THE CHANDRA SOURCE CATALOG
Creators
- Evans, Ian N.1
- Primini, Francis A.1
- Glotfelty, Kenny J.1
- Anderson, Craig S.1
- Bonaventura, Nina R.1
- Chen, Judy C.1
- Doe, Stephen M.1
- Evans, Janet D.1
- Fabbiano, Giuseppina1
- Galle, Elizabeth C.1
- Gibbs, Danny G.1
- Grier, John D.1
- Hain, Roger M.1
- Harbo, Peter N.1
- He Xiangqun1
- Karovska, Margarita1
- Kashyap, Vinay L.1
- Davis, John E.2
- Houck, John C.2
- Hall, Diane M.3
- and others
- 1. Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)
- 2. MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States)
- 3. Northrop Grumman, 60 Garden Street, Cambridge, MA 02138 (United States)
Description
The Chandra Source Catalog (CSC) is a general purpose virtual X-ray astrophysics facility that provides access to a carefully selected set of generally useful quantities for individual X-ray sources, and is designed to satisfy the needs of a broad-based group of scientists, including those who may be less familiar with astronomical data analysis in the X-ray regime. The first release of the CSC includes information about 94,676 distinct X-ray sources detected in a subset of public Advanced CCD Imaging Spectrometer imaging observations from roughly the first eight years of the Chandra mission. This release of the catalog includes point and compact sources with observed spatial extents ∼<30''. The catalog (1) provides access to the best estimates of the X-ray source properties for detected sources, with good scientific fidelity, and directly supports scientific analysis using the individual source data; (2) facilitates analysis of a wide range of statistical properties for classes of X-ray sources; and (3) provides efficient access to calibrated observational data and ancillary data products for individual X-ray sources, so that users can perform detailed further analysis using existing tools. The catalog includes real X-ray sources detected with flux estimates that are at least 3 times their estimated 1σ uncertainties in at least one energy band, while maintaining the number of spurious sources at a level of ∼<1 false source per field for a 100 ks observation. For each detected source, the CSC provides commonly tabulated quantities, including source position, extent, multi-band fluxes, hardness ratios, and variability statistics, derived from the observations in which the source is detected. In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively, including source images, event lists, light curves, and spectra from each observation in which a source is detected.
Availability note (English)
Available from http://dx.doi.org/10.1088/0067-0049/189/1/37Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal, Supplement Series
- Journal Volume
- 189
- Journal Issue
- 1
- Journal Page Range
- p. 37-82
- ISSN
- 0067-0049
- CODEN
- APJSA2
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42049688
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; CATALOGS; COSMIC X-RAY SOURCES; DATA ANALYSIS; SPECTROMETERS
- Descriptors DEC
- COSMIC RAY SOURCES; DOCUMENT TYPES; MEASURING INSTRUMENTS; PHYSICS