Maqola

The optical SN 2012bz associated with the long GRB 120422A

A. MelandriINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyE. PianINAF – Trieste Astronomical Observatory, via G.B. Tiepolo 11, 34143 Trieste, ItalyP. FerreroInstituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, SpainV. D’EliaASI, Science Data Centre, via Galileo Galilei, 00044 Frascati, ItalyE. S. WalkerScuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, ItalyG. GhirlandaINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyS. CovinoINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyL. AmatiINAF, IASF Bologna, via P. Gobetti 101, 40129 Bologna, ItalyP. D’AvanzoINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyP. A. MazzaliINAF – Padova Astronomical Observatory, vicolo dell’Osservatorio 5, 35122 Padova, ItalyM. Della ValleINAF – Capodimonte Astronomical Observatory, Salita Moiariello 16, 80131 Napoli, ItalyC. GuidorziPhysics Department, University of Ferrara, via Saragat 1, Ferrara 44122, ItalyL. A. AntonelliINAF – Roma Astronomical Observatory, via Frascati 33, 00040 Monteporzio Catone, ItalyM. G. BernardiniINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyD. BersierARI, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH41 1LD, UKF. BufanoDepartamento de Ciencias Fisicas, Universidad Andrés Bello, Av. República 252, Santiago, ChileS. CampanaINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyA. J. Castro‐TiradoInstituto de Astrofísica de Andalucía, CSIC, Glorieta de la Astronomía s/n, 18.008 Granada, SpainG. ChincariniINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyJ. DengNational Astronomical Observatories, CAS – 100012 Beijing, PR ChinaA. V. FilippenkoDepartment of Astronomy, University of California, Berkeley, CA 94720-3411, USAD. FugazzaINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyG. GhiselliniINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyC. KouveliotouNASA Marshall Space Flight Center, Huntsville, Alabama 35805, USAKeiichi MaedaThe University of TokyoG. MarconiEuropean Southern Observatory, Alonso de Cordova 3107, Santiago, ChileN. MasettiINAF, IASF Bologna, via P. Gobetti 101, 40129 Bologna, ItalyK. NomotoThe University of TokyoE. PalazziINAF, IASF Bologna, via P. Gobetti 101, 40129 Bologna, ItalyF. PatatEuropean Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, GermanyS. PiranomonteINAF – Roma Astronomical Observatory, via Frascati 33, 00040 Monteporzio Catone, ItalyR. SalvaterraINAF, IASF Milano, via E. Bassini 15, 20133 Milano, ItalyI. SavianeKavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, 277-8583 Chiba, JapanR. StarlingDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKG. TagliaferriINAF – Brera Astronomical Observatory, via E. Bianchi 46, 23807 Merate (LC), ItalyMasaomi TanakaNational Astronomical Observatory of Japan, Mitaka, 181-8588 Tokyo, JapanS. D. VerganiBrera Astronomical Observatory

2012en

Ochiq kirishBronza

ABI

Annotatsiya

Aims. The association of Type Ic supernovae (SNe) with long-duration gamma-ray bursts (GRBs) is well established. We endeavor, through accurate ground-based observational campaigns, to characterize these SNe at increasingly high redshifts.

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Identifikatorlar

DOI: 10.1051/0004-6361/201219879

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