Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve

Qinan Wang; Patrick Armstrong; Yossef Zenati; Ryan Ridden-Harper; Armin Rest; Iair Arcavi; Charles D. Kilpatrick; Ryan J. Foley; Brad E. Tucker; Chris Lidman; Thomas L. Killestein; Melissa Shahbandeh; Joseph P. Anderson; Rodrigo Angulo; Chris Ashall; Jamison Burke; Ting Wan Chen; Sophie von Coelln; Kyle A. Dalrymple; Kyle W. Davis; Michael D. Fulton; Lluís Galbany; Estefania Padilla Gonzalez; Bore Gao; Mariusz Gromadzki; D. Andrew Howell; Nada Ihanec; Jacob E. Jencson; David O. Jones; Joseph D. Lyman; Curtis McCully; Tomás E. Müller-Bravo; Megan Newsome; Matt Nicholl; David O’Neill; Craig Pellegrino; Sofia Rest; Stephen J. Smartt; Ken Smith; Shubham Srivastav; Giacomo Terreran; Samaporn Tinyanont; David R. Young; Alfredo Zenteno

doi:10.3847/2041-8213/acb0d0

Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve

Qinan Wang, Patrick Armstrong, Yossef Zenati, Ryan Ridden-Harper, Armin Rest, Iair Arcavi, Charles D. Kilpatrick, Ryan J. Foley, Brad E. Tucker, Chris Lidman, Thomas L. Killestein, Melissa Shahbandeh, Joseph P. Anderson, Rodrigo Angulo, Chris Ashall, Jamison Burke, Ting Wan Chen, Sophie von Coelln, Kyle A. Dalrymple, Kyle W. DavisMichael D. Fulton, Lluís Galbany, Estefania Padilla Gonzalez, Bore Gao, Mariusz Gromadzki, D. Andrew Howell, Nada Ihanec, Jacob E. Jencson, David O. Jones, Joseph D. Lyman, Curtis McCully, Tomás E. Müller-Bravo, Megan Newsome, Matt Nicholl, David O’Neill, Craig Pellegrino, Sofia Rest, Stephen J. Smartt, Ken Smith, Shubham Srivastav, Giacomo Terreran, Samaporn Tinyanont, David R. Young, Alfredo Zenteno

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摘要

We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30-0.65 M _⊙ and an envelope radius of ∼120-300 R _⊙. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties.

原文	???core.languages.en_GB???
文章編號	L15
期刊	Astrophysical Journal Letters
卷	943
發行號	2
DOIs	https://doi.org/10.3847/2041-8213/acb0d0
出版狀態	已出版 - 1 2月 2023

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10.3847/2041-8213/acb0d0

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Wang, Q., Armstrong, P., Zenati, Y., Ridden-Harper, R., Rest, A., Arcavi, I., Kilpatrick, C. D., Foley, R. J., Tucker, B. E., Lidman, C., Killestein, T. L., Shahbandeh, M., Anderson, J. P., Angulo, R., Ashall, C., Burke, J., Chen, T. W., von Coelln, S., Dalrymple, K. A., ... Zenteno, A. (2023). Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve. Astrophysical Journal Letters, 943(2), 文章 L15. https://doi.org/10.3847/2041-8213/acb0d0

@article{73a3ab062eec449ca9bd5bbaf2f9c4ed,

title = "Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve",

abstract = "We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30-0.65 M ⊙ and an envelope radius of ∼120-300 R ⊙. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties.",

author = "Qinan Wang and Patrick Armstrong and Yossef Zenati and Ryan Ridden-Harper and Armin Rest and Iair Arcavi and Kilpatrick, {Charles D.} and Foley, {Ryan J.} and Tucker, {Brad E.} and Chris Lidman and Killestein, {Thomas L.} and Melissa Shahbandeh and Anderson, {Joseph P.} and Rodrigo Angulo and Chris Ashall and Jamison Burke and Chen, {Ting Wan} and {von Coelln}, Sophie and Dalrymple, {Kyle A.} and Davis, {Kyle W.} and Fulton, {Michael D.} and Llu{\'i}s Galbany and Gonzalez, {Estefania Padilla} and Bore Gao and Mariusz Gromadzki and Howell, {D. Andrew} and Nada Ihanec and Jencson, {Jacob E.} and Jones, {David O.} and Lyman, {Joseph D.} and Curtis McCully and M{\"u}ller-Bravo, {Tom{\'a}s E.} and Megan Newsome and Matt Nicholl and David O{\textquoteright}Neill and Craig Pellegrino and Sofia Rest and Smartt, {Stephen J.} and Ken Smith and Shubham Srivastav and Giacomo Terreran and Samaporn Tinyanont and Young, {David R.} and Alfredo Zenteno",

