Levenhagen 2017 Virtual Observatory Resource

Authors

1. Levenhagen, Diaz, Coelho, Hubeny, ApJ Volume 231, Issue 1, article id. 1, 6 pp. (2017).

Published by

SVO CAB

Abstract

A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.

Keywords

1. star

Bibliographic source HTTP

http://specmodels.iag.usp.br/

See also HTML

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

IVOA Identifier IVOID

ivo://svo.cab/models/levenhagen

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=levenhagen17&