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Spectroscopic classification of two Supernovae Type Ia and one Type II by the Nearby Supernova Factory II

ATel #4331; 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 23 Aug 2012; 19:17 UT
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    |          |       |       | 
LSQ12eks                | 23:01:04.13 | -06:41:42.7 | 20120819  |   LSQ     | 18.61 | 20120822 | 0.094    |  Ia   |  1.4  |  
LSQ12ekl                | 23:11:25.46 | -01:51:54.4 | 20120819  |   LSQ     | 19.74 | 20120822 | 0.082    |  Ia   |  -8   |  
PSN J01273145+1449058   | 01:27:31.45 |  14:49:05.8 | 20120820  |   ISSP    | 18.4  | 20120822 | 0.022[1] |  II   |  4.4  |  
[1] Grogin and Geller 2000, AJ, 119, 32