Stripe 82-XL: the $\sim$54.8 deg$^2$ and $\sim$18.8 Ms Chandra and XMM-Newton point source catalog and number of counts Article Swipe
Alessandro Peca
,
N. Cappelluti
,
Stephanie LaMassa
,
C. Megan Urry
,
Massimo Moscetti
,
Stefano Marchesi
,
D. B. Sanders
,
Connor Auge
,
Aritra Ghosh
,
Tonima Tasnim Ananna
,
N. Torres-Albà
,
Ezequiel Treister
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2407.09617
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2407.09617
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 $\gtrsim 4σ$. 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 $\sim54.8$ deg$^2$ of non-overlapping 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$\times 10^{-16}$ (2.4$\times 10^{-15}$), 2.9$\times 10^{-15}$ (1.5$\times 10^{-14}$), and 1.4$\times 10^{-15}$ (9.5$\times 10^{-15}$) 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 $1.2\times 10^{38}$ to $1.6\times 10^{47}$ erg s$^{-1}$ in the 2-10 keV band (median X-ray luminosity, $7.2\times 10^{43}$ erg s$^{-1}$), and spectroscopic redshifts up to $z\sim6$. By using hardness ratios, we derived Active Galactic Nuclei (AGNs) obscuration obtaining a median value of $N_H=21.6_{-1.6}^{+1.0}$, and an overall, obscured fraction ($\log N_H/\mathrm{cm^{-2}}>22$) of $\sim 36.9\%$. 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.
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Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2407.09617
- https://arxiv.org/pdf/2407.09617
- OA Status
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- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
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https://doi.org/10.48550/arxiv.2407.09617Digital Object Identifier
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Stripe 82-XL: the $\sim$54.8 deg$^2$ and $\sim$18.8 Ms Chandra and XMM-Newton point source catalog and number of countsWork title
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preprintOpenAlex work type
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enPrimary language
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2024Year of publication
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2024-07-12Full publication date if available
- Authors
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Alessandro Peca, N. Cappelluti, Stephanie LaMassa, C. Megan Urry, Massimo Moscetti, Stefano Marchesi, D. B. Sanders, Connor Auge, Aritra Ghosh, Tonima Tasnim Ananna, N. Torres-Albà, Ezequiel TreisterList of authors in order
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https://arxiv.org/abs/2407.09617Publisher landing page
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https://arxiv.org/pdf/2407.09617Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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| abstract_inverted_index.s$^{-1}$ | 92, 134 |
| abstract_inverted_index.surveys, | 121 |
| abstract_inverted_index.valuable | 196 |
| abstract_inverted_index.$z\sim6$. | 152 |
| abstract_inverted_index.(S82-XL), | 11 |
| abstract_inverted_index.10^{-15}$ | 83, 88 |
| abstract_inverted_index.10^{-16}$ | 79 |
| abstract_inverted_index.benchmark | 184 |
| abstract_inverted_index.cm$^{-2}$ | 93 |
| abstract_inverted_index.extensive | 191 |
| abstract_inverted_index.featuring | 12 |
| abstract_inverted_index.flux-area | 114 |
| abstract_inverted_index.including | 41 |
| abstract_inverted_index.obtaining | 164 |
| abstract_inverted_index.parameter | 115 |
| abstract_inverted_index.redshifts | 149 |
| abstract_inverted_index.$1.2\times | 128 |
| abstract_inverted_index.$1.6\times | 131 |
| abstract_inverted_index.$7.2\times | 143 |
| abstract_inverted_index.$\sim54.8$ | 53 |
| abstract_inverted_index.(half-area | 75 |
| abstract_inverted_index.1.4$\times | 87 |
| abstract_inverted_index.10^{-15}$) | 90 |
| abstract_inverted_index.2.9$\times | 82 |
| abstract_inverted_index.3.4$\times | 78 |
| abstract_inverted_index.XMM-Newton | 49 |
| abstract_inverted_index.additional | 42 |
| abstract_inverted_index.especially | 195 |
| abstract_inverted_index.identified | 22 |
| abstract_inverted_index.rest-frame | 125 |
| abstract_inverted_index.s$^{-1}$), | 146 |
| abstract_inverted_index.(1.5$\times | 84 |
| abstract_inverted_index.(2.4$\times | 80 |
| abstract_inverted_index.(9.5$\times | 89 |
| abstract_inverted_index.10^{-14}$), | 85 |
| abstract_inverted_index.10^{-15}$), | 81 |
| abstract_inverted_index.identifying | 122 |
| abstract_inverted_index.luminosity, | 142 |
| abstract_inverted_index.obscuration | 163 |
| abstract_inverted_index.telescopes. | 50 |
| abstract_inverted_index.luminosities | 126 |
| abstract_inverted_index.significance | 25 |
| abstract_inverted_index.comprehensive | 14, 198 |
| abstract_inverted_index.respectively. | 107 |
| abstract_inverted_index.spectroscopic | 148 |
| abstract_inverted_index.multiwavelength | 192 |
| abstract_inverted_index.non-overlapping | 56 |
| abstract_inverted_index.publicly-available | 7 |
| abstract_inverted_index.$N_H=21.6_{-1.6}^{+1.0}$, | 169 |
| abstract_inverted_index.N_H/\mathrm{cm^{-2}}>22$) | 176 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 12 |
| citation_normalized_percentile |