Home > Research > Publications & Outputs > SN2017jgh: a high-cadence complete shock coolin...

Research

Links

Text available via DOI:

Keywords

View graph of relations

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

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Published

Standard

SN2017jgh: a high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope. / Armstrong, P.; Tucker, B. E.; Rest, A. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 507, No. 3, 01.11.2021, p. 3125-3138.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

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, Munoz-Elgueta, N, Rojas-Bravo, C, Vargas-Gonzalez, 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, Bodi, A, Bognar, Z, Brimacombe, J, Brown, P, Cseh, B, Galbany, L, Hiramatsu, D, Holoien, TW-S, Howell, DA, Jha, SW, Konyves-Toth, R, Kriskovics, L, McCully, C, Milne, P, Munoz, J, Pan, Y, Pal, A, Sai, H, Sarneczky, K, Smith, N, Sodor, A, Szabo, R, Szakats, R, Valenti, S, Vinko, 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

APA

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

Vancouver

Armstrong P, Tucker BE, Rest A, Ridden-Harper R, Zenati Y, Piro AL et al. SN2017jgh: a high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope. Monthly Notices of the Royal Astronomical Society. 2021 Nov 1;507(3):3125-3138. doi: 10.1093/mnras/stab2138

Author

Armstrong, P. ; Tucker, B. E. ; Rest, A. et al. / SN2017jgh: a high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope. In: Monthly Notices of the Royal Astronomical Society. 2021 ; Vol. 507, No. 3. pp. 3125-3138.

Bibtex

@article{20fee2dc82ce418b9f09ead7bec9f8f5,
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. Munoz-Elgueta and C. Rojas-Bravo and J. Vargas-Gonzalez 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. Bodi and Zs Bognar and J. Brimacombe and P. Brown and B. Cseh and L. Galbany and D. Hiramatsu and Holoien, {T. W-S} and Howell, {D. Andrew} and Jha, {S. W.} and R. Konyves-Toth and L. Kriskovics and C. McCully and P. Milne and J. Munoz and Y. Pan and A. Pal and H. Sai and K. Sarneczky and N. Smith and A. Sodor and R. Szabo and R. Szakats and S. Valenti and J. Vinko and X. Wang and K. Zhang and G. Zsidi",
year = "2021",
month = nov,
day = "1",
doi = "10.1093/mnras/stab2138",
language = "English",
volume = "507",
pages = "3125--3138",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "3",

}

RIS

TY - JOUR

T1 - SN2017jgh: 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 - Munoz-Elgueta, N.

AU - Rojas-Bravo, C.

AU - Vargas-Gonzalez, 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 - Bodi, A.

AU - Bognar, Zs

AU - Brimacombe, J.

AU - Brown, P.

AU - Cseh, B.

AU - Galbany, L.

AU - Hiramatsu, D.

AU - Holoien, T. W-S

AU - Howell, D. Andrew

AU - Jha, S. W.

AU - Konyves-Toth, R.

AU - Kriskovics, L.

AU - McCully, C.

AU - Milne, P.

AU - Munoz, J.

AU - Pan, Y.

AU - Pal, A.

AU - Sai, H.

AU - Sarneczky, K.

AU - Smith, N.

AU - Sodor, A.

AU - Szabo, R.

AU - Szakats, R.

AU - Valenti, S.

AU - Vinko, 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

U2 - 10.1093/mnras/stab2138

DO - 10.1093/mnras/stab2138

M3 - Journal article

VL - 507

SP - 3125

EP - 3138

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -