TheoSSA TMAP Web Interface

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.
Range of the atmosphere's effective temperatures to include. If you only specify one bound, you get a half-infinite interval.
Range of surface gravities to include. If you only specify one bound, you get a half-infinite interval.
Range of mass loss rates to include. If you only specify one bound, you get a half-infinite interval.
Mass fraction of an element. You may leave out either upper or lower bound.
Mass fraction of an element. You may leave out either upper or lower bound.
Mass fraction of an element. You may leave out either upper or lower bound.
No selection matches all, multiple values legal.
Common name of object observed.
Sort by
Limit to items.
When publishing research making use of this service, please acknowledge: "The TheoSSA service (http://dc.g-vo.org/theossa) used to retrieve theoretical spectra for this paper was constructed as part of the activities of the German Astrophysical Virtual Observatory."