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The eROSITA Final Equatorial-Depth Survey (eFEDS): The AGN Catalogue and its X-ray Spectral Properties

Authors :
Liu, Teng
Buchner, Johannes
Nandra, Kirpal
Merloni, Andrea
Dwelly, Tom
Sanders, Jeremy S.
Salvato, Mara
Arcodia, Riccardo
Brusa, Marcella
Wolf, Julien
Georgakakis, Antonis
Boller, Thomas
Krumpe, Mirko
Lamer, Georg
Waddell, Sophia
Urrutia, Tanya
Schwope, Axel
Robrade, Jan
Wilms, Jörn
Dauser, Thomas
Comparat, Johan
Toba, Yoshiki
Ichikawa, Kohei
Iwasawa, Kazushi
Shen, Yue
Medel, Hector Ibarra
Source :
A&A 661, A5 (2022)
Publication Year :
2021

Abstract

Context: After the successful launch of the Spectrum-Roentgen-Gamma (SRG) mission in July 2019, eROSITA, the soft X-ray instrument aboard SRG, performed scanning observations of a large contiguous field, namely the eROSITA Final Equatorial Depth Survey (eFEDS), ahead of the planned four-year all-sky survey. eFEDS yielded a large sample of X-ray sources with very rich multi-band photometric and spectroscopic coverage. Aims: We present here the eFEDS Active Galactic Nuclei (AGN) catalog and the eROSITA X-ray spectral properties of the eFEDS sources. Methods: Using a Bayesian method, we perform a systematic X-ray spectral analysis for all eFEDS sources. The appropriate model is chosen based on the source classification and the spectral quality, and, in the case of AGN, including the possibility of intrinsic (rest-frame) absorption and/or soft excess emission. Hierarchical Bayesian modeling (HBM) is used to estimate the spectral parameter distribution of the sample. Results: X-ray spectral properties are presented for all eFEDS X-ray sources. There are 21952 candidate AGN, which comprise 79% of the eFEDS sample. Despite a large number of faint sources with low photon counts, our spectral fitting provides meaningful measurements of fluxes, luminosities, and spectral shapes for a majority of the sources. This AGN catalog is dominated by X-ray unobscured sources, with an obscured (logNH>21.5) fraction of 10% derived by HBM. The power-law slope of the catalog can be described by a Gaussian distribution of 1.94+-0.22. Above a photon counts threshold of 500, nine out of 50 AGN have soft excess detected. For the sources with blue UV to optical color (type-I AGN), the X-ray emission is well correlated with the UV emission with the usual anti-correlation between the X-ray to UV spectral slope {\alpha}_{OX} and the UV luminosity.<br />Comment: Submitted to A&A for the Special Issue: The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG Mission 24 pages, 23 figures

Details

Database :
arXiv
Journal :
A&A 661, A5 (2022)
Publication Type :
Report
Accession number :
edsarx.2106.14522
Document Type :
Working Paper
Full Text :
https://doi.org/10.1051/0004-6361/202141643