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IRAS90 recognises several different system of data units, which
may be specified using the following strings:
- pW/(M**2)
- - Flux values in Pico-Watts per square metre.
(1pW = 10-12W)
- (pW/M**2)/sr
- - Surface brightness values in Pico-Watts per
square metre, per steradian.
- Jy
- - Flux density values in Janskys.
- Jy/sr
- - Surface brightness values in Janskys per steradian.
- MJy/sr
- - Surface brightness values in Mega-Janskys per steradian.
- Jy/PIXEL
- - Surface brightness values in Janskys per pixel
- (pW/M**2)/PIXEL
- - Surface brightness values in Pico-Watts per
square metre, per pixel.
Note, the possible effects of varying pixel size should be borne
in mind when using either of the last two systems of units,
especially if dealing with very large areas of the sky. If this
may be a problem, then an equal area projection should be used
(see section
) when creating the pixel
values.
Some of these units are only available when dealing with CRDD
files (eg ``Jy''), and some when dealing with images (eg Jy/PIXEL).
Conversions between flux and flux density values use the detector bandwidths
described in section
. Conversions between flux density and
surface brightness values use the effective detector solid angles described in
section
.
Next: Time and Date Strings
Up: Using IRAS90 - Details
Previous: Point Spread Functions
IRAS90 --- IRAS Survey and PO Data Analysis Package --- Reference Guide
Starlink User Note 163
David S. Berry, W Gong, D C Parsons
19 February 1995
E-mail:ussc@star.rl.ac.uk
Copyright © 2008 Science and Technology Facilities Council