A collection of model light curves calculated using TURTLS.
If you make use of any of these models, please cite Magee et al. 2018, which describes TURTLS in detail.
@ARTICLE{2018A&A...614A.115M,
author = {{Magee}, M.~R. and {Sim}, S.~A. and {Kotak}, R. and {Kerzendorf}, W.~E.},
title = "{Modelling the early time behaviour of type Ia supernovae: effects of the $^{56}$Ni distribution}",
journal = {\aap},
keywords = {supernovae: general, radiative transfer, methods: numerical, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2018,
month = jun,
volume = {614},
eid = {A115},
pages = {A115},
doi = {10.1051/0004-6361/201832675},
archivePrefix = {arXiv},
eprint = {1803.04436},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...614A.115M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you make use of the 56Ni distribution models, please cite Magee et al. 2020.
@ARTICLE{2020A&A...634A..37M,
author = {{Magee}, M.~R. and {Maguire}, K. and {Kotak}, R. and {Sim}, S.~A. and
{Gillanders}, J.~H. and {Prentice}, S.~J. and {Skillen}, K.},
title = "{Determining the $^{56}$Ni distribution of type Ia supernovae from observations within days of explosion}",
journal = {\aap},
keywords = {supernovae: general, radiative transfer, Astrophysics - High Energy Astrophysical Phenomena},
year = 2020,
month = feb,
volume = {634},
eid = {A37},
pages = {A37},
doi = {10.1051/0004-6361/201936684},
archivePrefix = {arXiv},
eprint = {1912.07603},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...634A..37M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you make use of the 56Ni clump models, please cite Magee & Maguire 2020.
@ARTICLE{2020A&A...642A.189M,
author = {{Magee}, M.~R. and {Maguire}, K.},
title = "{An investigation of $^{56}$Ni shells as the source of early light curve bumps in type Ia supernovae}",
journal = {\aap},
keywords = {radiative transfer, supernovae: general, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = oct,
volume = {642},
eid = {A189},
pages = {A189},
doi = {10.1051/0004-6361/202037870},
archivePrefix = {arXiv},
eprint = {2007.02101},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...642A.189M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you make use of the double detonation models, please cite Magee et al. 2021.
@ARTICLE{2021MNRAS.502.3533M,
author = {{Magee}, M.~R. and {Maguire}, K. and {Kotak}, R. and {Sim}, S.~A.},
title = "{Exploring the diversity of double-detonation explosions for Type Ia supernovae: effects of the post-explosion helium shell composition}",
journal = {\mnras},
keywords = {radiative transfer, supernovae: general, Astrophysics - High Energy Astrophysical Phenomena},
year = 2021,
month = apr,
volume = {502},
number = {3},
pages = {3533-3553},
doi = {10.1093/mnras/stab201},
archivePrefix = {arXiv},
eprint = {2101.09792},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.3533M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you make use of the companion interaction models, please cite Magee et al. 2022.
@ARTICLE{2022MNRAS.513.3035M,
author = {{Magee}, M.~R. and {Cuddy}, C. and {Maguire}, K. and {Deckers}, M. and {Dhawan}, S. and {Frohmaier}, C. and {Miller}, A.~A. and {Nordin}, J. and {Coughlin}, M.~W. and {Feinstein}, F. and {Riddle}, R.},
title = "{The detection efficiency of Type Ia supernovae from the Zwicky Transient Facility: limits on the intrinsic rate of early flux excesses}",
journal = {\mnras},
keywords = {radiative transfer, supernovae: general, Astrophysics - High Energy Astrophysical Phenomena},
year = 2022,
month = jun,
volume = {513},
number = {2},
pages = {3035-3049},
doi = {10.1093/mnras/stac1045},
archivePrefix = {arXiv},
eprint = {2204.09705},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.513.3035M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}