Author: "Pearson, T" / Publication Year Range: Last 3 years - Searchworks@Jio Institute Digital Library Search Results

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142 results on '"Pearson, T"'

1. A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour

Author: Raiteri, C. M., Villata, M., Carnerero, M. I., Kurtanidze, S. O., Mirzaqulov, D. O., Benítez, E., Bonnoli, G., Carosati, D., Acosta-Pulido, J. A., Agudo, I., Andreeva, T. S., Apolonio, G., Bachev, R., Borman, G. A., Bozhilov, V., Brown, L. F., Carbonell, W., Casadio, C., Chen, W. P., Damljanovic, G., Ehgamberdiev, S. A., Elsaesser, D., Escudero, J., Feige, M., Fuentes, A., Gabellini, D., Gazeas, K., Giroletti, M., Grishina, T. S., Gupta, A. C., Gurwell, M. A., Hagen-Thorn, V. A., Hamed, G. M., Hiriart, D., Hodges, M., ivanidze, R. Z., Ivanov, D. V., Joner, M. D., Jorstad, S. G., Jovanovic, M. D., Kiehlmann, S., Kimeridze, G. N., Kopatskaya, E. N., Kovalev, Yu. A., Kovalev, Y. Y., Kurtanidze, O. M., Kurtenkov, A., Larionova, E. G., Lessing, A., Lin, H. C., López, J. M., Lorey, C., Ludwig, J., Marchili, N., Marchini, A., Marscher, A. P., Matsumoto, K., Max-Moerbeck, W., Mihov, B., Minev, M., Mingaliev, M. G., Modaressi, A., Morozova, D. A., Mortari, F., Mufakharov, T. V., Myserlis, I., Nikolashvili, M. G., Pearson, T. J., Popkov, A. V., Rahimov, I. A., Readhead, A. C. S., Reinhart, D., Reeves, R., Righini, S., Romanov, F. D., Savchenko, S. S., Semkov, E., Shishkina, E. V., Sigua, L. A., Slavcheva-Mihova, L., Sotnikova, Yu. V., Steineke, R., Stojanovic, M., Strigachev, A., Takey, A., Traianou, E., Troitskaya, Yu. V., Troitskiy, I. S., Tsai, A. L., Valcheva, A., Vasilyev, A. A., Verna, G., Vince, O., Vrontaki, K., Weaver, Z. R., Webb, J., Yuldoshev, Q. X., Zaharieva, E., and Zhovtan, A. V.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Blazars are beamed active galactic nuclei known for their strong multi-wavelength variability on timescales from years down to minutes. We aim to investigate the suitability of the twisting jet model presented in previous works to explain the multi-wavelength behaviour of BL Lacertae, the prototype of one of the blazar classes. According to this model, the jet is inhomogeneous, curved, and twisting, and the long-term variability is due to changes in the Doppler factor due to variations in the orientation of the jet-emitting regions. We analysed optical data of the source obtained during monitoring campaigns organised by the Whole Earth Blazar Telescope (WEBT) in 2019-2022, together with radio data from the WEBT and other teams, and gamma-ray data from the Fermi satellite. In this period, BL Lacertae underwent an extraordinary activity phase, reaching its historical optical and gamma-ray brightness maxima. The application of the twisting jet model to the source light curves allows us to infer the wiggling motion of the optical, radio, and gamma-ray jet-emitting regions. The optical-radio correlation shows that the changes in the radio viewing angle follow those in the optical viewing angle by about 120 days, and it suggests that the jet is composed of plasma filaments, which is in agreement with some radio high-resolution observations of other sources. The gamma-ray emitting region is found to be co-spatial with the optical one, and the analysis of the gamma-optical correlation is consistent with both the geometric interpretation and a synchrotron self-Compton (SSC) origin of the high-energy photons. We propose a geometric scenario where the jet is made up of a pair of emitting plasma filaments in a sort of double-helix curved rotating structure, whose wiggling motion produces changes in the Doppler beaming and can thus explain the observed multi-wavelength long-term variability., Comment: In press for A&A
Published: 2024

2. The Radio Spectra of High Luminosity Compact Symmetric Objects (CSO-2s): Implications for Studies of Compact Jetted Active Galactic Nuclei

Author: de la Parra, P. V., Readhead, A. C. S, Herbig, T., Kiehlmann, S., Lister, M. L., Pavlidou, V., Reeves, R. A., Siemiginowska, A., Sullivan, A. G., Surti, T., Synani, A., Tassis, K., Taylor, G. B., Wilkinson, P. N., Aller, M. F., Blandford, R. D., Globus, N., Lawrence, C. R., Molina, B., O'Neill, S., and Pearson, T. J.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract: This paper addresses, for the first time, a key aspect of the phenomenology of Compact Symmetric Objects (CSOs) -- the characteristics of their radio spectra. We present a radio-spectrum description of a complete sample of high luminosity CSOs (CSO-2s), which shows that they exhibit the \textit{complete} range of spectral types, including flat-spectrum sources ($\alpha \ge -0.5$), steep-spectrum sources ($\alpha < -0.5$), and peaked-spectrum sources. We show that there is no clear correlation between spectral type and size, but there is a correlation between the high-frequency spectral index and both object type and size. We also show that, to avoid biasing the data and to understand the various classes of jetted-AGN involved, the complete range of spectral types should be included in studying the general phenomenology of compact jetted-AGN, and that complete samples must be used, selected over a wide range of frequencies. We discuss examples that demonstrate these points. We find that the high-frequency spectral indices of CSO-2s span $-1.3 <\alpha_{\rm hi} < -0.3$, and hence that radio spectral signatures cannot be used to discriminate definitively between CSO-2s, binary galactic nuclei, and millilensed objects, unless they have $\alpha_{\rm hi} >-0.3$.
Published: 2024

3. PKS~J0805$-$0111: A Second Owens Valley Radio Observatory Blazar Showing Highly Significant Sinusoidal Radio Variability -- The Tip of the Iceberg

Author: de la Parra, P. V., Kiehlmann, S., Mroz, P., Readhead, A. C. S., Synani, A., Begelman, M. C., Blandford, R. D., Ding, Y., Harrison, F., Liodakis, I., Max-Moerbeck, W., Pavlidou, V., Reeves, R., Vallisneri, M., Aller, M. F., Graham, M. J., Hovatta, T., Lawrence, C. R., Lazio, T. J. W., Mahabal, A. A., Molina, B., O'Neill, S., Pearson, T. J., Ravi, V., Tassis, K., and Zensus, J. A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract: Owens Valley Radio Observatory (OVRO) observations of supermassive black hole binary (SMBHB) candidate PKS~2131$-$021 revealed, for the first time, six likely characteristics of the phenomenology exhibited by SMBHB in blazars, of which the most unexpected and critical is sinusoidal flux density variations. We have now identified a second blazar, PKS~J0805$-$0111, showing significant sinusoidal variations, with an observed period that translates to $1.422 \pm 0.005$ yr in the rest frame of the $z = 1.388$ object. We generate $10^6$ simulated light curves to reproduce the radio variability characteristics of PKS~J0805$-$0111, and show that the global probability, considering the \textit{look-elsewhere effect}, indicates that the observed periodicity can be attributed to the red noise tail of the power spectral density, with a $p_0$ value of $7.8 \times 10^{-5}$ (i.e. 3.78$\sigma$). PKS J0805$-$0111 displays all six characteristics observed in PKS 2131$-$021. Taking into account the well-defined OVRO sample size, the false positive probability $\sim 0.22$, but the rare behavior makes this a strong SMBHB candidate. The discovery of a second SMBHB candidate exhibiting these rare characteristics reveals that PKS~2131$-$021 is not a unique, isolated case. With these two strong cases we are clearly seeing only the tip of the iceberg. We estimate that the number of SMBHB candidates amongst blazars $\sim$ 1 in 100.
Published: 2024

4. COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at 'Cosmic Half-past Eleven'

Author: Chung, D. T., Breysse, P. C., Cleary, K. A., Dunne, D. A., Lunde, J. G. S., Padmanabhan, H., Stutzer, N. -O., Tolgay, D., Bond, J. R., Church, S. E., Eriksen, H. K., Gaier, T., Gundersen, J. O., Harper, S. E., Harris, A. I., Hobbs, R., Ihle, H. T., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Wehus, I. K., and Woody, D. P.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: The Carbon monOxide Mapping Array Project (COMAP) Pathfinder survey continues to demonstrate the feasibility of line-intensity mapping using high-redshift carbon monoxide (CO) line emission traced at cosmological scales. The latest COMAP Pathfinder power spectrum analysis is based on observations through the end of Season 2, covering the first three years of Pathfinder operations. We use our latest constraints on the CO(1-0) line-intensity power spectrum at $z\sim3$ to update corresponding constraints on the cosmological clustering of CO line emission and thus the cosmic molecular gas content at a key epoch of galaxy assembly. We first mirror the COMAP Early Science interpretation, considering how Season 2 results translate to limits on the shot noise power of CO fluctuations and the bias of CO emission as a tracer of the underlying dark matter distribution. The COMAP Season 2 results place the most stringent limits on the CO tracer bias to date, at $\langle{Tb}\rangle<4.8$ $\mu$K. These limits narrow the model space significantly compared to previous CO line-intensity mapping results while maintaining consistency with small-volume interferometric surveys of resolved line candidates. The results also express a weak preference for CO emission models used to guide fiducial forecasts from COMAP Early Science, including our data-driven priors. We also consider directly constraining a model of the halo-CO connection, and show qualitative hints of capturing the total contribution of faint CO emitters through the improved sensitivity of COMAP data. With continued observations and matching improvements in analysis, the COMAP Pathfinder remains on track for a detection of cosmological clustering of CO emission., Comment: 9 pages + bibliography and appendices (13 pages total); 9 figures, 1 table; v2 reflects minor changes made for version submitted to A&A, with no changes to top-line results
Published: 2024

5. COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrum

Author: Stutzer, N. -O., Lunde, J. G. S., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Ihle, H. T., Padmanabhan, H., Tolgay, D., Wehus, I. K., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Harper, S. E., Hobbs, R., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., and Woody, D. P.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present updated constraints on the cosmological 3D power spectrum of carbon monoxide CO(1-0) emission in the redshift range $2.4$-$3.4$. The constraints are derived from the two first seasons of Carbon monOxide Mapping Array Project (COMAP) Pathfinder line-intensity mapping observations aiming to trace star-formation during the Epoch of Galaxy Assembly. These results improve on the previous Early Science (ES) results through both increased data volume and improved data processing methodology. On the methodological side, we now perform cross-correlations between groups of detectors (''feed-groups''), as opposed to cross-correlations between single feeds, and this new feed-group pseudo power spectrum (FGPXS) is constructed to be more robust against systematic effects. In terms of data volume, the effective mapping speed is significantly increased due to an improved observational strategy as well as better data selection methodology. The updated spherically- and field-averaged FGPXS, $\tilde{C}(k)$, is consistent with zero, at a probability-to-exceed of around $34\,\%$, with an excess of $2.7\,\sigma$ in the most sensitive bin. Our power spectrum estimate is about an order of magnitude more sensitive in our six deepest bins across ${0.09\,\mathrm{Mpc}^{-1} < k < 0.73\,\mathrm{Mpc}^{-1}}$, as compared to the feed-feed pseudo power spectrum (FPXS) of COMAP ES. Each of these bins individually constrains the CO power spectrum to ${kP_\mathrm{CO}(k)< 2400-4900\,\mathrm{\mu K^2 Mpc^{2}}}$ at $95\,\%$ confidence. To monitor potential contamination from residual systematic effects, we analyze a set of 312 difference-map null tests and find that these are consistent with the instrumental noise prediction. In sum, these results provide the strongest direct constraints on the cosmological 3D CO(1-0) power spectrum published to date., Comment: 17 pages, 10 figures, v2 reflects changes made for version submitted to Astronomy and Astrophysics, addition of additional figure clarifying methodology, no change to final results
Published: 2024

6. COMAP Pathfinder -- Season 2 results I. Improved data selection and processing

Author: Lunde, J. G. S., Stutzer, N. -O., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Harper, S. E., Ihle, H. T., Lamb, J. W., Pearson, T. J., Philip, L., Wehus, I. K., Woody, D. P., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Hobbs, R., Kim, J., Lawrence, C. R., Murray, N., Padmanabhan, H., Readhead, A. C. S., Rennie, T. J., and Tolgay, D.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The CO Mapping Array Project (COMAP) Pathfinder is performing line intensity mapping of CO emission to trace the distribution of unresolved galaxies at redshift $z \sim 3$. We present an improved version of the COMAP data processing pipeline and apply this to the first two seasons of observations. This analysis improves on the COMAP Early Science (ES) results in several key aspects. On the observational side, all second season scans were made in constant-elevation mode, after noting that the previous Lissajous scans were associated with increased systematic errors; those scans accounted for 50% of the total Season 1 data volume. Secondly, all new observations were restricted to an elevation range of 35-65 degrees, to minimize sidelobe ground pickup. On the data processing side, more effective data cleaning in both the time- and map-domain has allowed us to eliminate all data-driven power spectrum-based cuts. This increases the overall data retention and reduces the risk of signal subtraction bias. On the other hand, due to the increased sensitivity, two new pointing-correlated systematic errors have emerged, and we introduce a new map-domain PCA filter to suppress these. Subtracting only 5 out of 256 PCA modes, we find that the standard deviation of the cleaned maps decreases by 67% on large angular scales, and after applying this filter, the maps appear consistent with instrumental noise. Combining all these improvements, we find that each hour of raw Season 2 observations yields on average 3.2 times more cleaned data compared to ES analysis. Combining this with the increase in raw observational hours, the effective amount of data available for high-level analysis is a factor of 8 higher than in ES. The resulting maps have reached an uncertainty of $25$-$50\,\mu K$ per voxel, providing by far the strongest constraints on cosmological CO line emission published to date., Comment: 23 pages, 22 figures, for submission to Astronomy and Astrophysics
Published: 2024

7. Foster parents’ experiences with animal companions while fostering children and youth

Author: Wiens, Jeanette, Pearson, T., and Whalen, C.
Subjects: human-animal bond, animal companion, social work practice, foster parent, foster care
Abstract: This qualitative exploratory inquiry examined foster parents’ perspectives of the impact companion animals had on the children/youth in their care. Six foster parents were interviewed and six themes, including 12 subthemes, were uncovered: (1) provision of companionship (unconditional love); (2) strengthening of the foster home environment (environmental connection, increased feelings of safety); (3) teaching empathy (responsibility, compassion); (4) emotional regulation (grief, emotional support, calming presence); (5) benefits to foster parents (friendship, affection, emotional support, additional support); and (6) challenges. These findings have important implications for social work practice. Specific recommendations based on the findings are presented.
Published: 2024
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8. The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium

Author: Pelgrims, V., Mandarakas, N., Skalidis, R., Tassis, K., Panopoulou, G. V., Pavlidou, V., Blinov, D., Kiehlmann, S., Clark, S. E., Hensley, B. S., Romanopoulos, S., Basyrov, A., Eriksen, H. K., Falalaki, M., Ghosh, T., Gjerløw, E., Kypriotakis, J. A., Maharana, S., Papadaki, A., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., and Wehus, I. K.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present the first degree-scale tomography map of the dusty magnetized interstellar medium (ISM) from stellar polarimetry and distance measurements. We used the RoboPol polarimeter at Skinakas Observatory to conduct a survey of starlight polarization in a region of the sky of 4 square degrees. We propose a Bayesian method to decompose the stellar-polarization source field along the distance to invert the 3D volume occupied by the observed stars. We used it to obtain the first 3D map of the dusty magnetized ISM. Specifically, we produced a tomography map of the orientation of the plane-of-sky (POS) component of the magnetic field threading the diffuse, dusty regions responsible for the stellar polarization. For the targeted region centered on Galactic coordinates $(l,b) \approx (103.3^\circ, 22.3^\circ)$, we identified several ISM clouds. Most of the lines of sight intersect more than one cloud. A very nearby component was detected in the foreground of a dominant component from which most of the polarization signal comes. Farther clouds, with a distance of up to 2~kpc, were similarly detected. Some of them likely correspond to intermediate-velocity clouds seen in HI spectra in this region of the sky. We found that the orientation of the POS component of the magnetic field changes along distance for most of the lines of sight. Our study demonstrates that starlight polarization data coupled to distance measures have the power to reveal the great complexity of the dusty magnetized ISM in 3D and, in particular, to provide local measurements of the POS component of the magnetic field. This demonstrates that the inversion of large data volumes, as expected from the PASIPHAE survey, will provide the necessary means to move forward in the modeling of the Galactic magnetic field and of the dusty magnetized ISM as a contaminant in observations of the cosmic microwave background polarization., Comment: Preprint of the accepted version at Astronomy & Astrophysics. The 3D map obtained in this paper can be visualized online at https://pasiphae.science/visualization and a video featuring it is accessible at https://www.youtube.com/watch?v=dB_6J1zhmPI
Published: 2024
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9. The RoboPol sample of optical polarimetric standards

Author: Blinov, D., Maharana, S., Bouzelou, F., Casadio, C., Gjerløw, E., Jormanainen, J., Kiehlmann, S., Kypriotakis, J. A., Liodakis, I., Mandarakas, N., Markopoulioti, L., Panopoulou, G. V., Pelgrims, V., Pouliasi, A., Romanopoulos, S., Skalidis, R., Anche, R. M., Angelakis, E., Antoniadis, J., Medhi, B. J., Hovatta, T., Kus, A., Kylafis, N., Mahabal, A., Myserlis, I., Paleologou, E., Papadakis, I., Pavlidou, V., Papamastorakis, I., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., Reig, P., Słowikowska, A., Tassis, K., and Zensus, J. A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Optical polarimeters are typically calibrated using measurements of stars with known and stable polarization parameters. However, there is a lack of such stars available across the sky. Many of the currently available standards are not suitable for medium and large telescopes due to their high brightness. Moreover, as we find, some of the used polarimetric standards are in fact variable or have polarization parameters that differ from their cataloged values. Our goal is to establish a sample of stable standards suitable for calibrating linear optical polarimeters with an accuracy down to $10^{-3}$ in fractional polarization. For five years, we have been running a monitoring campaign of a sample of standard candidates comprised of 107 stars distributed across the northern sky. We analyzed the variability of the linear polarization of these stars, taking into account the non-Gaussian nature of fractional polarization measurements. For a subsample of nine stars, we also performed multiband polarization measurements. We created a new catalog of 65 stars (see Table 2) that are stable, have small uncertainties of measured polarimetric parameters, and can be used as calibrators of polarimeters at medium- and large-size telescopes.
Published: 2023
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10. Bright-Moon Sky as a Wide-Field Linear Polarimetric Flat Source for Calibration

Author: Maharana, S., Kiehlmann, S., Blinov, D., Pelgrims, V., Pavlidou, V., Tassis, K., Kypriotakis, J. A., Ramaprakash, A. N., Anche, R. M., Basyrov, A., Deka, K., Eriksen, H. K., Ghosh, T., Gjerløw, E., Mandarakas, N., Ntormousi, E., Panopoulou, G. V., Papadaki, A., Pearson, T., Potter, S. B., Readhead, A. C. S., Skalidis, R., and Wehus, I. K.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Next-generation wide-field optical polarimeters like the Wide-Area Linear Optical Polarimeters (WALOPs) have a field of view (FoV) of tens of arcminutes. For efficient and accurate calibration of these instruments, wide-field polarimetric flat sources will be essential. Currently, no established wide-field polarimetric standard or flat sources exist. This paper tests the feasibility of using the polarized sky patches of the size of around ten-by-ten arcminutes, at a distance of up to 20 degrees from the Moon, on bright-Moon nights as a wide-field linear polarimetric flat source. We observed 19 patches of the sky adjacent to the bright-Moon with the RoboPol instrument in the SDSS-r broadband filter. These were observed on five nights within two days of the full-Moon across two RoboPol observing seasons. We find that for 18 of the 19 patches, the uniformity in the measured normalized Stokes parameters $q$ and $u$ is within 0.2 %, with 12 patches exhibiting uniformity within 0.07 % or better for both $q$ and $u$ simultaneously, making them reliable and stable wide-field linear polarization flats. We demonstrate that the sky on bright-Moon nights is an excellent wide-field linear polarization flat source. Various combinations of the normalized Stokes parameters $q$ and $u$ can be obtained by choosing suitable locations of the sky patch with respect to the Moon, Comment: 8 pages including appendix, 6 figures and 3 tables. Submitted to Astronomy and Astrophysics for review. Comments are welcome
Published: 2023
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11. The C-Band All-Sky Survey (C-BASS): New Constraints on the Integrated Radio Spectrum of M 31

Author: Harper, Stuart E., Barr, Adam, Dickinson, C., Peel, M. W., Cepeda-Arroita, Roke, Copley, C. J., Grumitt, R. D. P., Leahy, J. Patrick, Jonas, J. L., Jones, Michael E., Leech, J., Pearson, T. J., Readhead, A. C. S., and Taylor, Angela C.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The Andromeda galaxy (M31) is our closest neighbouring spiral galaxy, making it an ideal target for studying the physics of the interstellar medium in a galaxy very similar to our own. Using new observations of M31 at 4.76GHz by the C-Band All-Sky Survey (C-BASS), and all available radio data at $1^\circ$ resolution, we produce the integrated spectrum and put new constraints on the synchrotron spectral index and anomalous microwave emission (AME) from M31. We use aperture photometry and spectral modelling to fit for the integrated spectrum of M31, and subtract a comprehensive model of nearby background radio sources. The AME in M31 is detected at $3\sigma$ significance with a peak near 30GHz and flux density $0.27\pm0.09$Jy. The synchrotron spectral index of M31 is flatter than our own Galaxy at $\alpha = -0.66 \pm 0.03$ with no strong evidence of spectral curvature. The emissivity of AME, averaged over the total emission from M31 is lower than typical AME sources in our Galaxy, implying that AME is not uniformly distributed throughout M31 and instead is likely confined to sub-regions -- this will need to be confirmed using future higher resolution observations around 20--30GHz., Comment: 16 pages, 6 figures. Accepted by MNRAS
Published: 2023
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12. The Evolution of Compact Symmetric Objects -- A Possible Connection with Tidal Disruption Events

Author: Readhead, A. C. S., Ravi, V., Blandford, R. D., Sullivan, A. G., Somalwar, J., Liodakis, I., Lister, M. L., Taylor, G. B., Wilkinson, P. N., Globus, N., Kiehlmann, S., Lawrence, C. R., O'Neill, S., Pavlidou, V., Pearson, T. J., Sheldahl, E., Siemiginowska, A., and Tassis, K.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract: Compact Symmetric Objects (CSOs) form a distinct class of jetted active galactic nuclei (jetted-AGN). We examine a carefully selected sample of 54 CSOs, and confirm that there are two unrelated classes: an edge-dimmed, low-luminosity class (CSO 1), and an edge-brightened, high-luminosity class (CSO 2). Using statistically significant blind tests, we show that CSO 2s themselves consist of two morphologically distinct classes: CSO 2.0, having prominent hot-spots at the leading edges of narrow jets and/or narrow lobes; and CSO 2.2, without prominent hot-spots, and with broad jets and/or lobes. An intermediate class, CSO 2.1, exhibits mixed properties. The four classes occupy different, overlapping, portions of the luminosity-size plane, with the sizes of largest CSOs being $\sim 500$pc. We advance the hypothesis that CSO 2.0s are young and evolve through CSO 2.1s into CSO 2.2s, which are old (up to $\sim 5000$ yr). Thus CSOs do not evolve into larger types of jetted-AGN, but spend their whole life cycle as CSOs. The radio emission region energies in the CSO 2s we have studied range from $\sim 10^{-4}\, M_\odot {c}^2$ to $\sim 7 \, M_\odot {c}^2$. We show that the transient nature of CSO 2s, and their birthrate, can be explained through ignition in the tidal disruption events of giant stars. We also consider possibilities for tapping the spin energy of the supermassive black hole, and tapping the energy of the accretion disk, in a manner similar to, but not the same as, that which occurs in dwarf novae. Our results demonstrate conclusively that CSOs constitute a large family of AGN in which we have thus far studied only the brightest. More comprehensive radio studies, with higher sensitivity, resolution, and dynamic range, will revolutionize our understanding of AGN and the central engines that power them., Comment: 41 pages, 13 figures, 10 tables
Published: 2023

13. Compact Symmetric Objects: A Distinct Population of Jetted Active Galaxies

Author: Kiehlmann, S., Readhead, A. C. S., O'Neill, S., Wilkinson, P. N., Lister, M. L., Liodakis, I., Bruzewski, S., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., and Taylor, G. B.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Compact Symmetric Objects (CSOs) are a class of compact, jetted Active Galactic Nuclei (AGN) whose jet axes are not aligned close to the line of sight, and whose observed emission is not predominantly relativistically boosted towards us. Using complete samples of CSOs, we present three independent lines of evidence, based on their relative numbers, their redshift distributions, and their size distributions, which show conclusively that most CSOs do not evolve into larger-scale radio sources. Thus CSOs belong to a distinct population of jetted-AGN. This population should be characterized as "short-lived", as opposed to "young". We show that there is a sharp upper cutoff in the CSO size distribution at $\approx$ 500 pc, which cannot result from random episodic fueling events. There is clearly something that limits the fueling to $\lesssim 100 M_\odot$. Possible origins of CSOs, if not related to the fueling, must be related to the accretion disk, or the collimation of the relativistic jets. CSOs may well have a variety of origins, with each of the above mechanisms producing subsets of CSOs. Whatever the physical mechanism(s) might be, the distinct differences between CSOs and other jetted-AGN provide crucial insights into the formation and evolution of relativistic jets in AGN and the supermassive black holes that drive them., Comment: 27 pages, 9 figures, 6 tables
Published: 2023

14. Towards a Comprehensive Catalog of Bona Fide Compact Symmetric Objects

Author: Kiehlmann, S., Lister, M. L., Readhead, A. C. S., Liodakis, I., O'Neill, S., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., Taylor, G. B., and Wilkinson, P. N.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract: Compact Symmetric Objects (CSOs) are jetted Active Galactic Nuclei (AGN) with overall projected size < 1 kpc. The classification was introduced to distinguish these objects from the majority of known compact jetted-AGN, where the observed emission is relativistically boosted towards the observer. The original classification criteria for CSOs were: (i) evidence of emission on both sides of the center of activity, and (ii) overall size < 1 kpc. However some relativistically boosted objects with jet axes close to the line of sight appear symmetric and have been mis-classified as CSOs in the literature, thereby undermining the CSO classification. We introduce two new CSO classification criteria based on (iii) flux density variability, and (iv) the apparent velocity of components moving along the jets. As a first step towards creating a comprehensive catalog of "bona fide" CSOs, in this paper we identify 79 bona fide CSOs that meet our expanded CSO selection criteria. This sample of bona fide CSOs can be used for astrophysical studies of CSOs without fear of contamination by objects incorrectly identified as CSOs. We define three complete sub-samples of the 79 CSOs, which are suitable for statistical tests, and show that the fraction of CSOs in flux density limited samples with $\rm S_{5~GHz}$ > 700 mJy is between 6.4% and 8.2%., Comment: 21 pages, 7 figures, 3 tables
Published: 2023

15. The hunt for extraterrestrial high-energy neutrino counterparts

Author: Liodakis, I., Hovatta, T., Pavlidou, V., Readhead, A. C. S., Blandford, R. D., Kiehlmann, S., Lindfors, E., Max-Moerbeck, W., Pearson, T. J., and Petropoulou, M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The origin of Petaelectronvolt (PeV) astrophysical neutrinos is fundamental to our understanding of the high-energy Universe. Apart from the technical challenges of operating detectors deep below ice, oceans, and lakes, the phenomenological challenges are even greater than those of gravitational waves; the sources are unknown, hard to predict, and we lack clear signatures. Neutrino astronomy therefore represents the greatest challenge faced by the astronomy and physics communities thus far. The possible neutrino sources range from accretion disks and tidal disruption events, to relativistic jets and galaxy clusters with blazar TXS~0506+056 the most compelling association thus far. Since that association, immense effort has been put into proving or disproving that jets are indeed neutrino emitters, but to no avail. By generating simulated neutrino counterpart samples, we explore the potential of detecting a significant correlation of neutrinos with jets from active galactic nuclei. We find that, given the existing challenges, even our best experiments could not have produced a $>3\sigma$ result. Larger programs over the next few years will be able to detect a significant correlation only if the brightest radio sources, rather than all jetted active galactic nuclei, are neutrino emitters. We discuss the necessary strategies required to steer future efforts into successful experiments., Comment: 8 pages, 1 figure, 1 table, accepted for publication in A&A
Published: 2022
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16. Starlight-polarization-based tomography of the magnetized interstellar medium: PASIPHAE's line-of-sight inversion method

Author: Pelgrims, V., Panopoulou, G. V., Tassis, K., Pavlidou, V., Basyrov, A., Blinov, D., Gjerløw, E., Kiehlmann, S., Mandarakas, N., Papadaki, A., Skalidis, R., Tsouros, A., Anche, R. M., Eriksen, H. K., Ghosh, T., Kypriotakis, J. A., Maharana, S., Ntormousi, E., Pearson, T. J., Potter, S. B., Ramaprakash, A. N., Readhead, A. C. S., and Wehus, I. K.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the first Bayesian method for tomographic decomposition of the plane-of-sky orientation of the magnetic field with the use of stellar polarimetry and distance. This standalone tomographic inversion method presents an important step forward in reconstructing the magnetized interstellar medium (ISM) in 3D within dusty regions. We develop a model in which the polarization signal from the magnetized and dusty ISM is described by thin layers at various distances. Our modeling makes it possible to infer the mean polarization (amplitude and orientation) induced by individual dusty clouds and to account for the turbulence-induced scatter in a generic way. We present a likelihood function that explicitly accounts for uncertainties in polarization and parallax. We develop a framework for reconstructing the magnetized ISM through the maximization of the log-likelihood using a nested sampling method. We test our Bayesian inversion method on mock data taking into account realistic uncertainties from Gaia and as expected for the optical polarization survey PASIPHAE according to the currently planned observing strategy. We demonstrate that our method is effective at recovering the cloud properties as soon as the polarization induced by a cloud to its background stars is higher than $\sim 0.1\%$ for the adopted survey exposure time and level of systematic uncertainty. Our method makes it possible to recover not only the mean polarization properties but also to characterize the intrinsic scatter, thus creating new ways to characterize ISM turbulence and the magnetic field strength. Finally, we apply our method to an existing data set of starlight polarization with known line-of-sight decomposition, demonstrating agreement with previous results and an improved quantification of uncertainties in cloud properties., Comment: Closely matches the published version: A&A 670, A164, 2023 The accompanying code (BISP-1) is available at https://github.com/vpelgrims/Bisp_1
Published: 2022
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17. Polarization and variability of compact sources measured in Planck time-ordered data

Author: Rocha, G., Keskitalo, R., Partridge, B., Marscher, A., O'Dea, C., Pearson, T. J., and Górski, K. M.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: This paper introduces a new Planck Catalog of Polarized and Variable Compact Sources (PCCS-PV) comprising 153 sources, the majority of which are extragalactic. The data include both the total flux density and linear polarization measured by Planck with frequency coverage from 30 to 353 GHz, and temporal spacing ranging from days to years. We classify most sources as beamed, extragalactic radio sources; the catalog also includes several radio galaxies, Seyfert galaxies, and Galactic and Magellanic Cloud sources, including H IIi regions and planetary nebulae. An advanced extraction method applied directly to the multifrequency Planck time-ordered data, rather than the mission sky maps, was developed to allow an assessment of the variability of polarized sources. Our analysis of the time-ordered data from the Planck mission, tod2flux, allowed us to catalog the time-varying emission and polarization properties for these sources at the full range of polarized frequencies employed by Planck, 30 to 353 GHz. PCCS-PV provides the time- and frequency-dependent, polarized flux densities for all 153 sources. To illustrate some potential applications of the PCCS- PV, we conducted preliminary comparisons of our measurements of selected sources with published data from other astronomical instruments. In summary, we find general agreement between the Planck and the Institut de Radioastronomie Millim\'etrique (IRAM) polarization measurements as well as with the Mets\"ahovi 37 GHz values at closely similar epochs. These combined measurements also show the value of PCCS-PV results and the PCCS2 catalog for filling in missing spectral (or temporal) coverage and helping to define the spectral energy distributions of extragalactic sources. In turn, these results provide useful clues as to the physical properties of the sources., Comment: 18 pages, accepted for publication in Astronomy & Astrophysics
Published: 2022
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18. The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky

Author: Harper, S. E., Dickinson, C., Barr, A., Cepeda-Arroita, R., Grumitt, R. D. P., Heilgendorff, H. M., Jew, L., Jonas, J. L., Jones, M. E., Leahy, J. P., Leech, J., Pearson, T. J., Peel, M. W., Readhead, A. C. S., and Taylor, A. C.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The C-Band All-Sky Survey (C-BASS) has observed the Galaxy at 4.76GHz with an angular resolution of $0.73^\circ$ full-width half-maximum, and detected Galactic synchrotron emission with high signal-to-noise ratio over the entire northern sky ($\delta > -15^{\circ}$). We present the results of a spatial correlation analysis of Galactic foregrounds at mid-to-high ($b > 10^\circ$) Galactic latitudes using a preliminary version of the C-BASS intensity map. We jointly fit for synchrotron, dust, and free-free components between $20$ and $1000$GHz and look for differences in the Galactic synchrotron spectrum, and the emissivity of anomalous microwave emission (AME) when using either the C-BASS map or the 408MHz all-sky map to trace synchrotron emission. We find marginal evidence for a steepening ($\left<\Delta\beta\right> = -0.06\pm0.02$) of the Galactic synchrotron spectrum at high frequencies resulting in a mean spectral index of $\left<\beta\right> = -3.10\pm0.02$ over $4.76-22.8$GHz. Further, we find that the synchrotron emission can be well modelled by a single power-law up to a few tens of GHz. Due to this, we find that the AME emissivity is not sensitive to changing the synchrotron tracer from the 408MHz map to the 4.76GHz map. We interpret this as strong evidence for the origin of AME being spinning dust emission., Comment: 20 pages, 13 figures, published with MNRAS
Published: 2022
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19. Investigating the blazar TXS 0506+056 through sharp multi-wavelength eyes during 2017-2019

Author: MAGIC Collaboration, Acciari, V. A., Aniello, T., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batković, I., González, J. Becerra, Bednarek, W., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bökenkamp, H., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Del Popolo, A., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Fariña, L., Fattorini, A., Font, L., Fruck, C., Fukami, S., Fukazawa, Y., López, R. J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Hassan, T., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Iotov, R., Ishio, K., Iwamura, Y., Martínez, I. Jiménez, Jormanainen, J., Jouvin, L., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Linhoff, L., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Mariotti, M., Martínez, M., Aguilar, A. Mas, Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Nakamori, T., Nava, L., Neustroev, V., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Persic, M., Pihet, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schmuckermaier, F., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strišković, J., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Takeishi, R., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Viale, I., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Yamamoto, T., Zarić, D., Collaboration, OVRO, Hodges, M., Hovatta, T., Kiehlmann, S., Liodakis, I., Max-Moerbeck, W., Pearson, T. J., Readhead, A. C. S., Reeves, R. A., Collaboration, Metsähovi, Lähteenmaäki, A., Tornikoski, M., Tammi, J., D'Ammando, F., and Marchini, A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The blazar TXS 0506+056 got into the spotlight of the astrophysical community in September 2017, when a high-energy neutrino detected by IceCube (IceCube-170922A) was associated at the 3 $\sigma$ level to a $\gamma$-ray flare from this source. This multi-messenger photon-neutrino association remains, as per today, the most significant one ever observed. TXS 0506+056 was a poorly studied object before the IceCube-170922A event. To better characterize its broad-band emission, we organized a multi-wavelength campaign lasting 16 months (November 2017 to February 2019), covering the radio-band (Mets\"ahovi, OVRO), the optical/UV (ASAS-SN, KVA, REM, Swift/UVOT), the X-rays (Swift/XRT, NuSTAR), the high-energy $\gamma$ rays (Fermi/LAT) and the very-high-energy (VHE) $\gamma$ rays (MAGIC). In $\gamma$ rays, the behaviour of the source was significantly different from the 2017 one: MAGIC observations show the presence of flaring activity during December 2018, while the source only shows an excess at the 4$\sigma$ level during the rest of the campaign (74 hours of accumulated exposure); Fermi/LAT observations show several short (days-to-week timescale) flares, different from the long-term brightening of 2017. No significant flares are detected at lower energies. The radio light curve shows an increasing flux trend, not seen in other wavelengths. We model the multi-wavelength spectral energy distributions in a lepto-hadronic scenario, in which the hadronic emission emerges as Bethe-Heitler and pion-decay cascade in the X-rays and VHE $\gamma$ rays. According to the model presented here, the December 2018 $\gamma$-ray flare was connected to a neutrino emission that was too brief and not bright enough to be detected by current neutrino instruments., Comment: 18 pages, 6 figures; V2 to match published version, typo fixed
Published: 2022
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20. New Tests of Millilensing in the Blazar PKS 1413+135

Author: Peirson, A. L., Liodakis, I., Readhead, A. C. S., Lister, M. L., Perlman, E. S., Aller, M. F., Blandford, R. D., Grainge, K. J. B., Green, D. A., Gurwell, M. A., Hodges, M. W., Hovatta, T., Kiehlmann, S., Lähteenmäki, A., Max-Moerbeck, W., Mcaloone, T., O'Neill, S., Pavlidou, V., Pearson, T. J., Ravi, V., Reeves, R. A., Scott, P. F., Taylor, G. B., Titterington, D. J., Tornikoski, M., Vedantham, H. K., Wilkinson, P. N., Williams, D. T., and Zensus, J. A.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Symmetric Achromatic Variability (SAV) is a rare form of radio variability in blazars that has been attributed to gravitational millilensing by a ~$10^2 - 10^5$ $M_\odot$ mass condensate. Four SAVs have been identified between 1980 and 2020 in the long-term radio monitoring data of the blazar PKS 1413+135. We show that all four can be fitted with the same, unchanging, gravitational lens model. If SAV is due to gravitational millilensing, PKS 1413+135 provides a unique system for studying active galactic nuclei with unprecedented microarcsecond resolution, as well as for studying the nature of the millilens itself. We discuss two possible candidates for the putative millilens: a giant molecular cloud hosted in the intervening edge-on spiral galaxy, and an undetected dwarf galaxy with a massive black hole. We find a significant dependence of SAV crossing time on frequency, which could indicate a fast shock moving in a slower underlying flow. We also find tentative evidence for a 989-day periodicity in the SAVs, which, if real, makes possible the prediction of future SAVs: the next three windows for possible SAVs begin in August 2022, May 2025, and February 2028., Comment: Accepted to ApJ
Published: 2022
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21. Prediction of (p,n) Charge-Exchange Reactions with Uncertainty Quantification

Author: Whitehead, T. R., Poxon-Pearson, T., Nunes, F. M., and Potel, G.
Subjects: Nuclear Theory, Nuclear Experiment
Abstract: Background: Charge-exchange reactions are a powerful tool for exploring nuclear structure and nuclear astrophysics, however, a robust charge-exchange reaction theory with quantified uncertainties is essential to extracting reliable physics. Purpose: The goal of this work is to determine the uncertainties due to optical potentials used in the theory for charge-exchange reactions to isobaric analogue states. Method: We implement a two-body reaction model to study (p,n) charge-exchange transitions and perform a Bayesian analysis. We study the (p,n) reaction to the isobaric analog states of $^{14}$C, $^{48}$Ca, and $^{90}$Zr targets over a range of beam energies. We compare predictions using standard phenomenological optical potentials with those obtained microscopically. Results: Charge-exchange cross sections are reasonably reproduced by modern optical potentials. However, when uncertainties in the optical potentials are accounted for, the resulting predictions of charge-exchange cross sections have very large uncertainties. Conclusions: The charge-exchange reaction cross section is strongly sensitive to the input interactions, making it a good candidate to further constrain nuclear forces and aspects of bulk nuclear matter. However, further constraints on the optical potentials are necessary for a robust connection between this tool and the underlying isovector properties of nuclei.
Published: 2021
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22. Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

Author: MAGIC Collaboration, Acciari, V. A., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batković, I., González, J. Becerra, Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Fattorini, A., Ferrara, G., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., López, R. J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jiménez, I., Jormanainen, J., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Perennes, C., Persic, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Zarić, D., de Palma, F., D'Ammando, F., Barnacka, A., Sahu, D. K., Hodges, M., Hovatta, T., Kiehlmann, S., Max-Moerbeck, W., Readhead, A. C. S., Reeves, R., Pearson, T. J., Lähteenmäki, A., Björklund, I., Tornikoski, M., Tammi, J., Suutarinen, S., Hada, K., and Niinuma, K.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract: We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016-2020. Optical, X-ray and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very-high-energy (VHE, >= 100 GeV) gamma-ray emission. The lack of enhancement in radio emission measured by OVRO indicates the multi-zone nature of the emission from this object. We constrain the VHE duty cycle of the source to be < 16 2014-like flares per year (95% confidence). For the first time for this source, a broadband low-state SED is constructed with a deep exposure up to the VHE range. A flux upper limit on the low-state VHE gamma-ray emission of an order of magnitude below that of the 2014 flare is determined. The X-ray data are used to fit the column density of (8.10 +- 0.93 stat ) x 10^21 cm^-2 of the dust in the lensing galaxy. VLBI observations show a clear radio core and jet components in both lensed images, yet no significant movement of the components is seen. The radio measurements are used to model the source-lens-observer geometry and determine the magnifications and time delays for both components. The quiescent emission is modeled with the high-energy bump explained as a combination of synchrotron-self-Compton and external Compton emission from a region located outside of the broad line region. The bulk of the low-energy emission is explained as originating from a tens-of-parsecs scale jet., Comment: 21 pages, 12 figures, 5 tables, accepted for publication in MNRAS
Published: 2021
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23. The Unanticipated Phenomenology of the Blazar PKS~2131$-$021: A Unique Super-Massive Black Hole Binary Candidate

Author: O'Neill, S., Kiehlmann, S., Readhead, A. C. S., Aller, M. F., Blandford, R. D., Liodakis, I., Lister, M. L., Mróz, P., O'Dea, C. P., Pearson, T. J., Ravi, V., Vallisneri, M., Cleary, K. A., Graham, M. J., Grainge, K. J. B., Hodges, M. W., Hovatta, T., Lähteenmäki, A., Lamb, J. W., Lazio, T. J. W., Max-Moerbeck, W., Pavlidou, V., Prince, T. A., Reeves, R. A., Tornikoski, M., de la Para, P. Vergara, and Zensus, J. A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Most large galaxies host supermassive black holes in their nuclei and are subject to mergers, which can produce a supermassive black hole binary (SMBHB), and hence periodic signatures due to orbital motion. We report unique periodic radio flux density variations in the blazar PKS~2131$-$021, which strongly suggest an SMBHB with an orbital separation of $\sim 0.001-0.01$ pc. Our 45.1-year radio light curve shows two epochs of strong sinusoidal variation with the same period and phase to within $<2\%$ and $\sim 10\%$, respectively, straddling a 20-year period when this variation was absent. Our simulated light curves accurately reproduce the ``red noise'' of this object, and Lomb-Scargle, weighted wavelet Z-transform, and least-squares sine wave analyses demonstrate conclusively, at the $4.6\sigma$ significance level, that the periodicity in this object is not due to random fluctuations in flux density. The observed period translates to $2.082\pm 0.003$ years in the rest frame at the $z=1.285$ redshift of PKS~2131$-$021. The periodic variation in PKS~2131$-$021 is remarkably sinusoidal. We present a model in which orbital motion, combined with the strong Doppler boosting of the approaching relativistic jet, produces a sine-wave modulation in the flux density which easily fits the observations. Given the rapidly-developing field of gravitational wave experiments with pulsar timing arrays, closer counterparts to PKS~2131$-$021 and searches using the techniques we have developed are strongly motivated. These results constitute a compelling demonstration that the phenomenology, not the theory, must provide the lead in this field., Comment: 24 pages, 13 figure, 3 Tables, accepted for publication in APJL
Published: 2021
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24. Erratum to: Searches for long-lived charged particles in pp collisions at s = 7 and 8 TeV

Author: Chatrchyan, S., Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Bergauer, T., Dragicevic, M., Erö, J., Fabjan, C., Friedl, M., Frühwirth, R., Ghete, V. M., Hörmann, N., Hrubec, J., Jeitler, M., Kiesenhofer, W., Knünz, V., Krammer, M., Krätschmer, I., Liko, D., Mikulec, I., Rabady, D., Rahbaran, B., Rohringer, C., Rohringer, H., Schöfbeck, R., Strauss, J., Taurok, A., Treberer-Treberspurg, W., Waltenberger, W., Wulz, C.-E., Mossolov, V., Shumeiko, N., Suarez Gonzalez, J., Alderweireldt, S., Bansal, M., Bansal, S., Cornelis, T., De Wolf, E. A., Janssen, X., Knutsson, A., Luyckx, S., Mucibello, L., Ochesanu, S., Roland, B., Rougny, R., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Van Spilbeeck, A., Blekman, F., Blyweert, S., D’Hondt, J., Kalogeropoulos, A., Keaveney, J., Maes, M., Olbrechts, A., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Onsem, G. P., Villella, I., Clerbaux, B., De Lentdecker, G., Favart, L., Gay, A. P. R., Hreus, T., Léonard, A., Marage, P. E., Mohammadi, A., Perniè, L., Reis, T., Seva, T., Thomas, L., Vander Velde, C., Vanlaer, P., Wang, J., Adler, V., Beernaert, K., Benucci, L., Cimmino, A., Costantini, S., Dildick, S., Garcia, G., Klein, B., Lellouch, J., Marinov, A., Mccartin, J., Ocampo Rios, A. A., Ryckbosch, D., Sigamani, M., Strobbe, N., Thyssen, F., Tytgat, M., Walsh, S., Yazgan, E., Zaganidis, N., Basegmez, S., Beluffi, C., Bruno, G., Castello, R., Caudron, A., Ceard, L., Delaere, C., du Pree, T., Favart, D., Forthomme, L., Giammanco, A., Hollar, J., Jez, P., Lemaitre, V., Liao, J., Militaru, O., Nuttens, C., Pagano, D., Pin, A., Piotrzkowski, K., Popov, A., Selvaggi, M., Vizan Garcia, J. M., Beliy, N., Caebergs, T., Daubie, E., Hammad, G. H., Alves, G. A., Correa Martins Junior, M., Martins, T., Pol, M. E., Souza, M. H. G., Aldá Júnior, W. L., Carvalho, W., Chinellato, J., Custódio, A., Da Costa, E. M., De Jesus Damiao, D., De Oliveira Martins, C., Fonseca De Souza, S., Malbouisson, H., Malek, M., Matos Figueiredo, D., Mundim, L., Nogima, H., Prado Da Silva, W. L., Santoro, A., Sznajder, A., Tonelli Manganote, E. J., Vilela Pereira, A., Bernardes, C. A., Dias, F. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Lagana, C., Marinho, F., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Genchev, V., Iaydjiev, P., Piperov, S., Rodozov, M., Sultanov, G., Vutova, M., Dimitrov, A., Hadjiiska, R., Kozhuharov, V., Litov, L., Pavlov, B., Petkov, P., Bian, J. G., Chen, G. M., Chen, H. S., Jiang, C. H., Liang, D., Liang, S., Meng, X., Tao, J., Wang, J., Wang, X., Wang, Z., Xiao, H., Xu, M., Asawatangtrakuldee, C., Ban, Y., Guo, Y., Li, W., Liu, S., Mao, Y., Qian, S. J., Teng, H., Wang, D., Zhang, L., Zou, W., Avila, C., Carrillo Montoya, C. A., Gomez, J. P., Gomez Moreno, B., Sanabria, J. C., Godinovic, N., Lelas, D., Plestina, R., Polic, D., Puljak, I., Antunovic, Z., Kovac, M., Brigljevic, V., Duric, S., Kadija, K., Luetic, J., Mekterovic, D., Morovic, S., Tikvica, L., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Finger, M., Finger, Jr., M., Assran, Y., Ellithi Kamel, A., Mahmoud, M. A., Mahrous, A., Radi, A., Kadastik, M., Müntel, M., Murumaa, M., Raidal, M., Rebane, L., Tiko, A., Eerola, P., Fedi, G., Voutilainen, M., Härkönen, J., Karimäki, V., Kinnunen, R., Kortelainen, M. J., Lampén, T., Lassila-Perini, K., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Peltola, T., Tuominen, E., Tuominiemi, J., Tuovinen, E., Wendland, L., Korpela, A., Tuuva, T., Besancon, M., Choudhury, S., Couderc, F., Dejardin, M., Denegri, D., Fabbro, B., Faure, J. L., Ferri, F., Ganjour, S., Givernaud, A., Gras, P., Hamel de Monchenault, G., Jarry, P., Locci, E., Malcles, J., Millischer, L., Nayak, A., Rander, J., Rosowsky, A., Titov, M., Baffioni, S., Beaudette, F., Benhabib, L., Bianchini, L., Bluj, M., Busson, P., Charlot, C., Daci, N., Dahms, T., Dalchenko, M., Dobrzynski, L., Florent, A., Granier de Cassagnac, R., Haguenauer, M., Miné, P., Mironov, C., Naranjo, I. N., Nguyen, M., Ochando, C., Paganini, P., Sabes, D., Salerno, R., Sirois, Y., Veelken, C., Zabi, A., Agram, J.-L., Andrea, J., Bloch, D., Bodin, D., Brom, J.-M., Chabert, E. C., Collard, C., Conte, E., Drouhin, F., Fontaine, J.-C., Gelé, D., Goerlach, U., Goetzmann, C., Juillot, P., Le Bihan, A.-C., Van Hove, P., Gadrat, S., Beauceron, S., Beaupere, N., Boudoul, G., Brochet, S., Chasserat, J., Chierici, R., Contardo, D., Depasse, P., El Mamouni, H., Fay, J., Gascon, S., Gouzevitch, M., Ille, B., Kurca, T., Lethuillier, M., Mirabito, L., Perries, S., Sgandurra, L., Sordini, V., Tschudi, Y., Vander Donckt, M., Verdier, P., Viret, S., Tsamalaidze, Z., Autermann, C., Beranek, S., Calpas, B., Edelhoff, M., Feld, L., Heracleous, N., Hindrichs, O., Klein, K., Ostapchuk, A., Perieanu, A., Raupach, F., Sammet, J., Schael, S., Sprenger, D., Weber, H., Wittmer, B., Zhukov, V., Ata, M., Caudron, J., Dietz-Laursonn, E., Duchardt, D., Erdmann, M., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Klingebiel, D., Kreuzer, P., Merschmeyer, M., Meyer, A., Olschewski, M., Padeken, K., Papacz, P., Pieta, H., Reithler, H., Schmitz, S. A., Sonnenschein, L., Steggemann, J., Teyssier, D., Thüer, S., Weber, M., Cherepanov, V., Erdogan, Y., Flügge, G., Geenen, H., Geisler, M., Haj Ahmad, W., Hoehle, F., Kargoll, B., Kress, T., Kuessel, Y., Lingemann, J., Nowack, A., Nugent, I. M., Perchalla, L., Pooth, O., Stahl, A., Aldaya Martin, M., Asin, I., Bartosik, N., Behr, J., Behrenhoff, W., Behrens, U., Bergholz, M., Bethani, A., Borras, K., Burgmeier, A., Cakir, A., Calligaris, L., Campbell, A., Costanza, F., Diez Pardos, C., Dooling, S., Dorland, T., Eckerlin, G., Eckstein, D., Flucke, G., Geiser, A., Glushkov, I., Gunnellini, P., Habib, S., Hauk, J., Hellwig, G., Jung, H., Kasemann, M., Katsas, P., Kleinwort, C., Kluge, H., Krämer, M., Krücker, D., Kuznetsova, E., Lange, W., Leonard, J., Lipka, K., Lohmann, W., Lutz, B., Mankel, R., Marfin, I., Melzer-Pellmann, I.-A., Meyer, A. B., Mnich, J., Mussgiller, A., Naumann-Emme, S., Novgorodova, O., Nowak, F., Olzem, J., Perrey, H., Petrukhin, A., Pitzl, D., Placakyte, R., Raspereza, A., Ribeiro Cipriano, P. M., Riedl, C., Ron, E., Sahin, M. Ö., Salfeld-Nebgen, J., Schmidt, R., Schoerner-Sadenius, T., Sen, N., Stein, M., Walsh, R., Wissing, C., Blobel, V., Enderle, H., Erfle, J., Gebbert, U., Görner, M., Gosselink, M., Haller, J., Heine, K., Höing, R. S., Kaussen, G., Kirschenmann, H., Klanner, R., Kogler, R., Lange, J., Marchesini, I., Peiffer, T., Pietsch, N., Rathjens, D., Sander, C., Schettler, H., Schleper, P., Schlieckau, E., Schmidt, A., Schröder, M., Schum, T., Seidel, M., Sibille, J., Sola, V., Stadie, H., Steinbrück, G., Thomsen, J., Troendle, D., Vanelderen, L., Barth, C., Baus, C., Berger, J., Böser, C., Chwalek, T., De Boer, W., Descroix, A., Dierlamm, A., Feindt, M., Guthoff, M., Hackstein, C., Hartmann, F., Hauth, T., Heinrich, M., Held, H., Hoffmann, K. H., Husemann, U., Katkov, I., Komaragiri, J. R., Kornmayer, A., Lobelle Pardo, P., Martschei, D., Mueller, S., Müller, Th., Niegel, M., Nürnberg, A., Oberst, O., Ott, J., Quast, G., Rabbertz, K., Ratnikov, F., Röcker, S., Schilling, F.-P., Schott, G., Simonis, H. J., Stober, F. M., Ulrich, R., Wagner-Kuhr, J., Wayand, S., Weiler, T., Zeise, M., Anagnostou, G., Daskalakis, G., Geralis, T., Kesisoglou, S., Kyriakis, A., Loukas, D., Markou, A., Markou, C., Ntomari, E., Gouskos, L., Mertzimekis, T. J., Panagiotou, A., Saoulidou, N., Stiliaris, E., Aslanoglou, X., Evangelou, I., Flouris, G., Foudas, C., Kokkas, P., Manthos, N., Papadopoulos, I., Paradas, E., Bencze, G., Hajdu, C., Hidas, P., Horvath, D., Radics, B., Sikler, F., Veszpremi, V., Vesztergombi, G., Zsigmond, A. J., Beni, N., Czellar, S., Molnar, J., Palinkas, J., Szillasi, Z., Karancsi, J., Raics, P., Trocsanyi, Z. L., Ujvari, B., Beri, S. B., Bhatnagar, V., Dhingra, N., Gupta, R., Kaur, M., Mehta, M. Z., Mittal, M., Nishu, N., Saini, L. K., Sharma, A., Singh, J. B., Kumar, Ashok, Kumar, Arun, Ahuja, S., Bhardwaj, A., Choudhary, B. C., Malhotra, S., Naimuddin, M., Ranjan, K., Saxena, P., Sharma, V., Shivpuri, R. K., Banerjee, S., Bhattacharya, S., Chatterjee, K., Dutta, S., Gomber, B., Jain, Sa., Jain, Sh., Khurana, R., Modak, A., Mukherjee, S., Roy, D., Sarkar, S., Sharan, M., Abdulsalam, A., Dutta, D., Kailas, S., Kumar, V., Mohanty, A. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Chatterjee, R. M., Ganguly, S., Ghosh, S., Guchait, M., Gurtu, A., Kole, G., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Mohanty, G. B., Parida, B., Sudhakar, K., Wickramage, N., Banerjee, S., Dugad, S., Arfaei, H., Bakhshiansohi, H., Etesami, S. M., Fahim, A., Hesari, H., Jafari, A., Khakzad, M., Mohammadi Najafabadi, M., Paktinat Mehdiabadi, S., Safarzadeh, B., Zeinali, M., Grunewald, M., Abbrescia, M., Barbone, L., Calabria, C., Chhibra, S. S., Colaleo, A., Creanza, D., De Filippis, N., De Palma, M., Fiore, L., Iaselli, G., Maggi, G., Maggi, M., Marangelli, B., My, S., Nuzzo, S., Pacifico, N., Pompili, A., Pugliese, G., Selvaggi, G., Silvestris, L., Singh, G., Venditti, R., Verwilligen, P., Zito, G., Abbiendi, G., Benvenuti, A. C., Bonacorsi, D., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Meneghelli, M., Montanari, A., Navarria, F. L., Odorici, F., Perrotta, A., Primavera, F., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Travaglini, R., Albergo, S., Chiorboli, M., Costa, S., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Frosali, S., Gallo, E., Gonzi, S., Gori, V., Lenzi, P., Meschini, M., Paoletti, S., Sguazzoni, G., Tropiano, A., Benussi, L., Bianco, S., Fabbri, F., Piccolo, D., Fabbricatore, P., Musenich, R., Tosi, S., Benaglia, A., De Guio, F., Di Matteo, L., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Lucchini, M. T., Malvezzi, S., Manzoni, R. A., Martelli, A., Menasce, D., Moroni, L., Paganoni, M., Pedrini, D., Ragazzi, S., Redaelli, N., Tabarelli de Fatis, T., Buontempo, S., Cavallo, N., De Cosa, A., Fabozzi, F., Iorio, A. O. M., Lista, L., Meola, S., Merola, M., Paolucci, P., Azzi, P., Bacchetta, N., Bisello, D., Branca, A., Carlin, R., Checchia, P., Dorigo, T., Dosselli, U., Galanti, M., Gasparini, F., Gasparini, U., Giubilato, P., Gozzelino, A., Gulmini, M., Kanishchev, K., Lacaprara, S., Lazzizzera, I., Margoni, M., Maron, G., Meneguzzo, A. T., Pazzini, J., Pozzobon, N., Ronchese, P., Simonetto, F., Torassa, E., Tosi, M., Vanini, S., Zotto, P., Zucchetta, A., Zumerle, G., Gabusi, M., Ratti, S. P., Riccardi, C., Vitulo, P., Biasini, M., Bilei, G. M., Fanò, L., Lariccia, P., Mantovani, G., Menichelli, M., Nappi, A., Romeo, F., Saha, A., Santocchia, A., Spiezia, A., Androsov, K., Azzurri, P., Bagliesi, G., Boccali, T., Broccolo, G., Castaldi, R., D’Agnolo, R. T., Dell’Orso, R., Fiori, F., Foà, L., Giassi, A., Kraan, A., Ligabue, F., Lomtadze, T., Martini, L., Messineo, A., Palla, F., Rizzi, A., Serban, A. T., Spagnolo, P., Squillacioti, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Vernieri, C., Barone, L., Cavallari, F., Del Re, D., Diemoz, M., Grassi, M., Longo, E., Margaroli, F., Meridiani, P., Micheli, F., Nourbakhsh, S., Organtini, G., Paramatti, R., Rahatlou, S., Soffi, L., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Biino, C., Cartiglia, N., Casasso, S., Costa, M., Demaria, N., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Musich, M., Obertino, M. M., Ortona, G., Pastrone, N., Pelliccioni, M., Potenza, A., Romero, A., Ruspa, M., Sacchi, R., Solano, A., Staiano, A., Tamponi, U., Belforte, S., Candelise, V., Casarsa, M., Cossutti, F., Della Ricca, G., Gobbo, B., La Licata, C., Marone, M., Montanino, D., Penzo, A., Schizzi, A., Zanetti, A., Kim, T. Y., Nam, S. K., Chang, S., Kim, D. H., Kim, G. N., Kim, J. E., Kong, D. J., Oh, Y. D., Park, H., Son, D. C., Kim, J. Y., Kim, Zero J., Song, S., Choi, S., Gyun, D., Hong, B., Jo, M., Kim, H., Kim, T. J., Lee, K. S., Park, S. K., Roh, Y., Choi, M., Kim, J. H., Park, C., Park, I. C., Park, S., Ryu, G., Choi, Y., Choi, Y. K., Goh, J., Kim, M. S., Kwon, E., Lee, B., Lee, J., Lee, S., Seo, H., Yu, I., Grigelionis, I., Juodagalvis, A., Castilla-Valdez, H., De La Cruz-Burelo, E., Heredia-de La Cruz, I., Lopez-Fernandez, R., Martínez-Ortega, J., Sanchez-Hernandez, A., Villasenor-Cendejas, L. M., Carrillo Moreno, S., Vazquez Valencia, F., Salazar Ibarguen, H. A., Casimiro Linares, E., Morelos Pineda, A., Reyes-Santos, M. A., Krofcheck, D., Bell, A. J., Butler, P. H., Doesburg, R., Reucroft, S., Silverwood, H., Ahmad, M., Asghar, M. I., Butt, J., Hoorani, H. R., Khalid, S., Khan, W. A., Khurshid, T., Qazi, S., Shah, M. A., Shoaib, M., Bialkowska, H., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Romanowska-Rybinska, K., Szleper, M., Wrochna, G., Zalewski, P., Brona, G., Bunkowski, K., Cwiok, M., Dominik, W., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Wolszczak, W., Almeida, N., Bargassa, P., David, A., Faccioli, P., Ferreira Parracho, P. G., Gallinaro, M., Rodrigues Antunes, J., Seixas, J., Varela, J., Vischia, P., Bunin, P., Gavrilenko, M., Golutvin, I., Gorbunov, I., Kamenev, A., Karjavin, V., Konoplyanikov, V., Kozlov, G., Lanev, A., Malakhov, A., Matveev, V., Moisenz, P., Palichik, V., Perelygin, V., Shmatov, S., Skatchkov, N., Smirnov, V., Zarubin, A., Evstyukhin, S., Golovtsov, V., Ivanov, Y., Kim, V., Levchenko, P., Murzin, V., Oreshkin, V., Smirnov, I., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Vorobyev, An., Andreev, Yu., Dermenev, A., Gninenko, S., Golubev, N., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Erofeeva, M., Gavrilov, V., Lychkovskaya, N., Popov, V., Safronov, G., Semenov, S., Spiridonov, A., Stolin, V., Vlasov, E., Zhokin, A., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Leonidov, A., Mesyats, G., Rusakov, S. V., Vinogradov, A., Belyaev, A., Boos, E., Bunichev, V., Dubinin, M., Dudko, L., Ershov, A., Gribushin, A., Klyukhin, V., Kodolova, O., Lokhtin, I., Markina, A., Obraztsov, S., Savrin, V., Snigirev, A., Azhgirey, I., Bayshev, I., Bitioukov, S., Kachanov, V., Kalinin, A., Konstantinov, D., Krychkine, V., Petrov, V., Ryutin, R., Sobol, A., Tourtchanovitch, L., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, P., Ekmedzic, M., Krpic, D., Milosevic, J., Aguilar-Benitez, M., Alcaraz Maestre, J., Battilana, C., Calvo, E., Cerrada, M., Chamizo Llatas, M., Colino, N., De La Cruz, B., Delgado Peris, A., Domínguez Vázquez, D., Fernandez Bedoya, C., Fernández Ramos, J. P., Ferrando, A., Flix, J., Fouz, M. C., Garcia-Abia, P., Gonzalez Lopez, O., Goy Lopez, S., Hernandez, J. M., Josa, M. I., Merino, G., Navarro De Martino, E., Puerta Pelayo, J., Quintario Olmeda, A., Redondo, I., Romero, L., Santaolalla, J., Soares, M. S., Willmott, C., Albajar, C., de Trocóniz, J. F., Brun, H., Cuevas, J., Fernandez Menendez, J., Folgueras, S., Gonzalez Caballero, I., Lloret Iglesias, L., Piedra Gomez, J., Brochero Cifuentes, J. A., Cabrillo, I. J., Calderon, A., Chuang, S. H., Duarte Campderros, J., Fernandez, M., Gomez, G., Gonzalez Sanchez, J., Graziano, A., Jorda, C., Lopez Virto, A., Marco, J., Marco, R., Martinez Rivero, C., Matorras, F., Munoz Sanchez, F. J., Rodrigo, T., Rodríguez-Marrero, A. Y., Ruiz-Jimeno, A., Scodellaro, L., Vila, I., Vilar Cortabitarte, R., Abbaneo, D., Auffray, E., Auzinger, G., Bachtis, M., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Benitez, J. F., Bernet, C., Bianchi, G., Bloch, P., Bocci, A., Bonato, A., Bondu, O., Botta, C., Breuker, H., Camporesi, T., Cerminara, G., Christiansen, T., Coarasa Perez, J. A., Colafranceschi, S., d’Enterria, D., Dabrowski, A., De Roeck, A., De Visscher, S., Di Guida, S., Dobson, M., Dupont-Sagorin, N., Elliott-Peisert, A., Eugster, J., Funk, W., Georgiou, G., Giffels, M., Gigi, D., Gill, K., Giordano, D., Girone, M., Giunta, M., Glege, F., Gomez-Reino Garrido, R., Gowdy, S., Guida, R., Hammer, J., Hansen, M., Harris, P., Hartl, C., Hinzmann, A., Innocente, V., Janot, P., Karavakis, E., Kousouris, K., Krajczar, K., Lecoq, P., Lee, Y.-J., Lourenço, C., Magini, N., Malberti, M., Malgeri, L., Mannelli, M., Masetti, L., Meijers, F., Mersi, S., Meschi, E., Moser, R., Mulders, M., Musella, P., Nesvold, E., Orsini, L., Palencia Cortezon, E., Perez, E., Perrozzi, L., Petrilli, A., Pfeiffer, A., Pierini, M., Pimiä, M., Piparo, D., Plagge, M., Polese, G., Quertenmont, L., Racz, A., Reece, W., Rolandi, G., Rovelli, C., Rovere, M., Sakulin, H., Santanastasio, F., Schäfer, C., Schwick, C., Segoni, I., Sekmen, S., Sharma, A., Siegrist, P., Silva, P., Simon, M., Sphicas, P., Spiga, D., Stoye, M., Tsirou, A., Veres, G. I., Vlimant, J. R., Wöhri, H. K., Worm, S. D., Zeuner, W. D., Bertl, W., Deiters, K., Erdmann, W., Gabathuler, K., Horisberger, R., Ingram, Q., Kaestli, H. C., König, S., Kotlinski, D., Langenegger, U., Renker, D., Rohe, T., Bachmair, F., Bäni, L., Bortignon, P., Buchmann, M. A., Casal, B., Chanon, N., Deisher, A., Dissertori, G., Dittmar, M., Donegà, M., Dünser, M., Eller, P., Freudenreich, K., Grab, C., Hits, D., Lecomte, P., Lustermann, W., Marini, A. C., Martinez Ruiz del Arbol, P., Mohr, N., Moortgat, F., Nägeli, C., Nef, P., Nessi-Tedaldi, F., Pandolfi, F., Pape, L., Pauss, F., Peruzzi, M., Ronga, F. J., Rossini, M., Sala, L., Sanchez, A. K., Starodumov, A., Stieger, B., Takahashi, M., Tauscher, L., Thea, A., Theofilatos, K., Treille, D., Urscheler, C., Wallny, R., Weber, H. A., Amsler, C., Chiochia, V., Favaro, C., Ivova Rikova, M., Kilminster, B., Millan Mejias, B., Otiougova, P., Robmann, P., Snoek, H., Taroni, S., Tupputi, S., Verzetti, M., Cardaci, M., Chen, K. 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M., Rogerson, S., Rose, A., Seez, C., Sharp, P., Sparrow, A., Tapper, A., Vazquez Acosta, M., Virdee, T., Wakefield, S., Wardle, N., Whyntie, T., Chadwick, M., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, P., Leggat, D., Leslie, D., Martin, W., Reid, I. D., Symonds, P., Teodorescu, L., Turner, M., Dittmann, J., Hatakeyama, K., Kasmi, A., Liu, H., Scarborough, T., Charaf, O., Cooper, S. I., Henderson, C., Rumerio, P., Avetisyan, A., Bose, T., Fantasia, C., Heister, A., Lawson, P., Lazic, D., Rohlf, J., Sperka, D., St. John, J., Sulak, L., Alimena, J., Bhattacharya, S., Christopher, G., Cutts, D., Demiragli, Z., Ferapontov, A., Garabedian, A., Heintz, U., Kukartsev, G., Laird, E., Landsberg, G., Luk, M., Narain, M., Segala, M., Sinthuprasith, T., Speer, T., Breedon, R., Breto, G., Calderon De La Barca Sanchez, M., Chauhan, S., Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Gardner, M., Houtz, R., Ko, W., Kopecky, A., Lander, R., Mall, O., Miceli, T., Nelson, R., Pellett, D., Ricci-Tam, F., Rutherford, B., Searle, M., Smith, J., Squires, M., Tripathi, M., Wilbur, S., Yohay, R., Andreev, V., Cline, D., Cousins, R., Erhan, S., Everaerts, P., Farrell, C., Felcini, M., Hauser, J., Ignatenko, M., Jarvis, C., Rakness, G., Schlein, P., Takasugi, E., Traczyk, P., Valuev, V., Weber, M., Babb, J., Clare, R., Dinardo, M. E., Ellison, J., Gary, J. W., Hanson, G., Liu, H., Long, O. R., Luthra, A., Nguyen, H., Paramesvaran, S., Sturdy, J., Sumowidagdo, S., Wilken, R., Wimpenny, S., Andrews, W., Branson, J. G., Cerati, G. B., Cittolin, S., Evans, D., Holzner, A., Kelley, R., Lebourgeois, M., Letts, J., Macneill, I., Mangano, B., Padhi, S., Palmer, C., Petrucciani, G., Pieri, M., Sani, M., Sharma, V., Simon, S., Sudano, E., Tadel, M., Tu, Y., Vartak, A., Wasserbaech, S., Würthwein, F., Yagil, A., Yoo, J., Barge, D., Bellan, R., Campagnari, C., D’Alfonso, M., Danielson, T., Flowers, K., Geffert, P., George, C., Golf, F., Incandela, J., Justus, C., Kalavase, P., Kovalskyi, D., Krutelyov, V., Lowette, S., Magaña Villalba, R., Mccoll, N., Pavlunin, V., Ribnik, J., Richman, J., Rossin, R., Stuart, D., To, W., West, C., Apresyan, A., Bornheim, A., Bunn, J., Chen, Y., Di Marco, E., Duarte, J., Kcira, D., Ma, Y., Mott, A., Newman, H. B., Rogan, C., Spiropulu, M., Timciuc, V., Veverka, J., Wilkinson, R., Xie, S., Yang, Y., Zhu, R. Y., Azzolini, V., Calamba, A., Carroll, R., Ferguson, T., Iiyama, Y., Jang, D. W., Liu, Y. F., Paulini, M., Russ, J., Vogel, H., Vorobiev, I., Cumalat, J. P., Drell, B. R., Ford, W. T., Gaz, A., Luiggi Lopez, E., Nauenberg, U., Smith, J. G., Stenson, K., Ulmer, K. A., Wagner, S. R., Alexander, J., Chatterjee, A., Eggert, N., Gibbons, L. K., Hopkins, W., Khukhunaishvili, A., Kreis, B., Mirman, N., Nicolas Kaufman, G., Patterson, J. R., Ryd, A., Salvati, E., Sun, W., Teo, W. D., Thom, J., Thompson, J., Tucker, J., Weng, Y., Winstrom, L., Wittich, P., Winn, D., Abdullin, S., Albrow, M., Anderson, J., Apollinari, G., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Burkett, K., Butler, J. N., Chetluru, V., Cheung, H. W. K., Chlebana, F., Cihangir, S., Elvira, V. D., Fisk, I., Freeman, J., Gao, Y., Gottschalk, E., Gray, L., Green, D., Gutsche, O., Hare, D., Harris, R. M., Hirschauer, J., Hooberman, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kunori, S., Kwan, S., Leonidopoulos, C., Linacre, J., Lincoln, D., Lipton, R., Lykken, J., Maeshima, K., Marraffino, J. M., Martinez Outschoorn, V. I., Maruyama, S., Mason, D., McBride, P., Mishra, K., Mrenna, S., Musienko, Y., Newman-Holmes, C., O’Dell, V., Prokofyev, O., Ratnikova, N., Sexton-Kennedy, E., Sharma, S., Spalding, W. J., Spiegel, L., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vidal, R., Whitmore, J., Wu, W., Yang, F., Yun, J. C., Acosta, D., Avery, P., Bourilkov, D., Chen, M., Cheng, T., Das, S., De Gruttola, M., Di Giovanni, G. P., Dobur, D., Drozdetskiy, A., Field, R. D., Fisher, M., Fu, Y., Furic, I. K., Hugon, J., Kim, B., Konigsberg, J., Korytov, A., Kropivnitskaya, A., Kypreos, T., Low, J. F., Matchev, K., Milenovic, P., Mitselmakher, G., Muniz, L., Remington, R., Rinkevicius, A., Skhirtladze, N., Snowball, M., Yelton, J., Zakaria, M., Gaultney, V., Hewamanage, S., Lebolo, L. M., Linn, S., Markowitz, P., Martinez, G., Rodriguez, J. L., Adams, T., Askew, A., Bochenek, J., Chen, J., Diamond, B., Gleyzer, S. V., Haas, J., Hagopian, S., Hagopian, V., Johnson, K. F., Prosper, H., Veeraraghavan, V., Weinberg, M., Baarmand, M. M., Dorney, B., Hohlmann, M., Kalakhety, H., Yumiceva, F., Adams, M. R., Apanasevich, L., Bazterra, V. E., Betts, R. R., Bucinskaite, I., Callner, J., Cavanaugh, R., Evdokimov, O., Gauthier, L., Gerber, C. E., Hofman, D. J., Khalatyan, S., Kurt, P., Lacroix, F., Moon, D. H., O’Brien, C., Silkworth, C., Strom, D., Turner, P., Varelas, N., Akgun, U., Albayrak, E. A., Bilki, B., Clarida, W., Dilsiz, K., Duru, F., Griffiths, S., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Newsom, C. R., Ogul, H., Onel, Y., Ozok, F., Sen, S., Tan, P., Tiras, E., Wetzel, J., Yetkin, T., Yi, K., Barnett, B. A., Blumenfeld, B., Bolognesi, S., Fehling, D., Giurgiu, G., Gritsan, A. V., Guo, Z. J., Hu, G., Maksimovic, P., Swartz, M., Whitbeck, A., Baringer, P., Bean, A., Benelli, G., Kenny, III, R. P., Murray, M., Noonan, D., Sanders, S., Stringer, R., Wood, J. S., Barfuss, A. F., Chakaberia, I., Ivanov, A., Khalil, S., Makouski, M., Maravin, Y., Shrestha, S., Svintradze, I., Gronberg, J., Lange, D., Rebassoo, F., Wright, D., Baden, A., Calvert, B., Eno, S. C., Gomez, J. A., Hadley, N. J., Kellogg, R. G., Kolberg, T., Lu, Y., Marionneau, M., Mignerey, A. C., Pedro, K., Peterman, A., Skuja, A., Temple, J., Tonjes, M. B., Tonwar, S. C., Apyan, A., Bauer, G., Busza, W., Butz, E., Cali, I. A., Chan, M., Dutta, V., Gomez Ceballos, G., Goncharov, M., Kim, Y., Klute, M., Lai, Y. S., Levin, A., Luckey, P. D., Ma, T., Nahn, S., Paus, C., Ralph, D., Roland, C., Roland, G., Stephans, G. S. F., Stöckli, F., Sumorok, K., Sung, K., Velicanu, D., Wolf, R., Wyslouch, B., Yang, M., Yilmaz, Y., Yoon, A. S., Zanetti, M., Zhukova, V., Dahmes, B., De Benedetti, A., Franzoni, G., Gude, A., Haupt, J., Kao, S. C., Klapoetke, K., Kubota, Y., Mans, J., Pastika, N., Rusack, R., Sasseville, M., Singovsky, A., Tambe, N., Turkewitz, J., Cremaldi, L. M., Kroeger, R., Perera, L., Rahmat, R., Sanders, D. A., Summers, D., Avdeeva, E., Bloom, K., Bose, S., Claes, D. R., Dominguez, A., Eads, M., Gonzalez Suarez, R., Keller, J., Kravchenko, I., Lazo-Flores, J., Malik, S., Meier, F., Snow, G. R., Dolen, J., Godshalk, A., Iashvili, I., Jain, S., Kharchilava, A., Kumar, A., Rappoccio, S., Wan, Z., Alverson, G., Barberis, E., Baumgartel, D., Chasco, M., Haley, J., Massironi, A., Nash, D., Orimoto, T., Trocino, D., Wood, D., Zhang, J., Anastassov, A., Hahn, K. A., Kubik, A., Lusito, L., Mucia, N., Odell, N., Pollack, B., Pozdnyakov, A., Schmitt, M., Stoynev, S., Velasco, M., Won, S., Berry, D., Brinkerhoff, A., Chan, K. M., Hildreth, M., Jessop, C., Karmgard, D. J., Kolb, J., Lannon, K., Luo, W., Lynch, S., Marinelli, N., Morse, D. M., Pearson, T., Planer, M., Ruchti, R., Slaunwhite, J., Valls, N., Wayne, M., Wolf, M., Antonelli, L., Bylsma, B., Durkin, L. S., Hill, C., Hughes, R., Kotov, K., Ling, T. Y., Puigh, D., Rodenburg, M., Smith, G., Vuosalo, C., Williams, G., Winer, B. L., Wolfe, H., Berry, E., Elmer, P., Halyo, V., Hebda, P., Hegeman, J., Hunt, A., Jindal, P., Koay, S. A., Lopes Pegna, D., Lujan, P., Marlow, D., Medvedeva, T., Mooney, M., Olsen, J., Piroué, P., Quan, X., Raval, A., Saka, H., Stickland, D., Tully, C., Werner, J. S., Zenz, S. C., Zuranski, A., Brownson, E., Lopez, A., Mendez, H., Ramirez Vargas, J. E., Alagoz, E., Benedetti, D., Bolla, G., Bortoletto, D., De Mattia, M., Everett, A., Hu, Z., Jones, M., Jung, K., Koybasi, O., Kress, M., Leonardo, N., Maroussov, V., Merkel, P., Miller, D. H., Neumeister, N., Shipsey, I., Silvers, D., Svyatkovskiy, A., Vidal Marono, M., Wang, F., Xu, L., Yoo, H. D., Zablocki, J., Zheng, Y., Guragain, S., Parashar, N., Adair, A., Akgun, B., Ecklund, K. M., Geurts, F. J. M., Li, W., Padley, B. P., Redjimi, R., Roberts, J., Zabel, J., Betchart, B., Bodek, A., Covarelli, R., de Barbaro, P., Demina, R., Eshaq, Y., Ferbel, T., Garcia-Bellido, A., Goldenzweig, P., Han, J., Harel, A., Miner, D. C., Petrillo, G., Vishnevskiy, D., Zielinski, M., Bhatti, A., Ciesielski, R., Demortier, L., Goulianos, K., Lungu, G., Malik, S., Mesropian, C., Arora, S., Barker, A., Chou, J. P., Contreras-Campana, C., Contreras-Campana, E., Duggan, D., Ferencek, D., Gershtein, Y., Gray, R., Halkiadakis, E., Hidas, D., Lath, A., Panwalkar, S., Park, M., Patel, R., Rekovic, V., Robles, J., Rose, K., Salur, S., Schnetzer, S., Seitz, C., Somalwar, S., Stone, R., Thomas, S., Walker, M., Cerizza, G., Hollingsworth, M., Spanier, S., Yang, Z. C., York, A., Eusebi, R., Flanagan, W., Gilmore, J., Kamon, T., Khotilovich, V., Montalvo, R., Osipenkov, I., Pakhotin, Y., Perloff, A., Roe, J., Safonov, A., Sakuma, T., Suarez, I., Tatarinov, A., Toback, D., Akchurin, N., Damgov, J., Dragoiu, C., Dudero, P. R., Jeong, C., Kovitanggoon, K., Lee, S. W., Libeiro, T., Volobouev, I., Appelt, E., Delannoy, A. G., Greene, S., Gurrola, A., Johns, W., Maguire, C., Mao, Y., Melo, A., Sharma, M., Sheldon, P., Snook, B., Tuo, S., Velkovska, J., Arenton, M. W., Boutle, S., Cox, B., Francis, B., Goodell, J., Hirosky, R., Ledovskoy, A., Lin, C., Neu, C., Wood, J., Gollapinni, S., Harr, R., Karchin, P. E., Kottachchi Kankanamge Don, C., Lamichhane, P., Sakharov, A., Anderson, M., Belknap, D. A., Borrello, L., Carlsmith, D., Cepeda, M., Dasu, S., Friis, E., Grogg, K. S., Grothe, M., Hall-Wilton, R., Herndon, M., Hervé, A., Kaadze, K., Klabbers, P., Klukas, J., Lanaro, A., Lazaridis, C., Loveless, R., Mohapatra, A., Mozer, M. U., Ojalvo, I., Pierro, G. A., Ross, I., Savin, A., Smith, W. H., and Swanson, J.
Published: 2022
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25. Compact Symmetric Objects. I. Toward a Comprehensive Bona Fide Catalog

Author: Kiehlmann, S., primary, Lister, M. L., additional, Readhead, A. C. S, additional, Liodakis, I., additional, O’Neill, Sandra, additional, Pearson, T. J., additional, Sheldahl, Evan, additional, Siemiginowska, Aneta, additional, Tassis, K., additional, Taylor, G. B., additional, and Wilkinson, P. N., additional
Published: 2024
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26. Compact Symmetric Objects. II. Confirmation of a Distinct Population of High-luminosity Jetted Active Galaxies

Author: Kiehlmann, S., primary, Readhead, A. C. S., additional, O’Neill, S., additional, Wilkinson, P. N., additional, Lister, M. L., additional, Liodakis, I., additional, Bruzewski, S., additional, Pavlidou, V., additional, Pearson, T. J., additional, Sheldahl, E., additional, Siemiginowska, A., additional, Tassis, K., additional, and Taylor, G. B., additional
Published: 2024
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27. Compact Symmetric Objects. III. Evolution of the High-luminosity Branch and a Possible Connection with Tidal Disruption Events

Author: Readhead, A. C. S, primary, Ravi, V., additional, Blandford, R. D., additional, Sullivan, A. G., additional, Somalwar, J., additional, Begelman, M. C., additional, Birkinshaw, M., additional, Liodakis, I., additional, Lister, M. L., additional, Pearson, T. J., additional, Taylor, G. B., additional, Wilkinson, P. N., additional, Globus, N., additional, Kiehlmann, S., additional, Lawrence, C. R., additional, Murphy, D., additional, O’Neill, S., additional, Pavlidou, V., additional, Sheldahl, E., additional, Siemiginowska, A., additional, and Tassis, K., additional
Published: 2024
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28. The RoboPol sample of optical polarimetric standards

Author: Blinov, D., primary, Maharana, S., additional, Bouzelou, F., additional, Casadio, C., additional, Gjerløw, E., additional, Jormanainen, J., additional, Kiehlmann, S., additional, Kypriotakis, J. A., additional, Liodakis, I., additional, Mandarakas, N., additional, Markopoulioti, L., additional, Panopoulou, G. V., additional, Pelgrims, V., additional, Pouliasi, A., additional, Romanopoulos, S., additional, Skalidis, R., additional, Anche, R. M., additional, Angelakis, E., additional, Antoniadis, J., additional, Medhi, B. J., additional, Hovatta, T., additional, Kus, A., additional, Kylafis, N., additional, Mahabal, A., additional, Myserlis, I., additional, Paleologou, E., additional, Papadakis, I., additional, Pavlidou, V., additional, Papamastorakis, I., additional, Pearson, T. J., additional, Potter, S. B., additional, Ramaprakash, A. N., additional, Readhead, A. C. S., additional, Reig, P., additional, Słowikowska, A., additional, Tassis, K., additional, and Zensus, J. A., additional
Published: 2023
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29. The C-Band all-sky survey (C-BASS): New constraints on the integrated radio spectrum of M 31

Author: Harper, Stuart E, primary, Barr, Adam, additional, Dickinson, C, additional, Peel, M W, additional, Cepeda-Arroita, Roke, additional, Copley, C J, additional, Grumitt, R D P, additional, Leahy, J Patrick, additional, Jonas, J L, additional, Jones, Michael E, additional, Leech, J, additional, Pearson, T J, additional, Readhead, A C S, additional, and Taylor, Angela C, additional
Published: 2023
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30. (504) Correlation of Donor Electrocardiogram Abnormalities with Donor Echocardiograms and Angiograms: The Donor Heart Study

Author: Tapaskar, N., primary, Wayda, B., additional, Luikart, H., additional, Malinoski, D., additional, Groat, T., additional, Nguyen, J., additional, Nieto, J., additional, Wood, R.P., additional, Neidlinger, N., additional, Salehi, A., additional, Geraghty, P., additional, Nicely, B., additional, Jendrisak, M., additional, Belcher, J., additional, Pearson, T., additional, Zaroff, J., additional, and Khush, K., additional
Published: 2023
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31. Prediction of Donor Heart Acceptance for Transplant: Results From the Donor Heart Study

Author: Wayda, B., primary, Weng, Y., additional, Zhang, S., additional, Luikart, H., additional, Pearson, T., additional, Wood, R., additional, Nieto, J., additional, Nicely, B., additional, Geraghty, P., additional, Belcher, J., additional, Nguyen, J., additional, Zaroff, J., additional, and Khush, K., additional
Published: 2023
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32. Compact Symmetric Objects -- I Towards a Comprehensive Bona Fide Catalog

Author: Kiehlmann, S., Lister, M. L., Readhead, A. C. S., Liodakis, I., O'Neill, S., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., Taylor, G. B., Wilkinson, P. N., Kiehlmann, S., Lister, M. L., Readhead, A. C. S., Liodakis, I., O'Neill, S., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., Taylor, G. B., and Wilkinson, P. N.
Abstract: Compact Symmetric Objects (CSOs) are jetted Active Galactic Nuclei (AGN) with overall projected size <1 kpc. The classification was introduced to distinguish these objects from the majority of compact jetted-AGN in centimeter wavelength very long baseline interferometry observations, where the observed emission is relativistically boosted towards the observer. The original classification criteria for CSOs were: (i) evidence of emission on both sides of the center of activity, and (ii) overall size <1 kpc. However some relativistically boosted objects with jet axes close to the line of sight appear symmetric and have been mis-classified as CSOs, thereby undermining the CSO classification. This is because two essential CSO properties, pointed out in the original papers, have been neglected: (iii) low variability, and (iv) low apparent speeds along the jets. As a first step towards creating a comprehensive catalog of ``bona fide'' CSOs, we identify 79 bona fide CSOs, including 15 objects claimed as confirmed CSOs here for the first time, that match the CSO selection criteria. This sample of bona fide CSOs can be used for astrophysical studies of CSOs without contamination by mis-classified CSOs. We show that the fraction of CSOs in complete flux density limited AGN samples with S$_{\rm 5\,GHz}$ >700 mJy is between $(6.8\pm1.6)$% and $(8.5\pm1.8)$%., Comment: 28 pages, 9 figures, 3 tables, accepted for publication
Published: 2023

33. Compact Symmetric Objects -- II Confirmation of a Distinct Population of High-Luminosity Jetted Active Galaxies

Author: Kiehlmann, S., Readhead, A. C. S., O'Neill, S., Wilkinson, P. N., Lister, M. L., Liodakis, I., Bruzewski, S., Pavlidou, V., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., Taylor, G. B., Kiehlmann, S., Readhead, A. C. S., O'Neill, S., Wilkinson, P. N., Lister, M. L., Liodakis, I., Bruzewski, S., Pavlidou, V., Pearson, T. J., Sheldahl, E., Siemiginowska, A., Tassis, K., and Taylor, G. B.
Abstract: Compact Symmetric Objects (CSOs) are compact (<1 kpc), jetted Active Galactic Nuclei (AGN), whose jet axes are not aligned close to the line of sight, and whose observed emission is not predominantly relativistically boosted towards us. Two classes of CSOs have previously been identified: approximately one fifth are edge-dimmed and designated as CSO 1s, while the rest are edge brightened and designated as CSO 2s. This paper focuses almost exclusively on CSO 2s. Using complete samples of CSO 2s we present three independent lines of evidence, based on their relative numbers, redshift distributions, and size distributions, which show conclusively that the vast majority (> 99%) of CSO 2s do not evolve into larger-scale radio sources. These CSO 2s belong to a distinct population of jetted-AGN, which should be characterized as ``short-lived'' compared to the classes of larger jetted-AGN, as opposed to ``young''. We show that there is a sharp upper cutoff in the CSO 2 size distribution at $\approx 500$ pc. The distinct differences between most CSO 2s and other jetted-AGN provides a crucial new time domain window on the formation and evolution of relativistic jets in AGN and the supermassive black holes that drive them., Comment: 29 pages, 10 figures, 7 tables, accepted for publication
Published: 2023

34. Compact Symmetric Objects -- III Evolution of the High-Luminosity Branch and a Possible Connection with Tidal Disruption Events

Author: Readhead, A. C. S., Ravi, V., Blandford, R. D., Sullivan, A. G., Somalwar, J., Begelman, M. C., Birkinshaw, M., Liodakis, I., Lister, M. L., Pearson, T. J., Taylor, G. B., Wilkinson, P. N., Globus, N., Kiehlmann, S., Lawrence, C. R., Murphy, D., O'Neill, S., Pavlidou, V., Sheldahl, E., Siemiginowska, A., Tassis, K., Readhead, A. C. S., Ravi, V., Blandford, R. D., Sullivan, A. G., Somalwar, J., Begelman, M. C., Birkinshaw, M., Liodakis, I., Lister, M. L., Pearson, T. J., Taylor, G. B., Wilkinson, P. N., Globus, N., Kiehlmann, S., Lawrence, C. R., Murphy, D., O'Neill, S., Pavlidou, V., Sheldahl, E., Siemiginowska, A., and Tassis, K.
Abstract: We use a sample of 54 Compact Symmetric Objects (CSOs) to confirm that there are two unrelated CSO classes: an edge-dimmed, low-luminosity class (CSO~1), and an edge-brightened, high-luminosity class (CSO~2). Using blind tests, we show that CSO~2s consist of three sub-classes: CSO 2.0, having prominent hot-spots at the leading edges of narrow jets and/or narrow lobes; CSO~2.2, without prominent hot-spots, and with broad jets and/or lobes; and CSO~2.1, which exhibit mixed properties. Most CSO 2s do not evolve into larger jetted-AGN, but spend their whole life-cycle as CSOs of size $\lesssim$500 pc and age $\lesssim$5000 yr. The minimum energies needed to produce the radio luminosity and structure in CSO~2s range from $\sim~10^{-4}\,M_\odot{c}^2$ to $\sim7\,M_\odot{c}^2$. We show that the transient nature of most CSO~2s, and their birthrate, can be explained through ignition in the tidal disruption events of giant stars. We also consider possibilities of tapping the spin energy of the supermassive black hole, and tapping the energy of the accretion disk. Our results demonstrate that CSOs constitute a large family of AGN in which we have thus far studied only the brightest. More comprehensive CSO studies, with higher sensitivity, resolution, and dynamic range, will revolutionize our understanding of AGN and the central engines that power them., Comment: 44 pages, 16 figures, 9 tables, accepted for publication
Published: 2023

35. Starlight-polarization-based tomography of the magnetized ISM: PASIPHAE's line-of-sight inversion method

Author: Pelgrims, V., primary, Panopoulou, G. V., additional, Tassis, K., additional, Pavlidou, V., additional, Basyrov, A., additional, Blinov, D., additional, Gjerlow, E., additional, Kiehlmann, S., additional, Mandarakas, N., additional, Papadaki, A., additional, Skalidis, R., additional, Tsouros, A., additional, Anche, R. M., additional, Eriksen, H. K., additional, Ghosh, T., additional, Kypriotakis, J. A., additional, Maharana, S., additional, Ntormousi, E., additional, Pearson, T. J., additional, Potter, S. B., additional, Ramaprakash, A. N., additional, Readhead, A. C. S., additional, and Wehus, I. K., additional
Published: 2023
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36. Polarization and variability of compact sources measured in Planck time-ordered data

Author: Rocha, G., primary, Keskitalo, R., additional, Partridge, B., additional, Marscher, A., additional, O’Dea, C., additional, Pearson, T. J., additional, and Górski, K. M., additional
Published: 2023
Full Text: View/download PDF

37. Erratum to: Searches for long-lived charged particles in pp collisions at <math> <msqrt> <mi>s</mi> </msqrt> </math> $$ \sqrt{\textrm{s}} $$ = 7 and 8 TeV

