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comb_analysis [2022/02/22 10:51]
theoastro
comb_analysis [2022/02/27 08:46] (current)
theoastro
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   *  the Hubble Constant.   *  the Hubble Constant.
  
-In the following, we will take as an example the EOS analysis.+In the following, we will take the EOS analysis as an example.
  
 ==== EOS analysis ==== ==== EOS analysis ====
Line 21: Line 21:
  
 EM data will house the posteriors of the electromagnetic data you will produce: in particular the lc.csv (./example_files/csv_lightcurve/outdir/macroeventID, where macroeventID in range(0, 100)) light curves. We now compute posteriors using NMMA on this simulated set of 100 events, of which we assume a fraction is detectable by Zwicky Transient Facility (ZTF). The result can be find at ./output/EMdata EM data will house the posteriors of the electromagnetic data you will produce: in particular the lc.csv (./example_files/csv_lightcurve/outdir/macroeventID, where macroeventID in range(0, 100)) light curves. We now compute posteriors using NMMA on this simulated set of 100 events, of which we assume a fraction is detectable by Zwicky Transient Facility (ZTF). The result can be find at ./output/EMdata
 +
 +for macroeventID in {0..99}
 +
 +  do
 +    mkdir -p ./output/EMdata/outdir/$macroeventID/
 +    light_curve_analysis --model Bu2019lm --svd-path ./svdmodels --gptype tensorflow --outdir ./output/EMdata/outdir/$macroeventID --label injection_Bu2019lm --prior ./priors/Bu2019lm.prior --tmin 0 --tmax 7 --dt 0.5 --error-budget 1.0 --nlive 256 --Ebv-max 0 --injection ./output/injection.json --injection-num $macroeventID --injection-detection-limit 22,22,22 --injection-outfile ./output/EMdata/outdir/$macroeventID/lc.csv --generation-seed 42 --filters g,r,i --ztf-sampling --ztf-uncertainties --plot --remove-nondetections --optimal-augmentation --optimal-augmentation-filters u,g,r,i,z,y,J,H,K --optimal-augmentation-N 100
 +  done
  
  
Last modified: le 2022/02/22 10:51