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Background Estimates in Sensitivity PlotsAlso see:
The background estimates were generated using a prototype version
of the Spitzer background estimator. Three lines of sight were chosen
to represent low, medium, and high background.
LINE OF SIGHT PARAMETERS
BACKGROUND CONTRIBUTIONSThe background model includes the zodiacal light, interstellar medium (cirrus), and the cosmic infrared background (at wavelengths greater than 100 microns). The contributions of each component can be seen in the figure below. The zodiacal light dominates IRAC and IRS wavelengths for all these lines of sight. For MIPS 70 microns, there are comparable interstellar and zodiacal contributions, while at 160 microns, the interstellar contribution dominates.
Figure:
BRIGHTNESS VALUESThe background spectra were integrated over the Spitzer passbands and the results are reported as per the Spitzer calibration convention (same as IRAS, ISO, COBE) below. The first column is the mnemonic wavelength for the band and the second column is the quoted surface brightness of that band. For reference, the color corrections ranged from 0.98 to 1.08.
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This file was last modified on Fri Jan 9 11:11:35 2009.