skymodel – simulation microwave components¶
Main¶
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Computes an all-sky map of the simulated microwave sky at the specified frequency. |
Extragalactic components¶
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Computes an all-sky CIB map at a given frequency and nside based on . |
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Computes an all-sky radio point source map at a given frequency and nside based on the simulations provided by Sehgal et al. (2010), which have been recalibrated by the SO collaboration. |
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Function that computes a CMB map from a power spectrum. |
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Function which compute tSZ maps at different frequencies and different nside. |
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Function which computes kSZ maps at different frequencies and different nside. |
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Computes a map that contains all ~250,000 point sources from the IRAS PS catalog. |
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Computes a map that contains all ~1,800,000 point sources from the NVSS PS catalog (Condon et al. 1998). |
Galactic foregrounds¶
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Computes an all-sky galactic foregrounds noise map at a given frequency and nside using the Python Sky model (PySM, Thorne et al. 2017), which is build from Planck data. |
Noises¶
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Function which create a White noise map for a given noise/arcmin or noise/radians. |
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Computes an all-sky atmospheric noise map at a given frequency and nside based on the SO noise model presented by the SO Collaboration (2019) and using the model parameters provided by Choi et al. (2019). |
Other¶
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Convert observed signal at given frequencies to different units. |
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Computes the size of Healpy pixels in function of the nside of the map. |
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Draws uniformly sampled tuples of coordinates on the sphere. |
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Creates gnomic projections of HEALPix all-sky maps. |
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Computes a sigmoid-shaped filer high-pass window in spherical harmonic space. |
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Returns the specified all-sky survey map. |