A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu

Z. Cano; A. De Ugarte Postigo; A. Pozanenko; Nathaniel Butler; C. C. Thöne; C. Guidorzi; T. Krühler; J. Gorosabel; P. Jakobsson; G. Leloudas; D. Malesani; J. Hjorth; A. Melandri; C. Mundell; K. Wiersema; P. D'Avanzo; S. Schulze; A. Gomboc; A. Johansson; W. Zheng; D. A. Kann; F. Knust; K. Varela; C. W. Akerlof; J. Bloom; O. Burkhonov; E. Cooke; J. A. De Diego; G. Dhungana; C. Farina; F. V. Ferrante; H. A. Flewelling; O. D. Fox; J. Fynbo; N. Gehrels; L. Georgiev; J. J. González; J. Greiner; T. Güver; O. Hartoog; N. Hatch; M. Jelinek; R. Kehoe; S. Klose; E. Klunko; D. Kopač; A. Kutyrev; Y. Krugly; W. H. Lee; A. Levan; V. Linkov; A. Matkin; N. Minikulov; I. Molotov; J. X. Prochaska; M. G. Richer; C. G. Román-Zúñiga; V. Rumyantsev; R. Sánchez-Ramírez; I. Steele; N. R. Tanvir; A. Volnova; A. M. Watson; D. Xu; F. Yuan

doi:10.1051/0004-6361/201423920

A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu

Z. Cano, A. De Ugarte Postigo, A. Pozanenko, Nathaniel Butler, C. C. Thöne, C. Guidorzi, T. Krühler, J. Gorosabel, P. Jakobsson, G. Leloudas, D. Malesani, J. Hjorth, A. Melandri, C. Mundell, K. Wiersema, P. D'Avanzo, S. Schulze, A. Gomboc, A. Johansson, W. ZhengD. A. Kann, F. Knust, K. Varela, C. W. Akerlof, J. Bloom, O. Burkhonov, E. Cooke, J. A. De Diego, G. Dhungana, C. Farina, F. V. Ferrante, H. A. Flewelling, O. D. Fox, J. Fynbo, N. Gehrels, L. Georgiev, J. J. González, J. Greiner, T. Güver, O. Hartoog, N. Hatch, M. Jelinek, R. Kehoe, S. Klose, E. Klunko, D. Kopač, A. Kutyrev, Y. Krugly, W. H. Lee, A. Levan, V. Linkov, A. Matkin, N. Minikulov, I. Molotov, J. X. Prochaska, M. G. Richer, C. G. Román-Zúñiga, V. Rumyantsev, R. Sánchez-Ramírez, I. Steele, N. R. Tanvir, A. Volnova, A. M. Watson, D. Xu, F. Yuan

Earth and Space Exploration, School of (SESE)

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

62 Scopus citations

Abstract

We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. For GRB 130215A/SN 2013ez, we also present optical spectroscopy at t - t₀ = 16.1 d, which covers rest-frame 3000-6250 Å. Based on Fe ii λ5169 and Si ii λ6355, our spectrum indicates an unusually low expansion velocity of ~4000-6350 km s^-1, the lowest ever measured for a GRB-SN. Additionally, we determined the brightness and shape of each accompanying SN relative to a template supernova (SN 1998bw), which were used to estimate the amount of nickel produced via nucleosynthesis during each explosion. We find that our derived nickel masses are typical of other GRB-SNe, and greater than those of SNe Ibc that are not associated with GRBs. For GRB 130831A/SN 2013fu, we used our well-sampled R-band light curve (LC) to estimate the amount of ejecta mass and the kinetic energy of the SN, finding that these too are similar to other GRB-SNe. For GRB 130215A, we took advantage of contemporaneous optical/NIR observations to construct an optical/NIR bolometric LC of the afterglow. We fit the bolometric LC with the millisecond magnetar model of Zhang & Mészáros (2001, ApJ, 552, L35), which considers dipole radiation as a source of energy injection to the forward shock powering the optical/NIR afterglow. Using this model we derive an initial spin period of P = 12 ms and a magnetic field of B = 1.1 × 10¹⁵ G, which are commensurate with those found for proposed magnetar central engines of other long-duration GRBs.

Original language	English (US)
Article number	A19
Journal	Astronomy and Astrophysics
Volume	568
DOIs	https://doi.org/10.1051/0004-6361/201423920
State	Published - Aug 2014

Keywords

Gamma-ray burst: general
Gamma-ray burst: individual: SN 2013ez
Supernovae: general
Supernovae: individual: SN 2013fu

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1051/0004-6361/201423920

Cite this

Cano, Z., De Ugarte Postigo, A., Pozanenko, A., Butler, N., Thöne, C. C., Guidorzi, C., Krühler, T., Gorosabel, J., Jakobsson, P., Leloudas, G., Malesani, D., Hjorth, J., Melandri, A., Mundell, C., Wiersema, K., D'Avanzo, P., Schulze, S., Gomboc, A., Johansson, A., ... Yuan, F. (2014). A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. Astronomy and Astrophysics, 568, Article A19. https://doi.org/10.1051/0004-6361/201423920

Cano, Z, De Ugarte Postigo, A, Pozanenko, A, Butler, N, Thöne, CC, Guidorzi, C, Krühler, T, Gorosabel, J, Jakobsson, P, Leloudas, G, Malesani, D, Hjorth, J, Melandri, A, Mundell, C, Wiersema, K, D'Avanzo, P, Schulze, S, Gomboc, A, Johansson, A, Zheng, W, Kann, DA, Knust, F, Varela, K, Akerlof, CW, Bloom, J, Burkhonov, O, Cooke, E, De Diego, JA, Dhungana, G, Farina, C, Ferrante, FV, Flewelling, HA, Fox, OD, Fynbo, J, Gehrels, N, Georgiev, L, González, JJ, Greiner, J, Güver, T, Hartoog, O, Hatch, N, Jelinek, M, Kehoe, R, Klose, S, Klunko, E, Kopač, D, Kutyrev, A, Krugly, Y, Lee, WH, Levan, A, Linkov, V, Matkin, A, Minikulov, N, Molotov, I, Prochaska, JX, Richer, MG, Román-Zúñiga, CG, Rumyantsev, V, Sánchez-Ramírez, R, Steele, I, Tanvir, NR, Volnova, A, Watson, AM, Xu, D & Yuan, F 2014, 'A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu', Astronomy and Astrophysics, vol. 568, A19. https://doi.org/10.1051/0004-6361/201423920

@article{71251c407e234d33acea1e19a798eb2b,

title = "A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu",

abstract = "We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. For GRB 130215A/SN 2013ez, we also present optical spectroscopy at t - t0 = 16.1 d, which covers rest-frame 3000-6250 {\AA}. Based on Fe ii λ5169 and Si ii λ6355, our spectrum indicates an unusually low expansion velocity of ~4000-6350 km s-1, the lowest ever measured for a GRB-SN. Additionally, we determined the brightness and shape of each accompanying SN relative to a template supernova (SN 1998bw), which were used to estimate the amount of nickel produced via nucleosynthesis during each explosion. We find that our derived nickel masses are typical of other GRB-SNe, and greater than those of SNe Ibc that are not associated with GRBs. For GRB 130831A/SN 2013fu, we used our well-sampled R-band light curve (LC) to estimate the amount of ejecta mass and the kinetic energy of the SN, finding that these too are similar to other GRB-SNe. For GRB 130215A, we took advantage of contemporaneous optical/NIR observations to construct an optical/NIR bolometric LC of the afterglow. We fit the bolometric LC with the millisecond magnetar model of Zhang & M{\'e}sz{\'a}ros (2001, ApJ, 552, L35), which considers dipole radiation as a source of energy injection to the forward shock powering the optical/NIR afterglow. Using this model we derive an initial spin period of P = 12 ms and a magnetic field of B = 1.1 × 1015 G, which are commensurate with those found for proposed magnetar central engines of other long-duration GRBs.",

keywords = "Gamma-ray burst: general, Gamma-ray burst: individual: SN 2013ez, Supernovae: general, Supernovae: individual: SN 2013fu",

author = "Z. Cano and {De Ugarte Postigo}, A. and A. Pozanenko and Nathaniel Butler and Th{\"o}ne, {C. C.} and C. Guidorzi and T. Kr{\"u}hler and J. Gorosabel and P. Jakobsson and G. Leloudas and D. Malesani and J. Hjorth and A. Melandri and C. Mundell and K. Wiersema and P. D'Avanzo and S. Schulze and A. Gomboc and A. Johansson and W. Zheng and Kann, {D. A.} and F. Knust and K. Varela and Akerlof, {C. W.} and J. Bloom and O. Burkhonov and E. Cooke and {De Diego}, {J. A.} and G. Dhungana and C. Farina and Ferrante, {F. V.} and Flewelling, {H. A.} and Fox, {O. D.} and J. Fynbo and N. Gehrels and L. Georgiev and Gonz{\'a}lez, {J. J.} and J. Greiner and T. G{\"u}ver and O. Hartoog and N. Hatch and M. Jelinek and R. Kehoe and S. Klose and E. Klunko and D. Kopa{\v c} and A. Kutyrev and Y. Krugly and Lee, {W. H.} and A. Levan and V. Linkov and A. Matkin and N. Minikulov and I. Molotov and Prochaska, {J. X.} and Richer, {M. G.} and Rom{\'a}n-Z{\'u}{\~n}iga, {C. G.} and V. Rumyantsev and R. S{\'a}nchez-Ram{\'i}rez and I. Steele and Tanvir, {N. R.} and A. Volnova and Watson, {A. M.} and D. Xu and F. Yuan",

note = "Funding Information: I am very grateful to Max de Pasquale for countless discussions regarding GRB physics, and Antonia Rowlinson for equally stimulating conversations regarding magnetars. We thank the referee for their insightful comments on the original manuscript. Z.C. gratefully acknowledges support by a Project Grant from the Icelandic Research Fund. The Dark Cosmology Centre is funded by the Danish National Research Foundation. The research activity of AdUP, CT, RSR, and JGor is supported by Spanish research project AYA2012-39362-C02-02. J.Gor and RSR are also supported by project AYA2012-39727-C03-01. AdUP acknowledges support by the European Commission under the Marie Curie Career Integration Grant programme (FP7-PEOPLE-2012-CIG 322307). T.K. acknowledges support by the European Commission under the Marie Curie Intra-European Fellowship Programme. The research activity of AM and PDA is supported by ASI grant INAF I/004/11/. A.P., A.V. acknowledge partial support by RFBR grants 12-02-01336, 14-02-10015, and A.M., I.M. acknowledge support by RFBR grant 13-01-92204. D.A.K. acknowledges support by the Max-Planck Institut f{\"u}r Extraterrestrische Physik, Garching, and the Th{\"u}ringer Landessternwarte Tautenburg. J.X.P. acknowledges support from NASA Swift Grant NNX13AJ67G. J.P.U.F. acknowledges support from the ERC-StG grant EGGS-278202. Based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrof{\'i}sica de Canarias. Based on observations made with the Gran Telescopio Canarias (GTC), instaled in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrof{\'i}sica de Canarias, in the island of La Palma. The Liverpool Telescope is operated by Liverpool John Moores University at the Observatorio del Roque de los Muchachos of the Instituto de Astrof{\'i}sica de Canarias. The Faulkes Telescopes are owned by Las Cumbres Observatory. C.G.M. acknowledges support from the Royal Society, the Wolfson Foundation and the Science and Technology Facilities Council. The ROTSE-IIIb telescope is operated by Southern Methodist University at McDonald Observatory, Ft. Davis, Texas. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. Additionally, we thank the RATIR project team and the staff of the Observatorio Astronmico Nacional on Sierra San Pedro M{\'a}rtir. RATIR is a collaboration between the University of California, the Universidad Nacional Auton{\'o}ma de M{\'e}xico, NASA Goddard Space Flight Center, and Arizona State University, benefiting from the loan of an H2RG detector and hardware and software support from Teledyne Scientific and Imaging. RATIR, the automation of the Harold L. Johnson Telescope of the Observatorio Astron{\'o}mico Nacional on Sierra San Pedro M{\'a}rtir, and the operation of both are funded through NASA grants NNX09AH71G, NNX09AT02G, NNX10AI27G, and NNX12AE66G, CONACyT grants INFR-2009-01-122785 and CB-2008-101958, UNAM PAPIIT grant IN113810, and UC MEXUS-CONACyT grant CN 09-283. S.S. acknowledges support from CONICYT through FONDECYT grant 3140534, from Basal-CATA PFB-06/2007, Iniciativa Cientifica Milenio grant P10-064-F (Millennium Center for Supernova Science), and by Project IC120009 “Millennium Institute of Astrophysics (MAS)” of Iniciativa Cient{\'i}fica Milenio del Ministerio de Economa, Fomento y Turismo de Chile, with input from “Fondo de Innovaci{\'o}n para la Competitividad, del Ministerio de Econom{\'i}a, Fomento y Turismo de Chile”. Part of this work is based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Minist{\'e}rio da Ci{\^e}ncia, Tecnologia e Inova{\c c}{\~a}o (Brazil) and Ministerio de Ciencia, Tecnolog{\'i}a e Innovaci{\'o}n Productiva (Argentina). Part of the fundingfor GROND (both hardware as well as personnel) was generously granted from the Leibniz-Prize to G. Hasinger (DFG grant HA 1850/28-1).",

year = "2014",

month = aug,

doi = "10.1051/0004-6361/201423920",

language = "English (US)",

volume = "568",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

TY - JOUR

T1 - A trio of gamma-ray burst supernovae

T2 - GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu

AU - Cano, Z.

