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comb_analysis [2022/02/22 10:51] theoastro |
comb_analysis [2022/02/27 08:46] (current) theoastro |
* the Hubble Constant. | * the Hubble Constant. |
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In the following, we will take as an example the EOS analysis. | In the following, we will take the EOS analysis as an example. |
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==== EOS analysis ==== | ==== EOS analysis ==== |
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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 |
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| for macroeventID in {0..99} |
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| 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 |
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