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Merge pull request #347 from litebird/co_maps
Update Mbs
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#PYSM model for ame (a2) | ||
#two population, one with fixed peak emissivity, the other with variable | ||
#temperature and polarization | ||
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[ame_TP] | ||
[ame_TP.comp1] | ||
class = "SpDustPol" | ||
map_I = "pysm_2/ame_t_new.fits" | ||
unit_I = "uK_RJ" | ||
freq_ref_I = "22.8 GHz" | ||
emissivity = "pysm_2/emissivity.txt" | ||
freq_peak = "pysm_2/ame_nu_peak_0.fits" | ||
freq_ref_peak = "30 GHz" | ||
pol_frac = 0.02 | ||
angle_Q = "pysm_2/dust_q_new.fits" | ||
angle_U = "pysm_2/dust_u_new.fits" | ||
[ame_TP.comp2] | ||
class = "SpDustPol" | ||
map_I = "pysm_2/ame2_t_new.fits" | ||
unit_I = "uK_RJ" | ||
freq_ref_I = "41 GHz" | ||
emissivity = "pysm_2/emissivity.txt" | ||
freq_peak = "33.35 GHz" | ||
freq_ref_peak = "30 GHz" | ||
pol_frac = 0.02 | ||
angle_Q = "pysm_2/dust_q_new.fits" | ||
angle_U = "pysm_2/dust_u_new.fits" |
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[co1] | ||
class = "COLines" | ||
has_polarization = false |
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[co2] | ||
class = "COLines" | ||
has_polarization = true | ||
polarization_fraction = 0.001 |
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[co3] | ||
class = "COLines" | ||
has_polarization = true | ||
polarization_fraction = 0.001 | ||
include_high_galactic_latitude_clouds = true |
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#PYSM model for dust (d10) | ||
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[dust_poltens_var_spec] | ||
class = "ModifiedBlackBody" | ||
map_I = "dust_gnilc/gnilc_dust_template_nside{nside}_2023.02.10.fits" | ||
map_mbb_index = "dust_gnilc/gnilc_dust_beta_nside{nside}_2023.06.06.fits" | ||
map_mbb_temperature = "dust_gnilc/gnilc_dust_Td_nside{nside}_2023.06.06.fits" | ||
freq_ref_I = "353 GHz" | ||
freq_ref_P = "353 GHz" | ||
max_nside = 8192 |
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#PYSM model for dust (d11) | ||
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[dust_poltens_var_spec_random] | ||
class = "ModifiedBlackBodyRealization" | ||
amplitude_modulation_temp_alm = "dust_gnilc/raw/gnilc_dust_temperature_modulation_alms_lmax768.fits.gz" | ||
amplitude_modulation_pol_alm = "dust_gnilc/raw/gnilc_dust_polarization_modulation_alms_lmax768.fits.gz" | ||
largescale_alm = "dust_gnilc/raw/gnilc_dust_largescale_template_logpoltens_alm_nside2048_lmax1024_complex64.fits.gz" | ||
small_scale_cl = "dust_gnilc/raw/gnilc_dust_small_scales_logpoltens_cl_lmax16384.fits.gz" | ||
largescale_alm_mbb_index = "dust_gnilc/raw/gnilc_dust_largescale_template_beta_alm_nside2048_lmax1024.fits.gz" | ||
small_scale_cl_mbb_index = "dust_gnilc/raw/gnilc_dust_small_scales_beta_cl_lmax16384_2023.06.06.fits.gz" | ||
largescale_alm_mbb_temperature = "dust_gnilc/raw/gnilc_dust_largescale_template_Td_alm_nside2048_lmax1024.fits.gz" | ||
small_scale_cl_mbb_temperature = "dust_gnilc/raw/gnilc_dust_small_scales_Td_cl_lmax16384_2023.06.06.fits.gz" | ||
freq_ref = "353 GHz" | ||
# Remove the galplane_fix option to skip applying the galactic plane fix | ||
galplane_fix = "dust_gnilc/raw/gnilc_dust_galplane.fits.gz" | ||
galplane_fix_beta_Td = "dust_gnilc/raw/gnilc_dust_beta_Td_galplane.fits.gz" | ||
# Configuration for reproducing d10 | ||
# seeds = [8192,777,888] | ||
# synalm_lmax = 16384 | ||
max_nside = 8192 |
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#PYSM model for dust (d12) | ||
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[dust_layers] | ||
class = "ModifiedBlackBodyLayers" | ||
map_layers = "mkd_dust/2048/thermaldust_ampl{layer}.fits" | ||
freq_ref = "353 GHz" | ||
map_mbb_index = "mkd_dust/2048/thermaldust_specind{layer}.fits" | ||
map_mbb_temperature = "mkd_dust/2048/thermaldust_temp{layer}.fits" | ||
num_layers = 6 | ||
color_correction = 0.911 | ||
unit_layers = "MJy/sr" | ||
unit_mbb_temperature = "K" | ||
max_nside = 2048 |
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#PYSM model for dust (d2) | ||
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[dust_var_spec_mean1p59_std0p2] | ||
class = "ModifiedBlackBody" | ||
map_I = "pysm_2/dust_t_new.fits" | ||
map_Q = "pysm_2/dust_q_new.fits" | ||
map_U = "pysm_2/dust_u_new.fits" | ||
unit_I = "uK_RJ" | ||
unit_Q = "uK_RJ" | ||
unit_U = "uK_RJ" | ||
map_mbb_index = "pysm_2/beta_mean1p59_std0p2.fits" | ||
map_mbb_temperature = "pysm_2/dust_temp.fits" | ||
unit_mbb_temperature = "K" | ||
freq_ref_I = "545 GHz" | ||
freq_ref_P = "353 GHz" |
