SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey
G. LeloudasDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, DenmarkE. ChatzopoulosDepartment of Astronomy, University of Texas at Austin, Austin, TX, USAB. DildayDepartment of Physics, University of California, Santa Barbara, Broida Hall, Santa Barbara, CA 93106-9530, USAJ. GorosabelInstituto de Astrofísica de Andalucía (IAA-CSIC), Granada, SpainJozsef VinkoDepartment of Astronomy, University of Texas at Austin, Austin, TX, USAAnna GallazziDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, DenmarkJ. C. WheelerDepartment of Astronomy, University of Texas at Austin, Austin, TX, USABruce A. BassettAfrican Institute for Mathematical sciences, Muizenberg, Cape Town, South AfricaJ. FischerUniversity of Pennsylvania, 209 South 33rd Street, PA 19104, USAJ. FriemanCenter for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510, USAJ. P. U. FynboDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, DenmarkA. GoobarDepartment of Physics, Stockholm University, Albanova University Centre, 10691 Stockholm, SwedenM. JelínekInstituto de Astrofísica de Andalucía (IAA-CSIC), Granada, SpainD. MalesaniDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, DenmarkR. C. NicholInstitute of Cosmology and Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth, PO1 3FX, UKJ. NordinE. O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720, USAL. ÖstmanInstitut de Física d’Altes Energies, Universitat Autonoma de Barcelona, 08193 Bellaterra (Barcelona), SpainM. ŠakoUniversity of Pennsylvania, 209 South 33rd Street, PA 19104, USADonald P. SchneiderDepartment of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USAM. SmithAfrican Institute for Mathematical sciences, Muizenberg, Cape Town, South AfricaJ. SollermanDepartment of Astronomy, Stockholm University, Albanova University Centre, 10691 Stockholm, SwedenM. StritzingerDepartment of Astronomy, Stockholm University, Albanova University Centre, 10691 Stockholm, SwedenC. C. ThöneInstituto de Astrofísica de Andalucía (IAA-CSIC), Granada, SpainA. de Ugarte PostigoDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, Denmark
2012en
ABI
Annotatsiya
Context. A new class of super-luminous transients has recently been identified. These objects reach absolute luminosities of Mu < −21, lack hydrogen in their spectra, and are exclusively discovered by non-targeted surveys because they are associated with very faint galaxies.
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