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Showing results 5651 to 5700 out of 6155

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IDNameRepsClassRADECObj. TypeRedshiftHost NameHost RedshiftDiscovering Group/sClassifying Group/sAssociated Group/sDisc. Internal NameDisc. Instrument/sClass. Instrument/sTNS ATPublicEnd Prop. PeriodObject SpectraDiscovery MagDiscovery Mag Filtersort ascendingDiscovery Date (UT)SenderRemarksSourcesBibcodeExt. catalog/s
5691SN 2011dq00:59:47.750-07:34:20.50SN IINGC 337 NY16.32011-05-15 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2749; PositionRef=CBET 2749; Orig Type=II ]
5693SN 2011ds20:02:20.930-20:13:13.40SN IIAnon. NY16.62011-05-13 00:00:00[Discoverer=Howerton, Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2751; PositionRef=CBET 2751; Orig Type=II ]
5696SN 2011dv116:12:04.620+14:12:33.19SN Ia0.031NGC 6078 DAO_OTSPlaskett - PlaskettNY116.22011-06-28 00:00:00[Discoverer=Ciabattari; DiscoveryRef=CBET 2755; PositionRef=CBET 2755; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20912018-06-08 22:30:12DAO_OTSDave BalamDAO_OTSSN Ia0.0311DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20962011-06-30 05:54:21Plaskett_Plaskett3600BalamBalamDAO_OTS tns_2011dv_2011-06-30_05-54-21_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011dv_2011-06-30_05-54-21_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 J16120400+1412330 = SN 2011dv, obtained on June 30.27 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova about five days past maximum light. Cross-correlation with a library of supernova spectra using the SNID code indicates that 2011dv is most similar to the type-Ia supernova 2006gz at five days past maximum light.
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20962011-06-30 05:54:21Plaskett / Plaskett3600BalamBalamDAO_OTS tns_2011dv_2011-06-30_05-54-21_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011dv_2011-06-30_05-54-21_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 J16120400+1412330 = SN 2011dv, obtained on June 30.27 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova about five days past maximum light. Cross-correlation with a library of supernova spectra using the SNID code indicates that 2011dv is most similar to the type-Ia supernova 2006gz at five days past maximum light.
5697SN 2011dw16:31:39.451+41:29:22.88SN IIAnon. NY17.52011-06-24 00:00:00[Discoverer=Pelloni, Newton, Puckett; DiscoveryRef=CBET 2756; PositionRef=CBET 2756; Orig Type=II? ]
5698SN 2011dx03:37:05.611-05:01:56.32SN IaNGC 1376 NY16.52011-06-27 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2759; PositionRef=CBET 2759; Orig Type=Ia ]
5699SN 2011dy23:29:20.131+03:23:08.59SN IIUGC 12628 NY16.82011-06-28 00:00:00[Discoverer=Briggs, Newton, Puckett; DiscoveryRef=CBET 2760; PositionRef=CBET 2760; Orig Type=II ]
5700SN 2011dz116:12:44.820+28:17:03.19SN Ia0.025UGC 10273 DAO_OTSPlaskett - PlaskettNY116.42011-06-26 00:00:00[Discoverer=Vida et al. (La Sagra Sky Survey); DiscoveryRef=CBET 2761; PositionRef=CBET 2761; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20922018-06-08 22:37:40DAO_OTSDave BalamDAO_OTSSN Ia0.0251DAO_OTS
Spectra
IDObs-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.
Spectra
IDObs-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.
5701SN 2011E00:26:19.231-04:29:42.40SN IIMCG -01-2-14 NY15.82011-01-07 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2628; PositionRef=CBET 2628; Orig Type=II ]
5703SN 2011eb01:57:36.581-57:48:00.79SN IaNGC 782 NY15.22011-07-09 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2764; PositionRef=CBET 2764; Orig Type=Ia ]
5704SN 2011ec22:41:37.570-57:36:08.78SN IaAnon. NY172011-05-14 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2765; PositionRef=CBET 2765; Orig Type=Ia ]
5705SN 2011ed19:15:34.339-54:37:39.50SN IaIC 4839 NY15.52011-03-26 00:00:00[Discoverer=Martin; DiscoveryRef=CBET 2767; PositionRef=CBET 2767; Orig Type=Ia ]
5708SN 2011eg118:42:54.209+53:02:41.50SN IIP0.028UGC 11343 DAO_OTSPlaskett - PlaskettNY217.52011-07-23 00:00:00[Discoverer=Newton, Sehgal, Puckett; DiscoveryRef=CBET 2774; PositionRef=CBET 2774; Orig Type=IIp ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20932018-06-08 22:45:52DAO_OTSDave BalamDAO_OTSSN IIP0.0282DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20982011-07-24 07:16:41Plaskett_Plaskett8000BalamBalamDAO_OTS tns_2011eg_2011-07-24_07-16-41_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011eg_2011-07-24_07-16-41_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 J18425421+5302415 = SN 2011eg, obtained on July 23.48 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-II-plateau supernova several 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 2011eg is most similar to the type-II-plateau supernova 2004et at 4 days past maximum light. A second spectrogram taken on July 28.35 shows 2011eg to be a type-IIp supernova most similar to SN 1999em within several weeks of maximum light.
