Difference: SpirePhotometerBeamProfile (5 vs. 6)
Revision 62013-11-15 - BernhardSchulz
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SPIRE Photometer Beam ProfilesSummary of beam profile analysis and solid angle revision ( Bernhard Schulz, September 2012) | ||||||||
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Radial Beam Profile ModelDatasets to construct the radial beam profile model are available below. These allow to take into account the color dependent FWHM of the true beam profiles. | ||||||||
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| > > | An implementation of the beam profile model in IDL is available for download . | |||||||
The radial beam profile model for SPIRE was developed and described by Griffin et al. 2013. The peak normalized monochromatic flux, depending on the distance from the peak (Theta) can be described as:
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| < < | A value of -0.85 should be adopted for gamma, which controls the dependence of the FWHM of the variable part of the beam on wavelength. The reference frequency nu_eff is the isophotal frequency for the product of the spectrum of Neptune and the respective SPIRE spectral filter profile. | |||||||
| > > | A value of -0.85 should be adopted for gamma, which controls the dependence of the FWHM of the variable part of the beam on wavelength. The reference frequency nu_eff is the isophotal frequency for the product of the spectrum of Neptune and the respective SPIRE spectral filter profile. The frequencies 1217.27, 867.75, 610.87 GHz for PSW, PMW, PLW respectively make the model beam profile consistent with the measured Neptune beam using the spectral indices 1.29, 1.42, 1.47 respectively to describe the Neptune SED in the three filter bands. | |||||||
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