The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe

Wei Kang Zheng; Benjamin E. Stahl; Thomas De Jaeger; Alexei V. Filippenko; Shan Qin Wang; Wen Pei Gan; Thomas G. Brink; Ivan Altunin; Raphael Baer-Way; Andrew Bigley; Kyle Blanchard; Peter K. Blanchard; James Bradley; Samantha K. Cargill; Chadwick Casper; Teagan Chapman; Vidhi Chander; Sanyum Channa; Byung Yun Choi; Nick Choksi; Matthew Chu; Kelsey I. Clubb; Daniel P. Cohen; Paul A. Dalba; Asia Degraw; Maxime De Kouchkovsky; Michael Ellison; Edward Falcon; Ori D. Fox; Kiera Fuller; Mohan Ganeshalingam; Nachiket Girish; Carolina Gould; Goni Halevi; Andrew Halle; Kevin T. Hayakawa; Romain Hardy; Julia Hestenes; Andrew M. Hoffman; Michael Hyland; Benjamin T. Jeffers; Connor Jennings; Michael T. Kandrashoff; Anthony Khodanian; Minkyu Kim; Haejung Kim; Michelle E. Kislak; Daniel Krishnan; Sahana Kumar; Snehaa Ganesh Kumar; Joel Leja; Erin J. Leonard; Gary Z. Li; Weidong Li; Ji Shun Lian; Evelyn Liu; Thomas B. Lowe; Philip Lu; Emily Ma; Michelle N. Mason; Michael May; Kyle McAllister; Emma McGinness; Shaunak Modak; Jeffrey Molloy; Yukei S. Murakami; Omnarayani Nayak; Derek Perera; Kenia Pina; Druv Punjabi; Andrew Rikhter; Timothy W. Ross; Jackson Sipple; Costas Soler; Samantha Stegman; Haynes Stephens; James Sunseri; Kevin Tang; Stephen Taylor; Patrick Thrasher; Schuyler D. Van Dyk; Xiang Gao Wang; Jeremy Wayland; Andrew Wilkins; Abel Yagubyan; Heechan Yuk; Sameen Yunus; Keto D. Zhang

doi:10.1093/mnras/stac723

The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe

Wei Kang Zheng, Benjamin E. Stahl, Thomas De Jaeger, Alexei V. Filippenko, Shan Qin Wang, Wen Pei Gan, Thomas G. Brink, Ivan Altunin, Raphael Baer-Way, Andrew Bigley, Kyle Blanchard, Peter K. Blanchard, James Bradley, Samantha K. Cargill, Chadwick Casper, Teagan Chapman, Vidhi Chander, Sanyum Channa, Byung Yun Choi, Nick ChoksiMatthew Chu, Kelsey I. Clubb, Daniel P. Cohen, Paul A. Dalba, Asia Degraw, Maxime De Kouchkovsky, Michael Ellison, Edward Falcon, Ori D. Fox, Kiera Fuller, Mohan Ganeshalingam, Nachiket Girish, Carolina Gould, Goni Halevi, Andrew Halle, Kevin T. Hayakawa, Romain Hardy, Julia Hestenes, Andrew M. Hoffman, Michael Hyland, Benjamin T. Jeffers, Connor Jennings, Michael T. Kandrashoff, Anthony Khodanian, Minkyu Kim, Haejung Kim, Michelle E. Kislak, Daniel Krishnan, Sahana Kumar, Snehaa Ganesh Kumar, Joel Leja, Erin J. Leonard, Gary Z. Li, Weidong Li, Ji Shun Lian, Evelyn Liu, Thomas B. Lowe, Philip Lu, Emily Ma, Michelle N. Mason, Michael May, Kyle McAllister, Emma McGinness, Shaunak Modak, Jeffrey Molloy, Yukei S. Murakami, Omnarayani Nayak, Derek Perera, Kenia Pina, Druv Punjabi, Andrew Rikhter, Timothy W. Ross, Jackson Sipple, Costas Soler, Samantha Stegman, Haynes Stephens, James Sunseri, Kevin Tang, Stephen Taylor, Patrick Thrasher, Schuyler D. Van Dyk, Xiang Gao Wang, Jeremy Wayland, Andrew Wilkins, Abel Yagubyan, Heechan Yuk, Sameen Yunus, Keto D. Zhang

Astronomy & Astrophysics

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Abstract

We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.

