A catalogue of cataclysmic variables from 20 yr of the Sloan Digital Sky Survey with new classifications, periods, trends, and oddities

Author:

Inight Keith1ORCID,Gänsicke Boris T1ORCID,Breedt Elmé2ORCID,Israel Henry T3,Littlefair Stuart P3ORCID,Manser Christopher J14,Marsh Tom R1ORCID,Mulvany Tim1,Pala Anna Francesca5ORCID,Thorstensen John R6

Affiliation:

1. Department of Physics, University of Warwick , Coventry, CV4 7AL , UK

2. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA , United Kingdom

3. Department of Physics and Astronomy, University of Sheffield , Sheffield S3 7RH , UK

4. Astrophysics Group, Department of Physics , Imperial College London, Prince Consort Rd, London SW7 2AZ , UK

5. European Space Agency, European Space Astronomy Centre , Camino Bajo del Castillo s/n, Villanueva de la Cañada, E-28692 Madrid , Spain

6. Department of Physics and Astronomy , Dartmouth College, Hanover NH 03755 , USA

Abstract

ABSTRACT We present a catalogue of 507 cataclysmic variables (CVs) observed in SDSS I to IV including 70 new classifications collated from multiple archival data sets. This represents the largest sample of CVs with high-quality and homogeneous optical spectroscopy. We have used this sample to derive unbiased space densities and period distributions for the major sub-types of CVs. We also report on some peculiar CVs, period bouncers and also CVs exhibiting large changes in accretion rates. We report 70 new CVs, 59 new periods, 178 unpublished spectra, and 262 new or updated classifications. From the SDSS spectroscopy, we also identified 18 systems incorrectly identified as CVs in the literature. We discuss the observed properties of 13 peculiar CVS, and we identify a small set of eight CVs that defy the standard classification scheme. We use this sample to investigate the distribution of different CV sub-types, and we estimate their individual space densities, as well as that of the entire CV population. The SDSS I to IV sample includes 14 period bounce CVs or candidates. We discuss the variability of CVs across the Hertzsprung–Russell diagram, highlighting selection biases of variability-based CV detection. Finally, we searched for, and found eight tertiary companions to the SDSS CVs. We anticipate that this catalogue and the extensive material included in the Supplementary Data will be useful for a range of observational population studies of CVs.

Funder

Alfred P. Sloan Foundation

National Science Foundation

U.S. Department of Energy

Brookhaven National Laboratory

Carnegie Mellon University

University of Florida

Johns Hopkins University

Lawrence Berkeley National Laboratory

New Mexico State University

New York University

Ohio State University

Pennsylvania State University

University of Portsmouth

Princeton University

University of Tokyo

University of Utah

Vanderbilt University

University of Virginia

University of Washington

Yale University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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