Author: Chatrchyan, S., Khachatryan, V., Sirunyan, A., Tumasyan, A., Adam, W., Bergauer, T., Dragicevic, M., Erö, J., Fabjan, C., Friedl, M., Frühwirth, R., Ghete, V., Hörmann, N., Hrubec, J., Jeitler, M., Kiesenhofer, W., Knünz, V., Krammer, M., Krätschmer, I., Liko, D., Mikulec, I., Rabady, D., Rahbaran, B., Rohringer, C., Rohringer, H., Schöfbeck, R., Strauss, J., Taurok, A., Treberer-Treberspurg, W., Waltenberger, W., Wulz, C.E., Mossolov, V., Shumeiko, N., Suarez Gonzalez, J., Alderweireldt, S., Bansal, M., Bansal, S., Cornelis, T., Wolf, E., Janssen, X., Knutsson, A., Luyckx, S., Mucibello, L., Ochesanu, S., Roland, B., Rougny, R., Haevermaet, H., Mechelen, P., Remortel, N., Spilbeeck, A., Blekman, F., Blyweert, S., D’Hondt, J., Kalogeropoulos, A., Keaveney, J., Maes, M., Olbrechts, A., Tavernier, S., Doninck, W., Mulders, P., Onsem, G., Villella, I., Clerbaux, B., Lentdecker, G., Favart, L., Gay, A., Hreus, T., Léonard, A., Marage, P., Mohammadi, A., Perniè, L., Reis, T., Seva, T., Thomas, L., Vander Velde, C., Vanlaer, P., Wang, J., Adler, V., Beernaert, K., Benucci, L., Cimmino, A., Costantini, S., Dildick, S., Garcia, G., Klein, B., Lellouch, J., Marinov, A., Mccartin, J., Ocampo Rios, A., Ryckbosch, D., Sigamani, M., Strobbe, N., Thyssen, F., Tytgat, M., Walsh, S., Yazgan, E., Zaganidis, N., Basegmez, S., Beluffi, C., Bruno, G., Castello, R., Caudron, A., Ceard, L., Delaere, C., Pree, T., Favart, D., Forthomme, L., Giammanco, A., Hollar, J., Jez, P., Lemaitre, V., Liao, J., Militaru, O., Nuttens, C., Pagano, D., Pin, A., Piotrzkowski, K., Popov, A., Selvaggi, M., Vizan Garcia, J., Beliy, N., Caebergs, T., Daubie, E., Hammad, G., Alves, G., Correa Martins Junior, M., Martins, T., Pol, M., Souza, M., Aldá Júnior, W., Carvalho, W., Chinellato, J., Custódio, A., Costa, E., De Jesus Damiao, D., De Oliveira Martins, C., Fonseca De Souza, S., Malbouisson, H., Malek, M., Matos Figueiredo, D., Mundim, L., Nogima, H., Prado Da Silva, W., Santoro, A., Sznajder, A., Tonelli Manganote, E., Vilela Pereira, A., Bernardes, C., Dias, F., Fernandez Perez Tomei, T., Gregores, E., Lagana, C., Marinho, F., Mercadante, P., Novaes, S., Padula, Sandra, Genchev, V., Iaydjiev, P., Piperov, S., Rodozov, M., Sultanov, G., Vutova, M., Dimitrov, A., Hadjiiska, R., Kozhuharov, V., Litov, L., Pavlov, B., Petkov, P., Bian, J., Chen, G., Chen, H., Jiang, C., Liang, D., Liang, S., Meng, X., Tao, J., Wang, X., Wang, Z., Xiao, H., Xu, M., Asawatangtrakuldee, C., Ban, Y., Guo, Y., Li, W., Liu, S., Mao, Y., Qian, S., Teng, H., Wang, D., Zhang, L., Zou, W., Avila, C., Carrillo Montoya, C., Gomez, J., Gomez Moreno, B., Sanabria, J., Godinovic, N., Lelas, D., Plestina, R., Polic, D., Puljak, I., Antunovic, Z., Kovac, M., Brigljevic, V., Duric, S., Kadija, K., Luetic, J., Mekterovic, D., Morovic, S., Tikvica, L., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P., Finger, M., Assran, Y., Ellithi Kamel, A., Mahmoud, M., Mahrous, A., Radi, A., Kadastik, M., Müntel, M., Murumaa, M., Raidal, M., Rebane, L., Tiko, A., Eerola, P., Fedi, G., Voutilainen, M., Härkönen, J., Karimäki, V., Kinnunen, R., Kortelainen, M., Lampén, T., Lassila-Perini, K., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Peltola, T., Tuominen, E., Tuominiemi, J., Tuovinen, E., Wendland, L., Korpela, A., Tuuva, T., Besancon, M., Choudhury, S., Couderc, F., Dejardin, M., Denegri, D., Fabbro, B., Faure, J., Ferri, F., Ganjour, S., Givernaud, A., Gras, P., Hamel de Monchenault, G., Jarry, P., Locci, E., Malcles, J., Millischer, L., Nayak, A., Rander, J., Rosowsky, A., Titov, M., Baffioni, S., Beaudette, F., Benhabib, L., Bianchini, L., Bluj, M., Busson, P., Charlot, C., Daci, N., Dahms, T., Dalchenko, M., Dobrzynski, L., Florent, A., Granier de Cassagnac, R., Haguenauer, M., Miné, P., Mironov, C., Naranjo, I., Nguyen, M., Ochando, C., Paganini, P., Sabes, D., Salerno, R., Sirois, Y., Veelken, C., Zabi, A., Agram, J.L., Andrea, J., Bloch, D., Bodin, D., Brom, J.M., Chabert, E., Collard, C., Conte, E., Drouhin, F., Fontaine, J.C., Gelé, D., Goerlach, U., Goetzmann, C., Juillot, P., Bihan, A.C., Hove, P., Gadrat, S., Beauceron, S., Beaupere, N., Boudoul, G., Brochet, S., Chasserat, J., Chierici, R., Contardo, D., Depasse, P., Mamouni, H., Fay, J., Gascon, S., Gouzevitch, M., Ille, B., Kurca, T., Lethuillier, M., Mirabito, L., Perries, S., Sgandurra, L., Sordini, V., Tschudi, Y., Vander Donckt, M., Verdier, P., Viret, S., Tsamalaidze, Z., Autermann, C., Beranek, S., Calpas, B., Edelhoff, M., Feld, L., Heracleous, N., Hindrichs, O., Klein, K., Ostapchuk, A., Perieanu, A., Raupach, F., Sammet, J., Schael, S., Sprenger, D., Weber, H., Wittmer, B., Zhukov, V., Ata, M., Caudron, J., Dietz-Laursonn, E., Duchardt, D., Erdmann, M., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Klingebiel, D., Kreuzer, P., Merschmeyer, M., Meyer, A., Olschewski, M., Padeken, K., Papacz, P., Pieta, H., Reithler, H., Schmitz, S., Sonnenschein, L., Steggemann, J., Teyssier, D., Thüer, S., Weber, M., Cherepanov, V., Erdogan, Y., Flügge, G., Geenen, H., Geisler, M., Haj Ahmad, W., Hoehle, F., Kargoll, B., Kress, T., Kuessel, Y., Lingemann, J., Nowack, A., Nugent, I., Perchalla, L., Pooth, O., Stahl, A., Aldaya Martin, M., Asin, I., Bartosik, N., Behr, J., Behrenhoff, W., Behrens, U., Bergholz, M., Bethani, A., Borras, K., Burgmeier, A., Cakir, A., Calligaris, L., Campbell, A., Costanza, F., Diez Pardos, C., Dooling, S., Dorland, T., Eckerlin, G., Eckstein, D., Flucke, G., Geiser, A., Glushkov, I., Gunnellini, P., Habib, S., Hauk, J., Hellwig, G., Jung, H., Kasemann, M., Katsas, P., Kleinwort, C., Kluge, H., Krämer, M., Krücker, D., Kuznetsova, E., Lange, W., Leonard, J., Lipka, K., Lohmann, W., Lutz, B., Mankel, R., Marfin, I., Melzer-Pellmann, I.A., Mnich, J., Mussgiller, A., Naumann-Emme, S., Novgorodova, O., Nowak, F., Olzem, J., Perrey, H., Petrukhin, A., Pitzl, D., Placakyte, R., Raspereza, A., Ribeiro Cipriano, P., Riedl, C., Ron, E., Sahin, M., Salfeld-Nebgen, J., Schmidt, R., Schoerner-Sadenius, T., Sen, N., Stein, M., Walsh, R., Wissing, C., Blobel, V., Enderle, H., Erfle, J., Gebbert, U., Görner, M., Gosselink, M., Haller, J., Heine, K., Höing, R., Kaussen, G., Kirschenmann, H., Klanner, R., Kogler, R., Lange, J., Marchesini, I., Peiffer, T., Pietsch, N., Rathjens, D., Sander, C., Schettler, H., Schleper, P., Schlieckau, E., Schmidt, A., Schröder, M., Schum, T., Seidel, M., Sibille, J., Sola, V., Stadie, H., Steinbrück, G., Thomsen, J., Troendle, D., Vanelderen, L., Barth, C., Baus, C., Berger, J., Böser, C., Chwalek, T., Boer, W., Descroix, A., Dierlamm, A., Feindt, M., Guthoff, M., Hackstein, C., Hartmann, F., Hauth, T., Heinrich, M., Held, H., Hoffmann, K., Husemann, U., Katkov, I., Komaragiri, J., Kornmayer, A., Lobelle Pardo, P., Martschei, D., Mueller, S., Müller, Th., Niegel, M., Nürnberg, A., Oberst, O., Ott, J., Quast, G., Rabbertz, K., Ratnikov, F., Röcker, S., Schilling, F.P., Schott, G., Simonis, H., Stober, F., Ulrich, R., Wagner-Kuhr, J., Wayand, S., Weiler, T., Zeise, M., Anagnostou, G., Daskalakis, G., Geralis, T., Kesisoglou, S., Kyriakis, A., Loukas, D., Markou, A., Markou, C., Ntomari, E., Gouskos, L., Mertzimekis, T., Panagiotou, A., Saoulidou, N., Stiliaris, E., Aslanoglou, X., Evangelou, I., Flouris, G., Foudas, C., Kokkas, P., Manthos, N., Papadopoulos, I., Paradas, E., Bencze, G., Hajdu, C., Hidas, P., Horvath, D., Radics, B., Sikler, F., Veszpremi, V., Vesztergombi, G., Zsigmond, A., Beni, N., Czellar, S., Molnar, J., Palinkas, J., Szillasi, Z., Karancsi, J., Raics, P., Trocsanyi, Z., Ujvari, B., Beri, S., Bhatnagar, V., Dhingra, N., Gupta, R., Kaur, M., Mehta, M., Mittal, M., Nishu, N., Saini, L., Sharma, A., Singh, J., Kumar, Ashok, Kumar, Arun, Ahuja, S., Bhardwaj, A., Choudhary, B., Malhotra, S., Naimuddin, M., Ranjan, K., Saxena, P., Sharma, V., Shivpuri, R., Banerjee, S., Bhattacharya, S., Chatterjee, K., Dutta, S., Gomber, B., Jain, Sa., Jain, Sh., Khurana, R., Modak, A., Mukherjee, S., Roy, D., Sarkar, S., Sharan, M., Abdulsalam, A., Dutta, D., Kailas, S., Kumar, V., Mohanty, A., Pant, L., Shukla, P., Topkar, A., Aziz, T., Chatterjee, R., Ganguly, S., Ghosh, S., Guchait, M., Gurtu, A., Kole, G., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Mohanty, G., Parida, B., Sudhakar, K., Wickramage, N., Dugad, S., Arfaei, H., Bakhshiansohi, H., Etesami, S., Fahim, A., Hesari, H., Jafari, A., Khakzad, M., Mohammadi Najafabadi, M., Paktinat Mehdiabadi, S., Safarzadeh, B., Zeinali, M., Grunewald, M., Abbrescia, M., Barbone, L., Calabria, C., Chhibra, S., Colaleo, A., Creanza, D., Filippis, N., Palma, M., Fiore, L., Iaselli, G., Maggi, G., Maggi, M., Marangelli, B., My, S., Nuzzo, S., Pacifico, N., Pompili, A., Pugliese, G., Selvaggi, G., Silvestris, L., Singh, G., Venditti, R., Verwilligen, P., Zito, G., Abbiendi, G., Benvenuti, A., Bonacorsi, D., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F., Cuffiani, M., Dallavalle, G., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Meneghelli, M., Montanari, A., Navarria, F., Odorici, F., Perrotta, A., Primavera, F., Rossi, A., Rovelli, T., Siroli, G., Tosi, N., Travaglini, R., Albergo, S., Chiorboli, M., Costa, S., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Frosali, S., Gallo, E., Gonzi, S., Gori, V., Lenzi, P., Meschini, M., Paoletti, S., Sguazzoni, G., Tropiano, A., Benussi, L., Bianco, S., Piccolo, D., Fabbricatore, P., Musenich, R., Tosi, S., Benaglia, A., Guio, F., Matteo, L., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Lucchini, M., Malvezzi, S., Manzoni, R., Martelli, A., Menasce, D., Moroni, L., Paganoni, M., Pedrini, D., Ragazzi, S., Redaelli, N., Tabarelli de Fatis, T., Buontempo, S., Cavallo, N., Cosa, A., Fabozzi, F., Iorio, A., Lista, L., Meola, S., Merola, M., Paolucci, P., Azzi, P., Bacchetta, N., Bisello, D., Branca, A., Carlin, R., Checchia, P., Dorigo, T., Dosselli, U., Galanti, M., Gasparini, F., Gasparini, U., Giubilato, P., Gozzelino, A., Gulmini, M., Kanishchev, K., Lacaprara, S., Lazzizzera, I., Margoni, M., Maron, G., Meneguzzo, A., Pazzini, J., Pozzobon, N., Ronchese, P., Simonetto, F., Torassa, E., Tosi, M., Vanini, S., Zotto, P., Zucchetta, A., Zumerle, G., Gabusi, M., Ratti, S., Riccardi, C., Vitulo, P., Biasini, M., Bilei, G., Fanò, L., Lariccia, P., Mantovani, G., Menichelli, M., Nappi, A., Romeo, F., Saha, A., Santocchia, A., Spiezia, A., Androsov, K., Azzurri, P., Bagliesi, G., Boccali, T., Broccolo, G., Castaldi, R., D’Agnolo, R., Dell’Orso, R., Fiori, F., Foà, L., Giassi, A., Kraan, A., Ligabue, F., Lomtadze, T., Martini, L., Messineo, A., Palla, F., Rizzi, A., Serban, A., Spagnolo, P., Squillacioti, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P., Vernieri, C., Barone, L., Cavallari, F., Re, D., Diemoz, M., Grassi, M., Longo, E., Margaroli, F., Meridiani, P., Micheli, F., Nourbakhsh, S., Organtini, G., Paramatti, R., Rahatlou, S., Soffi, L., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Biino, C., Cartiglia, N., Casasso, S., Costa, M., Demaria, N., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Musich, M., Obertino, M., Ortona, G., Pastrone, N., Pelliccioni, M., Potenza, A., Romero, A., Ruspa, M., Sacchi, R., Solano, A., Staiano, A., Tamponi, U., Belforte, S., Candelise, V., Casarsa, M., Cossutti, F., Della Ricca, G., Gobbo, B., Licata, C., Marone, M., Montanino, D., Penzo, A., Schizzi, A., Zanetti, A., Kim, T., Nam, S., Chang, S., Kim, D., Kim, G., Kim, J., Kong, D., Oh, Y., Park, H., Son, D., Kim, Zero, Song, S., Choi, S., Gyun, D., Hong, B., Jo, M., Kim, H., Lee, K., Park, S., Roh, Y., Choi, M., Park, C., Park, I., Ryu, G., Choi, Y., Goh, J., Kim, M., Kwon, E., Lee, B., Lee, J., Lee, S., Seo, H., Yu, I., Grigelionis, I., Juodagalvis, A., Castilla-Valdez, H., Cruz-Burelo, E., Heredia-de La Cruz, I., Lopez-Fernandez, R., Martínez-Ortega, J., Sanchez-Hernandez, A., Villasenor-Cendejas, L., Carrillo Moreno, S., Vazquez Valencia, F., Salazar Ibarguen, H., Casimiro Linares, E., Morelos Pineda, A., Reyes-Santos, M., Krofcheck, D., Bell, A., Butler, P., Doesburg, R., Reucroft, S., Silverwood, H., Ahmad, M., Asghar, M., Butt, J., Hoorani, H., Khalid, S., Khan, W., Khurshid, T., Qazi, S., Shah, M., Shoaib, M., Bialkowska, H., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Romanowska-Rybinska, K., Szleper, M., Wrochna, G., Zalewski, P., Brona, G., Bunkowski, K., Cwiok, M., Dominik, W., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Wolszczak, W., Almeida, N., Bargassa, P., David, A., Faccioli, P., Ferreira Parracho, P., Gallinaro, M., Rodrigues Antunes, J., Seixas, J., Varela, J., Vischia, P., Bunin, P., Gavrilenko, M., Golutvin, I., Gorbunov, I., Kamenev, A., Karjavin, V., Konoplyanikov, V., Kozlov, G., Lanev, A., 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Tourtchanovitch, L., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, P., Ekmedzic, M., Krpic, D., Milosevic, J., Aguilar-Benitez, M., Alcaraz Maestre, J., Battilana, C., Calvo, E., Cerrada, M., Chamizo Llatas, M., Colino, N., Cruz, B., Delgado Peris, A., Domínguez Vázquez, D., Fernandez Bedoya, C., Fernández Ramos, J., Ferrando, A., Flix, J., Fouz, M., Garcia-Abia, P., Gonzalez Lopez, O., Goy Lopez, S., Hernandez, J., Josa, M., Merino, G., Navarro De Martino, E., Puerta Pelayo, J., Quintario Olmeda, A., Redondo, I., Romero, L., Santaolalla, J., Soares, M., Willmott, C., Albajar, C., Trocóniz, J., Brun, H., Cuevas, J., Fernandez Menendez, J., Folgueras, S., Gonzalez Caballero, I., Lloret Iglesias, L., Piedra Gomez, J., Brochero Cifuentes, J., Cabrillo, I., Calderon, A., Chuang, S., Duarte Campderros, J., Fernandez, M., Gomez, G., Gonzalez Sanchez, J., Graziano, A., Jorda, C., Lopez Virto, A., Marco, J., Marco, R., Martinez Rivero, C., Matorras, F., Munoz Sanchez, F., Rodrigo, T., Rodríguez-Marrero, A., Ruiz-Jimeno, A., Scodellaro, L., Vila, I., Vilar Cortabitarte, R., Abbaneo, D., Auffray, E., Auzinger, G., Bachtis, M., Baillon, P., Ball, A., Barney, D., Bendavid, J., Benitez, J., Bernet, C., Bianchi, G., Bloch, P., Bocci, A., Bonato, A., Bondu, O., Botta, C., Breuker, H., Camporesi, T., Cerminara, G., Christiansen, T., Coarasa Perez, J., Colafranceschi, S., d’Enterria, D., Dabrowski, A., Roeck, A., Visscher, S., Guida, S., Dobson, M., Dupont-Sagorin, N., Elliott-Peisert, A., Eugster, J., Funk, W., Georgiou, G., Giffels, M., Gigi, D., Gill, K., Giordano, D., Girone, M., Giunta, M., Glege, F., Gomez-Reino Garrido, R., Gowdy, S., Guida, R., Hammer, J., Hansen, M., Harris, P., Hartl, C., Hinzmann, A., Innocente, V., Janot, P., Karavakis, E., Kousouris, K., Krajczar, K., Lecoq, P., Lee, Y.J., Lourenço, C., Magini, N., Malberti, M., Malgeri, L., Mannelli, M., Masetti, L., Meijers, F., Mersi, S., Meschi, E., Moser, R., Mulders, M., Musella, P., Nesvold, E., 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Magnan, A.M., Marrouche, J., Mathias, B., Nandi, R., Nash, J., Nikitenko, A., Pela, J., Pesaresi, M., Petridis, K., Pioppi, M., Raymond, D., Rogerson, S., Rose, A., Seez, C., Sharp, P., Sparrow, A., Tapper, A., Vazquez Acosta, M., Virdee, T., Wakefield, S., Wardle, N., Whyntie, T., Chadwick, M., Cole, J., Hobson, P., Khan, A., Kyberd, P., Leggat, D., Leslie, D., Martin, W., Reid, I., Symonds, P., Teodorescu, L., Turner, M., Dittmann, J., Hatakeyama, K., Kasmi, A., Liu, H., Scarborough, T., Charaf, O., Cooper, S., Henderson, C., Rumerio, P., Avetisyan, A., Bose, T., Fantasia, C., Heister, A., Lawson, P., Lazic, D., Rohlf, J., Sperka, D., St. John, J., Sulak, L., Alimena, J., Christopher, G., Cutts, D., Demiragli, Z., Ferapontov, A., Garabedian, A., Heintz, U., Kukartsev, G., Laird, E., Landsberg, G., Luk, M., Narain, M., Segala, M., Sinthuprasith, T., Speer, T., Breedon, R., Breto, G., Calderon De La Barca Sanchez, M., Chauhan, S., Chertok, M., Conway, J., Conway, R., Cox, P., Erbacher, R., Gardner, M., Houtz, R., Ko, W., Kopecky, A., Lander, R., Mall, O., Miceli, T., Nelson, R., Pellett, D., Ricci-Tam, F., Rutherford, B., Searle, M., Smith, J., Squires, M., Tripathi, M., Wilbur, S., Yohay, R., Cline, D., Cousins, R., Erhan, S., Everaerts, P., Farrell, C., Felcini, M., Hauser, J., Ignatenko, M., Jarvis, C., Rakness, G., Schlein, P., Takasugi, E., Traczyk, P., Valuev, V., Babb, J., Clare, R., Dinardo, M., Ellison, J., Gary, J., Hanson, G., Long, O., Luthra, A., Nguyen, H., Paramesvaran, S., Sturdy, J., Sumowidagdo, S., Wilken, R., Wimpenny, S., Andrews, W., Branson, J., Cerati, G., Cittolin, S., Evans, D., Holzner, A., Kelley, R., Lebourgeois, M., Letts, J., Macneill, I., Mangano, B., Padhi, S., Palmer, C., Petrucciani, G., Pieri, M., Sani, M., Simon, S., Sudano, E., Tadel, M., Tu, Y., Vartak, A., Wasserbaech, S., Würthwein, F., Yagil, A., Yoo, J., Barge, D., Bellan, R., Campagnari, C., D’Alfonso, M., Danielson, T., Flowers, K., Geffert, P., George, C., Golf, F., Incandela, J., Justus, C., Kalavase, P., Kovalskyi, D., Krutelyov, V., Lowette, S., Magaña Villalba, R., Mccoll, N., Pavlunin, V., Ribnik, J., Richman, J., Rossin, R., Stuart, D., To, W., West, C., Apresyan, A., Bornheim, A., Bunn, J., Chen, Y., Marco, E., Duarte, J., Kcira, D., Ma, Y., Mott, A., Newman, H., Rogan, C., Spiropulu, M., Timciuc, V., Veverka, J., Wilkinson, R., Xie, S., Yang, Y., Zhu, R., Azzolini, V., Calamba, A., Carroll, R., Ferguson, T., Iiyama, Y., Jang, D., Liu, Y., Paulini, M., Russ, J., Vogel, H., Vorobiev, I., Cumalat, J., Drell, B., Ford, W., Gaz, A., Luiggi Lopez, E., Nauenberg, U., Stenson, K., Ulmer, K., Wagner, S., Alexander, J., Chatterjee, A., Eggert, N., Gibbons, L., Hopkins, W., Khukhunaishvili, A., Kreis, B., Mirman, N., Nicolas Kaufman, G., Patterson, J., Ryd, A., Salvati, E., Sun, W., Teo, W., Thom, J., Thompson, J., Tucker, J., Weng, Y., Winstrom, L., Wittich, P., Winn, D., Abdullin, S., Albrow, M., Anderson, J., Apollinari, G., Bauerdick, L., Beretvas, A., Berryhill, J., Bhat, P., Burkett, K., Butler, J., Chetluru, V., Cheung, H., Chlebana, F., Cihangir, S., Elvira, V., Fisk, I., Freeman, J., Gao, Y., Gottschalk, E., Gray, L., Green, D., Gutsche, O., Hare, D., Harris, R., Hirschauer, J., Hooberman, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kunori, S., Kwan, S., Leonidopoulos, C., Linacre, J., Lincoln, D., Lipton, R., Lykken, J., Maeshima, K., Marraffino, J., Martinez Outschoorn, V., Maruyama, S., Mason, D., McBride, P., Mishra, K., Mrenna, S., Musienko, Y., Newman-Holmes, C., O’Dell, V., Prokofyev, O., Ratnikova, N., Sexton-Kennedy, E., Sharma, S., Spalding, W., Spiegel, L., Taylor, L., Tkaczyk, S., Tran, N., Uplegger, L., Vaandering, E., Vidal, R., Whitmore, J., Wu, W., Yang, F., Yun, J., Acosta, D., Avery, P., Bourilkov, D., Chen, M., Cheng, T., Das, S., Gruttola, M., Giovanni, G., Dobur, D., Drozdetskiy, A., Field, R., Fisher, M., Fu, Y., Furic, I., Hugon, J., Kim, B., Konigsberg, J., Korytov, A., Kropivnitskaya, A., Kypreos, T., Low, J., Matchev, K., Milenovic, P., Mitselmakher, G., Muniz, L., Remington, R., Rinkevicius, A., Skhirtladze, N., Snowball, M., Yelton, J., Zakaria, M., Gaultney, V., Hewamanage, S., Lebolo, L., Linn, S., Markowitz, P., Martinez, G., Rodriguez, J., Adams, T., Askew, A., Bochenek, J., Chen, J., Diamond, B., Gleyzer, S., Haas, J., Hagopian, S., Hagopian, V., Johnson, K., Prosper, H., Veeraraghavan, V., Weinberg, M., Baarmand, M., Dorney, B., Hohlmann, M., Kalakhety, H., Yumiceva, F., Adams, M., Apanasevich, L., Bazterra, V., Betts, R., Bucinskaite, I., Callner, J., Cavanaugh, R., Evdokimov, O., Gauthier, L., Gerber, C., Hofman, D., Khalatyan, S., Kurt, P., Lacroix, F., Moon, D., O’Brien, C., Silkworth, C., Strom, D., Turner, P., Varelas, N., Akgun, U., Albayrak, E., Bilki, B., Clarida, W., Dilsiz, K., Duru, F., Griffiths, S., Merlo, J.P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Newsom, C., Ogul, H., Onel, Y., Ozok, F., Sen, S., Tan, P., Tiras, E., Wetzel, J., Yetkin, T., Yi, K., Barnett, B., Blumenfeld, B., Bolognesi, S., Fehling, D., Giurgiu, G., Gritsan, A., Guo, Z., Hu, G., Maksimovic, P., Swartz, M., Whitbeck, A., Baringer, P., Bean, A., Benelli, G., Kenny, R., Murray, M., Noonan, D., Sanders, S., Stringer, R., Wood, J., Barfuss, A., Chakaberia, I., Ivanov, A., Khalil, S., Makouski, M., Maravin, Y., Shrestha, S., Svintradze, I., Gronberg, J., Lange, D., Rebassoo, F., Wright, D., Baden, A., Calvert, B., Eno, S., Hadley, N., Kellogg, R., Kolberg, T., Marionneau, M., Mignerey, A., Pedro, K., Peterman, A., Skuja, A., Temple, J., Tonjes, M., Tonwar, S., Apyan, A., Bauer, G., Busza, W., Butz, E., Cali, I., Chan, M., Dutta, V., Gomez Ceballos, G., Goncharov, M., Kim, Y., Klute, M., Lai, Y., Levin, A., Luckey, P., Ma, T., Nahn, S., Paus, C., Ralph, D., Roland, C., Roland, G., Stephans, G., Stöckli, F., Sumorok, K., Sung, K., Velicanu, D., Wolf, R., Wyslouch, B., Yang, M., Yilmaz, Y., Yoon, A., Zanetti, M., Zhukova, V., Dahmes, B., Benedetti, A., Franzoni, G., Gude, A., Haupt, J., Kao, S., Klapoetke, K., Kubota, Y., Mans, J., Pastika, N., Rusack, R., Sasseville, M., Singovsky, A., Tambe, N., Turkewitz, J., Cremaldi, L., Kroeger, R., Perera, L., Rahmat, R., Sanders, D., Summers, D., Avdeeva, E., Bloom, K., Bose, S., Claes, D., Dominguez, A., Eads, M., Gonzalez Suarez, R., Keller, J., Kravchenko, I., Lazo-Flores, J., Malik, S., Meier, F., Snow, G., Dolen, J., Godshalk, A., Iashvili, I., Jain, S., Kharchilava, A., Kumar, A., Rappoccio, S., Wan, Z., Alverson, G., Barberis, E., Baumgartel, D., Chasco, M., Haley, J., Massironi, A., Nash, D., Orimoto, T., Trocino, D., Wood, D., Zhang, J., Anastassov, A., Hahn, K., Kubik, A., Lusito, L., Mucia, N., Odell, N., Pollack, B., Pozdnyakov, A., Schmitt, M., Stoynev, S., Velasco, M., Won, S., Berry, D., Brinkerhoff, A., Chan, K., Hildreth, M., Jessop, C., Karmgard, D., Kolb, J., Lannon, K., Luo, W., Lynch, S., Marinelli, N., Morse, D., Pearson, T., Planer, M., Ruchti, R., Slaunwhite, J., Valls, N., Wayne, M., Wolf, M., Antonelli, L., Bylsma, B., Durkin, L., Hill, C., Hughes, R., Kotov, K., Ling, T., Puigh, D., Rodenburg, M., Smith, G., Vuosalo, C., Williams, G., Winer, B., Wolfe, H., Berry, E., Elmer, P., Halyo, V., Hebda, P., Hegeman, J., Hunt, A., Jindal, P., Koay, S., Lopes Pegna, D., Lujan, P., Marlow, D., Medvedeva, T., Mooney, M., Olsen, J., Piroué, P., Quan, X., Raval, A., Saka, H., Stickland, D., Tully, C., Werner, J., Zenz, S., Zuranski, A., Brownson, E., Lopez, A., Mendez, H., Ramirez Vargas, J., Alagoz, E., Benedetti, D., Bolla, G., Bortoletto, D., Mattia, M., Everett, A., Hu, Z., Jones, M., Jung, K., Koybasi, O., Kress, M., Leonardo, N., Maroussov, V., Merkel, P., Miller, D., Neumeister, N., Shipsey, I., Silvers, D., Svyatkovskiy, A., Vidal Marono, M., Wang, F., Xu, L., Yoo, H., Zablocki, J., Zheng, Y., Guragain, S., Parashar, N., Adair, A., Akgun, B., Ecklund, K., Geurts, F., Padley, B., Redjimi, R., Roberts, J., Zabel, J., Betchart, B., Bodek, A., Covarelli, R., Barbaro, P., Demina, R., Eshaq, Y., Ferbel, T., Garcia-Bellido, A., Goldenzweig, P., Han, J., Harel, A., Miner, D., Petrillo, G., Vishnevskiy, D., Zielinski, M., Bhatti, A., Ciesielski, R., Demortier, L., Goulianos, K., Lungu, G., Mesropian, C., Arora, S., Barker, A., Chou, J., Contreras-Campana, C., Contreras-Campana, E., Duggan, D., Ferencek, D., Gershtein, Y., Gray, R., Halkiadakis, E., Hidas, D., Lath, A., Panwalkar, S., Park, M., Patel, R., Rekovic, V., Robles, J., Rose, K., Salur, S., Schnetzer, S., Seitz, C., Somalwar, S., Stone, R., Thomas, S., Walker, M., Cerizza, G., Hollingsworth, M., Spanier, S., Yang, Z., York, A., Eusebi, R., Flanagan, W., Gilmore, J., Kamon, T., Khotilovich, V., Montalvo, R., Osipenkov, I., Pakhotin, Y., Perloff, A., Roe, J., Safonov, A., Sakuma, T., Suarez, I., Tatarinov, A., Toback, D., Akchurin, N., Damgov, J., Dragoiu, C., Dudero, P., Jeong, C., Kovitanggoon, K., Libeiro, T., Volobouev, I., Appelt, E., Delannoy, A., Greene, S., Gurrola, A., Johns, W., Maguire, C., Melo, A., Sharma, M., Sheldon, P., Snook, B., Tuo, S., Velkovska, J., Arenton, M., Boutle, S., Cox, B., Francis, B., Goodell, J., Hirosky, R., Ledovskoy, A., Lin, C., Neu, C., Gollapinni, S., Harr, R., Karchin, P., Kottachchi Kankanamge Don, C., Lamichhane, P., Sakharov, A., Anderson, M., Belknap, D., Borrello, L., Carlsmith, D., Cepeda, M., Dasu, S., Friis, E., Grogg, K., Grothe, M., Hall-Wilton, R., Herndon, M., Hervé, A., Kaadze, K., Klabbers, P., Klukas, J., Lanaro, A., Lazaridis, C., Loveless, R., Mohapatra, A., Mozer, M., Ojalvo, I., Pierro, G., Ross, I., Savin, A., Smith, W., and Swanson, J.
Subjects: Nuclear and High Energy Physics
Published: 2022

