BT-COND Virtual Observatory Resource

Authors

1. Hauschildt, P.H., Allard, F., Baron, E., ApJ 512, 377, 1999

Published by

SVO CAB

Abstract

The BT-COND Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation and no dust opacity (no dust settling) but updated abundances. Wavelengths have been converted to air wavelengths.

Keywords

1. star

Bibliographic source HTTP

http://phoenix.ens-lyon.fr/simulator/index.faces

See also HTML

http://svo.cab.inta-csic.es/

IVOA Identifier IVOID

ivo://svo.cab/models/bt-cond

Access

IVOA Simple Spectrum Search SSAP

For use with a VO-enabled spectral analysis program (e.g., Splat, VOSpec).
http://svo2.cab.inta-csic.es/theory/newov2/ssap.php?model=bt-cond&