Links to All Available ModelSets

To see plots and download individual FITS files for a given ModelSet, click on its ModelSet Description.

ModelSet name in pdrtpyModelSet Description
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=0
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=30
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=45
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=60
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=75
wk2006Wolfire/Kaufman 2006 constant density models, Z=3.0, losangle=0
wk2006Wolfire/Kaufman 2006 constant density models, Z=1.0, losangle=0
smcWolfire/Kaufman 2006 limited set of constant density models for Small Magellanic Cloud, Z=0.1, losangle=0
lmcWolfire/Kaufman 2020 limited set of constant density models for Large Magellanic Cloud, surface chemistry turned off, Z=0.5, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0

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