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| ===== Combined Analysis ===== | ===== Combined Analysis ===== | ||
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| + | NMMA is capable of performing combined analyses to constrain: | ||
| + | * the neutron star equation of state (EOS), and | ||
| + | * the Hubble Constant. | ||
| + | |||
| + | In the following, we will take the EOS analysis as an example. | ||
| + | |||
| + | ==== EOS analysis ==== | ||
| + | |||
| + | **Generate a simulation set** | ||
| + | |||
| + | First of all, you need to create an output directory, this output will host all the data that will be used to constrain the EOS. | ||
| + | mkdir -p ./output | ||
| + | |||
| + | Running the following command line will generate a json file (injection.json) with the BILBY processing of compact binary merging events. We take here binaries of type BNS (NSBH is also an option). This injection comprises a simulation set of parameters: '' | ||
| + | |||
| + | nmma_create_injection --prior-file ./ | ||
| + | |||
| + | **Light curve posterior** | ||
| + | |||
| + | EM data will house the posteriors of the electromagnetic data you will produce: in particular the lc.csv (./ | ||
| + | |||
| + | for macroeventID in {0..99} | ||
| + | |||
| + | do | ||
| + | mkdir -p ./ | ||
| + | light_curve_analysis --model Bu2019lm --svd-path ./svdmodels --gptype tensorflow --outdir ./ | ||
| + | done | ||
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Last modified: le 2022/02/22 10:23