AU - De Ugarte Postigo, A.

AU - Pozanenko, A.

AU - Butler, Nathaniel

AU - Thöne, C. C.

AU - Guidorzi, C.

AU - Krühler, T.

AU - Gorosabel, J.

AU - Jakobsson, P.

AU - Leloudas, G.

AU - Malesani, D.

AU - Hjorth, J.

AU - Melandri, A.

AU - Mundell, C.

AU - Wiersema, K.

AU - D'Avanzo, P.

AU - Schulze, S.

AU - Gomboc, A.

AU - Johansson, A.

AU - Zheng, W.

AU - Kann, D. A.

AU - Knust, F.

AU - Varela, K.

AU - Akerlof, C. W.

AU - Bloom, J.

AU - Burkhonov, O.

AU - Cooke, E.

AU - De Diego, J. A.

AU - Dhungana, G.

AU - Farina, C.

AU - Ferrante, F. V.

AU - Flewelling, H. A.

AU - Fox, O. D.

AU - Fynbo, J.

AU - Gehrels, N.

AU - Georgiev, L.

AU - González, J. J.

AU - Greiner, J.

AU - Güver, T.

AU - Hartoog, O.

AU - Hatch, N.

AU - Jelinek, M.

AU - Kehoe, R.

AU - Klose, S.

AU - Klunko, E.

AU - Kopač, D.

AU - Kutyrev, A.

AU - Krugly, Y.

AU - Lee, W. H.

AU - Levan, A.

AU - Linkov, V.

AU - Matkin, A.

AU - Minikulov, N.

AU - Molotov, I.

AU - Prochaska, J. X.

AU - Richer, M. G.

AU - Román-Zúñiga, C. G.

AU - Rumyantsev, V.

AU - Sánchez-Ramírez, R.

AU - Steele, I.

AU - Tanvir, N. R.

AU - Volnova, A.

AU - Watson, A. M.

AU - Xu, D.

AU - Yuan, F.

N1 - Funding Information: I am very grateful to Max de Pasquale for countless discussions regarding GRB physics, and Antonia Rowlinson for equally stimulating conversations regarding magnetars. We thank the referee for their insightful comments on the original manuscript. Z.C. gratefully acknowledges support by a Project Grant from the Icelandic Research Fund. The Dark Cosmology Centre is funded by the Danish National Research Foundation. The research activity of AdUP, CT, RSR, and JGor is supported by Spanish research project AYA2012-39362-C02-02. J.Gor and RSR are also supported by project AYA2012-39727-C03-01. AdUP acknowledges support by the European Commission under the Marie Curie Career Integration Grant programme (FP7-PEOPLE-2012-CIG 322307). T.K. acknowledges support by the European Commission under the Marie Curie Intra-European Fellowship Programme. The research activity of AM and PDA is supported by ASI grant INAF I/004/11/. A.P., A.V. acknowledge partial support by RFBR grants 12-02-01336, 14-02-10015, and A.M., I.M. acknowledge support by RFBR grant 13-01-92204. D.A.K. acknowledges support by the Max-Planck Institut für Extraterrestrische Physik, Garching, and the Thüringer Landessternwarte Tautenburg. J.X.P. acknowledges support from NASA Swift Grant NNX13AJ67G. J.P.U.F. acknowledges support from the ERC-StG grant EGGS-278202. Based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofísica de Canarias. Based on observations made with the Gran Telescopio Canarias (GTC), instaled in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias, in the island of La Palma. The Liverpool Telescope is operated by Liverpool John Moores University at the Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. The Faulkes Telescopes are owned by Las Cumbres Observatory. C.G.M. acknowledges support from the Royal Society, the Wolfson Foundation and the Science and Technology Facilities Council. The ROTSE-IIIb telescope is operated by Southern Methodist University at McDonald Observatory, Ft. Davis, Texas. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. Additionally, we thank the RATIR project team and the staff of the Observatorio Astronmico Nacional on Sierra San Pedro Mártir. RATIR is a collaboration between the University of California, the Universidad Nacional Autonóma de México, NASA Goddard Space Flight Center, and Arizona State University, benefiting from the loan of an H2RG detector and hardware and software support from Teledyne Scientific and Imaging. RATIR, the automation of the Harold L. Johnson Telescope of the Observatorio Astronómico Nacional on Sierra San Pedro Mártir, and the operation of both are funded through NASA grants NNX09AH71G, NNX09AT02G, NNX10AI27G, and NNX12AE66G, CONACyT grants INFR-2009-01-122785 and CB-2008-101958, UNAM PAPIIT grant IN113810, and UC MEXUS-CONACyT grant CN 09-283. S.S. acknowledges support from CONICYT through FONDECYT grant 3140534, from Basal-CATA PFB-06/2007, Iniciativa Cientifica Milenio grant P10-064-F (Millennium Center for Supernova Science), and by Project IC120009 “Millennium Institute of Astrophysics (MAS)” of Iniciativa Científica Milenio del Ministerio de Economa, Fomento y Turismo de Chile, with input from “Fondo de Innovación para la Competitividad, del Ministerio de Economía, Fomento y Turismo de Chile”. Part of this work is based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina). Part of the fundingfor GROND (both hardware as well as personnel) was generously granted from the Leibniz-Prize to G. Hasinger (DFG grant HA 1850/28-1).

