Computer Science
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..33390858d&link_type=abstract
VizieR On-line Data Catalog: J/A+A/339/858. Originally published in: 1998A&A...339..858D
Computer Science
Stars: Dwarfs, Stars: Giant, Parallaxes: Trigonometric, Effective Temperatures, Photometry: Infrared
Scientific paper
The results of calibration of the surface brightness, bolometric flux and effective temperature scales are presented for 537 dwarfs and giants selected as standards for the Infrared Space Observatory (ISO). Individual temperatures with small model-dependent corrections are derived at the target accuracy of 1%. The comparison with semiempirical values achieved by the Infrared Flux Method (IRFM) shows consistent results within the 1% level for F, G and K stars, but not for A-type stars. (2 data files).
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