UBVRIz light curves of 51 type II supernovae

Lluis Galbany; Mario Hamuy; Mark M. Phillips; Nicholas B. Suntzeff; José Maza; Thomas De Jaeger; Tania Moraga; Santiago González-Gaitán; Kevin Krisciunas; Nidia I. Morrell; Joanna Thomas-Osip; Wojtek Krzeminski; Luis González; Roberto Antezana; Marina Wishnjewski; Patrick McCarthy; Joseph P. Anderson; Claudia P. Gutiérrez; Maximilian Stritzinger; Gastón Folatelli; Claudio Anguita; Gaspar Galaz; Elisabeth M. Green; Chris Impey; Yong Cheol Kim; Sofia Kirhakos; Mathew A. Malkan; John S. Mulchaey; Andrew C. Phillips; Alessandro Pizzella; Charles F. Prosser; Brian P. Schmidt; Robert A. Schommer; William Sherry; Louis Gregory Strolger; Lisa A. Wells; Gerard M. Williger

doi:10.3847/0004-6256/151/2/33

UBVRIz light curves of 51 type II supernovae

Lluis Galbany, Mario Hamuy, Mark M. Phillips, Nicholas B. Suntzeff, José Maza, Thomas De Jaeger, Tania Moraga, Santiago González-Gaitán, Kevin Krisciunas, Nidia I. Morrell, Joanna Thomas-Osip, Wojtek Krzeminski, Luis González, Roberto Antezana, Marina Wishnjewski, Patrick McCarthy, Joseph P. Anderson, Claudia P. Gutiérrez, Maximilian Stritzinger, Gastón FolatelliClaudio Anguita, Gaspar Galaz, Elisabeth M. Green, Chris Impey, Yong Cheol Kim, Sofia Kirhakos, Mathew A. Malkan, John S. Mulchaey, Andrew C. Phillips, Alessandro Pizzella, Charles F. Prosser, Brian P. Schmidt, Robert A. Schommer, William Sherry, Louis Gregory Strolger, Lisa A. Wells, Gerard M. Williger

Department of Astronomy

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

66 Citations (Scopus)

Abstract

We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Calán/Tololo Supernova Program (C&T), the Supernova Optical and Infrared Survey (SOIRS), and the Carnegie Type II Supernova Survey (CATS). The photometry is based on template-subtracted images to eliminate any potential host galaxy light contamination, and calibrated from foreground stars. This work presents these photometric data, studies the color evolution using different bands, and explores the relation between the magnitude at maximum brightness and the brightness decline parameter (s) from maximum light through the end of the recombination phase. This parameter is found to be shallower for redder bands and appears to have the best correlation in the B band. In addition, it also correlates with the plateau duration, being shorter (longer) for larger (smaller) s values.

Original language	English
Article number	33
Journal	Astronomical Journal
Volume	151
Issue number	2
DOIs	https://doi.org/10.3847/0004-6256/151/2/33
Publication status	Published - 2016 Feb 1

Bibliographical note

Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved.

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.3847/0004-6256/151/2/33

Cite this

Galbany, L., Hamuy, M., Phillips, M. M., Suntzeff, N. B., Maza, J., Jaeger, T. D., Moraga, T., González-Gaitán, S., Krisciunas, K., Morrell, N. I., Thomas-Osip, J., Krzeminski, W., González, L., Antezana, R., Wishnjewski, M., McCarthy, P., Anderson, J. P., Gutiérrez, C. P., Stritzinger, M., ... Williger, G. M. (2016). UBVRIz light curves of 51 type II supernovae. Astronomical Journal, 151(2), [33]. https://doi.org/10.3847/0004-6256/151/2/33

@article{58e309608bef4f3cae353542ae51bbc9,

title = "UBVRIz light curves of 51 type II supernovae",

abstract = "We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Cal{\'a}n/Tololo Supernova Program (C&T), the Supernova Optical and Infrared Survey (SOIRS), and the Carnegie Type II Supernova Survey (CATS). The photometry is based on template-subtracted images to eliminate any potential host galaxy light contamination, and calibrated from foreground stars. This work presents these photometric data, studies the color evolution using different bands, and explores the relation between the magnitude at maximum brightness and the brightness decline parameter (s) from maximum light through the end of the recombination phase. This parameter is found to be shallower for redder bands and appears to have the best correlation in the B band. In addition, it also correlates with the plateau duration, being shorter (longer) for larger (smaller) s values.",

author = "Lluis Galbany and Mario Hamuy and Phillips, {Mark M.} and Suntzeff, {Nicholas B.} and Jos{\'e} Maza and Jaeger, {Thomas De} and Tania Moraga and Santiago Gonz{\'a}lez-Gait{\'a}n and Kevin Krisciunas and Morrell, {Nidia I.} and Joanna Thomas-Osip and Wojtek Krzeminski and Luis Gonz{\'a}lez and Roberto Antezana and Marina Wishnjewski and Patrick McCarthy and Anderson, {Joseph P.} and Guti{\'e}rrez, {Claudia P.} and Maximilian Stritzinger and Gast{\'o}n Folatelli and Claudio Anguita and Gaspar Galaz and Green, {Elisabeth M.} and Chris Impey and Kim, {Yong Cheol} and Sofia Kirhakos and Malkan, {Mathew A.} and Mulchaey, {John S.} and Phillips, {Andrew C.} and Alessandro Pizzella and Prosser, {Charles F.} and Schmidt, {Brian P.} and Schommer, {Robert A.} and William Sherry and Strolger, {Louis Gregory} and Wells, {Lisa A.} and Williger, {Gerard M.}",

year = "2016",

month = feb,

day = "1",

doi = "10.3847/0004-6256/151/2/33",

language = "English",

volume = "151",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "IOP Publishing Ltd.",

number = "2",

}

Galbany, L, Hamuy, M, Phillips, MM, Suntzeff, NB, Maza, J, Jaeger, TD, Moraga, T, González-Gaitán, S, Krisciunas, K, Morrell, NI, Thomas-Osip, J, Krzeminski, W, González, L, Antezana, R, Wishnjewski, M, McCarthy, P, Anderson, JP, Gutiérrez, CP, Stritzinger, M, Folatelli, G, Anguita, C, Galaz, G, Green, EM, Impey, C, Kim, YC, Kirhakos, S, Malkan, MA, Mulchaey, JS, Phillips, AC, Pizzella, A, Prosser, CF, Schmidt, BP, Schommer, RA, Sherry, W, Strolger, LG, Wells, LA & Williger, GM 2016, 'UBVRIz light curves of 51 type II supernovae', Astronomical Journal, vol. 151, no. 2, 33. https://doi.org/10.3847/0004-6256/151/2/33

TY - JOUR

T1 - UBVRIz light curves of 51 type II supernovae

AU - Galbany, Lluis

AU - Hamuy, Mario

AU - Phillips, Mark M.

AU - Suntzeff, Nicholas B.

AU - Maza, José

AU - Jaeger, Thomas De

AU - Moraga, Tania

AU - González-Gaitán, Santiago

AU - Krisciunas, Kevin

AU - Morrell, Nidia I.

AU - Thomas-Osip, Joanna

AU - Krzeminski, Wojtek

AU - González, Luis

AU - Antezana, Roberto

AU - Wishnjewski, Marina

AU - McCarthy, Patrick

AU - Anderson, Joseph P.

AU - Gutiérrez, Claudia P.

AU - Stritzinger, Maximilian

AU - Folatelli, Gastón

AU - Anguita, Claudio

AU - Galaz, Gaspar

AU - Green, Elisabeth M.

AU - Impey, Chris

AU - Kim, Yong Cheol

AU - Kirhakos, Sofia

AU - Malkan, Mathew A.

AU - Mulchaey, John S.

AU - Phillips, Andrew C.

AU - Pizzella, Alessandro

AU - Prosser, Charles F.

AU - Schmidt, Brian P.

AU - Schommer, Robert A.

AU - Sherry, William

AU - Strolger, Louis Gregory

AU - Wells, Lisa A.

AU - Williger, Gerard M.

PY - 2016/2/1

Y1 - 2016/2/1

N2 - We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Calán/Tololo Supernova Program (C&T), the Supernova Optical and Infrared Survey (SOIRS), and the Carnegie Type II Supernova Survey (CATS). The photometry is based on template-subtracted images to eliminate any potential host galaxy light contamination, and calibrated from foreground stars. This work presents these photometric data, studies the color evolution using different bands, and explores the relation between the magnitude at maximum brightness and the brightness decline parameter (s) from maximum light through the end of the recombination phase. This parameter is found to be shallower for redder bands and appears to have the best correlation in the B band. In addition, it also correlates with the plateau duration, being shorter (longer) for larger (smaller) s values.

AB - We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Calán/Tololo Supernova Program (C&T), the Supernova Optical and Infrared Survey (SOIRS), and the Carnegie Type II Supernova Survey (CATS). The photometry is based on template-subtracted images to eliminate any potential host galaxy light contamination, and calibrated from foreground stars. This work presents these photometric data, studies the color evolution using different bands, and explores the relation between the magnitude at maximum brightness and the brightness decline parameter (s) from maximum light through the end of the recombination phase. This parameter is found to be shallower for redder bands and appears to have the best correlation in the B band. In addition, it also correlates with the plateau duration, being shorter (longer) for larger (smaller) s values.

UR - http://www.scopus.com/inward/record.url?scp=84957954670&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84957954670&partnerID=8YFLogxK

U2 - 10.3847/0004-6256/151/2/33

DO - 10.3847/0004-6256/151/2/33

M3 - Article

AN - SCOPUS:84957954670

SN - 0004-6256

VL - 151

JO - Astronomical Journal

JF - Astronomical Journal

IS - 2

M1 - 33

ER -

UBVRIz light curves of 51 type II supernovae

Abstract

Bibliographical note

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this