no code implementations • 15 Dec 2020 • T. H. Reiprich, A. Veronica, F. Pacaud, M. E. Ramos-Ceja, N. Ota, J. Sanders, M. Kara, T. Erben, M. Klein, J. Erler, J. Kerp, D. N. Hoang, M. Brüggen, J. Marvil, L. Rudnick, V. Biffi, K. Dolag, J. Aschersleben, K. Basu, H. Brunner, E. Bulbul, K. Dennerl, D. Eckert, M. Freyberg, E. Gatuzz, V. Ghirardini, F. Käfer, A. Merloni, K. Migkas, K. Nandra, P. Predehl, J. Robrade, M. Salvato, B. Whelan, A. Diaz-Ocampo, D. Hernandez-Lang, A. Zenteno, M. J. I. Brown, J. D. Collier, J. M. Diego, A. M. Hopkins, A. Kapinska, B. Koribalski, T. Mroczkowski, R. P. Norris, A. O'Brien, E. Vardoulaki
We used dedicated SRG/eROSITA X-ray, ASKAP/EMU radio, and DECam optical observations of a 15 sq. deg region around the interacting galaxy cluster system A3391/95 to study the warm-hot gas in cluster outskirts and filaments, the surrounding large-scale structure and its formation process.
Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena
no code implementations • 30 Aug 2017 • S. De Vito, E. Esposito, M. Salvato, O. Popoola, F. Formisano, R. Jones, G. Di Francia
In this framework, several calibration approaches have been proposed and tested on a variety of proprietary devices and datasets; still, no thorough comparison is available to researchers.
1 code implementation • 8 Apr 2016 • C. Laigle, H. J. McCracken, O. Ilbert, B. C. Hsieh, I. Davidzon, P. Capak, G. Hasinger, J. D. Silverman, C. Pichon, J. Coupon, H. Aussel, D. Le Borgne, K. Caputi, P. Cassata, Y. -Y. Chang, F. Civano, J. Dunlop, J. Fynbo, J. S. kartaltepe, A. Koekemoer, O. Le Fevre, E. Le Floc'h, A. Leauthaud, S. Lilly, L. Lin, S. Marchesi, B. Milvang-Jensen, M. Salvato, D. B. Sanders, N. Scoville, V. Smolcic, M. Stockmann, Y. Taniguchi, L. Tasca, S. Toft, M. Vaccari, J. Zabl
We present the COSMOS2015 catalog which contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg$^{2}$ COSMOS field.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
1 code implementation • 17 Dec 2015 • P. Ranalli, E. Koulouridis, I. Georgantopoulos, S. Fotopoulou, L. -T. Hsu, M. Salvato, A. Comastri, M. Pierre, N. Cappelluti, F. J. Carrera, L. Chiappetti, N. Clerc, R. Gilli, K. Iwasawa, F. Pacaud, S. Paltani, E. Plionis, C. Vignali
The binned luminosity function and its evolution is determined with a variant of the Page-Carrera method, improved to include corrections for absorption and to account for the full probability distribution of photometric redshifts.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics