ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova

A. Pastorello; S. Taubenberger; N. Elias-Rosa; P. A. Mazzali; G. Pignata; E. Cappellaro; G. Garavini; S. Nobili; G. C. Anupama; D. D.R. Bayliss; S. Benetti; F. Bufano; N. K. Chakradhari; R. Kotak; A. Goobar; H. Navasardyan; F. Patat; D. K. Sahu; M. Salvo; B. P. Schmidt; V. Stanishev; M. Turatto; W. Hillebrandt

doi:10.1111/j.1365-2966.2007.11527.x

ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova

A. Pastorello^*
, S. Taubenberger
, N. Elias-Rosa
, P. A. Mazzali
, G. Pignata
, E. Cappellaro
, G. Garavini
, S. Nobili
, G. C. Anupama
, D. D.R. Bayliss
, S. Benetti
, F. Bufano
, N. K. Chakradhari
, R. Kotak
, A. Goobar
, H. Navasardyan
, F. Patat
, D. K. Sahu
, M. Salvo
, B. P. Schmidt

V. Stanishev, M. Turatto, W. Hillebrandt

^*Corresponding author for this work

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

91 Citations (Scopus)

Abstract

We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observations, spanning a period from about 12 d before to 3 months after maximum, have been obtained through the coordination of observational efforts of various nodes of the European Supernova Collaboration and including data obtained at the 2-m Himalayan Chandra Telescope. From the observed light curve we deduce that SN 2005cf is a fairly typical SN Ia with a post-maximum decline [Δm₁₅(B)_true = 1.12] close to the average value and a normal luminosity of M_B,max = -19.39 ±0.33. Models of the bolometric light curve suggest a synthesized ⁵⁶Ni mass of about 0.7 M_⊙. The negligible host galaxy interstellar extinction and its proximity make SN 2005cf a good Type Ia SN template.

Original language	English
Pages (from-to)	1301-1316
Number of pages	16
Journal	Monthly Notices of the Royal Astronomical Society
Volume	376
Issue number	3
DOIs	https://doi.org/10.1111/j.1365-2966.2007.11527.x
Publication status	Published - Apr 2007

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Pastorello, A., Taubenberger, S., Elias-Rosa, N., Mazzali, P. A., Pignata, G., Cappellaro, E., Garavini, G., Nobili, S., Anupama, G. C., Bayliss, D. D. R., Benetti, S., Bufano, F., Chakradhari, N. K., Kotak, R., Goobar, A., Navasardyan, H., Patat, F., Sahu, D. K., Salvo, M., ... Hillebrandt, W. (2007). ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova. Monthly Notices of the Royal Astronomical Society, 376(3), 1301-1316. https://doi.org/10.1111/j.1365-2966.2007.11527.x

@article{49532e19d86043abab33ae100612ec4c,

title = "ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova",

abstract = "We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observations, spanning a period from about 12 d before to 3 months after maximum, have been obtained through the coordination of observational efforts of various nodes of the European Supernova Collaboration and including data obtained at the 2-m Himalayan Chandra Telescope. From the observed light curve we deduce that SN 2005cf is a fairly typical SN Ia with a post-maximum decline [Δm15(B)true = 1.12] close to the average value and a normal luminosity of MB,max = -19.39 ±0.33. Models of the bolometric light curve suggest a synthesized 56Ni mass of about 0.7 M⊙. The negligible host galaxy interstellar extinction and its proximity make SN 2005cf a good Type Ia SN template.",

keywords = "Galaxies: individual: MCG-01-39-003, Galaxies: individual: NGC 5917, Supernovae: general, Supernovae: individual: SN 1992al, Supernovae: individual: SN 2001el, Supernovae: individual: SN 2005cf",