note = "Publisher Copyright: {\textcopyright} 2023. The Author(s). Published by the American Astronomical Society.",

year = "2023",

month = feb,

day = "1",

doi = "10.3847/2041-8213/acb0d0",

language = "???core.languages.en_GB???",

volume = "943",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

number = "2",

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Wang, Q, Armstrong, P, Zenati, Y, Ridden-Harper, R, Rest, A, Arcavi, I, Kilpatrick, CD, Foley, RJ, Tucker, BE, Lidman, C, Killestein, TL, Shahbandeh, M, Anderson, JP, Angulo, R, Ashall, C, Burke, J, Chen, TW, von Coelln, S, Dalrymple, KA, Davis, KW, Fulton, MD, Galbany, L, Gonzalez, EP, Gao, B, Gromadzki, M, Howell, DA, Ihanec, N, Jencson, JE, Jones, DO, Lyman, JD, McCully, C, Müller-Bravo, TE, Newsome, M, Nicholl, M, O’Neill, D, Pellegrino, C, Rest, S, Smartt, SJ, Smith, K, Srivastav, S, Terreran, G, Tinyanont, S, Young, DR & Zenteno, A 2023, 'Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve', Astrophysical Journal Letters, 卷 943, 編號 2, L15. https://doi.org/10.3847/2041-8213/acb0d0

TY - JOUR

T1 - Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve

AU - Wang, Qinan

AU - Armstrong, Patrick

AU - Zenati, Yossef

AU - Ridden-Harper, Ryan

AU - Rest, Armin

AU - Arcavi, Iair

AU - Kilpatrick, Charles D.

AU - Foley, Ryan J.

AU - Tucker, Brad E.

AU - Lidman, Chris

AU - Killestein, Thomas L.

AU - Shahbandeh, Melissa

AU - Anderson, Joseph P.

AU - Angulo, Rodrigo

AU - Ashall, Chris

AU - Burke, Jamison

AU - Chen, Ting Wan

AU - von Coelln, Sophie

AU - Dalrymple, Kyle A.

AU - Davis, Kyle W.

AU - Fulton, Michael D.

AU - Galbany, Lluís

AU - Gonzalez, Estefania Padilla

AU - Gao, Bore

AU - Gromadzki, Mariusz

AU - Howell, D. Andrew

AU - Ihanec, Nada

AU - Jencson, Jacob E.

AU - Jones, David O.

AU - Lyman, Joseph D.

AU - McCully, Curtis

AU - Müller-Bravo, Tomás E.

AU - Newsome, Megan

AU - Nicholl, Matt

AU - O’Neill, David

AU - Pellegrino, Craig

AU - Rest, Sofia

AU - Smartt, Stephen J.

AU - Smith, Ken

AU - Srivastav, Shubham

AU - Terreran, Giacomo

AU - Tinyanont, Samaporn

AU - Young, David R.

AU - Zenteno, Alfredo

PY - 2023/2/1

Y1 - 2023/2/1

N2 - We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30-0.65 M ⊙ and an envelope radius of ∼120-300 R ⊙. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties.

AB - We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30-0.65 M ⊙ and an envelope radius of ∼120-300 R ⊙. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties.

UR - http://www.scopus.com/inward/record.url?scp=85147341915&partnerID=8YFLogxK

U2 - 10.3847/2041-8213/acb0d0

DO - 10.3847/2041-8213/acb0d0

M3 - 期刊論文

AN - SCOPUS:85147341915

SN - 2041-8205

VL - 943

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L15

ER -

Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve

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