A revised zodiacal light model (ZodiSURF) adds wavelength-dependent analytical scattering phase function and albedo fitted to over 5,000 HST optical measurements, yielding ~4.5% uncertainty and revealing a 0.013 +/- 0.006 MJy/sr residual excess possibly from a dim spherical dust cloud.
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SIMLA delivers a complete set of cleaned mid-infrared spectral cubes (5.2-38 micron) from Spitzer/IRS mapping data for several hundred objects, processed via a novel pipeline and soon available at IRSA.
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SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
A revised zodiacal light model (ZodiSURF) adds wavelength-dependent analytical scattering phase function and albedo fitted to over 5,000 HST optical measurements, yielding ~4.5% uncertainty and revealing a 0.013 +/- 0.006 MJy/sr residual excess possibly from a dim spherical dust cloud.
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SIMLA: The Spitzer Infrared Spectrograph Mapping Legacy Archive
SIMLA delivers a complete set of cleaned mid-infrared spectral cubes (5.2-38 micron) from Spitzer/IRS mapping data for several hundred objects, processed via a novel pipeline and soon available at IRSA.