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Spectroscopic classification of two Type Ia SNe by the Nearby Supernova Factory II

ATel #4497; C. Buton, U. Feindt, M. Kerschhaggl, M. Kowalski (U. Bonn); S. Benitez, W. Hillebrandt, M. Kromer, M. Sasdelli, A. Sternberg, S. Taubenberger (MPA); D. Baugh, J. Chen, N. Chotard, C. Wu (THCA) C. Tao (CPPM & THCA), D. Fouchez, A. Tilquin (CPPM); E. Hadjiyska, D. Rabinowitz, C. Baltay, N. Ellman, R. McKinnon, A. Effron (Yale) F. Cellier-Holzem, A. Canto, P. Antilogus, S. Bongard, R. Pain (LPNHE); Y. Copin, E. Gangler, R. Pereira, M. Rigault, G. Smadja (IPNL); G. Aldering, D. Birchall, M. Childress, H. Fakhouri, A. Kim, J. Nordin, P. Nugent, S. Perlmutter, K. Runge, C. Saunders, N. Suzuki, R. C. Thomas (LBNL); E. Pecontal (CRAL);
on 18 Oct 2012; 20:02 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jakob Nordin (jnordin@lbl.gov)

Subjects: Optical, Supernovae

The Nearby Supernova Factory II (http://snfactory.lbl.gov) reports the following spectroscopic observations of supernovae based on spectra (range 320-1000 nm) obtained with the SuperNova Integral Field Spectrograph (Aldering et al 2002, SPIE, 4836, 61) on the University of Hawaii 2.2-meter telescope. Classifications were performed using Superfit (Howell et al 2002, BAAS, 34, 1256) or SNID (Blondin & Tonry, 2007, ApJ, 666, 1024). Heliocentric redshifts listed to two decimal places are measured from supernova features; all others are published values or measured by us from host galaxy features.

 
Name                              |  RA (J2000) | Dec (J2000) | Discovery | Discovery      | Disc. | Spectrum | Redshift    | Type  | Phase | Notes 
                                  |             |             |    Date   |   Source       | Mag   |  Date    |             |       |       | 
LSQ12fls                          | 02:21:33.79 | +02:38:34.8 | 20121016  |   LSQ          | 16.85 | 20121018 |    0.04     |  Ia   |  10   |  
SNNGC2370 (PSN J07250042+2347030) | 07:25:00.42 | +23:47:03.0 | 20121016  | CBAT(Shima)[1] | 17.0  | 20121018 | 0.018346[2] |  Ia   |   0   | Strongly reddened  
 
 
[1] www.cbat.eps.harvard.edu/unconf/followups/J07250042+2347030.html 
[2] RC3, de Vaucoulers et al, 1991