SN 2011df
RA/DEC (2000)
19:27:33.64 +54:23:11.29
291.89017 +54.38647
Type
SN Ia
Redshift
0.015
Discovery Date
2011-05-21 00:00:00
Public
Y
Host Name
NGC 6801
Comments
[Discoverer=Newton, Puckett; DiscoveryRef=CBET 2729; PositionRef=CBET 2729; Orig Type=Ia ]
Discovery Mag
17.6
IAU name
sn2011df
 2011-05-28 08:24:00 Plaskett Telescope / Plaskett (DAO_OTS)
Show H at z=vexp= km/s
Show He at z=vexp= km/s
Show He ii at z=vexp= km/s
Show O at z=vexp= km/s
Show O ii at z=vexp= km/s
Show O iii at z=vexp= km/s
Show Na at z=vexp= km/s
Show Mg at z=vexp= km/s
Show Mg ii at z=vexp= km/s
Show Si ii at z=vexp= km/s
Show S ii at z=vexp= km/s
Show Ca ii at z=vexp= km/s
Show Fe ii at z=vexp= km/s
Show Fe iii at z=vexp= km/s
Show Å at z=vexp= km/s
Show Å at z=vexp= km/s
Show Tellurics 
Show Galaxy lines at z=
Show WR-WN at z=vexp= km/s
Show WR-WC/O at z=vexp= km/s
   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (observed),0 (rest)
See separate spectra
Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
20952011-05-28 08:24:00Plaskett Telescope / Plaskett1848BalamBalamDAO_OTS tns_2011df_2011-05-28_08-24-00_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011df_2011-05-28_08-24-00_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTSD. 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; G. Sarty, University of Saskatchewan; and D. W. E. Green, Harvard University, report that a spectrogram (range 382-714 nm, resolution 0.3 nm) of PSN J19273364+5423113 = SN 2011df, obtained on May 28.36 UT with the 1.82-m Plaskett Telescope of the National Research Council of Canada, shows it to be a type-Ia supernova before 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 2011df is most similar to the type-Ia supernova 1989B a few days before maximum light.
Light Curves
No Data
AT Reportings
No Data
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
20902018-06-08 22:22:26DAO_OTSDave BalamDAO_OTSSN Ia0.015DAO_OTS

Comments