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Stripe 82-XL: The ∼54.8 deg 2 and ∼18.8 Ms Chandra and XMM-Newton Point-source Catalog and Number of Counts.

Authors :
Peca, Alessandro
Cappelluti, Nico
LaMassa, Stephanie
Urry, C. Megan
Moscetti, Massimo
Marchesi, Stefano
Sanders, David
Auge, Connor
Ghosh, Aritra
Ananna, Tonima Tasnim
Torres-Albà, Núria
Treister, Ezequiel
Source :
Astrophysical Journal. 10/20/2024, Vol. 974 Issue 2, p1-13. 13p.
Publication Year :
2024

Abstract

We present an enhanced version of the publicly available Stripe 82X catalog (S82-XL), featuring a comprehensive set of 22,737 unique X-ray point sources identified with a significance ≳4 σ. This catalog is four times larger than the original Stripe 82X catalog, by including additional archival data from the Chandra and XMM-Newton telescopes. Now covering ∼54.8 deg2 of nonoverlapping sky area, the S82-XL catalog roughly doubles the area and depth of the original catalog, with limiting fluxes (half-area fluxes) of 3.4 × 10−16 (2.4 × 10−15), 2.9 × 10−15 (1.5 × 10−14), and 1.4 × 10−15 (9.5 × 10−15) erg s−1 cm−2 across the soft (0.5–2 keV), hard (2–10 keV), and full (0.5–10 keV) bands, respectively. S82-XL occupies a unique region of flux-area parameter space compared to other X-ray surveys, identifying sources with rest-frame luminosities from 1.2 × 1038 to 1.6 × 1047 erg s−1 in the 2–10 keV band (median X-ray luminosity, 7.2 × 1043 erg s−1), and spectroscopic redshifts up to z ∼ 6. By using hardness ratios, we derived the obscuration of active galactic nuclei (AGNs), obtaining a median value of log (N H / cm − 2) = 21.6 − 1.6 + 1.0 and an overall, obscured fraction ( log (N H / cm − 2) > 22 ) of ∼36.9%. S82-XL serves as a benchmark in X-ray surveys and, with its extensive multiwavelength data, is especially valuable for comprehensive studies of luminous AGNs. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0004637X
Volume :
974
Issue :
2
Database :
Academic Search Index
Journal :
Astrophysical Journal
Publication Type :
Academic Journal
Accession number :
180254584
Full Text :
https://doi.org/10.3847/1538-4357/ad6df4