Catalog Service: Levenhagen 2017
Description
A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.
This section describes who is responsible for this resource
Publisher: SVO CABivo://svo.cab[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2010 Aug 17 12:36:47ZThis resource description was last updated on: 2019 Sep 04 08:31:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
This is a standard IVOA service for searches for spectra from this resource that were observed within a specified region of the sky.
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute