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Nearby Supernova Factory II classification of the SN Ia LSQ13ads and non-detection of LSQ13acp

ATel #5029; 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, E. Walker, 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, H. Fakhouri, A. Kim, J. Nordin, P. Nugent, S. Perlmutter, K. Runge, C. Saunders, N. Suzuki, R. C. Thomas (LBNL) E. Pecontal (CRAL); U. Feindt, M. Kowalski (U. Bonn); S. Benitez, W. Hillebrandt, M. Kromer, M. Sasdelli, A. Sternberg, S. Taubenberger (MPA);
on 30 Apr 2013; 03:15 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) |             |       |       | 
LSQ13ads    | 10:03:59.18 | -02:21:56.9 |  20130425   |   LSQ     | 17.94 |  20130429  |   0.047[1]  |  Ia   |   7   | .  
LSQ13acp    | 15:27:36.72 | +16:44:04.6 |  20130421   |   LSQ     | 18.71 |  20130429  |   N/A [2]   |  N/A  |  N/A  | Vmag>20  
[1]  2dF Galaxy Redshift Survey via NED 
[2] No object was present at the location of LSQ13acp brighter than V=20 mag.