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Sökning: WFRF:(Koulouridis E.) > (2022) > XXL-HSC: An updated...

XXL-HSC: An updated catalogue of high-redshift (z3.5) X-ray AGN in the XMM-XXL northern field: Constraints on the bright end of the soft log N -log S

Pouliasis, E. (författare)
National Observatory of Athens
Georgantopoulos, I. (författare)
National Observatory of Athens
Ruiz, A. (författare)
National Observatory of Athens
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Gilli, R. (författare)
Istituto nazionale di astrofisica (INAF)
Koulouridis, E. (författare)
National Observatory of Athens
Akiyama, M. (författare)
Tohoku University
Ueda, Y. (författare)
Kyoto University
Chiappetti, L. (författare)
Istituto nazionale di astrofisica (INAF)
Garrel, C. (författare)
Université Paris-Saclay,University Paris-Saclay
Horellou, Cathy, 1967 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Nagao, T. (författare)
Ehime University
Paltani, S. (författare)
Université de Genève,University of Geneva
Pierre, M. (författare)
Université Paris-Saclay,University Paris-Saclay
Toba, Y. (författare)
Academia Sinica Taiwan,Ehime University,Kyoto University
Vignali, C. (författare)
Universita di Bologna,University of Bologna,Istituto nazionale di astrofisica (INAF)
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 (creator_code:org_t)
2022-02-18
2022
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 658
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • 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. In this work, we built a high-redshift (z3.5) 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 (f0.52 keV>10 15 ergs 1 cm2). The samples of z 3.5, z4, and z5 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.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)

Nyckelord

Early Universe
Methods: statistical
Methods: data analysis
Methods: observational
Galaxies: active
X-rays: galaxies

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