SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

P. Armstrong; B. E. Tucker; A. Rest; R. Ridden-Harper; Y. Zenati; A. L. Piro; S. Hinton; C. Lidman; S. Margheim; G. Narayan; E. Shaya; P. Garnavich; D. Kasen; V. Villar; A. Zenteno; I. Arcavi; M. Drout; R. J. Foley; J. Wheeler; J. Anais; A. Campillay; D. Coulter; G. Dimitriadis; D. Jones; C. D. Kilpatrick; N. Muñoz-Elgueta; C. Rojas-Bravo; J. Vargas-González; J. Bulger; K. Chambers; M. Huber; T. Lowe; E. Magnier; B. J. Shappee; S. Smartt; K. W. Smith; T. Barclay; G. Barentsen; J. Dotson; M. Gully-Santiago; C. Hedges; S. Howell; A. Cody; K. Auchettl; A. Bódi; Zs Bognár; J. Brimacombe; P. Brown; B. Cseh; L. Galbany; D. Hiramatsu; T. W.S. Holoien; D. A. Howell; S. W. Jha; R. Könyves-Tóth; L. Kriskovics; C. McCully; P. Milne; J. Muñoz; Y. Pan; A. Pál; H. Sai; K. Sárneczky; N. Smith; Sódor; R. Szabó; R. Szakáts; S. Valenti; J. Vinkó; X. Wang; K. Zhang; G. Zsidi

doi:10.1093/mnras/stab2138

SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

P. Armstrong^*, B. E. Tucker^*, A. Rest^*, R. Ridden-Harper, Y. Zenati, A. L. Piro, S. Hinton, C. Lidman, S. Margheim, G. Narayan, E. Shaya, P. Garnavich, D. Kasen, V. Villar, A. Zenteno, I. Arcavi, M. Drout, R. J. Foley, J. Wheeler, J. AnaisA. Campillay, D. Coulter, G. Dimitriadis, D. Jones, C. D. Kilpatrick, N. Muñoz-Elgueta, C. Rojas-Bravo, J. Vargas-González, J. Bulger, K. Chambers, M. Huber, T. Lowe, E. Magnier, B. J. Shappee, S. Smartt, K. W. Smith, T. Barclay, G. Barentsen, J. Dotson, M. Gully-Santiago, C. Hedges, S. Howell, A. Cody, K. Auchettl, A. Bódi, Zs Bognár, J. Brimacombe, P. Brown, B. Cseh, L. Galbany, D. Hiramatsu, T. W.S. Holoien, D. A. Howell, S. W. Jha, R. Könyves-Tóth, L. Kriskovics, C. McCully, P. Milne, J. Muñoz, Y. Pan, A. Pál, H. Sai, K. Sárneczky, N. Smith, Sódor, R. Szabó, R. Szakáts, S. Valenti, J. Vinkó, X. Wang, K. Zhang, G. Zsidi

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

11 Scopus citations

Abstract

SN 2017jgh is a type IIb supernova discovered by Pan-STARRS during the C16/C17 campaigns of the Kepler/K2 mission. Here, we present the Kepler/K2 and ground based observations of SN 2017jgh, which captured the shock cooling of the progenitor shock breakout with an unprecedented cadence. This event presents a unique opportunity to investigate the progenitors of stripped envelope supernovae. By fitting analytical models to the SN 2017jgh light curve, we find that the progenitor of SN 2017jgh was likely a yellow supergiant with an envelope radius of ∼ 50-290R⊙, and an envelope mass of ∼ 0-1.7M⊙. SN 2017jgh likely had a shock velocity of ∼7500-10 300 km s-1. Additionally, we use the light curve of SN 2017jgh to investigate how early observations of the rise contribute to constraints on progenitor models. Fitting just the ground based observations, we find an envelope radius of ∼ 50-330R⊙, an envelope mass of ∼ 0.3-1.7M⊙ and a shock velocity of ∼9000-15 000 km s-1. Without the rise, the explosion time cannot be well constrained that leads to a systematic offset in the velocity parameter and larger uncertainties in the mass and radius. Therefore, it is likely that progenitor property estimates through these models may have larger systematic uncertainties than previously calculated.

Original language	English
Pages (from-to)	3125-3138
Number of pages	14
Journal	Monthly Notices of the Royal Astronomical Society
Volume	507
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stab2138
State	Published - 1 Nov 2021

Funding

Funders	Funder number
Ministerio de Ciencia, Innovación y Universidades
Israeli Council for Higher Education Alon Fellowship
Eötvös Loránd Tudományegyetem
Canada Research Chairs Program
University of Edinburgh
Johns Hopkins University
Australian Research Council Centre of Excellence
Max-Planck-Gesellschaft
Horizon 2020 Framework Programme
National Central University of Taiwan
United States-Israel Binational Science Foundation
Heising-Simons Foundation
Agencia Nacional de Investigacion y Desarrollo
Durham University
University of Maryland
Ministério da Ciência e Tecnologia
Queen's University Belfast
United States - Israel Binational Science Foundation
Ministerio de Ciencia, Tecnologia e Innovacion
Max Planck Institute for Astronomy
Smithsonian Astrophysical Observatory
Canadian Institute for Advanced Research
Magyar Tudományos Akadémia
European Research Council
Max Planck Institute for Extraterrestrial Physics
National Research, Development and Innovation Office
National Research Council Canada
Horizon 2020
Gordon and Betty Moore Foundation
University of Toronto	DGE1339067
National Aeronautics and Space Administration	NNX17AI64G, 80NSSC18K0302, NNX14AM74G, 80NSSC19K0112, NNX12AT65G
National Science Foundation	AST-2008108, AST- 1911074, 1339067, 852097, AST-1813176, 1911074, AST-1920392, HST-HF2-51458.001-A, AST- 1238877
Los Alamos National Laboratory	NOAO 2017B-0279, NOAO 2017B-0285
Natural Sciences and Engineering Research Council of Canada	grantRGPIN- 2019-06186
Space Telescope Science Institute	NNX08AR22G
Australian Research Council	CE170100013
NASA/K2	80NSSC18K0303, 80NSSC19K0113
MICIU	80NSSC19K1717, PID2020-115253GA-I00, RYC2019-027683
Nemzeti Kutatási Fejlesztési és Innovációs Hivatal	NKFIH PD-134784
Israel Science Foundation	2752/19
Academy of Sciences	GINOP 2.3.2-15- 2016-00033
European Commission	AST-1911151, AYA2017-84089, AST-1615455, 80NSSC19K0119, AST- 1911225
Korea Astronomy and Space Science Institute	GS-2017B-LP-13
David and Lucile Packard Foundation	HST-HF2-51462.001, NAS5-26555

Keywords

shock waves
supernovae: general
supernovae: individual
transients: supernovae

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10.1093/mnras/stab2138

Cite this

Armstrong, P., Tucker, B. E., Rest, A., Ridden-Harper, R., Zenati, Y., Piro, A. L., Hinton, S., Lidman, C., Margheim, S., Narayan, G., Shaya, E., Garnavich, P., Kasen, D., Villar, V., Zenteno, A., Arcavi, I., Drout, M., Foley, R. J., Wheeler, J., ... Zsidi, G. (2021). SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope. Monthly Notices of the Royal Astronomical Society, 507(3), 3125-3138. https://doi.org/10.1093/mnras/stab2138

@article{69ed015bfe5c47feb4a527db1d69df94,

title = "SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope",

abstract = "SN 2017jgh is a type IIb supernova discovered by Pan-STARRS during the C16/C17 campaigns of the Kepler/K2 mission. Here, we present the Kepler/K2 and ground based observations of SN 2017jgh, which captured the shock cooling of the progenitor shock breakout with an unprecedented cadence. This event presents a unique opportunity to investigate the progenitors of stripped envelope supernovae. By fitting analytical models to the SN 2017jgh light curve, we find that the progenitor of SN 2017jgh was likely a yellow supergiant with an envelope radius of ∼ 50-290R⊙, and an envelope mass of ∼ 0-1.7M⊙. SN 2017jgh likely had a shock velocity of ∼7500-10 300 km s-1. Additionally, we use the light curve of SN 2017jgh to investigate how early observations of the rise contribute to constraints on progenitor models. Fitting just the ground based observations, we find an envelope radius of ∼ 50-330R⊙, an envelope mass of ∼ 0.3-1.7M⊙ and a shock velocity of ∼9000-15 000 km s-1. Without the rise, the explosion time cannot be well constrained that leads to a systematic offset in the velocity parameter and larger uncertainties in the mass and radius. Therefore, it is likely that progenitor property estimates through these models may have larger systematic uncertainties than previously calculated.",

keywords = "shock waves, supernovae: general, supernovae: individual, transients: supernovae",

author = "P. Armstrong and Tucker, {B. E.} and A. Rest and R. Ridden-Harper and Y. Zenati and Piro, {A. L.} and S. Hinton and C. Lidman and S. Margheim and G. Narayan and E. Shaya and P. Garnavich and D. Kasen and V. Villar and A. Zenteno and I. Arcavi and M. Drout and Foley, {R. J.} and J. Wheeler and J. Anais and A. Campillay and D. Coulter and G. Dimitriadis and D. Jones and Kilpatrick, {C. D.} and N. Mu{\~n}oz-Elgueta and C. Rojas-Bravo and J. Vargas-Gonz{\'a}lez and J. Bulger and K. Chambers and M. Huber and T. Lowe and E. Magnier and Shappee, {B. J.} and S. Smartt and Smith, {K. W.} and T. Barclay and G. Barentsen and J. Dotson and M. Gully-Santiago and C. Hedges and S. Howell and A. Cody and K. Auchettl and A. B{\'o}di and Zs Bogn{\'a}r and J. Brimacombe and P. Brown and B. Cseh and L. Galbany and D. Hiramatsu and Holoien, {T. W.S.} and Howell, {D. A.} and Jha, {S. W.} and R. K{\"o}nyves-T{\'o}th and L. Kriskovics and C. McCully and P. Milne and J. Mu{\~n}oz and Y. Pan and A. P{\'a}l and H. Sai and K. S{\'a}rneczky and N. Smith and S{\'o}dor and R. Szab{\'o} and R. Szak{\'a}ts and S. Valenti and J. Vink{\'o} and X. Wang and K. Zhang and G. Zsidi",

note = "Publisher Copyright: {\textcopyright} 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2021",

month = nov,

day = "1",

doi = "10.1093/mnras/stab2138",

language = "אנגלית",

volume = "507",

pages = "3125--3138",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "3",

}

Armstrong, P, Tucker, BE, Rest, A, Ridden-Harper, R, Zenati, Y, Piro, AL, Hinton, S, Lidman, C, Margheim, S, Narayan, G, Shaya, E, Garnavich, P, Kasen, D, Villar, V, Zenteno, A, Arcavi, I, Drout, M, Foley, RJ, Wheeler, J, Anais, J, Campillay, A, Coulter, D, Dimitriadis, G, Jones, D, Kilpatrick, CD, Muñoz-Elgueta, N, Rojas-Bravo, C, Vargas-González, J, Bulger, J, Chambers, K, Huber, M, Lowe, T, Magnier, E, Shappee, BJ, Smartt, S, Smith, KW, Barclay, T, Barentsen, G, Dotson, J, Gully-Santiago, M, Hedges, C, Howell, S, Cody, A, Auchettl, K, Bódi, A, Bognár, Z, Brimacombe, J, Brown, P, Cseh, B, Galbany, L, Hiramatsu, D, Holoien, TWS, Howell, DA, Jha, SW, Könyves-Tóth, R, Kriskovics, L, McCully, C, Milne, P, Muñoz, J, Pan, Y, Pál, A, Sai, H, Sárneczky, K, Smith, N, Sódor, Szabó, R, Szakáts, R, Valenti, S, Vinkó, J, Wang, X, Zhang, K & Zsidi, G 2021, 'SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope', Monthly Notices of the Royal Astronomical Society, vol. 507, no. 3, pp. 3125-3138. https://doi.org/10.1093/mnras/stab2138

TY - JOUR

T1 - SN2017jgh

T2 - A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

AU - Armstrong, P.

AU - Tucker, B. E.

AU - Rest, A.

AU - Ridden-Harper, R.

AU - Zenati, Y.

AU - Piro, A. L.

AU - Hinton, S.

AU - Lidman, C.

AU - Margheim, S.

AU - Narayan, G.

AU - Shaya, E.

AU - Garnavich, P.

AU - Kasen, D.

AU - Villar, V.

AU - Zenteno, A.

AU - Arcavi, I.

AU - Drout, M.

AU - Foley, R. J.

AU - Wheeler, J.

AU - Anais, J.

AU - Campillay, A.

AU - Coulter, D.

AU - Dimitriadis, G.

AU - Jones, D.

AU - Kilpatrick, C. D.

