TheoSSA TMAP Web Interface Virtual Observatory Resource

Authors
  1. Rauch, T.
    2. Published by
    The GAVO DC team
Abstract
TheoSSA provides spectral energy distributions based on model
atmosphere calculations. Currently, we serve results obtained using
the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact
stars.
Keywords
  1. spectroscopy
  2. astronomical-simulations
  3. post-asymptotic-giant-branch-stars
  4. stellar-atmospheres
Bibliographic source Bibcode
2018MNRAS.475.3896R
See also HTML
http://dc.zah.uni-heidelberg.de/theossa/q/web/info
IVOA Identifier IVOID
ivo://org.gavo.dc/theossa/q/web
Document Object Identifer DOI

Access

Web browser access HTML
http://dc.zah.uni-heidelberg.de/theossa
https://dc.zah.uni-heidelberg.de/theossa
IVOA Table Access TAP
http://dc.zah.uni-heidelberg.de/tap
https://dc.zah.uni-heidelberg.de/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
Unknown endpoint
Capability for unknown standard ivo://ivoa.net/std/soda#sync-1.0. The VO Registry may have more details; look for IVOID ivo://org.gavo.dc/theossa/q/web.
Unknown endpoint
Capability for unknown standard ivo://ivoa.net/std/datalink#links-1.1. The VO Registry may have more details; look for IVOID ivo://org.gavo.dc/theossa/q/web.

History

2010-11-11T15:00:00Z
Resource record created
2022-01-13T13:38:11Z
updated

Contact

Name
Thomas Rauch
E-Mail
gavo@listserv.uni-tuebingen.de
Telephone
++49 7071 2978614