[761] | 1 | # SKYMIX NbComponents NSide_HealPix
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[878] | 2 | @SKYMIX 1 16
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[761] | 3 |
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| 4 | # READMAP FitsName
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| 5 | # To Read the already prepared (mixed) Output MAP from FITS file
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| 6 | # FitsName should be the complete path to the FITS file
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| 7 | READMAP xxx.fits
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| 8 |
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| 9 | # Defining the Detection filter pass - band
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| 10 | # GAUSSFILTER or FILTERFITSFILE card
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| 11 | # GAUSSFILTER -> Gaussian filter
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| 12 | # FILTERFITSFILE -> Filter (nu, T(nu)) from FITS file
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| 13 | # GAUSSFILTER Nu0 Sigma_Nu Tmax NuMin NuMax
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| 14 | # FILTERFITSFILE FileName NuMin NuMax
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| 15 | # FileName should be a complete path
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| 16 | @GAUSSFILTER 143 12 0.84 50. 300.
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| 17 |
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| 18 | # MAPPATH PathForFITS
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| 19 | # path for input Sky Component FITS files , and EmissionSpectra files
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[878] | 20 | MAPPATH /data/opus/Rz/SOPHYA/
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[761] | 21 |
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| 22 | # ---- Sky components ---------
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| 23 | # ---- HealPix maps ----
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| 24 | # MAPFITSFILEi FITSfilename Normalisation
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[878] | 25 | @MAPFITSFILE4 gauss.fits 1.0
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[761] | 26 |
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| 27 | # --- Emission Spectra definition -----
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| 28 | # SPECTRAFITSFILEi FITSfilename Fmin Fmax
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[878] | 29 | @SPECTRAFITSFILE4 pl.fits 100 600
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[761] | 30 |
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| 31 | # Other possible definition of emission spectra
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| 32 | # BLACKBODYi temperature
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[878] | 33 | # The blackbody object returns flux in units of watt/m2/sr/hz
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| 34 | # We thus scale the map (x 1.e17)
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| 35 | @MAPFITSFILE1 cossin.fits 1.e17
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| 36 |
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[761] | 37 | # For power-law spectra f = a ((nu-nu0)/dnu)^b)
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| 38 | # POWERLAWSPECTRAi a nu0 dnu b Fmin Fmax
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[878] | 39 | @MAPFITSFILE2 noise.fits 0.1
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| 40 | @POWERLAWSPECTRA2 1. 150. 50. -0.5 100. 500.
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[761] | 41 |
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[878] | 42 | # For an emission spectrum which depends on the position
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| 43 | # in the map -> synchrotron for instance nu^(-beta(theta,phi))
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| 44 | # MAPFITSFILE will still correspond to the brightness temperature
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| 45 | @MAPFITSFILE3 /exp/planck/Sync/Template408MHz.fits 0.2
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| 46 | #@MAPFITSFILE1 gauss.fits 0.2
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| 47 | # and the BETAFITSFILE will correspond to a map with the spectral
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| 48 | # index beta(theta,phi)
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| 49 | # 408 is the normalisation frequency of the map
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| 50 | # 32 is the nside of the map on which the integration over the
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| 51 | # spectralResponse of the detector will be performed
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| 52 | # for the full resolution, write the nside of the map
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| 53 | # or a negative value.
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| 54 | @BETAFITSFILE3 /exp/planck/Sync/SpectralIndex.fits 408e-3 16
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| 55 | #@BETAFITSFILE1 gauss.fits 408e-3 32
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| 56 |
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[1399] | 57 | # For adding a dipole component
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| 58 | # @DIPOLEx Theta Phi Amplitude [Temperature=Tcmb=2.726]
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| 59 | # CMB dipole parameters , theta, phi 3.358mK
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| 60 | # @DIPOLE4 0.73 -1.67 3.358e-3
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| 61 | @DIPOLE4 2.726
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| 62 |
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[761] | 63 | # Define the Debug level
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| 64 | @DEBUGLEVEL 0
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| 65 | # Define the Print level
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[878] | 66 | @PRINTLEVEL 5
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