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#PYSM model for dust (d3) | ||
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[dust_var_spec_mean1p59_std0p3] | ||
class = "ModifiedBlackBody" | ||
map_I = "pysm_2/dust_t_new.fits" | ||
map_Q = "pysm_2/dust_q_new.fits" | ||
map_U = "pysm_2/dust_u_new.fits" | ||
unit_I = "uK_RJ" | ||
unit_Q = "uK_RJ" | ||
unit_U = "uK_RJ" | ||
map_mbb_index = "pysm_2/beta_mean1p59_std0p3.fits" | ||
map_mbb_temperature = "pysm_2/dust_temp.fits" | ||
unit_mbb_temperature = "K" | ||
freq_ref_I = "545 GHz" | ||
freq_ref_P = "353 GHz" |
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#PYSM model for dust (d6) | ||
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[dust_decorrelated] | ||
class = "DecorrelatedModifiedBlackBody" | ||
correlation_length = 5.0 | ||
map_I = "pysm_2/dust_t_new.fits" | ||
map_Q = "pysm_2/dust_q_new.fits" | ||
map_U = "pysm_2/dust_u_new.fits" | ||
unit_I = "uK_RJ" | ||
unit_Q = "uK_RJ" | ||
unit_U = "uK_RJ" | ||
map_mbb_index = "pysm_2/dust_beta.fits" | ||
map_mbb_temperature = "pysm_2/dust_temp.fits" | ||
unit_mbb_temperature = "K" | ||
freq_ref_I = "545 GHz" | ||
freq_ref_P = "353 GHz" |
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#PYSM model for dust (d9) | ||
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[dust_poltens_fixed_spec] | ||
class = "ModifiedBlackBody" | ||
map_I = "dust_gnilc/gnilc_dust_template_nside{nside}_2023.02.10.fits" | ||
# from Planck 2018 XI | ||
map_mbb_index = 1.48 | ||
map_mbb_temperature = 19.6 | ||
unit_mbb_temperature = "K" | ||
freq_ref_I = "353 GHz" | ||
freq_ref_P = "353 GHz" | ||
max_nside = 8192 |
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#PSYM model for synchrotron (s2) | ||
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[synch_var_spec_lat] | ||
class = "PowerLaw" | ||
map_I = "pysm_2/synch_t_new.fits" | ||
map_Q = "pysm_2/synch_q_new.fits" | ||
map_U = "pysm_2/synch_u_new.fits" | ||
unit_I = "uK_RJ" | ||
unit_Q = "uK_RJ" | ||
unit_U = "uK_RJ" | ||
map_pl_index = "pysm_2/beta_latvar.fits" | ||
freq_ref_I = "408 MHz" | ||
freq_ref_P = "23 GHz" |
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#PSYM model for synchrotron (s3) | ||
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[synch_var_spec_curved] | ||
class = "CurvedPowerLaw" | ||
map_I = "pysm_2/synch_t_new.fits" | ||
map_Q = "pysm_2/synch_q_new.fits" | ||
map_U = "pysm_2/synch_u_new.fits" | ||
unit_I = "uK_RJ" | ||
unit_Q = "uK_RJ" | ||
unit_U = "uK_RJ" | ||
map_pl_index = "pysm_2/synch_beta.fits" | ||
freq_ref_I = "408 MHz" | ||
freq_ref_P = "23 GHz" | ||
spectral_curvature = -0.052 | ||
freq_curve = "23 GHz" |
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#PSYM model for synchrotron (s4) | ||
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[synch_poltens_fixed_spec] | ||
class = "PowerLaw" | ||
map_I = "synch/synch_template_nside{nside}_2023.02.25.fits" | ||
map_pl_index = -3.1 | ||
freq_ref_I = "23 GHz" | ||
freq_ref_P = "23 GHz" | ||
max_nside = 8192 |
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#PSYM model for synchrotron (s5) | ||
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[synch_poltens_var_spec] | ||
class = "PowerLaw" | ||
map_I = "synch/synch_template_nside{nside}_2023.02.25.fits" | ||
map_pl_index = "synch/synch_beta_nside{nside}_2023.02.16.fits" | ||
freq_ref_I = "23 GHz" | ||
freq_ref_P = "23 GHz" | ||
max_nside = 8192 |
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#PSYM model for synchrotron (s6) | ||
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[synch_var_spec_random] | ||
class = "PowerLawRealization" | ||
largescale_alm = "synch/raw/synch_largescale_template_logpoltens_alm_lmax128_2023.02.24.fits.gz" | ||
amplitude_modulation_temp_alm = "synch/raw/synch_temperature_modulation_alms_lmax64_2023.02.24.fits.gz" | ||
amplitude_modulation_pol_alm = "synch/raw/synch_polarization_modulation_alms_lmax64_2023.02.24.fits.gz" | ||
amplitude_modulation_beta_alm = "synch/raw/synch_amplitude_modulation_alms_lmax768.fits.gz" | ||
small_scale_cl = "synch/raw/synch_small_scales_cl_lmax16384_2023.02.24.fits.gz" | ||
largescale_alm_pl_index = "synch/raw/synch_largescale_beta_alm_nside512_lmax768.fits.gz" | ||
small_scale_cl_pl_index = "synch/raw/synch_small_scales_beta_cl_lmax16384.fits.gz" | ||
freq_ref = "23 GHz" | ||
max_nside = 8192 | ||
# Remove the galplane_fix option to skip applying the galactic plane fix | ||
galplane_fix = "synch/raw/synch_galplane.fits.gz" | ||
# Configuration for reproducing s5 | ||
# seeds = [555,444] | ||
# synalm_lmax = 16384 |
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