Nearby Supernova Factory II classification of five SNe Ia
ATel #5270; E. Pecontal (CRAL); U. Feindt, P. Greskovic, M. Kowalski, S. Lombardo (U. Bonn); S. Benitez, W. Hillebrandt, M. Kromer, M. Sasdelli, A. Sternberg, S. Taubenberger (MPA); D. Baugh, J. Chen, C. Wu (THCA); C. Tao (CPPM & THCA), D. Fouchez, A. Tilquin (CPPM); E. Hadjiyska, D. Rabinowitz, C. Baltay, N. Ellman, R. McKinnon, E. Walker, A. Effron (Yale); F. Cellier-Holzem, A. Canto, P. Antilogus, S. Bongard, M. Fleury, R. Pain (LPNHE) Y. Copin, N. Chotard, E. Gangler, R. Pereira, M. Rigault, G. Smadja (IPNL); G. Aldering, D. Birchall, H. Fakhouri, A. Kim, J. Nordin, P. Nugent, S. Perlmutter, D. Rubin, K. Runge, C. Saunders, C. Sofiatti, N. Suzuki, R. C. Thomas (LBNL);
on 13 Aug 2013; 06:11 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 (UTC) | Source | Mag | Date (UTC) | | | |
LSQ13bjy | 22:06:44.90 | +14:05:04.9 | 20130805 | LSQ | 19.49 | 20130812 | 0.11 | Ia | -1 |
LSQ13bjq | 22:00:48.53 | -13:07:17.2 | 20130807 | LSQ | 19.41 | 20130812 | 0.07 | Ia | -1 |
LSQ13bjs | 22:09:25.31 | -01:38:52.8 | 20130807 | LSQ | 18.44 | 20130812 | 0.04 | Ia | 5 |
LSQ13bka | 22:54:49.08 | +19:23:56.0 | 20130807 | LSQ | 19.33 | 20130812 | 0.07 | Ia | 0 |
LSQ13bjj | 02:12:05.18 | -25:44:40.2 | 20130804 | LSQ | 19.19 | 20130812 | 0.056[1] | Ia | -2 |
[1] Jones, D. et al 2009, MNRAS, 399, 683.