20992011-07-28 07:12:46Plaskett_Plaskett8000BalamBalamDAO_OTS tns_2011eg_2011-07-28_07-12-46_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011eg_2011-07-28_07-12-46_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20992011-07-28 07:12:46Plaskett / Plaskett8000BalamBalamDAO_OTS tns_2011eg_2011-07-28_07-12-46_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011eg_2011-07-28_07-12-46_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
20982011-07-24 07:16:41Plaskett / Plaskett8000BalamBalamDAO_OTS tns_2011eg_2011-07-24_07-16-41_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011eg_2011-07-24_07-16-41_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 J18425421+5302415 = SN 2011eg, obtained on July 23.48 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-II-plateau supernova several 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 2011eg is most similar to the type-II-plateau supernova 2004et at 4 days past maximum light. A second spectrogram taken on July 28.35 shows 2011eg to be a type-IIp supernova most similar to SN 1999em within several weeks of maximum light.
5709SN 2011eh11:18:31.541+57:58:36.80SN Ia-pecNGC 3613 NY16.22011-07-20 00:00:00[Discoverer=Tsuboi; DiscoveryRef=CBET 2776; PositionRef=CBET 2776; Orig Type=Ia-p ]
5712SN 2011ek102:25:48.890+18:31:59.99SN Ia0.01NGC 918 DAO_OTSPlaskett - PlaskettNY216.42011-08-04 00:00:00[Discoverer=Itagaki; DiscoveryRef=CBET 2783; PositionRef=CBET 2783; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20942018-06-09 05:05:36DAO_OTSDave BalamDAO_OTSSN Ia0.012DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21002011-08-05 09:49:17Plaskett_Plaskett1102BalamBalamDAO_OTS tns_2011ek_2011-08-05_09-49-17_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011ek_2011-08-05_09-49-17_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 J02254889+1832000 = 2011ek, obtained on Aug. 7.41 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova before maximum light. Comparison with a library of supernova spectra using the "superfit" matching program of Howell et al. (2005, Ap.J. 634, 1190) indicates that 2011ek is a normal type-Ia supernova most similar to SN 2002bo at 11 days before maximum light.
21012011-08-07 09:35:38Plaskett_Plaskett6444BalamBalamDAO_OTS tns_2011ek_2011-08-07_09-35-38_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011ek_2011-08-07_09-35-38_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21012011-08-07 09:35:38Plaskett / Plaskett6444BalamBalamDAO_OTS tns_2011ek_2011-08-07_09-35-38_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011ek_2011-08-07_09-35-38_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
21002011-08-05 09:49:17Plaskett / Plaskett1102BalamBalamDAO_OTS tns_2011ek_2011-08-05_09-49-17_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011ek_2011-08-05_09-49-17_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 J02254889+1832000 = 2011ek, obtained on Aug. 7.41 UT with the 1.82-m Plaskett Telescope of the NRCC, shows it to be a type-Ia supernova before maximum light. Comparison with a library of supernova spectra using the "superfit" matching program of Howell et al. (2005, Ap.J. 634, 1190) indicates that 2011ek is a normal type-Ia supernova most similar to SN 2002bo at 11 days before maximum light.
5714SN 2011em13:27:13.190+55:29:17.41SN IaNGC 5164 NY16.82011-08-04 00:00:00[Discoverer=Tsuboi; DiscoveryRef=CBET 2785; PositionRef=CBET 2785; Orig Type=Ia ]
5716SN 2011eo16:42:25.121+16:49:28.09SN IIPAnon. NY17.42011-04-13 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=IIP ]
5732SN 2011fd06:46:39.850+60:21:02.81SN IIPNGC 2273B NY152011-08-20 00:00:00[Discoverer=Dimai; DiscoveryRef=CBET 2791; PositionRef=CBET 2791; Orig Type=IIP ]
5733SN 2011fe14:03:05.810+54:16:25.39SN Ia NY17.22011-08-24 00:00:00[Discoverer=Nugent et al. (Palomar Transient Factory); DiscoveryRef=CBET 2792; PositionRef=CBET 2792; Orig Type=Ia ]
5734SN 2011ff122:45:02.280+34:00:15.01SN Ia0.023UGC 12179 DAO_OTSPlaskett - PlaskettNY116.82011-08-22 00:00:00[Discoverer=Leonini, Guerrini; DiscoveryRef=CBET 2793; PositionRef=CBET 2793; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20952018-06-09 05:12:39DAO_OTSDave BalamDAO_OTSSN Ia0.0231DAO_OTS
Spectra
IDObs-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.
