SN 2011ff
RA/DEC ()
22:45:02.280 +34:00:15.01
341.2595 +34.00417
Type
SN Ia
Redshift
0.023
Discovery Date
2011-08-22 00:00:00
Public
Y
Host Name
UGC 12179
Comments
[Discoverer=Leonini, Guerrini; DiscoveryRef=CBET 2793; PositionRef=CBET 2793; Orig Type=Ia ]
Discovery Mag
16.8
IAU name
sn2011ff

Spectra

 SN_2011ff - 2011-08-25 06:59:24 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
21022011-08-25 06:59:24Plaskett / Plaskett6894BalamBalamDAO_OTS tns_2011ff_2011-08-25_06-59-24_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011ff_2011-08-25_06-59-24_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 383-717 nm; resolution 0.3 nm) of PSN J22450228+3400150 = SN 2011ff, obtained on Aug. 25.33 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 2011ff is most similar to the type-Ia supernova 2004eo at 2 days past maximum light.
Light Curves
No Data
AT Reportings
No Data
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
20952018-06-09 05:12:39DAO_OTSDave BalamDAO_OTSSN Ia0.023DAO_OTS