Service: Synthetic Spectra Convolution Service
Description
Convolution of normalized synthetic stellar spectra. Up to 3 successive convolutions are allowed on a adjustable portion of a synthetic spectrum, in order to mimic an observable. These convolutions acount for macroturbulence velocity, rotational velocity and instrumental profile. Finally, the output can be Doppler-shifted in order to take into account a stellar radial velocity.
This section describes who is responsible for this resource
Publisher: OV-GSO Virtual Observatory servicesivo://ov-gso[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2014 May 20 05:28:23ZThis resource description was last updated on: 2024 Apr 03 08:16:45Z
This section describes what the resource is, what it contains, and how it might be relevant.
Related Resources:
This section describes the rights and usage information for this data.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
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