Closed dongj17 closed 2 weeks ago
Hi Jiang,
This is a parameter of the "psb_wild2020" star-formation history model. You can see how this model works at the link below, as far as I know it's exactly as described in the paper.
Cheers, Adam
Hi Jiang, An example fit_instructions for this SFH would look like this:
psb = {} # PSB model of Wild + 2020
psb["age"] = (4, 14.) # Vary age between 4 and 14 Gyr. In practice
# the code automatically limits this to the age of
# the Universe at the observed redshift.
psb["tau"] = (0.3, 10.) # Vary tau between 300 Myr and 10 Gyr
psb["massformed"] = (6, 13) # vary log_10(M*/M_solar) between 6 and 13
psb["burstage"] = (0,4) # age of burst from 0 to 4Gyr
psb["alpha"] = (0.01,1000) # decline of burst
psb["alpha_prior"] = "log_10"
psb["beta"] = 250. # rise of burst: fixed
psb["fburst"] = (0,1)
psb["metallicity"] = (0.01, 2.5) # vary Z between 0.01 and 2.5 Z_solar
fit_instructions["psb_wild2020"] = psb
Then the output fitted parameters for this SFH are stored in fit.posterior.samples: 'psb_wild2020:age', 'psb_wild2020:alpha', 'psb_wild2020:burstage', 'psb_wild2020:fburst', 'psb_wild2020:massformed', 'psb_wild2020:metallicity', 'psb_wild2020:tau'
Contact me by email if that isn't enough information.
Hi, Adam! I am currently performing photometric fitting on a lensed post-starburst galaxy. In the paper titled " The star formation histories of z ~1 post-starburst galaxies" (doi: 10.1093/mnras/staa674), there is a parameter "f_burst" in the equation (2). However, I couldn't find this parameter in the Bagpipes documentation. Could you please let me how to set this parameter?