38. The hunt for extraterrestrial high-energy neutrino counterparts

Author: Liodakis, I., primary, Hovatta, T., additional, Pavlidou, V., additional, Readhead, A.C.S., additional, Blandford, R. D., additional, Kiehlmann, S., additional, Lindfors, E., additional, Max-Moerbeck, W., additional, Pearson, T. J., additional, and Petropoulou, M., additional
Published: 2022
Full Text: View/download PDF

39. Prediction for ( p,n ) charge-exchange reactions with uncertainty quantification

Author: Whitehead, T. R., primary, Poxon-Pearson, T., additional, Nunes, F. M., additional, and Potel, G., additional
Published: 2022
Full Text: View/download PDF

40. The C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky

Author: Harper, S E, primary, Dickinson, C, additional, Barr, A, additional, Cepeda-Arroita, R, additional, Grumitt, R D P, additional, Heilgendorff, H M, additional, Jew, L, additional, Jonas, J L, additional, Jones, M E, additional, Leahy, J P, additional, Leech, J, additional, Pearson, T J, additional, Peel, M W, additional, Readhead, A C S, additional, and Taylor, A C, additional
Published: 2022
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41. Incidence, Predictors, and Reversibility of Left Ventricular Dysfunction After Brain Death: The Donor Heart Study

Author: Khush, K.K., primary, Malinoski, D., additional, Luikart, H., additional, Groat, T., additional, Nguyen, J., additional, Nieto, J., additional, Neidlinger, N., additional, Salehi, A., additional, Geraghty, P., additional, Rudich, S., additional, Nicely, B., additional, Jendrisak, M., additional, Belcher, J., additional, Pearson, T., additional, Wood, R., additional, Zhang, S., additional, Weng, Y., additional, Wayda, B., additional, and Zaroff, J., additional
Published: 2022
Full Text: View/download PDF

42. Investigating the Blazar TXS 0506+056 through Sharp Multiwavelength Eyes During 2017–2019

Author: Acciari, V. A., primary, Aniello, T., additional, Ansoldi, S., additional, Antonelli, L. A., additional, Arbet Engels, A., additional, Artero, M., additional, Asano, K., additional, Baack, D., additional, Babić, A., additional, Baquero, A., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Batković, I., additional, Becerra González, J., additional, Bednarek, W., additional, Bernardini, E., additional, Bernardos, M., additional, Berti, A., additional, Besenrieder, J., additional, Bhattacharyya, W., additional, Bigongiari, C., additional, Biland, A., additional, Blanch, O., additional, Bökenkamp, H., additional, Bonnoli, G., additional, Bošnjak, Ž., additional, Busetto, G., additional, Carosi, R., additional, Ceribella, G., additional, Cerruti, M., additional, Chai, Y., additional, Chilingarian, A., additional, Cikota, S., additional, Colombo, E., additional, Contreras, J. L., additional, Cortina, J., additional, Covino, S., additional, D’Amico, G., additional, D’Elia, V., additional, Vela, P. Da, additional, Dazzi, F., additional, De Angelis, A., additional, De Lotto, B., additional, Del Popolo, A., additional, Delfino, M., additional, Delgado, J., additional, Mendez, C. Delgado, additional, Depaoli, D., additional, Di Pierro, F., additional, Di Venere, L., additional, Do Souto Espiñeira, E., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Elsaesser, D., additional, Fallah Ramazani, V., additional, Fariña, L., additional, Fattorini, A., additional, Font, L., additional, Fruck, C., additional, Fukami, S., additional, Fukazawa, Y., additional, García López, R. J., additional, Garczarczyk, M., additional, Gasparyan, S., additional, Gaug, M., additional, Giglietto, N., additional, Giordano, F., additional, Gliwny, P., additional, Godinović, N., additional, Green, J. G., additional, Green, D., additional, Hadasch, D., additional, Hahn, A., additional, Hassan, T., additional, Heckmann, L., additional, Herrera, J., additional, Hoang, J., additional, Hrupec, D., additional, Hütten, M., additional, Inada, T., additional, Iotov, R., additional, Ishio, K., additional, Iwamura, Y., additional, Jiménez Martínez, I., additional, Jormanainen, J., additional, Jouvin, L., additional, Kerszberg, D., additional, Kobayashi, Y., additional, Kubo, H., additional, Kushida, J., additional, Lamastra, A., additional, Lelas, D., additional, Leone, F., additional, Lindfors, E., additional, Linhoff, L., additional, Lombardi, S., additional, Longo, F., additional, López-Coto, R., additional, López-Moya, M., additional, López-Oramas, A., additional, Loporchio, S., additional, Machado de Oliveira Fraga, B., additional, Maggio, C., additional, Majumdar, P., additional, Makariev, M., additional, Mallamaci, M., additional, Maneva, G., additional, Manganaro, M., additional, Mannheim, K., additional, Mariotti, M., additional, Martínez, M., additional, Mas Aguilar, A., additional, Mazin, D., additional, Menchiari, S., additional, Mender, S., additional, Mićanović, S., additional, Miceli, D., additional, Miener, T., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Molina, E., additional, Moralejo, A., additional, Morcuende, D., additional, Moreno, V., additional, Moretti, E., additional, Nakamori, T., additional, Nava, L., additional, Neustroev, V., additional, Nievas Rosillo, M., additional, Nigro, C., additional, Nilsson, K., additional, Nishijima, K., additional, Noda, K., additional, Nozaki, S., additional, Ohtani, Y., additional, Oka, T., additional, Otero-Santos, J., additional, Paiano, S., additional, Palatiello, M., additional, Paneque, D., additional, Paoletti, R., additional, Paredes, J. M., additional, Pavletić, L., additional, Peñil, P., additional, Persic, M., additional, Pihet, M., additional, Prada Moroni, P. G., additional, Prandini, E., additional, Priyadarshi, C., additional, Puljak, I., additional, Rhode, W., additional, Ribó, M., additional, Rico, J., additional, Righi, C., additional, Rugliancich, A., additional, Sahakyan, N., additional, Saito, T., additional, Sakurai, S., additional, Satalecka, K., additional, Saturni, F. G., additional, Schleicher, B., additional, Schmidt, K., additional, Schmuckermaier, F., additional, Schweizer, T., additional, Sitarek, J., additional, Šnidarić, I., additional, Sobczynska, D., additional, Spolon, A., additional, Stamerra, A., additional, Strišković, J., additional, Strom, D., additional, Strzys, M., additional, Suda, Y., additional, Surić, T., additional, Takahashi, M., additional, Takeishi, R., additional, Tavecchio, F., additional, Temnikov, P., additional, Terzić, T., additional, Teshima, M., additional, Tosti, L., additional, Truzzi, S., additional, Tutone, A., additional, Ubach, S., additional, van Scherpenberg, J., additional, Vanzo, G., additional, Vazquez Acosta, M., additional, Ventura, S., additional, Verguilov, V., additional, Viale, I., additional, Vigorito, C. F., additional, Vitale, V., additional, Vovk, I., additional, Will, M., additional, Wunderlich, C., additional, Yamamoto, T., additional, Zarić, D., additional, Hodges, M., additional, Hovatta, T., additional, Kiehlmann, S., additional, Liodakis, I., additional, Max-Moerbeck, W., additional, Pearson, T. J., additional, Readhead, A. C. S., additional, Reeves, R. A., additional, Lähteenmäki, A., additional, Tornikoski, M., additional, Tammi, J., additional, D’Ammando, F., additional, and Marchini, A., additional
Published: 2022
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43. New Tests of Milli-lensing in the Blazar PKS 1413 + 135

Author: Peirson, A. L., primary, Liodakis, I., additional, Readhead, A. C. S, additional, Lister, M. L., additional, Perlman, E. S., additional, Aller, M. F., additional, Blandford, R. D., additional, Grainge, K. J. B., additional, Green, D. A., additional, Gurwell, M. A., additional, Hodges, M. W., additional, Hovatta, T., additional, Kiehlmann, S., additional, Lähteenmäki, A., additional, Max-Moerbeck, W., additional, Mcaloone, T., additional, O’Neill, S., additional, Pavlidou, V., additional, Pearson, T. J., additional, Ravi, V., additional, Reeves, R. A., additional, Scott, P. F., additional, Taylor, G. B., additional, Titterington, D. J., additional, Tornikoski, M., additional, Vedantham, H. K., additional, Wilkinson, P. N., additional, Williams, D. T., additional, and Zensus, J. A., additional
Published: 2022
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44. Erratum to: Searches for long-lived charged particles in pp collisions at $ \sqrt{\textrm{s}} $= 7 and 8 TeV

Author: CMS Collaboration, Chatrchyan, S., Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Bergauer, T., Dragicevic, M., Erö, J., Fabjan, C., Friedl, M., Frühwirth, R., Ghete, V. M., Hörmann, N., Hrubec, J., Jeitler, M., Kiesenhofer, W., Knünz, V., Krammer, M., Krätschmer, I., Liko, D., Mikulec, I., Rabady, D., Rahbaran, B., Rohringer, C., Rohringer, H., Schöfbeck, R., Strauss, J., Taurok, A., Treberer-Treberspurg, W., Waltenberger, W., Wulz, C.-E., Mossolov, V., Shumeiko, N., Suarez Gonzalez, J., Alderweireldt, S., Bansal, M., Bansal, S., Cornelis, T., De Wolf, E. A., Janssen, X., Knutsson, A., Luyckx, S., Mucibello, L., Ochesanu, S., Roland, B., Rougny, R., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Van Spilbeeck, A., Blekman, F., Blyweert, S., D’Hondt, J., Kalogeropoulos, A., Keaveney, J., Maes, M., Olbrechts, A., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Onsem, G. P., Villella, I., Clerbaux, B., De Lentdecker, G., Favart, L., Gay, A. P. R., Hreus, T., Léonard, A., Marage, P. E., Mohammadi, A., Perniè, L., Reis, T., Seva, T., Thomas, L., Vander Velde, C., Vanlaer, P., Wang, J., Adler, V., Beernaert, K., Benucci, L., Cimmino, A., Costantini, S., Dildick, S., Garcia, G., Klein, B., Lellouch, J., Marinov, A., Mccartin, J., Ocampo Rios, A. A., Ryckbosch, D., Sigamani, M., Strobbe, N., Thyssen, F., Tytgat, M., Walsh, S., Yazgan, E., Zaganidis, N., Basegmez, S., Beluffi, C., Bruno, G., Castello, R., Caudron, A., Ceard, L., Delaere, C., Du Pree, T., Favart, D., Forthomme, L., Giammanco, A., Hollar, J., Jez, P., Lemaitre, V., Liao, J., Militaru, O., Nuttens, C., Pagano, D., Pin, A., Piotrzkowski, K., Popov, A., Selvaggi, M., Vizan Garcia, J. M., Beliy, N., Caebergs, T., Daubie, E., Hammad, G. H., Alves, G. A., Correa Martins Junior, M., Martins, T., Pol, M. E., Souza, M. H. G., Aldá Júnior, W. L., Carvalho, W., Chinellato, J., Custódio, A., Da Costa, E. M., De Jesus Damiao, D., De Oliveira Martins, C., Fonseca De Souza, S., Malbouisson, H., Malek, M., Matos Figueiredo, D., Mundim, L., Nogima, H., Prado Da Silva, W. L., Santoro, A., Sznajder, A., Tonelli Manganote, E. J., Vilela Pereira, A., Bernardes, C. A., Dias, F. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Lagana, C., Marinho, F., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Genchev, V., Iaydjiev, P., Piperov, S., Rodozov, M., Sultanov, G., Vutova, M., Dimitrov, A., Hadjiiska, R., Kozhuharov, V., Litov, L., Pavlov, B., Petkov, P., Bian, J. G., Chen, G. M., Chen, H. S., Jiang, C. H., Liang, D., Liang, S., Meng, X., Tao, J., Wang, X., Wang, Z., Xiao, H., Xu, M., Asawatangtrakuldee, C., Ban, Y., Guo, Y., Li, W., Liu, S., Mao, Y., Qian, S. J., Teng, H., Wang, D., Zhang, L., Zou, W., Avila, C., Carrillo Montoya, C. A., Gomez, J. P., Gomez Moreno, B., Sanabria, J. C., Godinovic, N., Lelas, D., Plestina, R., Polic, D., Puljak, I., Antunovic, Z., Kovac, M., Brigljevic, V., Duric, S., Kadija, K., Luetic, J., Mekterovic, D., Morovic, S., Tikvica, L., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Finger, M., Assran, Y., Ellithi Kamel, A., Mahmoud, M. A., Mahrous, A., Radi, A., Kadastik, M., Müntel, M., Murumaa, M., Raidal, M., Rebane, L., Tiko, A., Eerola, P., Fedi, G., Voutilainen, M., Härkönen, J., Karimäki, V., Kinnunen, R., Kortelainen, M. J., Lampén, T., Lassila-Perini, K., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Peltola, T., Tuominen, E., Tuominiemi, J., Tuovinen, E., Wendland, L., Korpela, A., Tuuva, T., Besancon, M., Choudhury, S., Couderc, F., Dejardin, M., Denegri, D., Fabbro, B., Faure, J. L., Ferri, F., Ganjour, S., Givernaud, A., Gras, P., Hamel De Monchenault, G., Jarry, P., Locci, E., Malcles, J., Millischer, L., Nayak, A., Rander, J., Rosowsky, A., Titov, M., Baffioni, S., Beaudette, F., Benhabib, L., Bianchini, L., Bluj, M., Busson, P., Charlot, C., Daci, N., Dahms, T., Dalchenko, M., Dobrzynski, L., Florent, A., Granier De Cassagnac, R., Haguenauer, M., Miné, P., Mironov, C., Naranjo, I. N., Nguyen, M., Ochando, C., Paganini, P., Sabes, D., Salerno, R., Sirois, Y., Veelken, C., Zabi, A., Agram, J.-L., Andrea, J., Bloch, D., Bodin, D., Brom, J.-M., Chabert, E. C., Collard, C., Conte, E., Drouhin, F., Fontaine, J.-C., Gelé, D., Goerlach, U., Goetzmann, C., Juillot, P., Le Bihan, A.-C., Van Hove, P., Gadrat, S., Beauceron, S., Beaupere, N., Boudoul, G., Brochet, S., Chasserat, J., Chierici, R., Contardo, D., Depasse, P., El Mamouni, H., Fay, J., Gascon, S., Gouzevitch, M., Ille, B., Kurca, T., Lethuillier, M., Mirabito, L., Perries, S., Sgandurra, L., Sordini, V., Tschudi, Y., Vander Donckt, M., Verdier, P., Viret, S., Tsamalaidze, Z., Autermann, C., Beranek, S., Calpas, B., Edelhoff, M., Feld, L., Heracleous, N., Hindrichs, O., Klein, K., Ostapchuk, A., Perieanu, A., Raupach, F., Sammet, J., Schael, S., Sprenger, D., Weber, H., Wittmer, B., Zhukov, V., Ata, M., Caudron, J., Dietz-Laursonn, E., Duchardt, D., Erdmann, M., Fischer, R., Güth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Klingebiel, D., Kreuzer, P., Merschmeyer, M., Meyer, A., Olschewski, M., Padeken, K., Papacz, P., Pieta, H., Reithler, H., Schmitz, S. A., Sonnenschein, L., Steggemann, J., Teyssier, D., Thüer, S., Weber, M., Cherepanov, V., Erdogan, Y., Flügge, G., Geenen, H., Geisler, M., Haj Ahmad, W., Hoehle, F., Kargoll, B., Kress, T., Kuessel, Y., Lingemann, J., Nowack, A., Nugent, I. M., Perchalla, L., Pooth, O., Stahl, A., Aldaya Martin, M., Asin, I., Bartosik, N., Behr, J., Behrenhoff, W., Behrens, U., Bergholz, M., Bethani, A., Borras, K., Burgmeier, A., Cakir, A., Calligaris, L., Campbell, A., Costanza, F., Diez Pardos, C., Dooling, S., Dorland, T., Eckerlin, G., Eckstein, D., Flucke, G., Geiser, A., Glushkov, I., Gunnellini, P., Habib, S., Hauk, J., Hellwig, G., Jung, H., Kasemann, M., Katsas, P., Kleinwort, C., Kluge, H., Krämer, M., Krücker, D., Kuznetsova, E., Lange, W., Leonard, J., Lipka, K., Lohmann, W., Lutz, B., Mankel, R., Marfin, I., Melzer-Pellmann, I.-A., Meyer, A. B., Mnich, J., Mussgiller, A., Naumann-Emme, S., Novgorodova, O., Nowak, F., Olzem, J., Perrey, H., Petrukhin, A., Pitzl, D., Placakyte, R., Raspereza, A., Ribeiro Cipriano, P. M., Riedl, C., Ron, E., Sahin, M. Ö., Salfeld-Nebgen, J., Schmidt, R., Schoerner-Sadenius, T., Sen, N., Stein, M., Walsh, R., Wissing, C., Blobel, V., Enderle, H., Erfle, J., Gebbert, U., Görner, M., Gosselink, M., Haller, J., Heine, K., Höing, R. S., Kaussen, G., Kirschenmann, H., Klanner, R., Kogler, R., Lange, J., Marchesini, I., Peiffer, T., Pietsch, N., Rathjens, D., Sander, C., Schettler, H., Schleper, P., Schlieckau, E., Schmidt, A., Schröder, M., Schum, T., Seidel, M., Sibille, J., Sola, V., Stadie, H., Steinbrück, G., Thomsen, J., Troendle, D., Vanelderen, L., Barth, C., Baus, C., Berger, J., Böser, C., Chwalek, T., De Boer, W., Descroix, A., Dierlamm, A., Feindt, M., Guthoff, M., Hackstein, C., Hartmann, F., Hauth, T., Heinrich, M., Held, H., Hoffmann, K. H., Husemann, U., Katkov, I., Komaragiri, J. R., Kornmayer, A., Lobelle Pardo, P., Martschei, D., Müller, Sarah, Müller, Th, Niegel, M., Nürnberg, A., Oberst, O., Ott, J., Quast, G., Rabbertz, K., Ratnikov, F., Röcker, S., Schilling, F.-P., Schott, G., Simonis, H. J., Stober, F. M., Ulrich, R., Wagner-Kuhr, J., Wayand, S., Weiler, T., Zeise, M., Anagnostou, G., Daskalakis, G., Geralis, T., Kesisoglou, S., Kyriakis, A., Loukas, D., Markou, A., Markou, C., Ntomari, E., Gouskos, L., Mertzimekis, T. J., Panagiotou, A., Saoulidou, N., Stiliaris, E., Aslanoglou, X., Evangelou, I., Flouris, G., Foudas, C., Kokkas, P., Manthos, N., Papadopoulos, I., Paradas, E., Bencze, G., Hajdu, C., Hidas, P., Horvath, D., Radics, B., Sikler, F., Veszpremi, V., Vesztergombi, G., Zsigmond, A. J., Beni, N., Czellar, S., Molnar, J., Palinkas, J., Szillasi, Z., Karancsi, J., Raics, P., Trocsanyi, Z. L., Ujvari, B., Beri, S. B., Bhatnagar, V., Dhingra, N., Gupta, R., Kaur, M., Mehta, M. Z., Mittal, M., Nishu, N., Saini, L. K., Sharma, A., Singh, J. B., Kumar, Ashok, Kumar, Arun, Ahuja, S., Bhardwaj, A., Choudhary, B. C., Malhotra, S., Naimuddin, M., Ranjan, K., Saxena, P., Sharma, V., Shivpuri, R. K., Banerjee, S., Bhattacharya, S., Chatterjee, K., Dutta, S., Gomber, B., Jain, Sa, Jain, Sh, Khurana, R., Modak, A., Mukherjee, S., Roy, D., Sarkar, S., Sharan, M., Abdulsalam, A., Dutta, D., Kailas, S., Kumar, V., Mohanty, A. K., Pant, L. M., Shukla, P., Topkar, A., Aziz, T., Chatterjee, R. M., Ganguly, S., Ghosh, S., Guchait, M., Gurtu, A., Kole, G., Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Mohanty, G. B., Parida, B., Sudhakar, K., Wickramage, N., Dugad, S., Arfaei, H., Bakhshiansohi, H., Etesami, S. M., Fahim, A., Hesari, H., Jafari, A., Khakzad, M., Mohammadi Najafabadi, M., Paktinat Mehdiabadi, S., Safarzadeh, B., Zeinali, M., Grunewald, M., Abbrescia, M., Barbone, L., Calabria, C., Chhibra, S. S., Colaleo, A., Creanza, D., De Filippis, N., De Palma, M., Fiore, L., Iaselli, G., Maggi, G., Maggi, M., Marangelli, B., My, S., Nuzzo, S., Pacifico, N., Pompili, A., Pugliese, G., Selvaggi, G., Silvestris, L., Singh, G., Venditti, R., Verwilligen, P., Zito, G., Abbiendi, G., Benvenuti, A. C., Bonacorsi, D., Braibant-Giacomelli, S., Brigliadori, L., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, P., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Meneghelli, M., Montanari, A., Navarria, F. L., Odorici, F., Perrotta, A., Primavera, F., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Travaglini, R., Albergo, S., Chiorboli, M., Costa, S., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Ciulli, V., Civinini, C., D’Alessandro, R., Focardi, E., Frosali, S., Gallo, E., Gonzi, S., Gori, V., Lenzi, P., Meschini, M., Paoletti, S., Sguazzoni, G., Tropiano, A., Benussi, L., Bianco, S., Piccolo, D., Fabbricatore, P., Musenich, R., Tosi, S., Benaglia, A., De Guio, F., Di Matteo, L., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, P., Lucchini, M. T., Malvezzi, S., Manzoni, R. A., Martelli, A., Menasce, D., Moroni, L., Paganoni, M., Pedrini, D., Ragazzi, S., Redaelli, N., Tabarelli De Fatis, T., Buontempo, S., Cavallo, N., De Cosa, A., Fabozzi, F., Iorio, A. O. M., Lista, L., Meola, S., Merola, M., Paolucci, P., Azzi, P., Bacchetta, N., Bisello, D., Branca, A., Carlin, R., Checchia, P., Dorigo, T., Dosselli, U., Galanti, M., Gasparini, F., Gasparini, U., Giubilato, P., Gozzelino, A., Gulmini, M., Kanishchev, K., Lacaprara, S., Lazzizzera, I., Margoni, M., Maron, G., Meneguzzo, A. T., Pazzini, J., Pozzobon, N., Ronchese, P., Simonetto, F., Torassa, E., Tosi, M., Vanini, S., Zotto, P., Zucchetta, A., Zumerle, G., Gabusi, M., Ratti, S. P., Riccardi, C., Vitulo, P., Biasini, M., Bilei, G. M., Fanò, L., Lariccia, P., Mantovani, G., Menichelli, M., Nappi, A., Romeo, F., Saha, A., Santocchia, A., Spiezia, A., Androsov, K., Azzurri, P., Bagliesi, G., Boccali, T., Broccolo, G., Castaldi, R., D’Agnolo, R. T., Dell’Orso, R., Fiori, F., Foà, L., Giassi, A., Kraan, A., Ligabue, F., Lomtadze, T., Martini, L., Messineo, A., Palla, F., Rizzi, A., Serban, A. T., Spagnolo, P., Squillacioti, P., Tenchini, R., Tonelli, G., Venturi, A., Verdini, P. G., Vernieri, C., Barone, L., Cavallari, F., Del Re, D., Diemoz, M., Grassi, M., Longo, E., Margaroli, F., Meridiani, P., Micheli, F., Nourbakhsh, S., Organtini, G., Paramatti, R., Rahatlou, S., Soffi, L., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Biino, C., Cartiglia, N., Casasso, S., Costa, M., Demaria, N., Mariotti, C., Maselli, S., Migliore, E., Monaco, V., Musich, M., Obertino, M. M., Ortona, G., Pastrone, N., Pelliccioni, M., Potenza, A., Romero, A., Ruspa, M., Sacchi, R., Solano, A., Staiano, A., Tamponi, U., Belforte, S., Candelise, V., Casarsa, M., Cossutti, F., Della Ricca, G., Gobbo, B., La Licata, C., Marone, M., Montanino, D., Penzo, A., Schizzi, A., Zanetti, A., Kim, T. Y., Nam, S. K., Chang, S., Kim, D. H., Kim, G. N., Kim, J. E., Kong, D. J., Oh, Y. D., Park, H., Son, D. C., Kim, J. Y., Kim, Zero J., Song, S., Choi, S., Gyun, D., Hong, B., Jo, M., Kim, H., Kim, T. J., Lee, K. S., Park, S. K., Roh, Y., Choi, M., Kim, J. H., Park, C., Park, I. C., Park, S., Ryu, G., Choi, Y., Choi, Y. K., Goh, J., Kim, M. S., Kwon, E., Lee, B., Lee, J., Lee, S., Seo, H., Yu, I., Grigelionis, I., Juodagalvis, A., Castilla-Valdez, H., De La Cruz-Burelo, E., Heredia-De La Cruz, I., Lopez-Fernandez, R., Martínez-Ortega, J., Sanchez-Hernandez, A., Villasenor-Cendejas, L. M., Carrillo Moreno, S., Vazquez Valencia, F., Salazar Ibarguen, H. A., Casimiro Linares, E., Morelos Pineda, A., Reyes-Santos, M. A., Krofcheck, D., Bell, A. J., Butler, P. H., Doesburg, R., Reucroft, S., Silverwood, H., Ahmad, M., Asghar, M. I., Butt, J., Hoorani, H. R., Khalid, S., Khan, W. A., Khurshid, T., Qazi, S., Shah, M. A., Shoaib, M., Bialkowska, H., Boimska, B., Frueboes, T., Górski, M., Kazana, M., Nawrocki, K., Romanowska-Rybinska, K., Szleper, M., Wrochna, G., Zalewski, P., Brona, G., Bunkowski, K., Cwiok, M., Dominik, W., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Wolszczak, W., Almeida, N., Bargassa, P., David, A., Faccioli, P., Ferreira Parracho, P. 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R., Jeong, C., Kovitanggoon, K., Lee, S. W., Libeiro, T., Volobouev, I., Appelt, E., Delannoy, A. G., Greene, S., Gurrola, A., Johns, W., Maguire, C., Melo, A., Sharma, M., Sheldon, P., Snook, B., Tuo, S., Velkovska, J., Arenton, M. W., Boutle, S., Cox, B., Francis, B., Goodell, J., Hirosky, R., Ledovskoy, A., Lin, C., Neu, C., Wood, J., Gollapinni, S., Harr, R., Karchin, P. E., Kottachchi Kankanamge Don, C., Lamichhane, P., Sakharov, A., Anderson, M., Belknap, D. A., Borrello, L., Carlsmith, D., Cepeda, M., Dasu, S., Friis, E., Grogg, K. S., Grothe, M., Hall-Wilton, R., Herndon, M., Hervé, A., Kaadze, K., Klabbers, P., Klukas, J., Lanaro, A., Lazaridis, C., Loveless, R., Mohapatra, A., Mozer, M. U., Ojalvo, I., Pierro, G. A., Ross, I., Savin, A., Smith, W. H., and Swanson, J.
Subjects: Physics, ddc:530
Published: 2022

