BT-DUSTY Virtual Observatory Resource

Authors

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

Published by

SVO CAB

Abstract

The BT-DUSTY Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling) and 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-dusty

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-dusty&