astropy / SPISEA

Stellar Population Synthesis Modeling
https://spisea.readthedocs.io/en/stable/index.html
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SiessGenevaPadova bug with mass_current #17

Closed jluastro closed 4 years ago

jluastro commented 4 years ago

Student encountered a bug trying to run the SiessGenevaPadova models... mass_current doesn't seem to exist?

Code:

pypopstar_ps1.py

Creates an isochrone using the pypopstar package

import sys import os import string import numpy as np import pandas as pd from astropy.io import ascii from astropy.io import fits import matplotlib.pyplot as plt from popstar import synthetic, evolution, atmospheres, reddening, ifmr from popstar.imf import imf, multiplicity

Define isochrone parameters logAges = [6.6, 7.6] # Age in log(years) AKs = 0 # extinction in mags

dist = 1000 # distance in parsec metallicity = 0 # Metallicity in [M/H]

Define evolution/atmosphere models and extinction law evo_model = evolution.MergedSiessGenevaPadova() evo_model_name = ['MIST', 'Padova']

atm_func = atmospheres.get_merged_atmosphere red_law = reddening.RedLawHosek18b()

Also specify filters for synthetic photometry (optional). Here we use # the HST WFC3-IR F127M, F139M, and F153M filters

filt_list = ['wfc3,ir,f127m', 'wfc3,ir,f139m', 'wfc3,ir,f153m']

Make Isochrone object. Note that is calculation will take a few minutes, unless the # isochrone has been generated previously.

for logAge in logAges: my_iso = synthetic.IsochronePhot(logAge, AKs, dist, metallicity=0, evo_model=evo_model, atm_func=atm_func, red_law=red_law, filters=filt_list) print(my_iso.save_file)

Bug: image

mwhosek commented 4 years ago

The SiessGenevaPadova are no longer supported by PyPopStar, as they have fallen out of date. It has been replaced by MergedBaraffePisaEkstromParsec