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Showing results 38451 to 38500 out of 45584

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IDNameRepsClassRADECObj. Typesort descendingRedshiftHost NameHost RedshiftReporting Group/sDiscovery Data Source/sClassifying Group/sAssociated Group/sDisc. Internal NameDisc. Instrument/sClass. Instrument/sTNS ATPublicEnd Prop. PeriodObject SpectraDiscovery MagDiscovery Mag FilterDiscovery Date (UT)SenderRemarksSourcesBibcodeExt. catalog/s
5671SN 2011cx12:14:22.159+33:55:09.52SN IaAnon. NY18.62011-05-02 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2733; PositionRef=CBET 2733; Orig Type=Ia ]
5672SN 2011cy14:58:37.099+02:20:59.10SN IaAnon. NY202011-05-07 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2733; PositionRef=CBET 2733; Orig Type=Ia ]
5679SN 2011de115:43:53.251+67:45:42.52SN Ia0.031UGC 10018 DAO_OTSPlaskett - PlaskettNY116.72011-05-22 00:00:00[Discoverer=Newton, Puckett; DiscoveryRef=CBET 2728; PositionRef=CBET 2728; Orig Type=Ia ]
Classification reports
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20892018-06-08 22:06:10DAO_OTSDave BalamDAO_OTSSN Ia0.0311DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20942011-05-28 06:25:12Plaskett_Plaskett2067BalamBalamDAO_OTS tns_2011de_2011-05-28_06-25-12_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011de_2011-05-28_06-25-12_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 J15435325+6745425 = SN 2011de, obtained on May 28.28 UT with the 1.82-m Plaskett Telescope of the NRCC, 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 2011de is most similar to the type-Ia supernova 2003du at one week before maximum light.
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20942011-05-28 06:25:12Plaskett / Plaskett2067BalamBalamDAO_OTS tns_2011de_2011-05-28_06-25-12_Plaskett_Telescope_Plaskett_DAO_OTS.txt tns_2011de_2011-05-28_06-25-12_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 J15435325+6745425 = SN 2011de, obtained on May 28.28 UT with the 1.82-m Plaskett Telescope of the NRCC, 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 2011de is most similar to the type-Ia supernova 2003du at one week before maximum light.
5680SN 2011df119:27:33.641+54:23:11.29SN Ia0.015NGC 6801 DAO_OTSPlaskett - PlaskettNY117.62011-05-21 00:00:00[Discoverer=Newton, Puckett; DiscoveryRef=CBET 2729; PositionRef=CBET 2729; Orig Type=Ia ]
Classification reports
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarks
20902018-06-08 22:22:26DAO_OTSDave BalamDAO_OTSSN Ia0.0151DAO_OTS
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20952011-05-28 08:24:00Plaskett_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.
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
20952011-05-28 08:24:00Plaskett / 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.
5683SN 2011di18:43:59.059-61:59:46.28SN IaIC 4754 NY17.52011-05-13 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2737; PositionRef=CBET 2737; Orig Type=Ia ]
5684SN 2011dj13:07:06.689-01:10:44.00SN IaAnon. NY15.82011-06-04 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2740; PositionRef=CBET 2740; Orig Type=Ia ]
5686SN 2011dl16:18:04.970+21:33:04.00SN IaUGC 10321 NY16.92011-06-17 00:00:00[Discoverer=Gorelli, Newton, Puckett; DiscoveryRef=CBET 2744; PositionRef=CBET 2744; Orig Type=Ia ]
5687SN 2011dm21:56:41.590+73:17:48.91SN IaUGC 11861 NY18.82011-06-15 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2745; PositionRef=CBET 2745; Orig Type=Ia ]
5688SN 2011dn19:58:35.530+02:36:16.31SN IaUGC 11501 NY16.82011-06-21 00:00:00[Discoverer=Leonini; DiscoveryRef=CBET 2746; PositionRef=CBET 2746; Orig Type=Ia ]
5689SN 2011do04:25:47.561-67:48:40.72SN IaAnon. NY14.82011-06-11 00:00:00[Discoverer=Parker; DiscoveryRef=CBET 2747; PositionRef=CBET 2747; Orig Type=Ia ]
5690SN 2011dp01:45:24.770-03:49:35.29SN IaAnon. NY16.12011-06-02 00:00:00[Discoverer=Monard; DiscoveryRef=CBET 2748; PositionRef=CBET 2748; Orig Type=Ia ]
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 reports
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.
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 ]
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 reports
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.
5702SN 2011ea12:27:36.379+04:09:49.50SN IaAnon. NY19.22011-07-01 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2762; PositionRef=CBET 2762; Orig Type=Ia ]
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 ]
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 reports
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.
5713SN 2011el03:00:18.199+05:49:24.89SN IaAnon. NY17.62011-08-01 00:00:00[Discoverer=Zheng et al. (ROTSE); DiscoveryRef=CBET 2784; PositionRef=CBET 2784; Orig Type=Ia ]
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 ]
5718SN 2011eq21:17:59.270-02:37:22.80SN IaAnon. NY192011-04-29 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ia ]
5719SN 2011er15:49:50.650+14:49:30.11SN IaAnon. NY18.92011-05-25 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ia ]
5721SN 2011et15:30:01.399+24:52:29.10SN IaAnon. NY18.82011-06-02 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ia ]
5725SN 2011ex15:48:51.749+62:57:48.89SN IaAnon. NY17.62011-06-13 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ia ]
5727SN 2011ez12:42:42.430+00:33:54.00SN IaAnon. NY18.92011-06-24 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ia ]
5731SN 2011fc23:01:36.379+32:20:06.90SN IaAnon. NY17.92011-07-11 00:00:00[Discoverer=Mikuz; DiscoveryRef=CBET 2788; PositionRef=CBET 2788; Orig Type=Ia ]
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 reports
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.
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 reports
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 ]
5744SN 2011fp00:15:25.610+17:19:11.89SN IaNGC 57 NY17.92011-08-29 00:00:00[Discoverer=Itagaki; DiscoveryRef=CBET 2820; PositionRef=CBET 2820; Orig Type=Ia ]
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 reports
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.
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 ]
5755SN 2011G12:09:41.810+56:31:11.39SN IaUGC 7144 NY19.32011-01-08 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2630; PositionRef=CBET 2630; Orig Type=Ia ]
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 ]
5762SN 2011gg00:46:21.079-09:09:27.68SN IaAnon. NY17.62011-09-20 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2839; PositionRef=CBET 2839; Orig Type=Ia ]
5764SN 2011gi00:32:43.001+26:06:51.59SN IaAnon. NY18.22011-09-21 00:00:00[Discoverer=Howerton, Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2842; PositionRef=CBET 2842; 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 ]
5766SN 2011gk02:02:19.020+19:39:39.60SN IaUGC 1523 NY182011-09-06 00:00:00[Discoverer=Moore, Sehgal, Puckett; DiscoveryRef=CBET 2845; PositionRef=CBET 2845; Orig Type=Ia ]
5767SN 2011gl05:01:43.070-15:23:24.68SN IaAnon. NY18.22011-09-23 00:00:00[Discoverer=Howerton, Drake et al. (Siding Spring Survey); DiscoveryRef=CBET 2846; PositionRef=CBET 2846; 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 ]
5769SN 2011gn07:06:28.289+77:52:31.80SN IaMCG +13-5-36 NY182011-09-30 00:00:00[Discoverer=Boles; DiscoveryRef=CBET 2848; PositionRef=CBET 2848; Orig Type=Ia ]
5772SN 2011gq21:42:28.440-16:06:30.49SN IaAnon. NY19.22011-09-26 00:00:00[Discoverer=Howerton, Drake et al. (Mount Lemmon Survey); DiscoveryRef=CBET 2856; PositionRef=CBET 2856; Orig Type=Ia ]
5773SN 2011gr00:20:45.979+06:56:05.21SN IaAnon. NY18.32011-09-18 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2858; PositionRef=CBET 2858; 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 ]
5776SN 2011gu23:06:02.801+34:06:36.68SN IaNGC 7485 NY182011-10-14 00:00:00[Discoverer=Martinelli, Mancini, Briganti; DiscoveryRef=CBET 2866; PositionRef=CBET 2866; Orig Type=Ia ]

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