, S., Beckett, V., Beckitt, R., Beckley, S., Beddall, H., Beddows, S., Beeby, D., Beeby, S., Beech, G., Beecroft, M., Beer, N., Beer, Sa, Beety, J., Bega, G., Begg, A., Begg, S., Beghini, S., Begum, A., Begum, S., Behan, T., Behrouzi, R., Beishon, J., Beith, C., Belcher, J., Belfield, H., Belfield, K., Belgaumkar, A., Bell, D., Bell, G., Bell, J., Bell, L., Bell, N., Bell, P., Bell, S., Bellamu, J., Bellamy, M., Bellamy, T., Bellini, A., Bellis, A., Bellis, F., Bendall, L., Benesh, N., Benetti, N., Bengu, S.A., Benham, L., Benison-Horner, G., Benkenstein, S., Benn, T., Bennett, A., Bennett, C., Bennett, D., Bennett, G., Bennett, K., Bennett, L., Bennett, M.R., Bennett, S., Bennion, K., Benoy, G., Benson, V., Bentley, A., Bentley, J., Benton, I., Beranova, E., Beresford, M., Bergin, C., Bergstrom, M., Bernatoniene, J., Berriman, T., Berry, Z., Best, F., Best, K., Bester, A.-M., Beuvink, Y., Bevan, E., Bevins, S., Bewick, T., Bexley, A., Beyatli, S., Beynon, F., Bhadi, A., Bhagani, S., Bhakta, S., Bhalla, R., Bhandal, K., Bhandari, A., Bhandari, L., Bhandari, L.N., Bhandari, S., Bhanich Supapol, J., Bhanot, A., Bhanot, R., Bhasin, S., Bhat, A., Bhat, P., Bhatnagar, R., Bhatt, K., Bhayani, J., Bhojwani, D., Bhuie, P., Bhuiyan, M.S., Bhuiyan, S., Bibby, A., Bibi, F., Bibi, N., Bibi, S., Bicanic, T., Bidgood, S., Bigg, J., Biggs, S., Biju, A., Bikov, A., Billingham, S., Billings, J., Binh, P., Binns, A., BinRofaie, M., Bintcliffe, O., Birch, C., Birch, J., Birchall, K., Bird, S., Birt, M., Bishop, C., Bishop, K., Bishop, L., Bisnauthsing, K., Biswas, N., Bittaye, M., Biuk, S., Blachford, K., Black, E., Black, H., Black, K., Black, M., Black, P., Black, V., Blackgrove, H., Blackledge, B., Blackler, J., Blackley, S., Blackman, H., Blackstock, C., Blair, C., Blakemore, F., Blamey, H., Bland, A., Blane, S., Blankley, S., Blaxill, P., Blaylock, K., Blazeby, J., Blencowe, N., Bloom, B., Bloomfield, J., Bloss, A., Blowers, A., Blows, S., Bloxham, H., Blrd, S., Blundell, L., Blunsum, A., Blunt, M., Blunt, T., Blyth, I., Blyth, K., Blythe, A., Blythe, K., Boahen, K.A., Boampoaa, M., Board, S., Boatemah, E., Bobie, B., Bobruk, K., Bodalia, P.N., Bodasing, N., Boden, M., Bodenham, T., Boehmer, G., Boffito, M., Bohanan, K., Bohmova, K., Bohnacker, N., Bokhandi, S., Bokhar, M., Bokhari, S., Bokhari, S.O., Bokobza, I., Boles, A., Bolger, C., Bonaconsa, C., Bond, C., Bond, H., Bond, S., Bond, T., Bone, A., Boniface, G., Bonney, J., Bonney, L., Booker, L., Boot, S., Boothroyd, M., Borbone, J., Borman, N., Bosence, S., Bostock, K., Botting, N., Bottrill, F., Bouattia, H., Bough, L., Boughton, H., Boult, Z., Boumrah, T., Bourke, M., Bourke, S., Bourne, M., Bousfield, R., Boustred, L., Bowes, A., Bowker, P., Bowker, T., Bowler, H., Bowman, L., Bowman, S., Bowmer, R., Bowring, A., Bowyer, H., Boyd, A., Boyd, J., Boyd, L., Boyer, N., Boyle, N., Boyle, P., Boyle, R., Boyles, L., 