SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS

Conor L. Ransome; V. Ashley Villar; Anna Tartaglia; Sebastian Javier Gonzalez; Wynn V. Jacobson-Galán; Charles D. Kilpatrick; Raffaella Margutti; Ryan J. Foley; Matthew Grayling; Yuan Qi Ni; Ricardo Yarza; Christine Ye; Katie Auchettl; Thomas de Boer; Kenneth C. Chambers; David A. Coulter; Maria R. Drout; Diego Farias; Christa Gall; Hua Gao; Mark E. Huber; Adaeze L. Ibik; David O. Jones; Nandita Khetan; Chien Cheng Lin; Collin A. Politsch; Sandra I. Raimundo; Armin Rest; Richard J. Wainscoat; S. Karthik Yadavalli; Yossef Zenati

doi:10.3847/1538-4357/ad2df7

SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS

Conor L. Ransome, V. Ashley Villar, Anna Tartaglia, Sebastian Javier Gonzalez, Wynn V. Jacobson-Galán, Charles D. Kilpatrick, Raffaella Margutti, Ryan J. Foley, Matthew Grayling, Yuan Qi Ni, Ricardo Yarza, Christine Ye, Katie Auchettl, Thomas de Boer, Kenneth C. Chambers, David A. Coulter, Maria R. Drout, Diego Farias, Christa Gall, Hua GaoMark E. Huber, Adaeze L. Ibik, David O. Jones, Nandita Khetan, Chien Cheng Lin, Collin A. Politsch, Sandra I. Raimundo, Armin Rest, Richard J. Wainscoat, S. Karthik Yadavalli, Yossef Zenati

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

Abstract

The nearby type II supernova, SN 2023ixf in M101 exhibits signatures of early time interaction with circumstellar material in the first week postexplosion. This material may be the consequence of prior mass loss suffered by the progenitor, which possibly manifested in the form of a detectable presupernova outburst. We present an analysis of long-baseline preexplosion photometric data in the g, w, r, i, z, and y filters from Pan-STARRS as part of the Young Supernova Experiment, spanning ∼5000 days. We find no significant detections in the Pan-STARRS preexplosion light curves. We train a multilayer perceptron neural network to classify presupernova outbursts. We find no evidence of eruptive presupernova activity to a limiting absolute magnitude of −7 mag. The limiting magnitudes from the full set of gwrizy (average absolute magnitude ≈ −8 mag) data are consistent with previous preexplosion studies. We use deep photometry from the literature to constrain the progenitor of SN 2023ixf, finding that these data are consistent with a dusty red supergiant progenitor with luminosity log L / L ⊙ ≈ 5.12

Original language	English
Article number	93
Journal	Astrophysical Journal
Volume	965
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ad2df7
State	Published - 1 Apr 2024
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ad2df7

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Ransome, C. L., Villar, V. A., Tartaglia, A., Gonzalez, S. J., Jacobson-Galán, W. V., Kilpatrick, C. D., Margutti, R., Foley, R. J., Grayling, M., Ni, Y. Q., Yarza, R., Ye, C., Auchettl, K., de Boer, T., Chambers, K. C., Coulter, D. A., Drout, M. R., Farias, D., Gall, C., ... Zenati, Y. (2024). SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS. Astrophysical Journal, 965(1), Article 93. https://doi.org/10.3847/1538-4357/ad2df7

@article{ce531d9631434a0a816602ac508e793e,

title = "SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS",

abstract = "The nearby type II supernova, SN 2023ixf in M101 exhibits signatures of early time interaction with circumstellar material in the first week postexplosion. This material may be the consequence of prior mass loss suffered by the progenitor, which possibly manifested in the form of a detectable presupernova outburst. We present an analysis of long-baseline preexplosion photometric data in the g, w, r, i, z, and y filters from Pan-STARRS as part of the Young Supernova Experiment, spanning ∼5000 days. We find no significant detections in the Pan-STARRS preexplosion light curves. We train a multilayer perceptron neural network to classify presupernova outbursts. We find no evidence of eruptive presupernova activity to a limiting absolute magnitude of −7 mag. The limiting magnitudes from the full set of gwrizy (average absolute magnitude ≈ −8 mag) data are consistent with previous preexplosion studies. We use deep photometry from the literature to constrain the progenitor of SN 2023ixf, finding that these data are consistent with a dusty red supergiant progenitor with luminosity log L / L ⊙ ≈ 5.12",

author = "Ransome, {Conor L.} and Villar, {V. Ashley} and Anna Tartaglia and Gonzalez, {Sebastian Javier} and Jacobson-Gal{\'a}n, {Wynn V.} and Kilpatrick, {Charles D.} and Raffaella Margutti and Foley, {Ryan J.} and Matthew Grayling and Ni, {Yuan Qi} and Ricardo Yarza and Christine Ye and Katie Auchettl and {de Boer}, Thomas and Chambers, {Kenneth C.} and Coulter, {David A.} and Drout, {Maria R.} and Diego Farias and Christa Gall and Hua Gao and Huber, {Mark E.} and Ibik, {Adaeze L.} and Jones, {David O.} and Nandita Khetan and Lin, {Chien Cheng} and Politsch, {Collin A.} and Raimundo, {Sandra I.} and Armin Rest and Wainscoat, {Richard J.} and Yadavalli, {S. Karthik} and Yossef Zenati",

