Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
lc_inference [2022/05/19 08:56]
theoastro 		lc_inference [2023/06/10 18:58] (current)
theoastro
Line 1: Line 1:
-===== Light curve inference =====+===== Inference of electromagnetic signals =====
  
 NMMA enables to perform parameter estimation in different electromagnetic regimes such as for kilonovae and gamma-ray burst afterglows. Similarly to light curve generation, the following models are available for kilonova inference: ''Bu2019nsbh'' (BH-NS model), ''Bu2019lm''  (BNS model), ''Me2017'' (BNS model), and ''Ka2017'' (BNS model).  NMMA enables to perform parameter estimation in different electromagnetic regimes such as for kilonovae and gamma-ray burst afterglows. Similarly to light curve generation, the following models are available for kilonova inference: ''Bu2019nsbh'' (BH-NS model), ''Bu2019lm''  (BNS model), ''Me2017'' (BNS model), and ''Ka2017'' (BNS model). 
Last modified: le 2022/05/19 08:56

Page Tools