Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
comb_analysis [2022/02/22 10:27] theoastro |
comb_analysis [2022/02/27 08:46] (current) theoastro |
||
---|---|---|---|
Line 5: | Line 5: | ||
* the Hubble Constant. | * the Hubble Constant. | ||
- | In the following, we will take as an example | + | In the following, we will take the EOS analysis |
+ | |||
+ | ==== 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 | ||
+ | |||
+ | |||
- | == EOS analysis == | ||
Last modified: le 2022/02/22 10:27