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; Ádám Sódor; R. Szabó; R. Szakáts; S. Valenti; J. Vinkó; X. Wang; K. Zhang; G. Zsidi

doi:https://doi.org/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, Ádám Sódor, R. Szabó, R. Szakáts, S. Valenti, J. Vinkó, X. Wang, K. Zhang, G. Zsidi

School of Physics and Astronomy

Tel Aviv University

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

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

Keywords

shock waves
supernovae: general
supernovae: individual
transients: supernovae

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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https://doi.org/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{e8a03a3591fb436998a14ad61a16f0ae,

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 {\'A}d{\'a}m 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 = "https://doi.org/10.1093/mnras/stab2138",

language = "الإنجليزيّة",

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, Á, 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, Ádám

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 - https://doi.org/10.1093/mnras/stab2138

DO - https://doi.org/10.1093/mnras/stab2138

M3 - مقالة

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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