sdapy.snerun.snelist.get_par¶
- snelist.get_par(objid, returnname=False, **kwargs)¶
get parameter of one SN
- Parameters
- objidstr
object ID string
- returnnamebool
get number or name of parameter
- parnamestr
a parameter name from self.parlist
- filt1str
used when e.g. parname is mag, or color
- filt2str
used only when e.g. parname is color, together with filt1
- quantlist
used to get fitting samples, e.g. 5th to 95th percentiles as the error
- peakwithstr
how to decide the peak
- expwithstr
how to decide the explosion epoch
- phase1str
used when parname is detlam, together with phase2
- phase2str
used when parname is detlam, together with phase1
- interpolationstr
what interpolation to be used when e.g. calculate magnitudes, colours, etc
- corr_mkwstr
when calculating absulte mag, if correct milky way extinction if there’re any
- corr_hoststr
when calculating absulte mag, if correct host galaxy extinction if there’re any
- indexint
if there’re multple models can provide, e.g. the nickel mass mni, which one to use
- enginestr
which engine models to be used
- modelstr
which models to be used
- sourcestr
which source to be used