GSC - Hubble Space Telescope Guide Star Catalog (1.1)


Overview

The GSC was constructed from 1477 Schmidt plates covering the standard survey grids plus 39 supplemental plates. The GSC as distributed on the cd-roms contains 25,126,027 entries for 18,819,291 objects with magnitudes between 8.5 and 15. Of these 15,169,873 are stars and 3,649,418 are not. The GSC as contained in the HEASARC database has been compressed to only have one entry per object. This compression process finds 18,818,613 objects, 678 objects fewer than advertised.

Each entry contains a position, a Quasi-V magnitude (`QV mag`) and a Quasi-B magnitude (`QB mag`). The former comes mostly from the northern Palomar survey, and the latter from the UK SERC Schmidt survey. Near equatorial regions, where the surveys overlap, both magnitudes are available. But for the majority of cases only one or the other will be given. A code (`CV` and `CB`) gives further information on the emulsion and filter used.

The default cone search radius is 1 arc minute. Be careful in selecting larger values for the cone search radius: for example, setting it to be 30 arcminutes will typically result in a sample that contains hundreds, if not thousands, of stars. We recommend that cone search radii of more than 30 arcminutes not be used.


Description

The GSC was constructed from 1477 Schmidt plates covering the standard survey grids plus 39 supplemental plates. The GSC as distributed on the cd-roms contains 25,126,027 entries for 18,819,291 objects with magnitudes between 8.5 and 15. Of these 15,169,873 are stars and 3,649,418 are not. The GSC as contained in the EXOSAT database has been compressed to only have one entry per object. This compression process finds 18,818,613 objects, 678 objects fewer than advertised.

Each entry contains a position, a Quasi-V magnitude (`QV mag`) and a Quasi-B magnitude (`QB mag`). The former comes mostly from the northern Palomar survey, and the latter from the UK SERC Schmidt survey. Near equatorial regions, where the surveys overlap, both magnitudes are available. But for the majority of cases only one or the other will be given. A code (`CV` and `CB`) gives further information on the emulsion and filter used.

We recommend that cone searches should not exceed a radius of 30 arc min, since, as you will quickly discover, a radius of 30 arc mins usually contains hundreds if not thousands of stars. To `cover' a larger area, then, you should do a mosaic of 30 arc minute searches with offset co-ordinates. Notice that the default cone search radius is 1 arc minute.


Parameters

RA
The Right Ascension of the star.

Dec
The Declination of the star.

LII
The galactic longitude of the star.

BII
The galactic latitude of the star.

QV_Mag
Each entry contains a position, a Quasi-V magnitude (`QV mag`) and a Quasi-B magnitude (`QB mag`). The former comes mostly from the northern Palomar survey, and the latter from the UK SERC Schmidt survey. Near equatorial regions, where the surveys overlap, both magnitudes are available. But for the majority of cases only one or the other will be given. A code (`CV` and `CB`) gives further information on the emulsion and filter used.

QV_Err
The uncertainty in the Quasi-V magnitude value.

QB_Mag
Each entry contains a position, a Quasi-V magnitude (`QV mag`) and a Quasi-B magnitude (`QB mag`). The former comes mostly from the northern Palomar survey, and the latter from the UK SERC Schmidt survey. Near equatorial regions, where the surveys overlap, both magnitudes are available. But for the majority of cases only one or the other will be given. A code (`CV` and `CB`) gives further information on the emulsion and filter used.

QB_Err
The uncertainty in the Quasi-B magnitude value.

CV
The bandpass codes used are (see ST Preprint no. 363, p. 102, table VI.):

------------------------------------------------------------------------
       Code     Emulsion     Filter
       ----     --------     ------
         1      IIaD         W12
         6      IIaD         GG495
         8      103aE        Red plexiglass
        10      IIaD         GG495
------------------------------------------------------------------------
Note that the passbands are (unfortunately) solely defined by the emulsion/filter combination; they bear only little resemblance to standard magnitudes (e.g., B or V). Since we do not have any color information (yet - wait 5 years until we have the next surveys), an individual transformation into a standard system is not possible.

CB
The bandpass codes used are (see ST Preprint no. 363, p. 102, table VI.):

------------------------------------------------------------------------
       Code     Emulsion     Filter
       ----     --------     ------
         0      IIIaJ        GG395
        11      103aO        GG400
        18      IIIaJ        GG385
------------------------------------------------------------------------
Note that the passbands are (unfortunately) solely defined by the emulsion/filter combination; they bear only little resemblance to standard magnitudes (e.g., B or V). Since we do not have any color information (yet - wait 5 years until we have the next surveys), an individual transformation into a standard system is not possible.

PCount
The number of plates used in calculating the position.

XClass
The classification flag uses the following codes:

------------------------------------------------------------------------
       Code     Meaning
       ----     -------
         1      Star
         2      Galaxy
         3      Non-Star
         5      Artifact
------------------------------------------------------------------------

Reference

The full details of the GSC catalog are contained in the Space Telescope Preprint No. 363.

Contact Person

Questions regarding the HST GSC database table can be addressed to the HEASARC User Hotline at request@athena.gsfc.nasa.gov.

Space Science Data System
Cosmic Journeys

Part of the NASA OSS
Structure and Evolution of the Universe theme.

Questions/Comments/Feedback
NASA's Privacy Statement
Tell me about black holes, astronomy, and more!

A service of the Laboratory for High Energy Astrophysics (LHEA) at NASA/ GSFC
and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory (SAO)

HEASARC Director: Dr. Nicholas E. White,
white@adhoc.gsfc.nasa.gov
HEASARC Associate Director: Dr. Steve Murray, ssm@head-cfa.harvard.edu
Technical Representative: Eunice Eng,
eunice.eng@gsfc.nasa.gov


Page Author: Browse Software Development Team <request@athena.gsfc.nasa.gov>
Last Modified: Monday, 16-Oct-2000 14:28:24 EDT