XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field
Abstract
X-rays offer a reliable method to identify active galactic nuclei (AGNs). However, in the high-redshift Universe, X-ray AGNs are poorly sampled due to their relatively low space density and the small areas covered by X-ray surveys. In addition to wide-area X-ray surveys, it is important to have deep optical data in order to locate the optical counterparts and determine their redshifts. Here, in this work, we built a high-redshift (z ≥ 3.5) X-ray-selected AGN sample in the XMM-XXL northern field using the most updated [0.5–2 keV] catalogue along with a plethora of new spectroscopic and multi-wavelength catalogues, including the deep optical Subaru Hyper Suprime-Cam (HSC) data, reaching magnitude limits i ~ 26 mag. We selected all the spectroscopically confirmed AGN and complement this sample with high-redshift candidates that are HSC g- and r-band dropouts. To confirm the dropouts, we derived their photometric redshifts using spectral energy distribution techniques. We obtained a sample of 54 high-z sources (28 with spec-z), the largest in this field so far (almost three times larger than in previous studies), and we estimated the possible contamination and completeness. We calculated the number counts (log N-log S) in different redshift bins and compared our results with previousmore »
- Authors:
-
- National Observatory of Athens (Greece)
- Istituto Nazionale di Astrofisica (INAF) (Italy)
- Tohoku Univ., Sendai (Japan)
- Kyoto Univ. (Japan)
- Centre National de la Recherche Scientifique (CNRS) (France); Commissariat a l'Energie Atomique (CEA) (France); Univ. Paris-Saclay, Gif-sur-Yvette (France); University Paris-Diderot (France)
- Chalmers University of Technology (Sweden)
- Ehime Univ., Matsuyama (Japan)
- Univ. of Geneva (Switzerland)
- Kyoto Univ. (Japan); Ehime Univ., Matsuyama (Japan); Academia Sinica, Taipei (Taiwan)
- Univ. of Bologna (Italy); Istituto Nazionale di Astrofisica (INAF) (Italy)
- Publication Date:
- Research Org.:
- US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)
- Sponsoring Org.:
- USDOE Office of Science (SC); Alfred P. Sloan Foundation
- OSTI Identifier:
- 1982304
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Astronomy and Astrophysics
- Additional Journal Information:
- Journal Volume: 658; Journal ID: ISSN 0004-6361
- Publisher:
- EDP Sciences
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; active galaxies; x-rays; data analysis; observational methods; statistical methods; early universe
Citation Formats
Pouliasis, E., Georgantopoulos, I., Ruiz, A., Gilli, R., Koulouridis, E., Akiyama, M., Ueda, Y., Chiappetti, L., Garrel, C., Horellou, C., Nagao, T., Paltani, S., Pierre, M., Toba, Y., and Vignali, C. XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field. United States: N. p., 2022.
Web. doi:10.1051/0004-6361/202142059.
Pouliasis, E., Georgantopoulos, I., Ruiz, A., Gilli, R., Koulouridis, E., Akiyama, M., Ueda, Y., Chiappetti, L., Garrel, C., Horellou, C., Nagao, T., Paltani, S., Pierre, M., Toba, Y., & Vignali, C. XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field. United States. https://doi.org/10.1051/0004-6361/202142059
Pouliasis, E., Georgantopoulos, I., Ruiz, A., Gilli, R., Koulouridis, E., Akiyama, M., Ueda, Y., Chiappetti, L., Garrel, C., Horellou, C., Nagao, T., Paltani, S., Pierre, M., Toba, Y., and Vignali, C. Fri .
"XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field". United States. https://doi.org/10.1051/0004-6361/202142059. https://www.osti.gov/servlets/purl/1982304.
@article{osti_1982304,
title = {XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field},
author = {Pouliasis, E. and Georgantopoulos, I. and Ruiz, A. and Gilli, R. and Koulouridis, E. and Akiyama, M. and Ueda, Y. and Chiappetti, L. and Garrel, C. and Horellou, C. and Nagao, T. and Paltani, S. and Pierre, M. and Toba, Y. and Vignali, C.},
abstractNote = {X-rays offer a reliable method to identify active galactic nuclei (AGNs). However, in the high-redshift Universe, X-ray AGNs are poorly sampled due to their relatively low space density and the small areas covered by X-ray surveys. In addition to wide-area X-ray surveys, it is important to have deep optical data in order to locate the optical counterparts and determine their redshifts. Here, in this work, we built a high-redshift (z ≥ 3.5) X-ray-selected AGN sample in the XMM-XXL northern field using the most updated [0.5–2 keV] catalogue along with a plethora of new spectroscopic and multi-wavelength catalogues, including the deep optical Subaru Hyper Suprime-Cam (HSC) data, reaching magnitude limits i ~ 26 mag. We selected all the spectroscopically confirmed AGN and complement this sample with high-redshift candidates that are HSC g- and r-band dropouts. To confirm the dropouts, we derived their photometric redshifts using spectral energy distribution techniques. We obtained a sample of 54 high-z sources (28 with spec-z), the largest in this field so far (almost three times larger than in previous studies), and we estimated the possible contamination and completeness. We calculated the number counts (log N-log S) in different redshift bins and compared our results with previous studies and models. We provide the strongest high-redshift AGN constraints yet at bright fluxes (f0.5 – 2 keV > 10–15 erg s–1 cm–2). The samples of z ≥ 3.5, z ≥ 4, and z ≥ 5 are in agreement with an exponential decline model similar to that witnessed at optical wavelengths. Our work emphasises the importance of using wide-area X-ray surveys with deep optical data to uncover high-redshift AGNs.},
doi = {10.1051/0004-6361/202142059},
journal = {Astronomy and Astrophysics},
number = ,
volume = 658,
place = {United States},
year = {Fri Feb 18 00:00:00 EST 2022},
month = {Fri Feb 18 00:00:00 EST 2022}
}
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