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A., Watson, A.J.R., Watson, E., Watson, F., Watson, J.G.R., Watson, L., Watson, P., Watson, R., Watson, K., Watters, M., Watterson, D., Wattimena, K., Watts, D., Watts, J., Watts, M., Waugh, V., Wayman, E., Wayman, M., Wazir, A., Weatherhead, M., Weatherly, N., Webb, C., Webb, H., Webb, K., Webb, S., Websdale, C., Webster, D., Webster, I., Webster, J., Webster, T., Wedlin, J., Wee, L., Weerakoon, R., Weerasinghe, T., Weeratunga, J., Weetman, M., Wei, S., Weichert, I., Welch, E., Welch, H., Welch, J., Welch, L., Welch, S., Welham, B., Weller, S., Wellings, L., Wells, B., Wellstead, S., Welsh, B., Welsh, R., Welters, I., Welton, R., Wenn, V., Wentworth, L., Wesonga, J., Wesseldine, K., West, J., West, M., West, R., West, S., Western, L., Westhead, R., Weston, H., Westwood, A., Westwood, K., Westwood, S., Wetherill, B., Wheaver, S., Wheeler, H., Whelan, B., Whelband, M., Whileman, A., Whitcher, A., White, A., White, B., White, C., White, D., White, J., White, K., White, M., White, N., White, S., White, T., Whitehead, C., Whitehorn, K., Whitehouse, A., Whitehouse, C., Whitehouse, T., Whiteley, J., Whiteley, L., Whiteley, S., Whitham, R., Whitlingum, G., Whitmore, D., Whittaker, E., Whittam, L., Whittington, A., Whittle, H., Whittle, R., Wiafe, E., Wiblin, L., Wickens, O., Widdrington, J., Wieboldt, J., Wieringa, H., Wiesender, C., Wiffen, L., Wight, A., Wignall, A., Wignall, C., Wilce, A., Wilcock, D., Wilcock, E., Wilcox, L., Wild, B., Wild, L., Wild, S., Wilde, M., Wilding, L., Wilding, P., Wildsmith, T., Wileman, J., Wiles, J., Wiles, K., Wilhelmsen, E., Wiliams, T., Wilkie, J., Wilkin, D., Wilkins, H., Wilkins, J., Wilkins, S., Wilkinson, I., Wilkinson, L., Wilkinson, N., Wilkinson, S., Wilkinson, T., Willetts, S., Williams, A., Williams, C., Williams, C.V., Williams, D., Williams, E., Williams, G., Williams, H., Williams, J., Williams, K., Williams, M., Williams, P., Williams, R., Williams, S., Williams, T., Williamson, A., Williamson, C., Williamson, D., Williamson, J., Williamson, J.D., Williamson, R., Williamson, H., Willis, E., Willis, H., Willis, J., Wills, L., Willsher, L., Willshire, C., Willson, F., Willson, J., Wilson, A., Wilson, B., Wilson, D., Wilson, I., Wilson, J., Wilson, K., Wilson, K.