2007CBET.1013....1B -
Central Bureau Electronic Telegrams, 1013, 1 (2007/July-0)
Supernovae 2007gf and 2007gg.
BUTON C., COPIN Y., GANGLER E., SMADJA G., ANTILOGUS P., PAIN R., PEREIRA R., WU C., ALDERING G., ARAGON C., BAILEY S., BONGARD S., CHILDRESS M., LOKEN S., NUGENT P., PERLMUTTER S., RUNGE K., THOMAS R.C., WEAVER B.A., BALTAY C., BAUER A., RABINOWITZ D., SCALZO R., RIGAUDIER G., PECONTAL E., BIRCHALL D. and HOLTZMAN J.
Abstract (from CDS):
The "Nearby Supernova Factory" collaboration (C. Buton, Y. Copin, E. Gangler, and G. Smadja, Institut de Physique Nucleaire de Lyon; P. Antilogus, R. Pain, R. Pereira, and C. Wu, Laboratoire de Physique Nucleaire et de Haute Energies de Paris; G. Aldering, C. Aragon, S. Bailey, S. Bongard, M. Childress, S. Loken, P. Nugent, S. Perlmutter, K. Runge, R. C. Thomas, and B. A. Weaver, Lawrence Berkeley National Laboratory, Berkeley; C. Baltay, A. Bauer, D. Rabinowitz, and R. Scalzo, Yale University; G. Rigaudier and E. Pecontal, Centre de Recherche Astronomique de Lyon; D. Birchall, Institute for Astronomy, University of Hawaii, Hilo; and J. Holtzman, New Mexico State University, Las Cruces) reports the discovery of two supernovae in images obtained during July 26-28 UT using the QUEST-II camera on the Palomar Oschin 1.2-m Schmidt telescope, operated by the Palomar-QUEST Consortium. Spectra (range 320-1000 nm) obtained with the SuperNova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope were used to classify the supernovae. A spectrum of 2007gf taken on July 29.4 showed it to be around maximum, and a spectrum of 2007gg on July 30.5 showed it to be one week past maximum. The R-band discovery magnitudes and astrometry below were derived from comparison with the USNO-B1.0 catalogue. SN 2007 UT R.A. (2000.0) Decl. Mag. z Type 2007gf July 26.4 23 17 48.71 +22 59 07.1 19.9 0.14 Ia 2007gg July 28.5 2 52 22.68 +16 31 40.3 19.1 0.04 Ib/c
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