AU - Muñoz-Elgueta, N.

AU - Rojas-Bravo, C.

AU - Vargas-González, J.

AU - Bulger, J.

AU - Chambers, K.

AU - Huber, M.

AU - Lowe, T.

AU - Magnier, E.

AU - Shappee, B. J.

AU - Smartt, S.

AU - Smith, K. W.

AU - Barclay, T.

AU - Barentsen, G.

AU - Dotson, J.

AU - Gully-Santiago, M.

AU - Hedges, C.

AU - Howell, S.

AU - Cody, A.

AU - Auchettl, K.

AU - Bódi, A.

AU - Bognár, Zs

AU - Brimacombe, J.

AU - Brown, P.

AU - Cseh, B.

AU - Galbany, L.

AU - Hiramatsu, D.

AU - Holoien, T. W.S.

AU - Howell, D. A.

AU - Jha, S. W.

AU - Könyves-Tóth, R.

AU - Kriskovics, L.

AU - McCully, C.

AU - Milne, P.

AU - Muñoz, J.

AU - Pan, Y.

AU - Pál, A.

AU - Sai, H.

AU - Sárneczky, K.

AU - Smith, N.

AU - Sódor,

AU - Szabó, R.

AU - Szakáts, R.

AU - Valenti, S.

AU - Vinkó, J.

AU - Wang, X.

AU - Zhang, K.

AU - Zsidi, G.

PY - 2021/11/1

Y1 - 2021/11/1

N2 - SN 2017jgh is a type IIb supernova discovered by Pan-STARRS during the C16/C17 campaigns of the Kepler/K2 mission. Here, we present the Kepler/K2 and ground based observations of SN 2017jgh, which captured the shock cooling of the progenitor shock breakout with an unprecedented cadence. This event presents a unique opportunity to investigate the progenitors of stripped envelope supernovae. By fitting analytical models to the SN 2017jgh light curve, we find that the progenitor of SN 2017jgh was likely a yellow supergiant with an envelope radius of ∼ 50-290R⊙, and an envelope mass of ∼ 0-1.7M⊙. SN 2017jgh likely had a shock velocity of ∼7500-10 300 km s-1. Additionally, we use the light curve of SN 2017jgh to investigate how early observations of the rise contribute to constraints on progenitor models. Fitting just the ground based observations, we find an envelope radius of ∼ 50-330R⊙, an envelope mass of ∼ 0.3-1.7M⊙ and a shock velocity of ∼9000-15 000 km s-1. Without the rise, the explosion time cannot be well constrained that leads to a systematic offset in the velocity parameter and larger uncertainties in the mass and radius. Therefore, it is likely that progenitor property estimates through these models may have larger systematic uncertainties than previously calculated.

AB - SN 2017jgh is a type IIb supernova discovered by Pan-STARRS during the C16/C17 campaigns of the Kepler/K2 mission. Here, we present the Kepler/K2 and ground based observations of SN 2017jgh, which captured the shock cooling of the progenitor shock breakout with an unprecedented cadence. This event presents a unique opportunity to investigate the progenitors of stripped envelope supernovae. By fitting analytical models to the SN 2017jgh light curve, we find that the progenitor of SN 2017jgh was likely a yellow supergiant with an envelope radius of ∼ 50-290R⊙, and an envelope mass of ∼ 0-1.7M⊙. SN 2017jgh likely had a shock velocity of ∼7500-10 300 km s-1. Additionally, we use the light curve of SN 2017jgh to investigate how early observations of the rise contribute to constraints on progenitor models. Fitting just the ground based observations, we find an envelope radius of ∼ 50-330R⊙, an envelope mass of ∼ 0.3-1.7M⊙ and a shock velocity of ∼9000-15 000 km s-1. Without the rise, the explosion time cannot be well constrained that leads to a systematic offset in the velocity parameter and larger uncertainties in the mass and radius. Therefore, it is likely that progenitor property estimates through these models may have larger systematic uncertainties than previously calculated.

KW - shock waves

KW - supernovae: general

KW - supernovae: individual

KW - transients: supernovae

UR - http://www.scopus.com/inward/record.url?scp=85115408172&partnerID=8YFLogxK

U2 - 10.1093/mnras/stab2138

DO - 10.1093/mnras/stab2138

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AN - SCOPUS:85115408172

SN - 0035-8711

VL - 507

SP - 3125

EP - 3138

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

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