The broad-lined Type Ic supernova 2003jd

S. Valenti; S. Benetti; E. Cappellaro; F. Patat; P. Mazzali; M. Turatto; K. Hurley; K. Maeda; A. Gal-Yam; R. J. Foley; A. V. Filippenko; A. Pastorello; P. Challis; F. Frontera; A. Harutyunyan; M. Iye; K. Kawabata; R. P. Kirshner; W. Li; Y. M. Lipkin; T. Matheson; K. Nomoto; E. O. Ofek; Y. Ohyama; E. Pian; D. Poznanski; M. Salvo; D. N. Sauer; B. P. Schmidt; A. Soderberg; L. Zampieri

doi:10.1111/j.1365-2966.2007.12647.x

The broad-lined Type Ic supernova 2003jd

S. Valenti^*, S. Benetti, E. Cappellaro, F. Patat, P. Mazzali, M. Turatto, K. Hurley, K. Maeda, A. Gal-Yam, R. J. Foley, A. V. Filippenko, A. Pastorello, P. Challis, F. Frontera, A. Harutyunyan, M. Iye, K. Kawabata, R. P. Kirshner, W. Li, Y. M. LipkinT. Matheson, K. Nomoto, E. O. Ofek, Y. Ohyama, E. Pian, D. Poznanski, M. Salvo, D. N. Sauer, B. P. Schmidt, A. Soderberg, L. Zampieri

^*Corresponding author for this work

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

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Abstract

The results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj) and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of M_ej = 3.0 ± 1 M_⊙ and a kinetic energy of E_k(tot) = 7⁺³_-2 × 10⁵¹ erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time-stretch factor. Finally, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB). Journal compilation

Original language	English
Pages (from-to)	1485-1500
Number of pages	16
Journal	Monthly Notices of the Royal Astronomical Society
Volume	383
Issue number	4
DOIs	https://doi.org/10.1111/j.1365-2966.2007.12647.x
State	Published - Feb 2008
Externally published	Yes

Funding

Funders	Funder number
National Science Foundation	0607485

Keywords

Supernovae: general
Supernovae: individual: 1996aq
Supernovae: individual: 2003jd

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10.1111/j.1365-2966.2007.12647.x

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Valenti, S., Benetti, S., Cappellaro, E., Patat, F., Mazzali, P., Turatto, M., Hurley, K., Maeda, K., Gal-Yam, A., Foley, R. J., Filippenko, A. V., Pastorello, A., Challis, P., Frontera, F., Harutyunyan, A., Iye, M., Kawabata, K., Kirshner, R. P., Li, W., ... Zampieri, L. (2008). The broad-lined Type Ic supernova 2003jd. Monthly Notices of the Royal Astronomical Society, 383(4), 1485-1500. https://doi.org/10.1111/j.1365-2966.2007.12647.x

@article{63dacf4697b449cfaeb4599da8ffd3a4,

title = "The broad-lined Type Ic supernova 2003jd",

abstract = "The results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj) and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of Mej = 3.0 ± 1 M⊙ and a kinetic energy of Ek(tot) = 7+3-2 × 1051 erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time-stretch factor. Finally, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB). Journal compilation",

keywords = "Supernovae: general, Supernovae: individual: 1996aq, Supernovae: individual: 2003jd",

author = "S. Valenti and S. Benetti and E. Cappellaro and F. Patat and P. Mazzali and M. Turatto and K. Hurley and K. Maeda and A. Gal-Yam and Foley, {R. J.} and Filippenko, {A. V.} and A. Pastorello and P. Challis and F. Frontera and A. Harutyunyan and M. Iye and K. Kawabata and Kirshner, {R. P.} and W. Li and Lipkin, {Y. M.} and T. Matheson and K. Nomoto and Ofek, {E. O.} and Y. Ohyama and E. Pian and D. Poznanski and M. Salvo and Sauer, {D. N.} and Schmidt, {B. P.} and A. Soderberg and L. Zampieri",

year = "2008",

month = feb,

doi = "10.1111/j.1365-2966.2007.12647.x",

language = "אנגלית",

volume = "383",

pages = "1485--1500",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "4",

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Valenti, S, Benetti, S, Cappellaro, E, Patat, F, Mazzali, P, Turatto, M, Hurley, K, Maeda, K, Gal-Yam, A, Foley, RJ, Filippenko, AV, Pastorello, A, Challis, P, Frontera, F, Harutyunyan, A, Iye, M, Kawabata, K, Kirshner, RP, Li, W, Lipkin, YM, Matheson, T, Nomoto, K, Ofek, EO, Ohyama, Y, Pian, E, Poznanski, D, Salvo, M, Sauer, DN, Schmidt, BP, Soderberg, A & Zampieri, L 2008, 'The broad-lined Type Ic supernova 2003jd', Monthly Notices of the Royal Astronomical Society, vol. 383, no. 4, pp. 1485-1500. https://doi.org/10.1111/j.1365-2966.2007.12647.x

TY - JOUR

T1 - The broad-lined Type Ic supernova 2003jd

AU - Valenti, S.

AU - Benetti, S.

AU - Cappellaro, E.

AU - Patat, F.

AU - Mazzali, P.

AU - Turatto, M.

AU - Hurley, K.

AU - Maeda, K.

AU - Gal-Yam, A.

AU - Foley, R. J.

AU - Filippenko, A. V.

AU - Pastorello, A.

AU - Challis, P.

AU - Frontera, F.

AU - Harutyunyan, A.

AU - Iye, M.

AU - Kawabata, K.

AU - Kirshner, R. P.

AU - Li, W.

AU - Lipkin, Y. M.

AU - Matheson, T.

AU - Nomoto, K.

AU - Ofek, E. O.

AU - Ohyama, Y.

AU - Pian, E.

AU - Poznanski, D.

AU - Salvo, M.

AU - Sauer, D. N.

AU - Schmidt, B. P.

AU - Soderberg, A.

AU - Zampieri, L.

PY - 2008/2

Y1 - 2008/2

N2 - The results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj) and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of Mej = 3.0 ± 1 M⊙ and a kinetic energy of Ek(tot) = 7+3-2 × 1051 erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time-stretch factor. Finally, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB). Journal compilation

AB - The results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj) and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of Mej = 3.0 ± 1 M⊙ and a kinetic energy of Ek(tot) = 7+3-2 × 1051 erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time-stretch factor. Finally, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB). Journal compilation

KW - Supernovae: general

KW - Supernovae: individual: 1996aq

KW - Supernovae: individual: 2003jd

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JO - Monthly Notices of the Royal Astronomical Society

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ER -

The broad-lined Type Ic supernova 2003jd

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