[761] | 1 | # SKYMIX NbComponents NSide_HealPix
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| 2 | SKYMIX 3 128
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| 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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| 20 | MAPPATH /data/opus/Rz/SOPHYA/
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| 21 |
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| 22 |
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| 23 | # ---- Sky components ---------
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| 24 | # ---- HealPix maps ----
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| 25 | # MAPFITSFILEi FITSfilename Normalisation
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| 26 | @MAPFITSFILE1 gauss.fits 1.0
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| 27 |
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| 28 | # --- Emission Spectra definition -----
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| 29 | # SPECTRAFITSFILEi FITSfilename Fmin Fmax
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| 30 | @SPECTRAFITSFILE1 pl.fits 100 600
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| 31 |
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| 32 | # Other possible definition of emission spectra
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| 33 | # BLACKBODYi temperature
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| 34 | # The blackbody object returns flux in units of watt/m2/sr/hz
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| 35 | # We thus scale the map (x 1.e17)
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| 36 | @MAPFITSFILE2 cossin.fits 1.e17
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| 37 | @BLACKBODY2 2.726
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| 38 |
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| 39 | # For power-law spectra f = a ((nu-nu0)/dnu)^b)
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| 40 | # POWERLAWSPECTRAi a nu0 dnu b Fmin Fmax
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| 41 | @MAPFITSFILE3 noise.fits 0.1
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| 42 | @POWERLAWSPECTRA3 1. 150. 50. -0.5 100. 500.
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| 43 |
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| 44 | # Define the Debug level
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| 45 | @DEBUGLEVEL 0
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| 46 | # Define the Print level
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| 47 | @PRINTLEVEL 5
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