The final SDSS-IV/SPIDERS X-ray point source spectroscopic catalogue
J. Comparat, A. Merloni, T. Dwelly, M. Salvato, A. Schwope, D. Coffey,, J. Wolf, R. Arcodia, T. Liu, J. Buchner, K. Nandra, A. Georgakakis, N. Clerc,, M. Brusa, J. R. Brownstein, D. P. Schneider, K. Pan, D. Bizyaev

TL;DR
This paper presents the largest systematic spectroscopic catalog of X-ray sources from SDSS-IV/SPIDERS, providing classifications, redshifts, and insights into AGN properties, supporting future eROSITA survey studies.
Contribution
It offers a comprehensive, high-quality spectroscopic catalog of X-ray sources, including classifications and redshifts for nearly all observed objects, and analyzes AGN properties systematically.
Findings
98.9% of observed objects are classified
97.8% have secure redshifts
AGN spectra show systematic differences in H-beta profiles
Abstract
We look to provide a detailed description of the SPectroscopic IDentification of ERosita Sources (SPIDERS) survey, an SDSS-IV programme aimed at obtaining spectroscopic classification and redshift measurements for complete samples of sufficiently bright X-ray sources. We describe the SPIDERS X-ray Point Source Spectroscopic Catalogue, considering its store of 11,092 observed spectra drawn from a parent sample of 14,759 ROSAT and XMM sources over an area of 5,129 deg covered in SDSS-IV by the eBOSS survey. This programme represents the largest systematic spectroscopic observation of an X-ray selected sample. A total of 10,970 (98.9\%) of the observed objects are classified and 10,849 (97.8\%) have secure redshifts. The majority of the spectra (10,070 objects) are active galactic nuclei (AGN), 522 are cluster galaxies, and 294 are stars. The observed AGN redshift distribution is in…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
