From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory

Research output: Contribution to journal › Journal article › Research › peer-review

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From core collapse to superluminous : the rates of massive stellar explosions from the Palomar Transient Factory. / Frohmaier, C.; Angus, C. R.; Vincenzi, M.; Sullivan, M.; Smith, M.; Nugent, P. E.; Cenko, S. B.; Gal-Yam, A.; Kulkarni, S. R.; Law, N. M.; Quimby, R. M.

In: Monthly Notices of the Royal Astronomical Society, Vol. 500, No. 4, 01.02.2021, p. 5142-5158.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Frohmaier, C, Angus, CR, Vincenzi, M, Sullivan, M, Smith, M, Nugent, PE, Cenko, SB, Gal-Yam, A, Kulkarni, SR, Law, NM & Quimby, RM 2021, 'From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 4, pp. 5142-5158. https://doi.org/10.1093/mnras/staa3607

APA

Frohmaier, C., Angus, C. R., Vincenzi, M., Sullivan, M., Smith, M., Nugent, P. E., Cenko, S. B., Gal-Yam, A., Kulkarni, S. R., Law, N. M., & Quimby, R. M. (2021). From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory. Monthly Notices of the Royal Astronomical Society, 500(4), 5142-5158. https://doi.org/10.1093/mnras/staa3607

Vancouver

Frohmaier C, Angus CR, Vincenzi M, Sullivan M, Smith M, Nugent PE et al. From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory. Monthly Notices of the Royal Astronomical Society. 2021 Feb 1;500(4):5142-5158. https://doi.org/10.1093/mnras/staa3607

Author

Frohmaier, C. ; Angus, C. R. ; Vincenzi, M. ; Sullivan, M. ; Smith, M. ; Nugent, P. E. ; Cenko, S. B. ; Gal-Yam, A. ; Kulkarni, S. R. ; Law, N. M. ; Quimby, R. M. / From core collapse to superluminous : the rates of massive stellar explosions from the Palomar Transient Factory. In: Monthly Notices of the Royal Astronomical Society. 2021 ; Vol. 500, No. 4. pp. 5142-5158.

Bibtex

@article{e278a20408f243d7bf4a7b5d74062220,
title = "From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory",
abstract = "We present measurements of the local core-collapse supernova (CCSN) rate using SN discoveries from the Palomar Transient Factory (PTF). We use a Monte Carlo simulation of hundreds of millions of SN light-curve realizations coupled with the detailed PTF survey detection efficiencies to forward model the SN rates in PTF. Using a sample of 86 CCSNe, including 26 stripped-envelope SNe (SESNe), we show that the overall CCSN volumetric rate is r(nu)(CC) = 9.10(-1.27)(+1.56) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3) at = 0.028, and the SESN volumetric rate is r(v)(SE) = 2.41(-0.64)(+0.81) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3). We further measure a volumetric rate for hydrogen-free superluminous SNe (SLSNe-I) using eight events at z",
keywords = "methods: data analysis, transients: supernovae, OBSERVATORY SUPERNOVA SEARCH, LIGHT CURVES, GALAXIES, STARS, PROGENITORS, DEPENDENCE, REDSHIFTS, EMISSION",
author = "C. Frohmaier and Angus, {C. R.} and M. Vincenzi and M. Sullivan and M. Smith and Nugent, {P. E.} and Cenko, {S. B.} and A. Gal-Yam and Kulkarni, {S. R.} and Law, {N. M.} and Quimby, {R. M.}",
year = "2021",
month = feb,
day = "1",
doi = "10.1093/mnras/staa3607",
language = "English",
volume = "500",
pages = "5142--5158",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "4",

}

RIS

TY - JOUR

T1 - From core collapse to superluminous

T2 - the rates of massive stellar explosions from the Palomar Transient Factory

AU - Frohmaier, C.

AU - Angus, C. R.

AU - Vincenzi, M.

AU - Sullivan, M.

AU - Smith, M.

AU - Nugent, P. E.

AU - Cenko, S. B.

AU - Gal-Yam, A.

AU - Kulkarni, S. R.

AU - Law, N. M.

AU - Quimby, R. M.

PY - 2021/2/1

Y1 - 2021/2/1

N2 - We present measurements of the local core-collapse supernova (CCSN) rate using SN discoveries from the Palomar Transient Factory (PTF). We use a Monte Carlo simulation of hundreds of millions of SN light-curve realizations coupled with the detailed PTF survey detection efficiencies to forward model the SN rates in PTF. Using a sample of 86 CCSNe, including 26 stripped-envelope SNe (SESNe), we show that the overall CCSN volumetric rate is r(nu)(CC) = 9.10(-1.27)(+1.56) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3) at = 0.028, and the SESN volumetric rate is r(v)(SE) = 2.41(-0.64)(+0.81) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3). We further measure a volumetric rate for hydrogen-free superluminous SNe (SLSNe-I) using eight events at z

AB - We present measurements of the local core-collapse supernova (CCSN) rate using SN discoveries from the Palomar Transient Factory (PTF). We use a Monte Carlo simulation of hundreds of millions of SN light-curve realizations coupled with the detailed PTF survey detection efficiencies to forward model the SN rates in PTF. Using a sample of 86 CCSNe, including 26 stripped-envelope SNe (SESNe), we show that the overall CCSN volumetric rate is r(nu)(CC) = 9.10(-1.27)(+1.56) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3) at = 0.028, and the SESN volumetric rate is r(v)(SE) = 2.41(-0.64)(+0.81) x 10(-5) SNe yr(-1) Mpc(-3) h(70)(3). We further measure a volumetric rate for hydrogen-free superluminous SNe (SLSNe-I) using eight events at z

KW - methods: data analysis

KW - transients: supernovae

KW - OBSERVATORY SUPERNOVA SEARCH

KW - LIGHT CURVES

KW - GALAXIES

KW - STARS

KW - PROGENITORS

KW - DEPENDENCE

KW - REDSHIFTS

KW - EMISSION

U2 - 10.1093/mnras/staa3607

DO - 10.1093/mnras/staa3607

M3 - Journal article

VL - 500

SP - 5142

EP - 5158

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 4

ER -

ID: 256626174