author = "A. Pastorello and S. Taubenberger and N. Elias-Rosa and Mazzali, \{P. A.\} and G. Pignata and E. Cappellaro and G. Garavini and S. Nobili and Anupama, \{G. C.\} and Bayliss, \{D. D.R.\} and S. Benetti and F. Bufano and Chakradhari, \{N. K.\} and R. Kotak and A. Goobar and H. Navasardyan and F. Patat and Sahu, \{D. K.\} and M. Salvo and Schmidt, \{B. P.\} and V. Stanishev and M. Turatto and W. Hillebrandt",

year = "2007",

month = apr,

doi = "10.1111/j.1365-2966.2007.11527.x",

language = "English",

volume = "376",

pages = "1301--1316",

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

issn = "0035-8711",

publisher = "Oxford University Press ",

number = "3",

}

Pastorello, A, Taubenberger, S, Elias-Rosa, N, Mazzali, PA, Pignata, G, Cappellaro, E, Garavini, G, Nobili, S, Anupama, GC, Bayliss, DDR, Benetti, S, Bufano, F, Chakradhari, NK, Kotak, R, Goobar, A, Navasardyan, H, Patat, F, Sahu, DK, Salvo, M, Schmidt, BP, Stanishev, V, Turatto, M & Hillebrandt, W 2007, 'ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova', Monthly Notices of the Royal Astronomical Society, vol. 376, no. 3, pp. 1301-1316. https://doi.org/10.1111/j.1365-2966.2007.11527.x

TY - JOUR

T1 - ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova

AU - Pastorello, A.

AU - Taubenberger, S.

AU - Elias-Rosa, N.

AU - Mazzali, P. A.

AU - Pignata, G.

AU - Cappellaro, E.

AU - Garavini, G.

AU - Nobili, S.

AU - Anupama, G. C.

AU - Bayliss, D. D.R.

AU - Benetti, S.

AU - Bufano, F.

AU - Chakradhari, N. K.

AU - Kotak, R.

AU - Goobar, A.

AU - Navasardyan, H.

AU - Patat, F.

AU - Sahu, D. K.

AU - Salvo, M.

AU - Schmidt, B. P.

AU - Stanishev, V.

AU - Turatto, M.

AU - Hillebrandt, W.

PY - 2007/4

Y1 - 2007/4

N2 - We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observations, spanning a period from about 12 d before to 3 months after maximum, have been obtained through the coordination of observational efforts of various nodes of the European Supernova Collaboration and including data obtained at the 2-m Himalayan Chandra Telescope. From the observed light curve we deduce that SN 2005cf is a fairly typical SN Ia with a post-maximum decline [Δm15(B)true = 1.12] close to the average value and a normal luminosity of MB,max = -19.39 ±0.33. Models of the bolometric light curve suggest a synthesized 56Ni mass of about 0.7 M⊙. The negligible host galaxy interstellar extinction and its proximity make SN 2005cf a good Type Ia SN template.

AB - We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observations, spanning a period from about 12 d before to 3 months after maximum, have been obtained through the coordination of observational efforts of various nodes of the European Supernova Collaboration and including data obtained at the 2-m Himalayan Chandra Telescope. From the observed light curve we deduce that SN 2005cf is a fairly typical SN Ia with a post-maximum decline [Δm15(B)true = 1.12] close to the average value and a normal luminosity of MB,max = -19.39 ±0.33. Models of the bolometric light curve suggest a synthesized 56Ni mass of about 0.7 M⊙. The negligible host galaxy interstellar extinction and its proximity make SN 2005cf a good Type Ia SN template.

KW - Galaxies: individual: MCG-01-39-003

KW - Galaxies: individual: NGC 5917

KW - Supernovae: general

KW - Supernovae: individual: SN 1992al

KW - Supernovae: individual: SN 2001el

KW - Supernovae: individual: SN 2005cf

UR - https://www.scopus.com/pages/publications/34147144032

U2 - 10.1111/j.1365-2966.2007.11527.x

DO - 10.1111/j.1365-2966.2007.11527.x

M3 - Article

SN - 0035-8711

VL - 376

SP - 1301

EP - 1316

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

ESC observations of SN 2005cf -I. Photometric evolution of a normal Type Ia supernova

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