Spectral Analysis in the Virtual Observatory
| dc.creator | Rauch, Thomas | |
| dc.creator | Nickelt, Iliya | |
| dc.date | 2009-01-27 | |
| dc.date.accessioned | 2026-07-07T12:34:50Z | |
| dc.date.available | 2026-07-07T12:34:50Z | |
| dc.description | In a collaboration of the German Astrophysical Virtual Observatory (GAVO) and AstroGrid-D, the German Astronomy Community Grid (GACG), we provide a VO service for the access and the calculation of stellar synthetic energy distributions (SEDs) based on static as well as expanding non-LTE model atmospheres. At three levels, a VO user may directly compare observed and theoretical SEDs: The easiest and fastest way is to use pre-calculated SEDs from the GAVO database. For individual objects, grids of model atmospheres and SEDs can be calculated on the compute resources of AstroGrid-D within reasonable wallclock time. Experienced VO users may even create own atomic-data files for a more detailed analyses. | |
| dc.description | 3 pages | |
| dc.identifier | https://arxiv.org/abs/0901.4202 | |
| dc.identifier | http://arxiv.org/abs/0901.4202 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/217582 | |
| dc.subject | Solar and Stellar Astrophysics | |
| dc.title | Spectral Analysis in the Virtual Observatory | |
| dc.type | text |