45. Searches for long-lived charged particles in pp collisions at root s = 7 and 8 TeV (vol 07, 122, 2013)

Author: Chatrchyan, S, Khachatryan, V, Sirunyan, Am, Tumasyan, A, Adam, W, Bergauer, T, Dragicevic, M, Ero, J, Fabjan, C, Friedl, M, Fruhwirth, R, Ghete, Vm, Hormann, N, Hrubec, J, Jeitler, M, Kiesenhofer, W, Knunz, V, Krammer, M, Kratschmer, I, Liko, D, Mikulec, I, Rabady, D, Rahbaran, B, Rohringer, C, Rohringer, H, Schofbeck, R, Strauss, J, Taurok, A, Treberer-Treberspurg, W, Waltenberger, W, Wulz, Ce, Mossolov, V, Shumeiko, N, Gonzalez, Js, Alderweireldt, S, Bansal, M, Bansal, S, Cornelis, T, De Wolf, Ea, Janssen, X, Knutsson, A, Luyckx, S, Mucibello, L, Ochesanu, S, Roland, B, Rougny, R, Van Haevermaet, H, Van Mechelen, P, Van Remortel, N, Van Spilbeeck, A, Blekman, F, Blyweert, S, D'Hondt, J, Kalogeropoulos, A, Keaveney, J, Maes, M, Olbrechts, A, Tavernier, S, Van Doninck, W, Van Mulders, P, Van Onsem, Gp, Villella, I, Clerbaux, B, De Lentdecker, G, Favart, L, Gay, Apr, Hreus, T, Leonard, A, Marage, Pe, Mohammadi, A, Pernie, L, Reis, T, Seva, T, Thomas, L, Vander Velde, C, Vanlaer, P, Wang, J, Adler, V, Beernaert, K, Benucci, L, Cimmino, A, Costantini, S, Dildick, S, Garcia, G, Klein, B, Lellouch, J, Marinov, A, Mccartin, J, Rios, Aao, Ryckbosch, D, Sigamani, M, Strobbe, N, Thyssen, F, Tytgat, M, Walsh, S, Yazgan, E, Zaganidis, N, Basegmez, S, Beluffi, C, Bruno, G, Castello, R, Caudron, A, Ceard, L, Delaere, C, du Pree, T, Favart, D, Forthomme, L, Giammanco, A, Hollar, J, Jez, P, Lemaitre, V, Liao, J, Militaru, O, Nuttens, C, Pagano, D, Pin, A, Piotrzkowski, K, Popov, A, Selvaggi, M, Garcia, Jmv, Beliy, N, Caebergs, T, Daubie, E, Hammad, Gh, Alves, Ga, Martins, Mc, Martins, T, Pol, Me, Souza, Mhg, Alda, Wl, Carvalho, W, Chinellato, J, Custodio, A, Da Costa, Em, Damiao, Dd, Martins, Cd, De Souza, Sf, Malbouisson, H, Malek, M, Figueiredo, Dm, Mundim, L, Nogima, H, Da Silva, Wlp, Santoro, A, Sznajder, A, Manganote, Ejt, Pereira, Av, Bernardes, Ca, Dias, Fa, Tomei, Trfp, Gregores, Em, Lagana, C, Marinho, F, Mercadante, Pg, Novaes, Sf, Padula, Ss, Genchev, V, Iaydjiev, P, Piperov, S, Rodozov, M, Sultanov, G, Vutova, M, Dimitrov, A, Hadjiiska, R, Kozhuharov, V, Litov, L, Pavlov, B, Petkov, P, Bian, Jg, Chen, Gm, Chen, Hs, Jiang, Ch, Liang, D, Liang, S, Meng, X, Tao, J, Wang, X, Wang, Z, Xiao, H, Xu, M, Asawatangtrakuldee, C, Ban, Y, Guo, Y, Li, W, Liu, S, Mao, Y, Qian, Sj, Teng, H, Wang, D, Zhang, L, Zou, W, Avila, C, Montoya, Cac, Gomez, Jp, Moreno, Bg, Sanabria, Jc, Godinovic, N, Lelas, D, Plestina, R, Polic, D, Puljak, I, Antunovic, Z, Kovac, M, Brigljevic, V, Duric, S, Kadija, K, Luetic, J, Mekterovic, D, Morovic, S, Tikvica, L, Attikis, A, Mavromanolakis, G, Mousa, J, Nicolaou, C, Ptochos, F, Razis, Pa, Finger, M, Assran, Y, Kamel, Ae, Mahmoud, Ma, Mahrous, A, Radi, A, Kadastik, M, Muntel, M, Murumaa, M, Raidal, M, Rebane, L, Tiko, A, Eerola, P, Fedi, G, Voutilainen, M, Harkonen, J, Karimaki, V, Kinnunen, R, Kortelainen, Mj, Lampen, T, Lassila-Perini, K, Lehti, S, Linden, T, Luukka, P, Maenpaa, T, Peltola, T, Tuominen, E, Tuominiemi, J, Tuovinen, E, Wendland, L, Korpela, A, Tuuva, T, Besancon, M, Choudhury, S, Couderc, F, Dejardin, M, Denegri, D, Fabbro, B, Faure, Jl, Ferri, F, Ganjour, S, Givernaud, A, Gras, P, de Monchenault, Gh, Jarry, P, Locci, E, Malcles, J, Millischer, L, Nayak, A, Rander, J, Rosowsky, A, Titov, M, Baffioni, S, Beaudette, F, Benhabib, L, Bianchini, L, Bluj, M, Busson, P, Charlot, C, Daci, N, Dahms, T, Dalchenko, M, Dobrzynski, L, Florent, A, de Cassagnac, Rg, Haguenauer, M, Mine, P, Mironov, C, Naranjo, In, Nguyen, M, Ochando, C, Paganini, P, Sabes, D, Salerno, R, Sirois, Y, Veelken, C, Zabi, A, Agram, Jl, Andrea, J, Bloch, D, Bodin, D, Brom, Jm, Chabert, Ec, Collard, C, Conte, E, Drouhin, F, Fontaine, Jc, Gele, D, Goerlach, U, Goetzmann, C, Juillot, P, Le Bihan, Ac, Van Hove, P, Gadrat, S, Beauceron, S, Beaupere, N, Boudoul, G, Brochet, S, Chasserat, J, Chierici, R, Contardo, D, Depasse, P, El Mamouni, H, Fay, J, Gascon, S, Gouzevitch, M, Ille, B, Kurca, T, Lethuillier, M, Mirabito, L, Perries, S, Sgandurra, L, Sordini, V, Tschudi, Y, Vander Donckt, M, Verdier, P, Viret, S, Tsamalaidze, Z, Autermann, C, Beranek, S, Calpas, B, Edelhoff, M, Feld, L, Heracleous, N, Hindrichs, O, Klein, K, Ostapchuk, A, Perieanu, A, Raupach, F, Sammet, J, Schael, S, Sprenger, D, Weber, H, Wittmer, B, Zhukov, V, Ata, M, Caudron, J, Dietz-Laursonn, E, Duchardt, D, Erdmann, M, Fischer, R, Guth, A, Hebbeker, T, Heidemann, C, Hoepfner, K, Klingebiel, D, Kreuzer, P, Merschmeyer, M, Meyer, A, Olschewski, M, Padeken, K, Papacz, P, Pieta, H, Reithler, H, Schmitz, Sa, Sonnenschein, L, Steggemann, J, Teyssier, D, Thuer, S, Weber, M, Cherepanov, V, Erdogan, Y, Flugge, G, Geenen, H, Geisler, M, Ahmad, Wh, Hoehle, F, Kargoll, B, Kress, T, Kuessel, Y, Lingemann, J, Nowack, A, Nugent, Im, Perchalla, L, Pooth, O, Stahl, A, Martin, Ma, Asin, I, Bartosik, N, Behr, J, Behrenhoff, W, Behrens, U, Bergholz, M, Bethani, A, Borras, K, Burgmeier, A, Cakir, A, Calligaris, L, Campbell, A, Costanza, F, Pardos, Cd, Dooling, S, Dorland, T, Eckerlin, G, Eckstein, D, Flucke, G, Geiser, A, Glushkov, I, Gunnellini, P, Habib, S, Hauk, J, Hellwig, G, Jung, H, Kasemann, M, Katsas, P, Kleinwort, C, Kluge, H, Kramer, M, Krucker, D, Kuznetsova, E, Lange, W, Leonard, J, Lipka, K, Lohmann, W, Lutz, B, Mankel, R, Marfin, I, Melzer-Pellmann, Ia, Meyer, Ab, Mnich, J, Mussgiller, A, Naumann-Emme, S, Novgorodova, O, Nowak, F, Olzem, J, Perrey, H, Petrukhin, A, Pitzl, D, Placakyte, R, Raspereza, A, Cipriano, Pmr, Riedl, C, Ron, E, Sahin, Mo, Salfeld-Nebgen, J, Schmidt, R, Schoerner-Sadenius, T, Sen, N, Stein, M, Walsh, R, Wissing, C, Blobel, V, Enderle, H, Erfle, J, Gebbert, U, Gorner, M, Gosselink, M, Haller, J, Heine, K, Hoing, Rs, Kaussen, G, Kirschenmann, H, Klanner, R, Kogler, R, Lange, J, Marchesini, I, Peiffer, T, Pietsch, N, Rathjens, D, Sander, C, Schettler, H, Schleper, P, Schlieckau, E, Schmidt, A, Schroder, M, Schum, T, Seidel, M, Sibille, J, Sola, V, Stadie, H, Steinbruck, G, Thomsen, J, Troendle, D, Vanelderen, L, Barth, C, Baus, C, Berger, J, Boser, C, Chwalek, T, De Boer, W, Descroix, A, Dierlamm, A, Feindt, M, Guthoff, M, Hackstein, C, Hartmann, F, Hauth, T, Heinrich, M, Held, H, Hoffmann, Kh, Husemann, U, Katkov, I, Komaragiri, Jr, Kornmayer, A, Pardo, Pl, Martschei, D, Mueller, S, Muller, T, Niegel, M, Nurnberg, A, Oberst, O, Ott, J, Quast, G, Rabbertz, K, Ratnikov, F, Rocker, S, Schilling, Fp, Schott, G, Simonis, Hj, Stober, Fm, Ulrich, R, Wagner-Kuhr, J, Wayand, S, Weiler, T, Zeise, M, Anagnostou, G, Daskalakis, G, Geralis, T, Kesisoglou, S, Kyriakis, A, Loukas, D, Markou, A, Markou, C, Ntomari, E, Gouskos, L, Mertzimekis, Tj, Panagiotou, A, Saoulidou, N, Stiliaris, E, Aslanoglou, X, Evangelou, I, Flouris, G, Foudas, C, Kokkas, P, Manthos, N, Papadopoulos, I, Paradas, E, Bencze, G, Hajdu, C, Hidas, P, Horvath, D, Radics, B, Sikler, F, Veszpremi, V, Vesztergombi, G, Zsigmond, Aj, Beni, N, Czellar, S, Molnar, J, Palinkas, J, Szillasi, Z, Karancsi, J, Raics, P, Trocsanyi, Zl, Ujvari, B, Beri, Sb, Bhatnagar, V, Dhingra, N, Gupta, R, Kaur, M, Mehta, Mz, Mittal, M, Nishu, N, Saini, Lk, Sharma, A, Singh, Jb, Kumar, A, Ahuja, S, Bhardwaj, A, Choudhary, Bc, Malhotra, S, Naimuddin, M, Ranjan, K, Saxena, P, Sharma, V, Shivpuri, Rk, Banerjee, S, Bhattacharya, S, Chatterjee, K, Dutta, S, Gomber, B, Jain, S, Khurana, R, Modak, A, Mukherjee, S, Roy, D, Sarkar, S, Sharan, M, Abdulsalam, A, Dutta, D, Kailas, S, Kumar, V, Mohanty, Ak, Pant, Lm, Shukla, P, Topkar, A, Aziz, T, Chatterjee, Rm, Ganguly, S, Ghosh, S, Guchait, M, Gurtu, A, Kole, G, Kumar, S, Maity, M, Majumder, G, Mazumdar, K, Mohanty, Gb, Parida, B, Sudhakar, K, Wickramage, N, Dugad, S, Arfaei, H, Bakhshiansohi, H, Etesami, Sm, Fahim, A, Hesari, H, Jafari, A, Khakzad, M, Najafabadi, Mm, Mehdiabadi, Sp, Safarzadeh, B, Zeinali, M, Grunewald, M, Abbrescia, M, Barbone, L, Calabria, C, Chhibra, Ss, Colaleo, A, Creanza, D, De Filippis, N, De Palma, M, Fiore, L, Iaselli, G, Maggi, G, Maggi, M, Marangelli, B, My, S, Nuzzo, S, Pacifico, N, Pompili, A, Pugliese, G, Selvaggi, G, Silvestris, L, Singh, G, Venditti, R, Verwilligen, P, Zito, G, Abbiendi, G, Benvenuti, Ac, Bonacorsi, D, Braibant-Giacomelli, S, Brigliadori, L, Campanini, R, Capiluppi, P, Castro, A, Cavallo, Fr, Cuffiani, M, Dallavalle, Gm, Fabbri, F, Fanfani, A, Fasanella, D, Giacomelli, P, Grandi, C, Guiducci, L, Marcellini, S, Masetti, G, Meneghelli, M, Montanari, A, Navarria, Fl, Odorici, F, Perrotta, A, Primavera, F, Rossi, Am, Rovelli, T, Siroli, Gp, Tosi, N, Travaglini, R, Albergo, S, Chiorboli, M, Costa, S, Giordano, F, Potenza, R, Tricomi, A, Tuve, C, Barbagli, G, Ciulli, V, Civinini, C, D'Alessandro, R, Focardi, E, Frosali, S, Gallo, E, Gonzi, S, Gori, V, Lenzi, P, Meschini, M, Paoletti, S, Sguazzoni, G, Tropiano, A, Benussi, L, Bianco, S, Piccolo, D, Fabbricatore, P, Musenich, R, Tosi, S, Benaglia, A, De Guio, F, Di Matteo, L, Fiorendi, S, Gennai, S, Ghezzi, A, Govoni, P, Lucchini, Mt, Malvezzi, S, Manzoni, Ra, Martelli, A, Menasce, D, Moroni, L, Paganoni, M, Pedrini, D, Ragazzi, S, Redaelli, N, de Fatis, Tt, Buontempo, S, Cavallo, N, De Cosa, A, Fabozzi, F, Iorio, Aom, Lista, L, Meola, S, Merola, M, Paolucci, P, Azzi, P, Bacchetta, N, Bisello, D, Branca, A, Carlin, R, Checchia, P, Dorigo, T, Dosselli, U, Galanti, M, Gasparini, F, Gasparini, U, Giubilato, P, Gozzelino, A, Gulmini, M, Kanishchev, K, Lacaprara, S, Lazzizzera, I, Margoni, M, Maron, G, Meneguzzo, At, Pazzini, J, Pozzobon, N, Ronchese, P, Simonetto, F, Torassa, E, Tosi, M, Vanini, S, Zotto, P, Zucchetta, A, Zumerle, G, Gabusi, M, Ratti, Sp, Riccardi, C, Vitulo, P, Biasini, M, Bilei, Gm, Fano, L, Lariccia, P, Mantovani, G, Menichelli, M, Nappi, A, Romeo, F, Saha, A, Santocchia, A, Spiezia, A, Androsov, K, Azzurri, P, Bagliesi, G, Boccali, T, Broccolo, G, Castaldi, R, D'Agnolo, Rt, Dell'Orso, R, Fiori, F, Foa, L, Giassi, A, Kraan, A, Ligabue, F, Lomtadze, T, Martini, L, Messineo, A, Palla, F, Rizzi, A, Serban, At, Spagnolo, P, Squillacioti, P, Tenchini, R, Tonelli, G, Venturi, A, Verdini, Pg, Vernieri, C, Barone, L, Cavallari, F, Del Re, D, Diemoz, M, Grassi, M, Longo, E, Margaroli, F, Meridiani, P, Micheli, F, Nourbakhsh, S, Organtini, G, Paramatti, R, Rahatlou, S, Soffi, L, Amapane, N, Arcidiacono, R, Argiro, S, Arneodo, M, Biino, C, Cartiglia, N, Casasso, S, Costa, M, Demaria, N, Mariotti, C, Maselli, S, Migliore, E, Monaco, V, Musich, M, Obertino, Mm, Ortona, G, Pastrone, N, Pelliccioni, M, Potenza, A, Romero, A, Ruspa, M, Sacchi, R, Solano, A, Staiano, A, Tamponi, U, Belforte, S, Candelise, V, Casarsa, M, Cossutti, F, Della Ricca, G, Gobbo, B, La Licata, C, Marone, M, Montanino, D, Penzo, A, Schizzi, A, Zanetti, A, Kim, Ty, Nam, Sk, Chang, S, Kim, Dh, Kim, Gn, Kim, Je, Kong, Dj, Yd, Oh, Park, H, Son, Dc, Kim, Jy, Kim, Zj, Song, S, Choi, S, Gyun, D, Hong, B, Jo, M, Kim, H, Kim, Tj, Lee, Ks, Park, Sk, Roh, Y, Choi, M, Kim, Jh, Park, C, Park, Ic, Park, S, Ryu, G, Choi, Y, Choi, Yk, Goh, J, Kim, Ms, Kwon, E, Lee, B, Lee, J, Lee, S, Seo, H, Yu, I, Grigelionis, I, Juodagalvis, A, Castilla-Valdez, H, De La Cruz-Burelo, E, Heredia-de La Cruz, I, Lopez-Fernandez, R, Martinez-Ortega, J, Sanchez-Hernandez, A, Villasenor-Cendejas, Lm, Moreno, Sc, Valencia, Fv, Ibarguen, Has, Linares, Ec, Pineda, Am, Reyes-Santos, Ma, Krofcheck, D, Bell, Aj, Butler, Ph, Doesburg, R, Reucroft, S, Silverwood, H, Ahmad, M, Asghar, Mi, Butt, J, Hoorani, Hr, Khalid, S, Khan, Wa, Khurshid, T, Qazi, S, Shah, Ma, Shoaib, M, Bialkowska, H, Boimska, B, Frueboes, T, Gorski, M, Kazana, M, Nawrocki, K, Romanowska-Rybinska, K, Szleper, M, Wrochna, G, Zalewski, P, Brona, G, Bunkowski, K, Cwiok, M, Dominik, W, Doroba, K, Kalinowski, A, Konecki, M, Krolikowski, J, Misiura, M, Wolszczak, W, Almeida, N, Bargassa, P, David, A, Faccioli, P, Parracho, Pgf, Gallinaro, M, Antunes, Jr, Seixas, J, Varela, J, Vischia, P, Bunin, P, Gavrilenko, M, Golutvin, I, Gorbunov, I, Kamenev, A, Karjavin, V, Konoplyanikov, V, Kozlov, G, Lanev, A, Malakhov, A, Matveev, V, Moisenz, P, Palichik, V, Perelygin, V, Shmatov, S, Skatchkov, N, Smirnov, V, Zarubin, A, Evstyukhin, S, Golovtsov, V, Ivanov, Y, Kim, V, Levchenko, P, Murzin, V, Oreshkin, V, Smirnov, I, Sulimov, V, Uvarov, L, Vavilov, S, Vorobyev, A, Andreev, Y, Dermenev, A, Gninenko, S, Golubev, N, Kirsanov, M, Krasnikov, N, Pashenkov, A, Tlisov, D, Toropin, A, Epshteyn, V, Erofeeva, M, Gavrilov, V, Lychkovskaya, N, Popov, V, Safronov, G, Semenov, S, Spiridonov, A, Stolin, V, Vlasov, E, Zhokin, A, Andreev, V, Azarkin, M, Dremin, I, Kirakosyan, M, Leonidov, A, Mesyats, G, Rusakov, Sv, Vinogradov, A, Belyaev, A, Boos, E, Bunichev, V, Dubinin, M, Dudko, L, Ershov, A, Gribushin, A, Klyukhin, V, Kodolova, O, Lokhtin, I, Markina, A, Obraztsov, S, Savrin, V, Snigirev, A, Azhgirey, I, Bayshev, I, Bitioukov, S, Kachanov, V, Kalinin, A, Konstantinov, D, Krychkine, V, Petrov, V, Ryutin, R, Sobol, A, Tourtchanovitch, L, Troshin, S, Tyurin, N, Uzunian, A, Volkov, A, Adzic, P, Ekmedzic, M, Krpic, D, Milosevic, J, Aguilar-Benitez, M, Alcaraz Maestre, J, Battilana, C, Calvo, E, Cerrada, M, Llatas, Mc, Colino, N, De La Cruz, B, Peris, Ad, Vazquez, Dd, Bedoya, Cf, Ramos, Jpf, Ferrando, A, Flix, J, Fouz, Mc, Garcia-Abia, P, Lopez, Og, Lopez, Sg, Hernandez, Jm, Josa, Mi, Merino, G, De Martino, En, Pelayo, Jp, Olmeda, Aq, Redondo, I, Romero, L, Santaolalla, J, Soares, Ms, Willmott, C, Albajar, C, de Troconiz, Jf, Brun, H, Cuevas, J, Menendez, Jf, Folgueras, S, Caballero, Ig, Iglesias, Ll, Cifuentes, Jab, Cabrillo, Ij, Calderon, A, Chuang, Sh, Campderros, Jd, Fernandez, M, Gomez, G, Sanchez, Jg, Graziano, A, Jorda, C, Virto, Al, Marco, J, Marco, R, Rivero, Cm, Matorras, F, Sanchez, Fjm, Rodrigo, T, Rodriguez-Marrero, Ay, Ruiz-Jimeno, A, Scodellaro, L, Vila, I, Cortabitarte, Rv, Abbaneo, D, Auffray, E, Auzinger, G, Bachtis, M, Baillon, P, Ball, Ah, Barney, D, Bendavid, J, Benitez, Jf, Bernet, C, Bianchi, G, Bloch, P, Bocci, A, Bonato, A, Bondu, O, Botta, C, Breuker, H, Camporesi, T, Cerminara, G, 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Published: 2022

46. Investigating the Blazar TXS 0506+056 through Sharp Multiwavelength Eyes During 2017-2019

Author: MAGIC Collaboration, Acciari, V. A., Aniello, T., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batković, I., González, J. Becerra, Bednarek, W., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bökenkamp, H., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Del Popolo, A., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Fariña, L., Fattorini, A., Font, L., Fruck, C., Fukami, S., Fukazawa, Y., López, R. J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Hassan, T., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Iotov, R., Ishio, K., Iwamura, Y., Martínez, I. Jiménez, Jormanainen, J., Jouvin, L., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Linhoff, L., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Mariotti, M., Martínez, M., Aguilar, A. Mas, Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Nakamori, T., Nava, L., Neustroev, V., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Persic, M., Pihet, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schmuckermaier, F., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strišković, J., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Takeishi, R., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Viale, I., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Yamamoto, T., Zarić, D., Collaboration, OVRO, Hodges, M., Hovatta, T., Kiehlmann, S., Liodakis, I., Max-Moerbeck, W., Pearson, T. J., Readhead, A. C. S., Reeves, R. A., Collaboration, Metsähovi, Lähteenmaäki, A., Tornikoski, M., Tammi, J., D'Ammando, F., Marchini, A., Metsähovi Radio Observatory, Department of Electronics and Nanoengineering, Aalto-yliopisto, Aalto University, Ministerio de Ciencia e Innovación (España), European Commission, Federal Ministry of Education and Research (Germany), Istituto Nazionale di Astrofisica, Istituto Nazionale di Fisica Nucleare, Swiss National Science Foundation, Department of Atomic Energy (India), Ministry of Education, Culture, Sports, Science and Technology (Japan), Ministry of Education and Science (Bulgaria), Academy of Finland, Generalitat de Catalunya, Croatian Science Foundation, and German Research Foundation
Subjects: High energy astrophysics, Jets, Blazars, Gamma-rays, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::High Energy Astrophysical Phenomena, gamma ray, VHE, FOS: Physical sciences, Bethe-Heitler, blazar, IceCube, X-ray, optical, High Energy Astrophysical Phenomena (astro-ph.HE), Astronomy and Astrophysics, neutrino, current, MAGIC, cascade, flux, Space and Planetary Science, ddc:520, spectral, Física nuclear, photon neutrino
Abstract: This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.--Full list of authors: Acciari, V. A.; Aniello, T.; Ansoldi, S.; Antonelli, L. A.; Arbet Engels, A.; Artero, M.; Asano, K.; Baack, D.; Babić, A.; Baquero, A.; Barres de Almeida, U.; Barrio, J. A.; Batković, I.; Becerra González, J.; Bednarek, W.; Bernardini, E.; Bernardos, M.; Berti, A.; Besenrieder, J.; Bhattacharyya, W.; Bigongiari, C.; Biland, A.; Blanch, O.; Bökenkamp, H.; Bonnoli, G.; Bošnjak, Ž.; Busetto, G.; Carosi, R.; Ceribella, G.; Cerruti, M.; Chai, Y.; Chilingarian, A.; Cikota, S.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D'Amico, G.; D'Elia, V.; Vela, P. Da; Dazzi, F.; De Angelis, A.; De Lotto, B.; Del Popolo, A.; Delfino, M.; Delgado, J.; Mendez, C. Delgado; Depaoli, D.; Di Pierro, F.; Di Venere, L.; Do Souto Espiñeira, E.; Dominis Prester, D.; Donini, A.; Dorner, D.; Doro, M.; Elsaesser, D.; Fallah Ramazani, V.; Fariña, L.; Fattorini, A.; Font, L.; Fruck, C.; Fukami, S.; Fukazawa, Y.; García López, R. J.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giglietto, N.; Giordano, F.; Gliwny, P.; Godinović, N.; Green, J. G.; Green, D.; Hadasch, D.; Hahn, A.; Hassan, T.; Heckmann, L.; Herrera, J.; Hoang, J.; Hrupec, D.; Hütten, M.; Inada, T.; Iotov, R.; Ishio, K.; Iwamura, Y.; Jiménez Martínez, I.; Jormanainen, J.; Jouvin, L.; Kerszberg, D.; Kobayashi, Y.; Kubo, H.; Kushida, J.; Lamastra, A.; Lelas, D.; Leone, F.; Lindfors, E.; Linhoff, L.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Machado de Oliveira Fraga, B.; Maggio, C.; Majumdar, P.; Makariev, M.; Mallamaci, M.; Maneva, G.; Manganaro, M.; Mannheim, K.; Mariotti, M.; Martínez, M.; Mas Aguilar, A.; Mazin, D.; Menchiari, S.; Mender, S.; Mićanović, S.; Miceli, D.; Miener, T.; Miranda, J. M.; Mirzoyan, R.; Molina, E.; Moralejo, A.; Morcuende, D.; Moreno, V.; Moretti, E.; Nakamori, T.; Nava, L.; Neustroev, V.; Nievas Rosillo, M.; Nigro, C.; Nilsson, K.; Nishijima, K.; Noda, K.; Nozaki, S.; Ohtani, Y.; Oka, T.; Otero-Santos, J.; Paiano, S.; Palatiello, M.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Pavletić, L.; Peñil, P.; Persic, M.; Pihet, M.; Prada Moroni, P. G.; Prandini, E.; Priyadarshi, C.; Puljak, I.; Rhode, W.; Ribó, M.; Rico, J.; Righi, C.; Rugliancich, A.; Sahakyan, N.; Saito, T.; Sakurai, S.; Satalecka, K.; Saturni, F. G.; Schleicher, B.; Schmidt, K.; Schmuckermaier, F.; Schweizer, T.; Sitarek, J.; Šnidarić, I.; Sobczynska, D.; Spolon, A.; Stamerra, A.; Strišković, J.; Strom, D.; Strzys, M.; Suda, Y.; Surić, T.; Takahashi, M.; Takeishi, R.; Tavecchio, F.; Temnikov, P.; Terzić, T.; Teshima, M.; Tosti, L.; Truzzi, S.; Tutone, A.; Ubach, S.; van Scherpenberg, J.; Vanzo, G.; Vazquez Acosta, M.; Ventura, S.; Verguilov, V.; Viale, I.; Vigorito, C. F.; Vitale, V.; Vovk, I.; Will, M.; Wunderlich, C.; Yamamoto, T.; Zarić, D.; Hodges, M.; Hovatta, T.; Kiehlmann, S.; Liodakis, I.; Max-Moerbeck, W.; Pearson, T. J.; Readhead, A. C. S.; Reeves, R. A.; Lähteenmäki, A.; Tornikoski, M.; Tammi, J.; D'Ammando, F.; Marchini, A.; MAGIC Collaboration; OVRO Collaboration; Metsahovi Collaboration., The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, when a high-energy neutrino detected by IceCube (IceCube-170922A) was associated at the 3σ level with a γ-ray flare from this source. This multi-messenger photon-neutrino association remains, as per today, the most significant association ever observed. TXS 0506+056 was a poorly studied object before the IceCube-170922A event. To better characterize its broadband emission, we organized a multiwavelength campaign lasting 16 months (2017 November to 2019 February), covering the radio band (Metsähovi, OVRO), the optical/UV (ASAS-SN, KVA, REM, Swift/UVOT), the X-rays (Swift/XRT, NuSTAR), the high-energy γ rays (Fermi/LAT), and the very high-energy (VHE) γ rays (MAGIC). In γ rays, the behavior of the source was significantly different from the behavior in 2017: MAGIC observations show the presence of flaring activity during 2018 December, while the source only shows an excess at the 4σ level during the rest of the campaign (74 hr of accumulated exposure); Fermi/LAT observations show several short (on a timescale of days to a week) flares, different from the long-term brightening of 2017. No significant flares are detected at lower energies. The radio light curve shows an increasing flux trend that is not seen in other wavelengths. We model the multiwavelength spectral energy distributions in a lepto-hadronic scenario, in which the hadronic emission emerges as Bethe-Heitler and pion-decay cascade in the X-rays and VHE γ rays. According to the model presented here, the 2018 December γ-ray flare was connected to a neutrino emission that was too brief and not bright enough to be detected by current neutrino instruments. © 2022. The Author(s). Published by the American Astronomical Society., The financial support of the German BMBF, MPG, and HGF; the Italian INFN and INAF; the Swiss National Fund SNF; the ERDF under the Spanish Ministerio de Ciencia e Innovación (MICINN) (PID2019-104114RB-C31, PID2019-104114RB-C32, PID2019-104114RB-C33, PID2019-105510GB-C31,PID2019-107847RB-C41, PID2019-107847RB-C42, PID2019-107847RB-C44, PID2019-107988GB-C22); the Indian Department of Atomic Energy; the Japanese ICRR, the University of Tokyo, JSPS, and MEXT; the Bulgarian Ministry of Education and Science, National RI Roadmap Project DO1-400/18.12.2020 and the Academy of Finland grant nr. 320045 is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia "Severo Ochoa" (SEV-2016-0588, SEV-2017-0709, CEX2019-000920-S), the Unidad de Excelencia "María de Maeztu" (CEX2019-000918-M, MDM-2015-0509-18-2) and by the CERCA program of the Generalitat de Catalunya; by the Croatian Science Foundation (HrZZ) Project IP-2016-06-9782 and the University of Rijeka Project 13.12.1.3.02; by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3; the Polish National Research Centre grant UMO-2016/22/M/ST9/00382; and by the Brazilian MCTIC, CNPq and FAPERJ. E.P. acknowledges funding from the Italian Ministry of Education, University and Research (MIUR) through the "Dipartimenti di eccellenza" project Science of the universe. M.C. has received financial support through the Postdoctoral Junior Leader Fellowship Programme from la Caixa Banking Foundation, grant No. LCF/BQ/LI18/11630012. This research has made use of data from the OVRO 40 m monitoring program, which was supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G, and NSF grants AST-0808050 and AST-1109911, and private funding from Caltech and the MPIfR. This publication makes use of data obtained at Metsähovi Radio Observatory, operated by Aalto University in Finland.
Published: 2022

47. The Unanticipated Phenomenology of the Blazar PKS 2131–021: A Unique Supermassive Black Hole Binary Candidate

Author: O’Neill, S., primary, Kiehlmann, S., additional, Readhead, A. C. S., additional, Aller, M. F., additional, Blandford, R. D., additional, Liodakis, I., additional, Lister, M. L., additional, Mróz, P., additional, O’Dea, C. P., additional, Pearson, T. J., additional, Ravi, V., additional, Vallisneri, M., additional, Cleary, K. A., additional, Graham, M. J., additional, Grainge, K. J. B., additional, Hodges, M. W., additional, Hovatta, T., additional, Lähteenmäki, A., additional, Lamb, J. W., additional, Lazio, T. J. W., additional, Max-Moerbeck, W., additional, Pavlidou, V., additional, Prince, T. A., additional, Reeves, R. A., additional, Tornikoski, M., additional, Vergara de la Parra, P., additional, and Zensus, J. A., additional
Published: 2022
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48. Revisiting the Distance to Radio Loops I and IV Using Gaia and Radio/Optical Polarization Data

Author: Panopoulou, G. V., primary, Dickinson, C., additional, Readhead, A. C. S., additional, Pearson, T. J., additional, and Peel, M. W., additional
Published: 2021
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49. Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

Author: Acciari, V A, primary, Ansoldi, S, additional, Antonelli, L A, additional, Arbet Engels, A, additional, Artero, M, additional, Asano, K, additional, Baack, D, additional, Babić, A, additional, Baquero, A, additional, Barres de Almeida, U, additional, Barrio, J A, additional, Batković, I, additional, Becerra González, J, additional, Bednarek, W, additional, Bellizzi, L, additional, Bernardini, E, additional, Bernardos, M, additional, Berti, A, additional, Besenrieder, J, additional, Bhattacharyya, W, additional, Bigongiari, C, additional, Biland, A, additional, Blanch, O, additional, Bonnoli, G, additional, Bošnjak, Ž, additional, Busetto, G, additional, Carosi, R, additional, Ceribella, G, additional, Cerruti, M, additional, Chai, Y, additional, Chilingarian, A, additional, Cikota, S, additional, Colak, S M, additional, Colombo, E, additional, Contreras, J L, additional, Cortina, J, additional, Covino, S, additional, D’Amico, G, additional, D’Elia, V, additional, Da Vela, P, additional, Dazzi, F, additional, De Angelis, A, additional, De Lotto, B, additional, Delfino, M, additional, Delgado, J, additional, Delgado Mendez, C, additional, Depaoli, D, additional, Di Pierro, F, additional, Di Venere, L, additional, Do Souto Espiñeira, E, additional, Dominis Prester, D, additional, Donini, A, additional, Dorner, D, additional, Doro, M, additional, Elsaesser, D, additional, Fallah Ramazani, V, additional, Fattorini, A, additional, Ferrara, G, additional, Fonseca, M V, additional, Font, L, additional, Fruck, C, additional, Fukami, S, additional, García López, R J, additional, Garczarczyk, M, additional, Gasparyan, S, additional, Gaug, M, additional, Giglietto, N, additional, Giordano, F, additional, Gliwny, P, additional, Godinović, N, additional, Green, J G, additional, Green, D, additional, Hadasch, D, additional, Hahn, A, additional, Heckmann, L, additional, Herrera, J, additional, Hoang, J, additional, Hrupec, D, additional, Hütten, M, additional, Inada, T, additional, Inoue, S, additional, Ishio, K, additional, Iwamura, Y, additional, Jiménez, I, additional, Jormanainen, J, additional, Jouvin, L, additional, Kajiwara, Y, additional, Karjalainen, M, additional, Kerszberg, D, additional, Kobayashi, Y, additional, Kubo, H, additional, Kushida, J, additional, Lamastra, A, additional, Lelas, D, additional, Leone, F, additional, Lindfors, E, additional, Lombardi, S, additional, Longo, F, additional, López-Coto, R, additional, López-Moya, M, additional, López-Oramas, A, additional, Loporchio, S, additional, Machado de Oliveira Fraga, B, additional, Maggio, C, additional, Majumdar, P, additional, Makariev, M, additional, Mallamaci, M, additional, Maneva, G, additional, Manganaro, M, additional, Mannheim, K, additional, Maraschi, L, additional, Mariotti, M, additional, Martínez, M, additional, Mazin, D, additional, Menchiari, S, additional, Mender, S, additional, Mićanović, S, additional, Miceli, D, additional, Miener, T, additional, Minev, M, additional, Miranda, J M, additional, Mirzoyan, R, additional, Molina, E, additional, Moralejo, A, additional, Morcuende, D, additional, Moreno, V, additional, Moretti, E, additional, Neustroev, V, additional, Nigro, C, additional, Nilsson, K, additional, Nishijima, K, additional, Noda, K, additional, Nozaki, S, additional, Ohtani, Y, additional, Oka, T, additional, Otero-Santos, J, additional, Paiano, S, additional, Palatiello, M, additional, Paneque, D, additional, Paoletti, R, additional, Paredes, J M, additional, Pavletić, L, additional, Peñil, P, additional, Perennes, C, additional, Persic, M, additional, Prada Moroni, P G, additional, Prandini, E, additional, Priyadarshi, C, additional, Puljak, I, additional, Rhode, W, additional, Ribó, M, additional, Rico, J, additional, Righi, C, additional, Rugliancich, A, additional, Saha, L, additional, Sahakyan, N, additional, Saito, T, additional, Sakurai, S, additional, Satalecka, K, additional, Saturni, F G, additional, Schleicher, B, additional, Schmidt, K, additional, Schweizer, T, additional, Sitarek, J, additional, Šnidarić, I, additional, Sobczynska, D, additional, Spolon, A, additional, Stamerra, A, additional, Strom, D, additional, Strzys, M, additional, Suda, Y, additional, Surić, T, additional, Takahashi, M, additional, Tavecchio, F, additional, Temnikov, P, additional, Terzić, T, additional, Teshima, M, additional, Tosti, L, additional, Truzzi, S, additional, Tutone, A, additional, Ubach, S, additional, van Scherpenberg, J, additional, Vanzo, G, additional, Vazquez Acosta, M, additional, Ventura, S, additional, Verguilov, V, additional, Vigorito, C F, additional, Vitale, V, additional, Vovk, I, additional, Will, M, additional, Wunderlich, C, additional, Zarić, D, additional, de Palma, F, additional, D’Ammando, F, additional, Barnacka, A, additional, Sahu, D K, additional, Hodges, M, additional, Hovatta, T, additional, Kiehlmann, S, additional, Max-Moerbeck, W, additional, Readhead, A C S, additional, Reeves, R, additional, Pearson, T J, additional, Lähteenmäki, A, additional, Björklund, I, additional, Tornikoski, M, additional, Tammi, J, additional, Suutarinen, S, additional, Hada, K, additional, and Niinuma, K, additional
Published: 2021
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50. C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky.

Author: Harper, S E, Dickinson, C, Barr, A, Cepeda-Arroita, R, Grumitt, R D P, Heilgendorff, H M, Jew, L, Jonas, J L, Jones, M E, Leahy, J P, Leech, J, Pearson, T J, Peel, M W, Readhead, A C S, and Taylor, A C
Subjects: SYNCHROTRON radiation, MICROWAVES, COSMIC background radiation, FREQUENCY spectra, SIGNAL-to-noise ratio, COSMIC rays, STATISTICAL correlation
Abstract: The C-Band All-Sky Survey (C-BASS) has observed the Galaxy at 4.76 GHz with an angular resolution of 0 |${_{.}^{\circ}}$| 73 full-width half-maximum, and detected Galactic synchrotron emission with high signal-to-noise ratio over the entire northern sky (δ > −15○). We present the results of a spatial correlation analysis of Galactic foregrounds at mid-to-high (b > 10○) Galactic latitudes using a preliminary version of the C-BASS intensity map. We jointly fit for synchrotron, dust, and free–free components between 20 and 1000 GHz and look for differences in the Galactic synchrotron spectrum, and the emissivity of anomalous microwave emission (AME) when using either the C-BASS map or the 408-MHz all-sky map to trace synchrotron emission. We find marginal evidence for a steepening (<Δ β > = −0.06 ± 0.02) of the Galactic synchrotron spectrum at high frequencies resulting in a mean spectral index of < β > = −3.10 ± 0.02 over 4.76–22.8 GHz. Further, we find that the synchrotron emission can be well modelled by a single power law up to a few tens of GHz. Due to this, we find that the AME emissivity is not sensitive to changing the synchrotron tracer from the 408-MHz map to the 4.76-GHz map. We interpret this as strong evidence for the origin of AME being spinning dust emission. [ABSTRACT FROM AUTHOR]
Published: 2022
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