Spectra
IDObs-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.
5735SN 2011fg23:23:20.590+16:47:41.32SN Ia-pecAnon. NY16.62011-08-20 00:00:00[Discoverer=Zheng et al. (ROTSE); DiscoveryRef=CBET 2794; PositionRef=CBET 2794; Orig Type=Ia-p ]
5736SN 2011fh12:56:14.009-29:29:54.82SN IInNGC 4806 NY14.52011-08-24 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2799; PositionRef=CBET 2799; Orig Type=IIn ]
5738SN 2011fj20:13:55.159-01:09:22.21SN IIUGC 11527 NY16.62011-08-28 00:00:00[Discoverer=Maza, Pignata et al. (CHASE); DiscoveryRef=CBET 2802; PositionRef=CBET 2802; Orig Type=II ]
5739SN 2011fk100:54:42.060+36:45:51.41SN Ia0.02UGC 549 DAO_OTSPlaskett - PlaskettNY116.62011-08-29 00:00:00[Discoverer=Ciabattari, Mazzoni; DiscoveryRef=CBET 2805; PositionRef=CBET 2805; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20962018-06-09 05:19:43DAO_OTSDave BalamDAO_OTSSN Ia0.021DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21032011-09-01 07:15:50Plaskett_Plaskett7000BalamBalamDAO_OTS tns_2011fk_2011-09-01_07-15-50_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011fk_2011-09-01_07-15-50_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21032011-09-01 07:15:50Plaskett / Plaskett7000BalamBalamDAO_OTS tns_2011fk_2011-09-01_07-15-50_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011fk_2011-09-01_07-15-50_Plaskett_Telescope_Plaskett_DAO_OTS.fitsObjectDAO_OTS
5741SN 2011fm19:06:50.170-61:41:57.70SN IaIC 4815 NY16.42011-08-22 00:00:00[Discoverer=Parker; DiscoveryRef=CBET 2807; PositionRef=CBET 2807; Orig Type=Ia ]
5743SN 2011fo20:30:15.881-34:48:32.51SN IIESO 400-33 NY16.92011-09-01 00:00:00[Discoverer=Pignata et al. (CHASE); DiscoveryRef=CBET 2816; PositionRef=CBET 2816; Orig Type=II ]
5747SN 2011fs122:17:19.519+35:34:50.02SN Ia0.022UGC 11975 DAO_OTSPlaskett - PlaskettNY116.82011-09-15 00:00:00[Discoverer=Jin, Gao; DiscoveryRef=CBET 2825; PositionRef=CBET 2825; Orig Type=Ia ]
Classification reportings
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
21002018-06-09 16:36:06DAO_OTSDave BalamDAO_OTSSN Ia0.0221DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21072011-09-24 03:58:04Plaskett_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.
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
21072011-09-24 03:58:04Plaskett / 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.
5748SN 2011ft17:52:42.979+29:04:10.60SN IbAnon. NY17.12011-08-30 00:00:00[Discoverer=Balanutsa, Lipunov (MASTER); DiscoveryRef=CBET 2826; PositionRef=CBET 2826; Orig Type=Ib ]
5749SN 2011fu02:08:21.410+41:29:12.30SN IIUGC 1626 NY15.82011-09-21 00:00:00[Discoverer=Ciabattari, Mazzoni; DiscoveryRef=CBET 2827; PositionRef=CBET 2827; Orig Type=II ]
5751SN 2011fw03:20:54.240+37:52:05.30SN IaMCG +06-8-15 NY17.22011-09-23 00:00:00[Discoverer=Ciabattari, Mazzoni; DiscoveryRef=CBET 2829; PositionRef=CBET 2829; Orig Type=Ia ]
5754SN 2011fz22:58:20.299+02:17:29.90SN Ib/cUGC 12271 NY16.62011-09-18 00:00:00[Discoverer=Howerton, Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2832; PositionRef=CBET 2832; Orig Type=Ib/c ]
5756SN 2011ga22:40:27.420+03:11:57.98SN IaAnon. NY17.32011-09-18 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2833; PositionRef=CBET 2833; Orig Type=Ia ]
5757SN 2011gb01:33:42.941+34:48:37.12SN IaAnon. NY16.12011-09-24 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2834; PositionRef=CBET 2834; Orig Type=Ia ]
5761SN 2011gf21:12:24.269-07:48:52.09SN IaAnon. NY16.62011-09-18 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2838; PositionRef=CBET 2838; Orig Type=Ia ]
5765SN 2011gj01:19:24.151+12:26:17.09SN IaUGC 849 NY17.52011-09-07 00:00:00[Discoverer=Peoples, Sehgal, Puckett; DiscoveryRef=CBET 2843; PositionRef=CBET 2843; Orig Type=Ia ]
5768SN 2011gm01:38:54.590-42:35:08.81SN IaNGC 644 NY15.82011-09-21 00:00:00[Discoverer=Parker; DiscoveryRef=CBET 2847; PositionRef=CBET 2847; Orig Type=Ia ]
5774SN 2011gs04:21:09.989+13:28:04.40SN IaAnon. NY17.42011-09-23 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2859; PositionRef=CBET 2859; Orig Type=Ia ]
5775SN 2011gt19:56:48.259-37:19:37.49SN IaIC 4913 NY162011-09-26 00:00:00[Discoverer=Howerton, Drake et al. (Siding Spring Survey); DiscoveryRef=CBET 2864; PositionRef=CBET 2864; Orig Type=Ia ]
5777SN 2011gv19:54:21.420-58:42:38.99SN IIPIC 4901 NY14.52011-10-19 00:00:00[Discoverer=Bock; DiscoveryRef=CBET 2868; PositionRef=CBET 2868; Orig Type=IIP ]
5778SN 2011gw07:28:17.021-62:21:18.90SN Ib/cIC 2200 NY17.42011-09-15 00:00:00[Discoverer=Pignata, Maza et al. (CHASE); DiscoveryRef=CBET 2869; PositionRef=CBET 2869; Orig Type=Ib/c ]
5780SN 2011gy03:29:35.299+40:52:03.40SN IaUGC 2756 NY15.82011-10-22 00:00:00[Discoverer=Jin, Gao; DiscoveryRef=CBET 2871; PositionRef=CBET 2871; Orig Type=Ia ]
5781SN 2011gz00:37:46.270-33:39:51.41SN IaAnon. NY15.92011-10-03 00:00:00[Discoverer=Maza, Pignata et al. (CHASE); DiscoveryRef=CBET 2872; PositionRef=CBET 2872; Orig Type=Ia ]
5782SN 2011H02:23:06.019+43:02:32.39SN IaUGC 1837 NY15.62011-01-04 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2634; PositionRef=CBET 2634; Orig Type=Ia ]
5785SN 2011hc20:12:10.070-11:21:57.71SN IaAnon. NY16.52011-10-23 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2882; PositionRef=CBET 2882; Orig Type=Ia ]
5786SN 2011hd09:58:48.300+34:47:03.30SN IaAnon. NY15.92011-10-24 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2884; PositionRef=CBET 2884; Orig Type=Ia ]
5790SN 2011hh02:57:04.610+49:47:43.30SN IaAnon. NY16.92011-10-26 00:00:00[Discoverer=Lipunov (MASTER); DiscoveryRef=CBET 2888; PositionRef=CBET 2888; Orig Type=Ia ]
5793SN 2011hk02:18:45.790-06:38:30.08SN IaIC 881 NY16.22011-10-31 00:00:00[Discoverer=Hirose; Itagaki; DiscoveryRef=CBET 2892; PositionRef=CBET 2892; Orig Type=Ia ]
5798SN 2011hp12:16:25.471-43:19:46.88SN IcNGC 4219 NY15.72011-11-03 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2899; PositionRef=CBET 2899; Orig Type=Ic ]
5800SN 2011hr08:54:46.030+39:32:16.12SN IaNGC 2691 NY16.92011-11-08 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2901; PositionRef=CBET 2901; Orig Type=Ia]
5801SN 2011hs22:57:11.770-43:23:04.81SN IIbIC 5267 NY15.52011-11-12 00:00:00[Discoverer=Parker; DiscoveryRef=CBET 2902; PositionRef=CBET 2902; Orig Type=IIb]
5802SN 2011ht10:08:10.589+51:50:57.01SN IInUGC 5460 NY172011-09-29 00:00:00[Discoverer=Boles; DiscoveryRef=CBET 2851; PositionRef=CBET 2851; Orig Type=IIn]

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