SN 2011fs
RA/DEC (2000)
22:17:19.52 +35:34:50.02
334.33133 +35.58056
Type
SN Ia
Redshift
0.022
Discovery Date
2011-09-15 00:00:00
Public
Y
Host Name
UGC 11975
Comments
[Discoverer=Jin, Gao; DiscoveryRef=CBET 2825; PositionRef=CBET 2825; Orig Type=Ia ]
Discovery Mag
16.8
IAU name
sn2011fs
 2011-09-24 03:58:04 Plaskett Telescope / Plaskett (DAO_OTS)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
21072011-09-24 03:58:04Plaskett Telescope / Plaskett4349BalamBalamDAO_OTS tns_2011fs_2011-09-24_03-58-04_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011fs_2011-09-24_03-58-04_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 362-693 nm, resolution 0.3 nm) of PSN J22171952+3534500 = SN 2011fs, obtained on Sept. 24.19 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova near 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 2011fs is most similar to the type-Ia supernova 1999aa at 5 days before maximum light.
Light Curves
No Data
AT Reportings
No Data
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
21002018-06-09 16:36:06DAO_OTSDave BalamDAO_OTSSN Ia0.022DAO_OTS