PISN light curve collection

All data presented on this page are calculated with the hydrodynamics radiative-transfer code STELLA (Blinnikov et al. 1998, 2000, 2006) by Sasha Kozyreva.

All questions, if any, please address to sasha.kozyreva @ gmail.com.

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Helium-core PISN models

KEPLER PISN models at zero metallicity by A. Heger

These light curves are calculated with STELLA and unpublished.

The results of radiative-transfer simulations computed with SEDONA for some of these models are published in Kasen, Heger, Woosley 2011

The stellar evolution models are from: Heger & Woosley 2002

model 56Ni [M⊙] He65 0.03 lbol tt SED He70 0.01 lbol tt SED He75 0.1 lbol tt SED He80 0.13 lbol tt SED He85 0.41 lbol tt SED He90 1.3 lbol tt SED He95 3 lbol tt SED He100 5.8 lbol tt SED He105 9.56 lbol tt SED He110 14 lbol tt SED He115 19 lbol tt SED He120 24.7 lbol tt SED He125 32. lbol tt SED He130 40 lbol tt SED

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H-poor/H-free PISNe

Initially hydrogenic GENEVA models at Z=0.001 by R. Hirschi

Kozyreva et al.2017 Gilmer et al.2017

model 56Ni [M⊙] P150 0.003 lbol tt SED P175 0.3 lbol tt SED P200 12 lbol tt SED P250 34 lbol tt SED

Note: The data presented on this page are different to those published in Gilmer et al.2017, because some numerical artefacts were corrected.

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Models with Hydrogen left in the envelope

Models at Z=0.001. N. Langer's stellar evolution code

Kozyreva et al. 2014

model Mfin/56Ni [M⊙] 150M 93/0.03 lbol tt SED 250M 167/19.3 lbol tt SED

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Modified models P150 and 150M

Kozyreva et al. 2018:

In this paper, we used modified models P150 (Gilmer et al. 2017) and 150M (Kozyreva et al. 2014) to match H-rich bright SN OGLE14-073. Both models have about 10 M⊙ of hydrogen mixed into the thick oxygen layer and 1.3 M⊙ of radioactive nickel ⁵⁶Ni.

model Mfin   56Ni [M⊙]   R [R⊙] P150-bf 91   1.37   1267 lbol tt SED 150M-bf 86   1.31   2000 lbol tt SED model R [R⊙] MH [M⊙] Eexpl [foe] 150M 3450 4.9 5 default model see files above 150M-3000R 3000 3.9 9 lbol tt 150M-14foe 2000 9.1 14 lbol tt 150M-He 2000 - 14 lbol tt model Ni mixed to Mr MH [M⊙] Eexpl [foe] P150 1267 R⊙ 4 3.8 6 default model see files above P150ni10 10 9.3 9 lbol tt P150ni30 30 9.3 9 lbol tt P150ni50 50 9.3 9 lbol tt

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The content of the lbol-files:

(1) time [days] (2) UBVRI-pseidobolometric [erg/s] (3) bolometric [erg/s] (4) X-ray-EUV <325Å (5) IR >890Å
Luminosities are in log10-scale.

The content of the tt-files:

(1) time [days] (2) Tbb [K] (3) Rbb [cm] (4) Teff [K] (7) Mbol (8) U (9) B (10) V (11) I (12)R

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In the case of making use of data from this website, please cite the Garching Core-Collapse Supernova Archive (by giving the link https://wwwmpa.mpa-garching.mpg.de/ccsnarchive/) as well as papers that are mentioned on this page. We made all possible efforts to ensure the correctness of the data in this archive. Errors, however, cannot be excluded. If any are found, we would appreciate being informed. — last update: