ATMO 2020, NEQ strong Virtual Observatory Resource

Authors
  1. Phillips et al. 2020
    2. Published by
    SVO CAB
Abstract

A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Non equilibrium chemistry (strong). Valid temperature range: 200-2000K. Only for solar metallicity.

Keywords
  1. star
Bibliographic source HTTP
https://ui.adsabs.harvard.edu/abs/2020A%26A...637A..38P
See also HTML
https://ui.adsabs.harvard.edu/abs/2020A%26A...637A..38P
IVOA Identifier IVOID
ivo://svo.cab/models/atmo2020/neq_strong

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=atmo2020_neq_strong&

History

2022-09-27T13:17:57.481
Resource record created

Contact

Name
Enrique Solano, LAEFF Archive Support Team
E-Mail
esm@cab.inta-csic.es