Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO

Autor: Fabrizio Gentile, Margherita Talia, Meriem Behiri, Giovanni Zamorani, Luigi Barchiesi, Cristian Vignali, Francesca Pozzi, Matthieu Bethermin, Andrea Enia, Andreas L. Faisst, Marika Giulietti, Carlotta Gruppioni, Andrea Lapi, Marcella Massardi, Vernesa Smolčić, Mattia Vaccari, Andrea Cimatti

Publikováno v: The Astrophysical Journal, Vol 962, Iss 1, p 26 (2024)

In the last decades, an increasing scientific interest has been growing in the elusive population of dark (i.e., lacking an optical/near-IR, hereafter NIR, counterpart) dusty star-forming galaxies (DSFGs). Although extremely promising for their likel

Externí odkaz: https://doaj.org/article/45ea0afc8b224f4a81b66733930ca393

Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations

Autor: Vernesa Smolčić, Keiichi Umetsu, Fabio Gastaldello, Keigo Tanaka, Dominique Eckert, Elinor Medezinski, Cathy Horellou, Craig L. Sarazin, Atsushi Yoshida, Sara Stanchfield, Kotaro Kohno, John ZuHone, Tony Mroczkowski, Chong Yang, Brian Mason, Marguerite Pierre, Satoshi Miyazaki, Mark Birkinshaw, Hiroki Akamatsu, Masamune Oguri, Mauro Sereno, Tetsu Kitayama, Jonathan Sievers, Charles Romero, Ayaka Honda, I-Non Chiu, Atsushi J. Nishizawa, Ikuyuki Mitsuishi, Yen-Ting Lin, Florian Pacaud, Kai-Yang Lin, Nobuhiro Okabe, Mark J. Devlin, Simon Dicker, Naomi Ota, Ryoichi Yamamoto

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (2), pp.1701-1732. ⟨10.1093/mnras/staa2330⟩
Monthly Notices of the Royal Astronomical Society, 2021, 501 (2), pp.1701-1732. ⟨10.1093/mnras/staa2330⟩
Okabe, N, Dicker, S, Eckert, D, Mroczkowski, T, Gastaldello, F, Lin, Y-T, Devlin, M, Romero, C E, Birkinshaw, M, Sarazin, C, Horellou, C, Kitayama, T, Umetsu, K, Sereno, M, Mason, B S, ZuHone, J A, Honda, A, Akamatsu, H, Chiu, I-N, Kohno, K, Lin, K-Y, Medezinski, E, Miyazaki, S, Mitsuishi, I, Nishizawa, A J, Oguri, M, Ota, N, Pacaud, F, Pierre, M, Sievers, J, Smolcic, V, Stanchfield, S, Tanaka, K, Yamamoto, R, Yang, C & Yoshida, A 2021, ' Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations ', Monthly Notices of the Royal Astronomical Society, vol. 501, no. 2, staa2330, pp. 1701–1732 . https://doi.org/10.1093/mnras/staa2330

We present results from simultaneous modeling of high angular resolution GBT/MUSTANG-2 90 GHz Sunyaev-Zel'dovich effect (SZE) measurements and XMM-XXL X-ray images of three rich galaxy clusters selected from the HSC-SSP Survey. The combination of hig

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfc7611f1fdb6c75cc1425bd089eac07
https://hal.archives-ouvertes.fr/hal-02431455

The XXL Survey. XLIII. The quasar radio loudness dichotomy exposed via radio luminosity functions obtained by combining results from COSMOS and XXL-S X-ray selected quasars

Autor: Sarah K. Leslie, J. Delhaize, Stefano Marchesi, Vernesa Smolčić, A. Butler, Jeyhan S. Kartaltepe, Manolis Plionis, Konstantinos Kolokythas, Eleni Vardoulaki, L. Ceraj, Marguerite Pierre, K. Tisanić, Mladen Novak, Cathy Horellou, Ivan Delvecchio, G. Zamorani

Publikováno v: Astronomy and Astrophysics
Volume 642

We studied a sample of 274 radio and X-ray selected quasars (XQSOs) detected in the COSMOS and XXL-S radio surveys at 3 GHz and 2.1 GHz, respectively. This sample was identified by adopting a conservative threshold in X-ray luminosity, Lx [2-10\ keV]

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b72f4d901c8155299079414ff46b5f89
https://repozitorij.pmf.unizg.hr/islandora/object/pmf:9070

The XXL Survey

Autor: Konstantinos Kolokythas, M. N. Bremer, K. Tisanić, Mark Birkinshaw, Cathy Horellou, Bruno Šlaus, H. J. A. Röttgering, Paolo Ciliegi, L. Ceraj, Mladen Novak, M. Huynh, Sotiria Fotopoulou, L. Chiappetti, Marguerite Pierre, Somak Raychaudhury, Hubertus Intema, Vernesa Smolčić, N. Jurlin

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy and astrophysics, 638:A46. EDP Sciences
Astronomy and Astrophysics
Volume 638
Astronomy and Astrophysics-A&A, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy & Astrophysics, 638, A46

We study the space density evolution of active galactic nuclei (AGN) using the 610 MHz radio survey of the XXL-North field, performed with the Giant Metrewave Radio Telescope. The survey covers an area of 30.4 deg2, with a beamsize of 6.5 arcsec. The

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b228e5bc7676e310a7490f807fc01607
https://hal-cea.archives-ouvertes.fr/cea-02863069/file/aa37258-19.pdf

A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population

Autor: J. A. Hodge, Fabian Walter, H. S. B. Algera, H. J. A. Röttgering, Ian Smail, Vernesa Smolčić, D. van der Vlugt, Dominik Riechers, J. F. Radcliffe, M. Novak

Publikováno v: Astrophysical journal, 2020, Vol.903(2), pp.139 [Peer Reviewed Journal]
The Astrophysical Journal, 903(2), 139

Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio AGN to be used to their fullest potential. We study the composition of the $\mu$Jy radio popul

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e231b55111549147ae420023d9d1735e