skymodel – simulation microwave components

Main

skymodel(freq[, sensitivity, components, ...])

Computes an all-sky map of the simulated microwave sky at the specified frequency.

Extragalactic components

simulate_cib(freq[, nside_out, lmax, ...])

Computes an all-sky CIB map at a given frequency and nside based on .

simulate_radio_ps(freq[, nside_out, lmax, ...])

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.

simulate_cmb(freq[, cl_file, lensed, ...])

Function that computes a CMB map from a power spectrum.

simulate_tSZ(freq[, nside_out, lmax, ...])

Function which compute tSZ maps at different frequencies and different nside.

simulate_kSZ(freq[, nside_out, lmax, ...])

Function which computes kSZ maps at different frequencies and different nside.

simulate_iras_ps(freq[, nside_out, ...])

Computes a map that contains all ~250,000 point sources from the IRAS PS catalog.

simulate_nvss_ps(freq[, nside_out, ...])

Computes a map that contains all ~1,800,000 point sources from the NVSS PS catalog (Condon et al. 1998).

Galactic foregrounds

simulate_gal_foregrounds(freq[, components, ...])

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

simulate_white_noise(freq, noise_level[, ...])

Function which create a White noise map for a given noise/arcmin or noise/radians.

simulate_atmosphere(freq[, nside_out, lmax, ...])

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

convert_units(freq, values[, cmb2mjy, ...])

Convert observed signal at given frequencies to different units.

px_size(nside[, arcmin])

Computes the size of Healpy pixels in function of the nside of the map.

sample_sphere_uniform(n[, mask, radec])

Draws uniformly sampled tuples of coordinates on the sphere.

project_maps(allsky_map, RA, DEC[, ...])

Creates gnomic projections of HEALPix all-sky maps.

sigmoid_filter(l_0, d_l, lmax)

Computes a sigmoid-shaped filer high-pass window in spherical harmonic space.

return_mask(survey[, nside_out, coord])

Returns the specified all-sky survey map.