-A., Wilson, L., Wilson, M., Wilson, S., Wilson, T., Win, K.L.Y., Win, M., Win, T., Win, T.T., Win, W.Y.W., Winckworth, L., Winder, L., Winder, P., Winearl, S., Winmill, H., Winn, S., Winpenny, C., Winslow, H., Winter, H., Winter, J., Winter-Goodwin, B., Winterton, J., Winwood, H., Wischhusen, J., Wisdom, S., Wise, M., Wiselka, M., Wiseman, R., Wiseman, S., Wishart, S., WIshlade, T., Witele, E., Withers, N., Wittes, J., Wixted, D., Wodehouse, T., Wolf, W., Wolff, N., Wolffsohn, K., Wolf-Roberts, R., Wolodimeroff, E., Wolstencroft, A., Wong, A., Wong, C., Wong, C.-H., Wong, C.-M., Wong, E., Wong, J.S.Y., Wong, K.Y., Wong, M.Y., Wong, N., Wong, S., Wong, T., Wongkyezeng, A.A., Wood, A., Wood, C., Wood, D., Wood, F., Wood, G., Wood, H., Wood, J., Wood, L., Wood, M., Wood, S., Wood, T., Woodall, K., Woodfield, R., Woodford, C., Woodford, E., Woodford, J., Woodhead, L., Woodhead, T., Woodland, P., Woodman, M., Woodmansey, S., Woods, C., Woods, J., Woods, K., Woods, S., Woodward, Z., Woolcock, M., Wooldridge, G., Woolf, R., Woollard, C., Woollen, L., Woolley, E., Woolley, J., Woosey, D., Wootton, D., Wootton, J., Worley, D., Worton, S., Wraight, J., Wray, M., Wren, K., Wren, L., Wrey Brown, C., Wright, C., Wright, D., Wright, F., Wright, H., Wright, I., Wright, L., Wright, R., Wright, S., Wright, T., Wroe, C., Wroe, H., Wu, H., Wu, P., Wubetu, J., Wulandari, F., Wulandari, R., Wurie, S., Wyatt, C., Wyn-Griffiths, F., Wynter, I., Xavier, B., Xhikola, A., Xia, B.E., Xia, Z., Yacoba, E., Yadav, S., Yakubi, M., Yan, M., Yanagisawa, Y., Yang, F., Yang, Y., Yanney, M., Yap, W.L., Yaqoob, N., Yasmin, S., Yates, B., Yates, D., Yates, E., Yates, H., Yates, T., Yates, M., Ye, J., Yearwood Martin, C., Yein, K., Yelnoorkar, F., Yen, L., Yen, L.M., Yeoh, A., Yeung, C.Y., Yew, P., Yewatkar, D., Ylquimiche Melly, L., Ynter, I., Yong, H., Yorke, J., Youens, J., Younes Ibrahim, A., Young, E., Young, G., Young, L., Yousafzar, A., Youssouf, S., Yousuf, A., Yovita, H., Yu, C., Yuan, J.S.J., Yufaniaputri, N., Yung, B., Yusef, D., Yusef, S., Yusuf, I., Zafar, A.-S., Zagalo, S., Zaher, S., Zahoor, A., Zainab, M., Zak, T., Zaki, K., Zakir, N., Zalewska, K., Zamalloa, A., Zaman, M., Zaman, S., Zamikula, J., Zammit, L., Zammit-Mangion, M., Zawadzka, M., Zayed, M., Zebracki, E., Zehnder, D., Zeidan, L., Zeinali, D., Zhang, J., Zhao, X., Zheng, D., Zhu, D., Zia, M., Zibdeh, O., Zill-E-Huma, R., Zin, E.T., Zincone, E., Zindoga, G., Zinkin, E., Zinyemba, V., Zipitis, C., Zitter, L., Zmierczak, A., Zubikarai, G., Zubir, A., Zuhra, N., Zulaikha, R., Zulfikar, S., Zullo, C., and Zuriaga-Alvaro, A.