Original language	English (US)
Pages (from-to)	3195-3214
Number of pages	20
Journal	Monthly Notices of the Royal Astronomical Society
Volume	512
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stac723
State	Published - May 1 2022

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1093/mnras/stac723

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Zheng, W. K., Stahl, B. E., De Jaeger, T., Filippenko, A. V., Wang, S. Q., Gan, W. P., Brink, T. G., Altunin, I., Baer-Way, R., Bigley, A., Blanchard, K., Blanchard, P. K., Bradley, J., Cargill, S. K., Casper, C., Chapman, T., Chander, V., Channa, S., Choi, B. Y., ... Zhang, K. D. (2022). The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe. Monthly Notices of the Royal Astronomical Society, 512(3), 3195-3214. https://doi.org/10.1093/mnras/stac723

@article{7ce53b3083284b63bd31764f0e48a958,

title = "The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe",

abstract = "We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.",

author = "Zheng, {Wei Kang} and Stahl, {Benjamin E.} and {De Jaeger}, Thomas and Filippenko, {Alexei V.} and Wang, {Shan Qin} and Gan, {Wen Pei} and Brink, {Thomas G.} and Ivan Altunin and Raphael Baer-Way and Andrew Bigley and Kyle Blanchard and Blanchard, {Peter K.} and James Bradley and Cargill, {Samantha K.} and Chadwick Casper and Teagan Chapman and Vidhi Chander and Sanyum Channa and Choi, {Byung Yun} and Nick Choksi and Matthew Chu and Clubb, {Kelsey I.} and Cohen, {Daniel P.} and Dalba, {Paul A.} and Asia Degraw and {De Kouchkovsky}, Maxime and Michael Ellison and Edward Falcon and Fox, {Ori D.} and Kiera Fuller and Mohan Ganeshalingam and Nachiket Girish and Carolina Gould and Goni Halevi and Andrew Halle and Hayakawa, {Kevin T.} and Romain Hardy and Julia Hestenes and Hoffman, {Andrew M.} and Michael Hyland and Jeffers, {Benjamin T.} and Connor Jennings and Kandrashoff, {Michael T.} and Anthony Khodanian and Minkyu Kim and Haejung Kim and Kislak, {Michelle E.} and Daniel Krishnan and Sahana Kumar and Kumar, {Snehaa Ganesh} and Joel Leja and Leonard, {Erin J.} and Li, {Gary Z.} and Weidong Li and Lian, {Ji Shun} and Evelyn Liu and Lowe, {Thomas B.} and Philip Lu and Emily Ma and Mason, {Michelle N.} and Michael May and Kyle McAllister and Emma McGinness and Shaunak Modak and Jeffrey Molloy and Murakami, {Yukei S.} and Omnarayani Nayak and Derek Perera and Kenia Pina and Druv Punjabi and Andrew Rikhter and Ross, {Timothy W.} and Jackson Sipple and Costas Soler and Samantha Stegman and Haynes Stephens and James Sunseri and Kevin Tang and Stephen Taylor and Patrick Thrasher and {Van Dyk}, {Schuyler D.} and Wang, {Xiang Gao} and Jeremy Wayland and Andrew Wilkins and Abel Yagubyan and Heechan Yuk and Sameen Yunus and Zhang, {Keto D.}",

note = "Publisher Copyright: {\textcopyright} 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2022",

month = may,

day = "1",

doi = "10.1093/mnras/stac723",

language = "English (US)",

volume = "512",

pages = "3195--3214",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "3",

}

Zheng, WK, Stahl, BE, De Jaeger, T, Filippenko, AV, Wang, SQ, Gan, WP, Brink, TG, Altunin, I, Baer-Way, R, Bigley, A, Blanchard, K, Blanchard, PK, Bradley, J, Cargill, SK, Casper, C, Chapman, T, Chander, V, Channa, S, Choi, BY, Choksi, N, Chu, M, Clubb, KI, Cohen, DP, Dalba, PA, Degraw, A, De Kouchkovsky, M, Ellison, M, Falcon, E, Fox, OD, Fuller, K, Ganeshalingam, M, Girish, N, Gould, C, Halevi, G, Halle, A, Hayakawa, KT, Hardy, R, Hestenes, J, Hoffman, AM, Hyland, M, Jeffers, BT, Jennings, C, Kandrashoff, MT, Khodanian, A, Kim, M, Kim, H, Kislak, ME, Krishnan, D, Kumar, S, Kumar, SG, Leja, J, Leonard, EJ, Li, GZ, Li, W, Lian, JS, Liu, E, Lowe, TB, Lu, P, Ma, E, Mason, MN, May, M, McAllister, K, McGinness, E, Modak, S, Molloy, J, Murakami, YS, Nayak, O, Perera, D, Pina, K, Punjabi, D, Rikhter, A, Ross, TW, Sipple, J, Soler, C, Stegman, S, Stephens, H, Sunseri, J, Tang, K, Taylor, S, Thrasher, P, Van Dyk, SD, Wang, XG, Wayland, J, Wilkins, A, Yagubyan, A, Yuk, H, Yunus, S & Zhang, KD 2022, 'The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 3, pp. 3195-3214. https://doi.org/10.1093/mnras/stac723

