Catalog Service: Kvant TTM/COMIS X-Ray Source Catalog
Description
A catalog of X-ray sources in the 2-30 keV energy band as observed by the TTM/COMIS (Coded Mask Imaging Spectrometer) telescope onboard the Mir-Kvant observatory is presented. Brief information about the 67 sources detected at a confidence level higher than 4 sigma between 1988 and 1998 is provided. X-ray properties and characteristic spectra of different types of sources are briefly described in the reference paper. This table was created by the HEASARC in April 2011 based on the <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/PAZh/26/355">CDS catalog J/PAZh/26/355</a> file table1.dat. This is a service provided by NASA HEASARC .
This section describes who is responsible for this resource
Publisher: NASA/GSFC HEASARCivo://nasa.heasarc/ASD[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2025 Apr 25 00:00:00ZThis resource description was last updated on: 2025 Apr 25 00:00:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
Related Resources:
This section describes the data's coverage over the sky, frequency, and time.
Reference Coordinate System: UTC-ICRS-TOPOXXivo://STClib/CoordSys#UTC-ICRS-TOPO[Res. ID]
Sky Coverage: Regions covered:
Wavebands covered:
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
VERB=1
VERB=3
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
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