2006CBET..629....1B -
Central Bureau Electronic Telegrams, 629, 1 (2006/September-0)
Supernovae 2006gd, 2006ge, 2006gf, 2006gg, 2006gh.
BASSETT B., BECKER A., BREWINGTON H., CHOI C., CINABRO D., DEJONGH F., DEMBICKY J., DEPOY D.L., DILDAY B., DOI M., FRIEMAN J., GARNAVICH P., HARVANEK M., HOGAN C., HOLTZMAN J., IM M., JHA S., KONISHI K., KRZESINSKI J., LAMPEITL H., KESSLER R., KETZEBACK B., LONG D., MALANUSHENKO O., MARRINER J., McMILLAN R., MIKNAITIS G., MOROKUMA T., NICHOL R., PAN K., PRIETO J.L., RICHMOND M., RIESS A., ROMANI R., SAKO M., SCHNEIDER D., SMITH M., SNEDDEN S., TAKANASHI N., TOKITA K., VAN DER HEYDEN K., WATTERS S., WHEELER C., YASUDA N., ZHENG C. and IHARA Y.
Abstract (from CDS):
Further to CBETs 611 and 627, B. Bassett, South African Astronomical Observatory (SAAO); A. Becker, University of Washington (UW); H. Brewington, Apache Point Observatory (APO); C. Choi, Seoul National University (SNU); D. Cinabro, Wayne State University; F. DeJongh, Fermilab; J. Dembicky, APO; D. L. DePoy, Ohio State University (OSU); B. Dilday, University of Chicago (UC); M. Doi, University of Tokyo (UoT); J. Frieman, Fermilab and UC; P. Garnavich, University of Notre Dame; M. Harvanek, APO; C. Hogan, UW; J. Holtzman, New Mexico State University; M. Im, SNU; S. Jha, Stanford University (SU); K. Konishi, UoT; J. Krzesinski, APO; H. Lampeitl, Space Telescope Science Institute (STScI); R. Kessler, UC; B. Ketzeback, D. Long, O. Malanushenko, and V. Malanushenko, APO; J. Marriner, Fermilab; R. McMillan, APO; G. Miknaitis, Fermilab; T. Morokuma, UoT; R. Nichol, University of Portsmouth (UP); K. Pan, APO; J. L. Prieto, OSU; M. Richmond, Rochester Institute of Technology; A. Riess, STScI; R. Romani, SU; M. Sako, University of Pennsylvania; D. Schneider, Pennsylvania State University; M. Smith, UP; S. Snedden, APO; N. Takanashi and K. Tokita, UoT; K. van der Heyden, SAAO; S. Watters, APO; C. Wheeler, University of Texas; N. Yasuda, UoT; and C. Zheng, SU, on behalf of the Sloan Digital Sky Survey II collaboration, report the discovery of five additional supernovae on multiple g, r, and i images taken with the SDSS 2.5-m telescope at Apache Point Observatory by the SDSS observing team. Spectroscopic observations with the Subaru 8-m telescope on Sept. 18 UT by N. Takanashi, Y. Ihara, T. Morokuma, K. Tokita, K. Konishi, and N. Yasuda indicate that four of the supernovae (2006ge, 2006gf, 2006gg, 2006gh) are type-Ia events, and one (2006gd) is a type-IIP event. The discovery and peak magnitudes tabulated below are all SDSS g magnitudes, with the exception of 2006gf (r magnitude, denoted by "r" in the table below). Spectroscopic redshifts are given in the column labelled "z". Peak magnitudes and dates (all 2006) are estimates from early fits to the multi-band light curves. SN Discov. R.A. (2000.0) Decl. Mag. z Estimated Peak Date UT Date Mag. 2006gd Aug. 28 1 10 26.39 - 1 04 04.8 22.8 0.15 Aug. 21 21.3 2006ge Aug. 28 21 49 35.79 + 0 00 03.8 21.7 0.28 Aug. 20 21.6 2006gf Sept.11 0 46 24.35 + 0 00 12.5 21.4r 0.12 Sept. 8 21.3r 2006gg Sept.12 0 28 12.51 + 0 07 04.8 21.3 0.20 Sept.21 20.7 2006gh Sept.12 0 54 46.94 - 0 15 03.1 21.2 0.25 Sept.16 21.1
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