In the framework of the Virtual Observatory, the GAVO project provides theoretical spectral energy distributions (SEDs) of TMAP NLTE model atmospheres within the GAVO TheoSSA service.
TheoSSA gives a VO user easy access to pre-calculated SED grids. In case that no suitable SED is available, the VO user is transferred to TMAW, the WWW interface to calculate individual SEDs from H+He+C+N+O+Ne+Mg models using TMAP. SEDs are automatically ingested in the GAVO database
2010, January
1st TMAW
model atmosphere was
calculated successfully on compute resources of
AstroGrid-D.
2010, September
1st extended TMAW
model-atmosphere grid was
calculated successfully on compute resources of
AstroGrid-D.
2013, February
A new tool,
TEUV,
to simulate interstellar absorption in EUV spectra,
and a new service,
TIRO,
to create model atoms for iron-group elements (Ca - Ni)
and to calculate respective bound-bound and bound-free
absorption cross-sections were registered.
2013, April
Sodium added to
TMAD.
2013, May
Sodium included in
TMAW.