PY - 2014/8

Y1 - 2014/8

N2 - We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. For GRB 130215A/SN 2013ez, we also present optical spectroscopy at t - t0 = 16.1 d, which covers rest-frame 3000-6250 Å. Based on Fe ii λ5169 and Si ii λ6355, our spectrum indicates an unusually low expansion velocity of ~4000-6350 km s-1, the lowest ever measured for a GRB-SN. Additionally, we determined the brightness and shape of each accompanying SN relative to a template supernova (SN 1998bw), which were used to estimate the amount of nickel produced via nucleosynthesis during each explosion. We find that our derived nickel masses are typical of other GRB-SNe, and greater than those of SNe Ibc that are not associated with GRBs. For GRB 130831A/SN 2013fu, we used our well-sampled R-band light curve (LC) to estimate the amount of ejecta mass and the kinetic energy of the SN, finding that these too are similar to other GRB-SNe. For GRB 130215A, we took advantage of contemporaneous optical/NIR observations to construct an optical/NIR bolometric LC of the afterglow. We fit the bolometric LC with the millisecond magnetar model of Zhang & Mészáros (2001, ApJ, 552, L35), which considers dipole radiation as a source of energy injection to the forward shock powering the optical/NIR afterglow. Using this model we derive an initial spin period of P = 12 ms and a magnetic field of B = 1.1 × 1015 G, which are commensurate with those found for proposed magnetar central engines of other long-duration GRBs.

AB - We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. For GRB 130215A/SN 2013ez, we also present optical spectroscopy at t - t0 = 16.1 d, which covers rest-frame 3000-6250 Å. Based on Fe ii λ5169 and Si ii λ6355, our spectrum indicates an unusually low expansion velocity of ~4000-6350 km s-1, the lowest ever measured for a GRB-SN. Additionally, we determined the brightness and shape of each accompanying SN relative to a template supernova (SN 1998bw), which were used to estimate the amount of nickel produced via nucleosynthesis during each explosion. We find that our derived nickel masses are typical of other GRB-SNe, and greater than those of SNe Ibc that are not associated with GRBs. For GRB 130831A/SN 2013fu, we used our well-sampled R-band light curve (LC) to estimate the amount of ejecta mass and the kinetic energy of the SN, finding that these too are similar to other GRB-SNe. For GRB 130215A, we took advantage of contemporaneous optical/NIR observations to construct an optical/NIR bolometric LC of the afterglow. We fit the bolometric LC with the millisecond magnetar model of Zhang & Mészáros (2001, ApJ, 552, L35), which considers dipole radiation as a source of energy injection to the forward shock powering the optical/NIR afterglow. Using this model we derive an initial spin period of P = 12 ms and a magnetic field of B = 1.1 × 1015 G, which are commensurate with those found for proposed magnetar central engines of other long-duration GRBs.

KW - Gamma-ray burst: general

KW - Gamma-ray burst: individual: SN 2013ez

KW - Supernovae: general

KW - Supernovae: individual: SN 2013fu

UR - http://www.scopus.com/inward/record.url?scp=84905638459&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84905638459&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201423920

DO - 10.1051/0004-6361/201423920

M3 - Article

AN - SCOPUS:84905638459

SN - 0004-6361

VL - 568

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A19

ER -

A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu

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Photometry of 3 {gamma}-ray burst supernovae

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A trio of gamma-ray burst supernovae: GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu

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Photometry of 3 {gamma}-ray burst supernovae

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