Catalog Service: Arches and Quintuplet Clusters Chandra X-Ray Point Source Catalog
Description
The Galactic centre (GC) provides a unique laboratory for a detailed examination of the interplay between massive star formation and the nuclear environment of our Galaxy. Here are presented some of the results from a 100-ks Chandra Advanced CCD Imaging Spectrometer (ACIS) observation of the Arches and Quintuplet star clusters in the form of a catalog of 244 point-like X-ray sources detected in the observation. The deep Chandra ACIS-I observation (Obs. ID: 4500) was carried out on 2004 June 9. The Arches cluster was placed about 1-arcmin away from the aim point to minimize the effect of the CCD gaps on mapping the extended X-ray emission around the cluster. This table was created by the HEASARC in July 2007 based on <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/371/38">CDS Catalog J/MNRAS/371/38</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 Feb 21 00:00:00ZThis resource description was last updated on: 2025 Feb 21 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