Published
2025
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92. Design and performance of the field cage for the XENONnT experiment

Author

Aprile, E., Abe, K., Maouloud, S. Ahmed, Althueser, L., Andrieu, B., Angelino, E., Angevaare, J. R., Antochi, V. C., Martin, D. Antón, Arneodo, F., Baudis, L., Baxter, A. L., Bazyk, M., Bellagamba, L., Biondi, R., Bismark, A., Brookes, E. J., Brown, A., Bruenner, S., Bruno, G., Budnik, R., Bui, T. K., Cai, C., Cardoso, J. M. R., Cichon, D., Chávez, A. P. Cimental, Colijn, A. P., Conrad, J., Cuenca-García, J. J., Cussonneau, J. P., DÁndrea, V., Decowski, M. P., Di Gangi, P., Diglio, S., Eitel, K., Elykov, A., Farrell, S., Ferella, A. D., Ferrari, C., Fischer, H., Flierman, M., Fulgione, W., Fuselli, C., Gaemers, P., Gaior, R., Rosso, A. Gallo, Galloway, M., Gao, F., Glade-Beucke, R., Grandi, L., Grigat, J., Guan, H., Guida, M., Hammann, R., Higuera, A., Hils, C., Hoetzsch, L., Hood, N. F., Howlett, J., Iacovacci, M., Itow, Y., Jakob, J., Joerg, F., Joy, A., Kara, M., Kavrigin, P., Kazama, S., Kobayashi, M., Koltman, G., Kopec, A., Kuger, F., Landsman, H., Lang, R. F., Levinson, L., Li, I., Li, S., Liang, S., Lindemann, S., Lindner, M., Liu, K., Loizeau, J., Lombardi, F., Long, J., Lopes, J. A. M., Ma, Y., Macolino, C., Mahlstedt, J., Mancuso, A., Manenti, L., Marignetti, F., Undagoitia, T. Marrodán, Martens, K., Masbou, J., Masson, D., Masson, E., Mastroianni, S., Messina, M., Miuchi, K., Molinario, A., Moriyama, S., Morå, K., Mosbacher, Y., Murra, M., Müller, J., Ni, K., Oberlack, U., Paetsch, B., Palacio, J., Pellegrini, Q., Peres, R., Peters, C., Pienaar, J., Pierre, M., Plante, G., Pollmann, T. R., Qi, J., Qin, J., García, D. Ramírez, Šarčević, N., Shi, J., Singh, R., Sanchez, L., Santos, J. M. F. dos, Sarnoff, I., Sartorelli, G., Schreiner, J., Schulte, D., Schulte, P., Eißing, H. Schulze, Schumann, M., Lavina, L. Scotto, Selvi, M., Semeria, F., Shagin, P., Shi, S., Shockley, E., Silva, M., Simgen, H., Takeda, A., Tan, P. -L., Terliuk, A., Thers, D., Toschi, F., Trinchero, G., Tunnell, C., Tönnies, F., Valerius, K., Volta, G., Weinheimer, C., Weiss, M., Wenz, D., Wittweg, C., Wolf, T., Wu, V. H. S., Xing, Y., Xu, D., Xu, Z., Yamashita, M., Yang, L., Ye, J., Yuan, L., Zavattini, G., Zhong, M., and Zhu, T.

Subjects
High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

The precision in reconstructing events detected in a dual-phase time projection chamber depends on an homogeneous and well understood electric field within the liquid target. In the XENONnT TPC the field homogeneity is achieved through a double-array field cage, consisting of two nested arrays of field shaping rings connected by an easily accessible resistor chain. Rather than being connected to the gate electrode, the topmost field shaping ring is independently biased, adding a degree of freedom to tune the electric field during operation. Two-dimensional finite element simulations were used to optimize the field cage, as well as its operation. Simulation results were compared to ${}^{83m}\mathrm{Kr}$ calibration data. This comparison indicates an accumulation of charge on the panels of the TPC which is constant over time, as no evolution of the reconstructed position distribution of events is observed. The simulated electric field was then used to correct the charge signal for the field dependence of the charge yield. This correction resolves the inconsistent measurement of the drift electron lifetime when using different calibrations sources and different field cage tuning voltages.

Published
2023
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93. Discovery of millihertz Quasi-Periodic Oscillations in the Low Mass X-Ray Binary XTE J1701$-$462 from a Search of the RXTE Legacy data set

Author

Tse, Kaho, Galloway, Duncan K., and Heger, Alexander

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report the detection of millihertz quasi-periodic oscillations ($\mathrm{mHz}$ QPOs) from the low-mass X-ray binary XTE J1701$-$462. The discovery came from a search of the legacy data set of the Rossi X-ray Timing Explorer, in order to detect the periodic signals in all observations of sources exhibiting thermonuclear bursts. We found that $47$ out of $860$ observations of XTE J1701$-$462; covering the 2006-7 outburst exhibits signals with a significance above the detection threshold, which was determined separately for each observation via a Monte Carlo approach. We chose the four strongest candidates, each with maximum power exceeding $4\sigma$ of the simulated wavelet noise power distribution, to demonstrate the properties of the QPOs. The frequencies of the signals in the four observations are $\sim 3.5\;\text{to}\;5.6\; \mathrm{mHz}$, and the fractional R.M.S. amplitudes vary between $0.74 \pm 0.05\,\%$ and $3.54 \pm 0.04\,\%$. Although previously reported signals in other sources typically disappear immediately before a burst, we do not observe this behaviour in XTE J1701$-$462. Instead, we found that the QPOs and bursts occurred in separate accretion regimes. When the persistent luminosity dropped near the end of the outburst, the source showed bursts and no QPOs were detected, which is the behaviour predicted by theory for the transition from stable to unstable burning. On the basis of this new detection, we reassess the cases for identifying these $\mathrm{mHz}$ QPOs in this and other sources as arising from marginally stable burning., Comment: 7 pages, 5 figures

Published
2023

94. Remarks on the size of apparent horizons

Author

Galloway, Gregory J.

Subjects
General Relativity and Quantum Cosmology, Mathematics - Differential Geometry
Abstract

Marginally outer trapped surfaces (also referred to as apparent horizons) that are stable in 3-dimensional initial data sets obeying the dominant energy condition strictly are known to satisfy an area bound. The main purpose of this note is to show (in several ways) that such surfaces also satisfy a diameter bound., Comment: 10 pages. v2: minor changes/corrections, reference added

Published
2023

95. A catalogue of unusually long thermonuclear bursts on neutron stars

Author

Alizai, Khaled, Chenevez, Jérôme, Cumming, Andrew, Degenaar, Nathalie, Falanga, Maurizio, Galloway, Duncan K., Zand, Jean J. M. in `t, Jaisawal, Gaurava K., Keek, Laurens, Kuulkers, Erik, Lampe, Nathanael, Schatz, Hendrik, and Serino, Motoko

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Rare, energetic (long) thermonuclear (Type I) X-ray bursts are classified either as intermediate-duration or superbursts, based on their duration. Intermediate-duration bursts lasting a few to tens of minutes are thought to arise from the thermonuclear runaway of a relatively thick (10^10 g/cm2) helium layer, while superbursts lasting hours are attributed to the detonation of an underlying carbon layer. We present a catalogue of 84 long thermonuclear bursts from 40 low-mass X-ray binaries, and defined from a new set of criteria distinguishing them from the more frequent short bursts. The three criteria are: (1) a total energy release larger than 10^40 erg, (2) a photospheric radius expansion phase longer than 10 s, and (3) a burst time-scale longer than 70 s. This work is based on a comprehensive systematic analysis of 70 bursts found with INTEGRAL, RXTE, Swift, BeppoSAX, MAXI, and NICER, as well as 14 long bursts from the literature that were detected with earlier generations of X-ray instruments. For each burst, we measure its peak flux and fluence, which eventually allows us to confirm the distinction between intermediate-duration bursts and superbursts. Additionally, we list 18 bursts that only partially meet the above inclusion criteria, possibly bridging the gap between normal and intermediate-duration bursts. With this catalogue, we significantly increase the number of long-duration bursts included in the MINBAR and thereby provide a substantial sample of these rare X-ray bursts for further study., Comment: Published in MNRAS, 20 pages, 7 figures, 4 tables

Published
2023
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96. JWST detection of heavy neutron capture elements in a compact object merger

