SN 2011dz
RA/DEC ()
16:12:44.820 +28:17:03.19
243.18675 +28.28422
Type
SN Ia
Redshift
0.025
Discovery Date
2011-06-26 00:00:00
Public
Y
Host Name
UGC 10273
Comments
[Discoverer=Vida et al. (La Sagra Sky Survey); DiscoveryRef=CBET 2761; PositionRef=CBET 2761; Orig Type=Ia ]
Discovery Mag
16.4
IAU name
sn2011dz

Spectra

 SN_2011dz - 2011-07-05 08:51:40 Plaskett / Plaskett (DAO_OTS)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
20972011-07-05 08:51:40Plaskett / Plaskett5815BalamBalamDAO_OTS tns_2011dz_2011-07-05_08-51-40_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011dz_2011-07-05_08-51-40_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS D. D. Balam, Dominion Astrophysical Observatory, National Research Council of Canada (NRCC); M. L. Graham, Las Cumbres Observatory Global Telescope, University of California at Santa Barbara; E. Y. Hsiao, Lawrence Berkeley Laboratory; and D. W. E. Green, Harvard University, report that a spectrogram (range 389-725 nm, resolution 0.3 nm) of PSN J16124482+2817032 = SN 2011dz, obtained on July 5.37 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova about 35 days past maximum light. Cross-correlation with a library of supernova spectra using the "Supernova Identification" code (Blondin and Tonry 2007, Ap.J. 666, 1024) indicates that 2011dz is most similar to the type-Ia supernova 2002ic at 35 days past maximum light.
Light Curves
No Data
AT Reportings
No Data
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
20922018-06-08 22:37:40DAO_OTSDave BalamDAO_OTSSN Ia0.025DAO_OTS