Catalog Service: Effective temperature scale of FGK stars
Description
The infrared flux method (IRFM) has been applied to a sample of 135 dwarf and 36 giant stars covering the following regions of the atmospheric parameter space: (1) the metal-rich ([Fe/H]>~0) end (consisting mostly of planet-hosting stars), (2) the cool (Teff<~5000K) metal-poor (-1<~[Fe/H]<~-3) dwarf region, and (3) the very metal-poor ([Fe/H]<~-2.5) end.
This section describes who is responsible for this resource
Publisher: CDS[+]ivo://CDS[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2007 Oct 27 11:27:21ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
Related Resources:
This section describes the data's coverage over the sky, frequency, and time.
Wavebands covered:
This section describes the rights and usage information for this data.
This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/ApJ/626/446/table2 (Input data adopted, effective temperatures and angular diameters derived in this work)
VERB=1
VERB=3
Cone search capability for table J/ApJ/626/446/table4 (Dwarf and subgiant stars with measured angular diameters)
Cone search capability for table J/ApJ/626/446/table3 (Giant stars with measured angular diameters in Richichi & Percheron (Cat. <J/A+A/386/492>) and Mozurkewich et al. (2003AJ....126.2502M))
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute