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Now efficient again (if run on pre-existing nemo run). Added tests of both forced photometry modes. Changed link to quickstart maps from UKZN server to dropbox.
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| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,121 @@ | ||
| # Nemo config file | ||
| # YAML format | ||
| # - use null to return None in Python | ||
| # - note that YAML is fussy about large numbers: use e.g. 1.0e+14 for M500MSun (not 1e14) | ||
|
|
||
| unfilteredMaps: | ||
| - {mapFileName: "maps/f150_1_10_8_map.fits", | ||
| weightsFileName: "maps/f150_1_10_8_ivar.fits", | ||
| obsFreqGHz: 149.6, units: 'uK', | ||
| beamFileName: "maps/s16_pa2_f150_nohwp_night_beam_profile_jitter.txt"} | ||
| - {mapFileName: "maps/f090_1_10_8_map.fits", | ||
| weightsFileName: "maps/f090_1_10_8_ivar.fits", | ||
| obsFreqGHz: 97.8, units: 'uK', | ||
| beamFileName: "maps/s16_pa3_f090_nohwp_night_beam_profile_jitter.txt"} | ||
|
|
||
| # Masks | ||
| #surveyMask: "maps/Jun2020/AdvACTSurveyMask_v7_galLatCut_S18-dust-artifacts-extended-post10mJy.fits" | ||
|
|
||
| # Instead of giving point source mask, can give catalog instead | ||
| maskPointSourcesFromCatalog: | ||
| - "PS_S18_f150_auto_rArcmin.fits" | ||
|
|
||
| # Detection/catalog options | ||
| thresholdSigma: 4.0 | ||
| minObjPix: 1 | ||
| findCenterOfMass: True | ||
| useInterpolator: True | ||
| rejectBorder: 0 | ||
| objIdent: 'ACT-CL' | ||
| longNames: False | ||
| removeRings: False | ||
|
|
||
| # Photometry options | ||
| photFilter: 'Arnaud_M2e14_z0p4' | ||
| fitQ: True | ||
|
|
||
| # Optionally override the GNFW parameters - if not present, Arnaud et al. (2010) parameters are used | ||
| # The example below is for the Planck Pressure Profile (PPP) | ||
| #GNFWParams: {P0: 6.41, c500: 1.81, gamma: 0.31, alpha: 1.33, beta: 4.13, tol: 1e-7, npts: 100} | ||
|
|
||
| # Mass measurement options - used by nemoMass and nemoSelFn scripts | ||
| # Writes out .fits file to nemoOutDir/nemoOutDir_M500.fits | ||
| # redshiftCatalog: A .fits table containing name, RADeg, decDeg, redshift, redshiftErr columns | ||
| # tenToA0, B0, Mpivot, sigma_int: Fixed scaling relation options (see H13 or ACTPol paper) | ||
| # rescaleFactor, rescaleFactorErr: For MCal masses, as in the ACTPol paper (i.e., just rescales M500 results by 1/rescaleFactor) | ||
| massOptions: {tenToA0: 4.95e-5, | ||
| B0: 0.08, | ||
| Mpivot: 3.0e+14, | ||
| sigma_int: 0.2, | ||
| relativisticCorrection: True, | ||
| rescaleFactor: 0.69, | ||
| rescaleFactorErr: 0.07, | ||
| redshiftCatalog: "DR5_cluster-catalog_v1.1.fits"} | ||
|
|
||
| # Selection function options - this calculation can also be enabled with the nemo -S switch | ||
| # NOTE: could eventually add 'completenessFraction' to 'massLimitMaps', which is why that's a dictionary list | ||
| # Use selFnFootprints to calculate average completeness in given sky areas - e.g., overlap with optical surveys | ||
| calcSelFn: False | ||
| selFnOptions: {fixedSNRCut: 5.0, | ||
| massLimitMaps: [{z: 0.5}]} | ||
|
|
||
| # Filter definitions: | ||
| # allFilters is a dictionary of parameters that will be copied into all mapFilters | ||
| # (these can be overridden by keys with the same name in mapFilters) | ||
| allFilters: {class: "ArnaudModelMatchedFilter", | ||
| params: {noiseParams: {method: "dataMap", | ||
| noiseGridArcmin: 40.}, | ||
| saveFilteredMaps: True, | ||
| saveRMSMap: True, | ||
| savePlots: False, | ||
| saveDS9Regions: False, | ||
| outputUnits: 'yc', | ||
| edgeTrimArcmin: 0.0} | ||
| } | ||
|
|
||
| # mapFilters is a list of all the different filters to apply | ||
| # (keys in mapFilters with the same name as those in allFilters take priority) | ||
| mapFilters: | ||
| #- {label: "Arnaud_M1e14_z0p2", | ||
| #params: {M500MSun: 1.0e+14, z: 0.2}} | ||
| #- {label: "Arnaud_M2e14_z0p2", | ||
| #params: {M500MSun: 2.0e+14, z: 0.2}} | ||
| #- {label: "Arnaud_M4e14_z0p2", | ||
| #params: {M500MSun: 4.0e+14, z: 0.2}} | ||
| #- {label: "Arnaud_M8e14_z0p2", | ||
| #params: {M500MSun: 8.0e+14, z: 0.2}} | ||
| #- {label: "Arnaud_M1e14_z0p4", | ||
| #params: {M500MSun: 1.0e+14, z: 0.4}} | ||
| - {label: "Arnaud_M2e14_z0p4", | ||
| params: {M500MSun: 2.0e+14, z: 0.4, | ||
| saveFilteredMaps: True, | ||
| savePlots: True}} | ||
| #- {label: "Arnaud_M4e14_z0p4", | ||
| #params: {M500MSun: 4.0e+14, z: 0.4}} | ||
| #- {label: "Arnaud_M8e14_z0p4", | ||
| #params: {M500MSun: 8.0e+14, z: 0.4}} | ||
| #- {label: "Arnaud_M1e14_z0p8", | ||
| #params: {M500MSun: 1.0e+14, z: 0.8}} | ||
| #- {label: "Arnaud_M2e14_z0p8", | ||
| #params: {M500MSun: 2.0e+14, z: 0.8}} | ||
| #- {label: "Arnaud_M4e14_z0p8", | ||
| #params: {M500MSun: 4.0e+14, z: 0.8}} | ||
| #- {label: "Arnaud_M8e14_z0p8", | ||
| #params: {M500MSun: 8.0e+14, z: 0.8}} | ||
| #- {label: "Arnaud_M1e14_z1p2", | ||
| #params: {M500MSun: 1.0e+14, z: 1.2}} | ||
| #- {label: "Arnaud_M2e14_z1p2", | ||
| #params: {M500MSun: 2.0e+14, z: 1.2}} | ||
| #- {label: "Arnaud_M4e14_z1p2", | ||
| #params: {M500MSun: 4.0e+14, z: 1.2}} | ||
| #- {label: "Arnaud_M8e14_z1p2", | ||
| #params: {M500MSun: 8.0e+14, z: 1.2}} | ||
|
|
||
| # Source injection test - this can also be enabled with the nemo -I switch | ||
| sourceInjectionIterations: 10 | ||
| sourcesPerTile: 50 | ||
| sourceInjectionModels: | ||
| - {redshift: 0.8, M500: 2.0e+14} | ||
| - {redshift: 0.4, M500: 2.0e+14} | ||
| - {redshift: 0.2, M500: 2.0e+14} | ||
| - {redshift: 0.1, M500: 2.0e+14} |
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