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, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=75, avlos=27.05, avperp=26.12
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=60, avlos=14.00, avperp=12.12
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=45, avlos=9.90, avperp=7.00
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=30, avlos=8.08, avperp=4.04
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=0, avlos=7.00
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=75
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=60
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=45
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=30
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0

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