ISSA Explanatory Supplement
II. IRAS SKY SURVEY ATLAS OVERVIEW
C. Product Description
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Figure II.C.1 ISSA Fields for || > 50°
in Equatorial Coordinates larger largest |
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Figure II.C.2 ISSA Fields for || > 20°
in Equatorial Coordinates larger largest |
For each field and IRAS wavelength (12, 25, 60 and 100 µm), there
is an intensity image for each confirming coverage (HCON-1, HCON-2 and
HCON-3) plus a co-added image of all the coverages.
Coverage and standard deviation images were also produced
and are available upon request at
IPAC.
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Figure II.C.3 ISSA Reject Fields
||<20° in Equatorial Coordinates larger largest |
The FITS intensity images are either 16 or 32 bits per sample. The number of bits per sample was determined by examining the intensity range and comparing it to 5% of median noise, where noise is the standard deviation of the mean of each pixel. If 16 bits is too small to hold the intensity range down to the 5% of median noise level, then the number of bits that will carry information down to that threshold is used. In FITS-formatted images, any number greater than 16 bits requires 32 bits per sample.
The size of each intensity image is either 0.5 or 1.0 Mbytes, depending
on noise level and dynamic range of signal.
The entire set of ISSA plus ISSA Reject images has a size of
4.2 Gbytes. The ISSA Reject Set comprises
about 1.4 Gbytes.
ISSA is available on permanent media through:
Coordinated Request and User Support Office (CRUSO) NASA/GSFC Code 633.4 Greenbelt, MD 20771.[NOTE: All released IRAS data products are available from IRSA.]