TY - JOUR

T1 - The Lick Observatory Supernova Search follow-up program

T2 - photometry data release of 70 SESNe

AU - Zheng, Wei Kang

AU - Stahl, Benjamin E.

AU - De Jaeger, Thomas

AU - Filippenko, Alexei V.

AU - Wang, Shan Qin

AU - Gan, Wen Pei

AU - Brink, Thomas G.

AU - Altunin, Ivan

AU - Baer-Way, Raphael

AU - Bigley, Andrew

AU - Blanchard, Kyle

AU - Blanchard, Peter K.

AU - Bradley, James

AU - Cargill, Samantha K.

AU - Casper, Chadwick

AU - Chapman, Teagan

AU - Chander, Vidhi

AU - Channa, Sanyum

AU - Choi, Byung Yun

AU - Choksi, Nick

AU - Chu, Matthew

AU - Clubb, Kelsey I.

AU - Cohen, Daniel P.

AU - Dalba, Paul A.

AU - Degraw, Asia

AU - De Kouchkovsky, Maxime

AU - Ellison, Michael

AU - Falcon, Edward

AU - Fox, Ori D.

AU - Fuller, Kiera

AU - Ganeshalingam, Mohan

AU - Girish, Nachiket

AU - Gould, Carolina

AU - Halevi, Goni

AU - Halle, Andrew

AU - Hayakawa, Kevin T.

AU - Hardy, Romain

AU - Hestenes, Julia

AU - Hoffman, Andrew M.

AU - Hyland, Michael

AU - Jeffers, Benjamin T.

AU - Jennings, Connor

AU - Kandrashoff, Michael T.

AU - Khodanian, Anthony

AU - Kim, Minkyu

AU - Kim, Haejung

AU - Kislak, Michelle E.

AU - Krishnan, Daniel

AU - Kumar, Sahana

AU - Kumar, Snehaa Ganesh

AU - Leja, Joel

AU - Leonard, Erin J.

AU - Li, Gary Z.

AU - Li, Weidong

AU - Lian, Ji Shun

AU - Liu, Evelyn

AU - Lowe, Thomas B.

AU - Lu, Philip

AU - Ma, Emily

AU - Mason, Michelle N.

AU - May, Michael

AU - McAllister, Kyle

AU - McGinness, Emma

AU - Modak, Shaunak

AU - Molloy, Jeffrey

AU - Murakami, Yukei S.

AU - Nayak, Omnarayani

AU - Perera, Derek

AU - Pina, Kenia

AU - Punjabi, Druv

AU - Rikhter, Andrew

AU - Ross, Timothy W.

AU - Sipple, Jackson

AU - Soler, Costas

AU - Stegman, Samantha

AU - Stephens, Haynes

AU - Sunseri, James

AU - Tang, Kevin

AU - Taylor, Stephen

AU - Thrasher, Patrick

AU - Van Dyk, Schuyler D.

AU - Wang, Xiang Gao

AU - Wayland, Jeremy

AU - Wilkins, Andrew

AU - Yagubyan, Abel

AU - Yuk, Heechan

AU - Yunus, Sameen

AU - Zhang, Keto D.

PY - 2022/5/1

Y1 - 2022/5/1

N2 - We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.

AB - We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.

UR - http://www.scopus.com/inward/record.url?scp=85131758671&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85131758671&partnerID=8YFLogxK

U2 - 10.1093/mnras/stac723

DO - 10.1093/mnras/stac723

M3 - Article

AN - SCOPUS:85131758671

SN - 0035-8711

VL - 512

SP - 3195

EP - 3214

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe

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