Cool DZ white dwarfs. I.

White dwarfs with metal lines in their spectra act as signposts for post-main-sequence planetary systems. Searching the Sloan Digital Sky Survey (SDSS) Data Release 12, we have identified 231 cool (300km/s. The implications of our results on remnant planetary systems are to be discussed in a separate paper.

Cone search capability for table J/MNRAS/467/4970/table3 (SDSS PSF photometry for all white dwarfs in our sample)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/467/4970
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/467/4970
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/467/4970
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/467/4970
Provenance
Creator Hollands M.A.; Koester D.; Alekseev V.; Herbert E.L.; Gansicke B.T.
Publisher CDS
Publication Year 2019
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy