Links to All Available ModelSets

Click on the description to explore a ModelSet (see plots, download FITS files).

ModelSet name in `pdrtpy`	ModelSet Description
wk2020	Wolfire/Kaufman 2020 constant density models, A_V=7, no freeze-out, Z=1.0
wk2006	Wolfire/Kaufman 2006 constant density models, Z=3.0
wk2006	Wolfire/Kaufman 2006 constant density models, Z=1.0
smc	Wolfire/Kaufman 2006 limited set of constant density models for Small Magellanic Cloud, Z=0.1
lmc	Wolfire/Kaufman 2020 limited set of constant density models for Large Magellanic Cloud, surface chemistry turned off, Z=0.5
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M_⊙, Z=1.0
kt2020	KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, non-clumpy, single clump 1000 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, non-clumpy, single clump 100 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, non-clumpy, single clump 10 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, non-clumpy, single clump 1 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, non-clumpy, single clump 0.1 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, clumpy, maximum clump mass = 1000 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, clumpy, maximum clump mass = 100 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, clumpy, maximum clump mass = 10 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, clumpy, maximum clump mass = 1 M_⊙, Z=1.0
kt2013wd01-7	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=3.1, clumpy, maximum clump mass = 0.1 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, non-clumpy, single clump 1000 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, non-clumpy, single clump 100 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, non-clumpy, single clump 10 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, non-clumpy, single clump 1 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, non-clumpy, single clump 0.1 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, clumpy, maximum clump mass = 1000 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, clumpy, maximum clump mass = 100 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, clumpy, maximum clump mass = 10 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, clumpy, maximum clump mass = 1 M_⊙, Z=1.0
kt2013wd01-25	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=5.5, clumpy, maximum clump mass = 0.1 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, non-clumpy, single clump 1000 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, non-clumpy, single clump 100 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, non-clumpy, single clump 10 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, non-clumpy, single clump 1 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, non-clumpy, single clump 0.1 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, clumpy, maximum clump mass = 1000 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, clumpy, maximum clump mass = 100 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, clumpy, maximum clump mass = 10 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, clumpy, maximum clump mass = 1 M_⊙, Z=1.0
kt2013wd01-21	KOSMA-tau 2013 models, Weingarter & Draine 2001 R_V=4.0, clumpy, maximum clump mass = 0.1 M_⊙, Z=1.0