Author

Levan, A., Gompertz, B. P., Salafia, O. S., Bulla, M., Burns, E., Hotokezaka, K., Izzo, L., Lamb, G. P., Malesani, D. B., Oates, S. R., Ravasio, M. E., Escorial, A. Rouco, Schneider, B., Sarin, N., Schulze, S., Tanvir, N. R., Ackley, K., Anderson, G., Brammer, G. B., Christensen, L., Dhillon, V. S., Evans, P. A., Fausnaugh, M., Fong, W. -F., Fruchter, A. S., Fryer, C., Fynbo, J. P. U., Gaspari, N., Heintz, K. E., Hjorth, J., Kennea, J. A., Kennedy, M. R., Laskar, T., Leloudas, G., Mandel, I., Martin-Carrillo, A., Metzger, B. D., Nicholl, M., Nugent, A., Palmerio, J. T., Pugliese, G., Rastinejad, J., Rhodes, L., Rossi, A., Smartt, S. J., Stevance, H. F., Tohuvavohu, A., van der Horst, A., Vergani, S. D., Watson, D., Barclay, T., Bhirombhakdi, K., Breedt, E., Breeveld, A. A., Brown, A. J., Campana, S., Chrimes, A. A., D'Avanzo, P., D'Elia, V., De Pasquale, M., Dyer, M. J., Galloway, D. K., Garbutt, J. A., Green, M. J., Hartmann, D. H., Jakobsson, P., Kerry, P., Langeroodi, D., Leung, J. K., Littlefair, S. P., Munday, J., O'Brien, P., Parsons, S. G., Pelisoli, I., Saccardi, A., Sahman, D. I., Salvaterra, R., Sbarufatti, B., Steeghs, D., Tagliaferri, G., Thöne, C. C., Postigo, A. de Ugarte, and Kann, D. A.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray bursts (GRBs), sources of high-frequency gravitational waves and likely production sites for heavy element nucleosynthesis via rapid neutron capture (the r-process). These heavy elements include some of great geophysical, biological and cultural importance, such as thorium, iodine and gold. Here we present observations of the exceptionally bright gamma-ray burst GRB 230307A. We show that GRB 230307A belongs to the class of long-duration gamma-ray bursts associated with compact object mergers, and contains a kilonova similar to AT2017gfo, associated with the gravitational-wave merger GW170817. We obtained James Webb Space Telescope mid-infrared (mid-IR) imaging and spectroscopy 29 and 61 days after the burst. The spectroscopy shows an emission line at 2.15 microns which we interpret as tellurium (atomic mass A=130), and a very red source, emitting most of its light in the mid-IR due to the production of lanthanides. These observations demonstrate that nucleosynthesis in GRBs can create r-process elements across a broad atomic mass range and play a central role in heavy element nucleosynthesis across the Universe., Comment: Submitted. Comments welcome! Nature (2023)

Published
2023
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97. Developing and testing Advance Choice Document implementation resources for Black African and Caribbean people with experience of compulsory psychiatric admission

Author

Jonathan Simpson, Abigail Babatunde, Alan Simpson, Steven Gilbert, Alex Ruck Keene, Lucy Stephenson, Kia-Chong Chua, Gareth Owen, Fiona Crowe, Pauline Edwards, Selena Galloway, Megan Fisher, Marcela Schilderman, Anita Bignell, Shubulade Smith, and Claire Henderson

Subjects
Advance choice documents, Advance directives, Advance statements, Mental health act, Black mental health, Mental health inequity, Psychiatry, RC435-571
Abstract

Abstract Background Advance Choice Documents (ACDs) have been recommended for use in England and Wales based on evidence from trials that show that they can reduce involuntary hospitalisation, which disproportionately affects Black African and Caribbean people. Our aim was therefore to develop and test ACD implementation resources and processes for Black people who have previously been involuntarily hospitalised and the people that support them. Methods Resource co-production workshops were held to inform the development of the ACD template and two types of training for all stakeholders, comprising a Recovery College course and simulation training. An ACD facilitator then used the ACD template developed through the workshops to create personalised ACDs with service users and mental health staff over a series of meetings. Interviews were then conducted with service user and staff participants and analysed to document their experience of the process and opinions on ACDs. Other implementation strategies were also employed alongside to support and optimise the creation of ACDs. Results Nine ACDs were completed and were largely reported as appropriate, acceptable, and feasible to service users and staff. Both reported it being an empowering process that encouraged hope for better future treatment and therefore better wellbeing. Uncertainty was also expressed about the confidence people had that ACDs would be adhered to/honoured, primarily due to staff workload. The information provision training and the skills training were generally considered to be informative by trainees. Conclusions The project has developed an ACD creation resource that was reported as agreeable to all stakeholders; however, the generalisability of the findings is limited due to the small sample size. The project also highlights the importance of staff and ACD facilitator capacity and good therapeutic relationships in ACD completion. Further research is needed to determine the adjustments needed for large scale use, including for those under age 18 and those under the care of forensic mental health services; and how to include carers/supporters more in the process.

