Stellar parameters and extinction

DOI

Astrometric surveys provide the opportunity to measure the absolute magnitudes of large numbers of stars, but only if the individual line-of-sight extinctions are known. Unfortunately, extinction is highly degenerate with stellar effective temperature when estimated from broad band optical/infrared photometry. To address this problem, I introduce a Bayesian method for estimating the intrinsic parameters of a star and its line-of-sight extinction.

Cone search capability for table J/MNRAS/411/435/h2mqcat (Stellar parameter estimates and uncertainties)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74110435
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/411/435
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/411/435
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/411/435
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/411/435
Provenance
Creator Bailer-Jones C.A.L.
Publisher CDS
Publication Year 2011
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; Natural Sciences; Observational Astronomy; Physics