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Guide to image dataThe sections linked below provide basic information on the data returned by the small area image extraction form, Get an Image, and on the GAIA software. More detailed discussions are planned.Updates to the on-line data and associated access software are listed in the Release History.
The pixel dataThe pixel data is returned as a (gzipped) standard FITS file. The original pixel data have been compressed using the H-transform by a factor of 20 without loss of resolution i.e. the pixel size is still 10 microns (0.7 arcsec). Pixel values range from 0 to 32767 and are representative of the plate density (derived from the measured transmission). A world coordinate system (WCS) has been written into the FITS file so that astronomical coordinates (as opposed to x and y) are readily available. The WCS system is defined for each extraction using the positions of objects taken from at least a 10 x 10 armin area in the object-catalogue. The objects in this catalogue were detected during the SuperCOSMOS Image Analysis Mode (IAM). Typically some 1000 objects define the xy-to-RA/Dec transformation and the coordinates of a given pixel are thought to be accurate to a few tenths of an arcsec. The object-catalogue dataThe image extraction form returns two fomats of object catalogues.
Only objects detected in the primary/selected waveband are returned. Magnitudes in any/all of the other wavebands are also returned if a given object in the primary colour pairs up with an object detected in the other wavebands. A secondary magnitude of 99.999 indicates one of the following:
Parameters in the FITS tables Description of FITS table object parametersFITS table 1The first table lists the most useful parameters and contains magnitudes of the objects in the other wavebands that have been paired with those detected in the primary (i.e. the one requested in the form) waveband/survey.Each object is desribed by the parameters listed below. Some of the parameters have links pointing to more detailed information. FITS tables can be examined using various software (eg using xcatview under CURSA)
FITS table 2The second table lists all 32 parameters as measured/extracted from plate in the primary (selected) waveband. Some of the parameters have links pointing to more detailed information. FITS tables can be examined using various software (eg using xcatview under CURSA)
Description of object parameters in tab-separated listThe image extraction form also returns a tab-separated ascii listing. This file contains 16 parameters (plus a running ID number) for each object. These parameters include proper motions, magnitudes in all wavebands (where available/detected) and a subset of the full 32 parameters recorded by SuperCOSMOS during its Image Analyis Mode (IAM) of the primary plate. The second table in the FITS file contains all 32.The tab-separated listing is formatted in the way it is so that it is directly readable by GAIA. At the top of the listing are a few lines of information (not garbage!) describing how GAIA should plot the object symbols, in this case ellipses, when the file is read in. The parameters returned are given below:
The GAIA softwareGAIA is one of many applications that can read the standard FITS images produced during the extraction. More than just an advanced image display tool, GAIA also provides for the plotting of object-catalogues and is therefore well-suited to the data being discussed (of course users may prefer to use another package: SAOIMAGE, SAOTNG, XV, etc). Currently GAIA requires object catalogues to be in a similar format to the tab-separated listing produced by the form. Future releases of GAIA will be able to read the catalogue already inlcluded as part of the FITS file. For more detailed information on GAIA (including how to get and install the package) go here .
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WFAU, Institute for Astronomy, M.Read@roe.ac.uk
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