note = "Publisher Copyright: {\textcopyright} 2024. The Author(s). Published by the American Astronomical Society.",

year = "2024",

month = apr,

day = "1",

doi = "10.3847/1538-4357/ad2df7",

language = "الإنجليزيّة",

volume = "965",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

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Ransome, CL, Villar, VA, Tartaglia, A, Gonzalez, SJ, Jacobson-Galán, WV, Kilpatrick, CD, Margutti, R, Foley, RJ, Grayling, M, Ni, YQ, Yarza, R, Ye, C, Auchettl, K, de Boer, T, Chambers, KC, Coulter, DA, Drout, MR, Farias, D, Gall, C, Gao, H, Huber, ME, Ibik, AL, Jones, DO, Khetan, N, Lin, CC, Politsch, CA, Raimundo, SI, Rest, A, Wainscoat, RJ, Yadavalli, SK & Zenati, Y 2024, 'SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS', Astrophysical Journal, vol. 965, no. 1, 93. https://doi.org/10.3847/1538-4357/ad2df7

TY - JOUR

T1 - SN 2023ixf in Messier 101

T2 - The Twilight Years of the Progenitor as Seen by Pan-STARRS

AU - Ransome, Conor L.

AU - Villar, V. Ashley

AU - Tartaglia, Anna

AU - Gonzalez, Sebastian Javier

AU - Jacobson-Galán, Wynn V.

AU - Kilpatrick, Charles D.

AU - Margutti, Raffaella

AU - Foley, Ryan J.

AU - Grayling, Matthew

AU - Ni, Yuan Qi

AU - Yarza, Ricardo

AU - Ye, Christine

AU - Auchettl, Katie

AU - de Boer, Thomas

AU - Chambers, Kenneth C.

AU - Coulter, David A.

AU - Drout, Maria R.

AU - Farias, Diego

AU - Gall, Christa

AU - Gao, Hua

AU - Huber, Mark E.

AU - Ibik, Adaeze L.

AU - Jones, David O.

AU - Khetan, Nandita

AU - Lin, Chien Cheng

AU - Politsch, Collin A.

AU - Raimundo, Sandra I.

AU - Rest, Armin

AU - Wainscoat, Richard J.

AU - Yadavalli, S. Karthik

AU - Zenati, Yossef

PY - 2024/4/1

Y1 - 2024/4/1

N2 - The nearby type II supernova, SN 2023ixf in M101 exhibits signatures of early time interaction with circumstellar material in the first week postexplosion. This material may be the consequence of prior mass loss suffered by the progenitor, which possibly manifested in the form of a detectable presupernova outburst. We present an analysis of long-baseline preexplosion photometric data in the g, w, r, i, z, and y filters from Pan-STARRS as part of the Young Supernova Experiment, spanning ∼5000 days. We find no significant detections in the Pan-STARRS preexplosion light curves. We train a multilayer perceptron neural network to classify presupernova outbursts. We find no evidence of eruptive presupernova activity to a limiting absolute magnitude of −7 mag. The limiting magnitudes from the full set of gwrizy (average absolute magnitude ≈ −8 mag) data are consistent with previous preexplosion studies. We use deep photometry from the literature to constrain the progenitor of SN 2023ixf, finding that these data are consistent with a dusty red supergiant progenitor with luminosity log L / L ⊙ ≈ 5.12

AB - The nearby type II supernova, SN 2023ixf in M101 exhibits signatures of early time interaction with circumstellar material in the first week postexplosion. This material may be the consequence of prior mass loss suffered by the progenitor, which possibly manifested in the form of a detectable presupernova outburst. We present an analysis of long-baseline preexplosion photometric data in the g, w, r, i, z, and y filters from Pan-STARRS as part of the Young Supernova Experiment, spanning ∼5000 days. We find no significant detections in the Pan-STARRS preexplosion light curves. We train a multilayer perceptron neural network to classify presupernova outbursts. We find no evidence of eruptive presupernova activity to a limiting absolute magnitude of −7 mag. The limiting magnitudes from the full set of gwrizy (average absolute magnitude ≈ −8 mag) data are consistent with previous preexplosion studies. We use deep photometry from the literature to constrain the progenitor of SN 2023ixf, finding that these data are consistent with a dusty red supergiant progenitor with luminosity log L / L ⊙ ≈ 5.12

UR - http://www.scopus.com/inward/record.url?scp=85190293501&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ad2df7

DO - 10.3847/1538-4357/ad2df7

M3 - مقالة

SN - 0004-637X

VL - 965

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 93

ER -

SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS

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