Published
2024
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98. A latent Axin2 +/Scx + progenitor pool is the central organizer of tendon healing

Author

Mor Grinstein, Stephanie L. Tsai, Daniel Montoro, Benjamin R. Freedman, Heather L. Dingwall, Steffany Villaseñor, Ken Zou, Moshe Sade-Feldman, Miho J. Tanaka, David J. Mooney, Terence D. Capellini, Jayaraj Rajagopal, and Jenna L. Galloway

Subjects
Medicine
Abstract

Abstract A tendon’s ordered extracellular matrix (ECM) is essential for transmitting force but is also highly prone to injury. How tendon cells embedded within and surrounding this dense ECM orchestrate healing is not well understood. Here, we identify a specialized quiescent Scx +/Axin2 + population in mouse and human tendons that initiates healing and is a major functional contributor to repair. Axin2 + cells express stem cell markers, expand in vitro, and have multilineage differentiation potential. Following tendon injury, Axin2 + -descendants infiltrate the injury site, proliferate, and differentiate into tenocytes. Transplantation assays of Axin2-labeled cells into injured tendons reveal their dual capacity to significantly proliferate and differentiate yet retain their Axin2 + identity. Specific loss of Wnt secretion in Axin2 + or Scx + cells disrupts their ability to respond to injury, severely compromising healing. Our work highlights an unusual paradigm, wherein specialized Axin2 + /Scx + cells rely on self-regulation to maintain their identity as key organizers of tissue healing.

Published
2024
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99. Urologic Cancer Drug Costs in Low- and Middle-Income Countries

Author

Lan Anh S. Galloway, Brian D. Cortese, and Ruchika Talwar

Subjects
drug costs, LMICs, novel hormonal therapy, bladder cancer, Wilms tumor, Diseases of the genitourinary system. Urology, RC870-923
Abstract

All 189 World Bank member countries are classified by their capita gross national income into one of four income groups. In this review, we aim to explore the economic burden and management of urologic oncology conditions in low- and middle-income countries (LMICs), emphasizing disparities and challenges in treatment access. The current World Bank classification system highlights economic stratification, showing significant health outcome disparities, particularly in urologic oncology conditions including kidney, bladder, and prostate cancer. First, this review focuses on the management of advanced prostate cancer in Asian LMICs, revealing higher mortality-to-incidence ratios and a greater prevalence of metastatic disease compared to high-income countries (HICs). The prohibitive costs of novel hormonal therapies (NHTs) like abiraterone and enzalutamide limit their use and exacerbate outcome disparities. Second, we review Wilms tumor treatment with chemotherapy in African countries, noting significant price variations for adapted and non-adapted regimens across different economic settings. The cost of chemotherapy agents, particularly dactinomycin, acts as a primary driver of treatment expenses, underscoring the economic challenges in providing high-quality care. Lastly, bladder cancer treatment costs in Brazil and Middle Eastern countries are examined, highlighting how detrimental the economic burden of intravesical therapies, like mitomycin C and Bacillus Calmette–Guérin (BCG), is on treatment accessibility. Overall, this literature review emphasizes the financial strain on healthcare systems and patients, particularly in regions facing economic instability and drug shortages, and underscores the need for international cooperation and effective resource allocation to address the economic barriers to urologic care in LMICs, aiming to improve health outcomes and ensure equitable access to advanced treatments.

Published
2024
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100. Supporting Social Strengths amid Emerging Bilingualism: Effects of Word Generation on Social Perspective Taking in English Learners' Writing

Author

Lisa B. Hsin, Emily Phillips Galloway, and Catherine E. Snow

Abstract

Bilinguals often outperform monolinguals at apprehending the perspectives of others--an apparent consequence of their experiences moving across linguistic and sociocultural contexts. Whether English learners' (ELs') use of such skill in academic writing may be affected by literacy curriculum is the focus of this study. The study explored students' use of social perspective taking (SPT) in writing by examining their responses to a novel argumentative writing task, the iPad--Take A Stand assessment (iTAS). The iTAS was designed to assess the efficacy of the Word Generation curriculum (WG), which provides supports for discussing and deploying multiple perspectives, during its 2012-2014 randomized controlled trial. iTAS essays produced in that study by 4th-7th-grade ELs and their non-EL peers were coded along two dimensions of SPT, acknowledgment and articulation. Analyses revealed a positive impact of WG irrespective of language status on social perspective acknowledgment, the less sophisticated dimension; in contrast, a 'bilingual boost' of the curriculum was detected in students' use of social perspective articulation, the more sophisticated dimension. These findings suggest ELs may draw on their SPT skills when constructing written arguments, at least in the presence of WG's sociocognitive and linguistic supports.

Published
2024
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