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Showing results 35601 to 35650 out of 41394

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IDsort descendingNameRepsClassRADECObj. TypeRedshiftHost NameHost RedshiftDiscovering Group/sClassifying Group/sAssociated Group/sDisc. Internal NameDisc. Instrument/sClass. Instrument/sTNS ATPublicEnd Prop. PeriodObject SpectraDiscovery MagDiscovery Mag FilterDiscovery Date (UT)SenderRemarksSourcesBibcodeExt. catalog/s
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 ]
5720SN 2011es13:43:54.950+25:32:52.91SN IIPAnon. NY19.92011-05-27 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=IIP ]
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 ]
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 ]
5717SN 2011ep17:03:41.779+32:45:52.60SN IcAnon. NY192011-04-14 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=Ic ]
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 ]
5715SN 2011en11:07:50.561+18:59:39.08SN IIPAnon. NY18.32011-03-25 00:00:00[Discoverer=Drake et al. (Catalina Real Time Transient Survey); DiscoveryRef=CBET 2787; PositionRef=CBET 2787; Orig Type=IIP ]
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 ]
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 ]
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.
5711SN 2011ej22:00:42.259-08:15:42.01SN IIPAnon. NY18.82011-07-03 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2778; PositionRef=CBET 2778; Orig Type=IIP ]
5710SN 2011ei20:34:22.620-31:58:23.59SN IIbNGC 6925 NY182011-07-25 00:00:00[Discoverer=Parker; DiscoveryRef=CBET 2777; PositionRef=CBET 2777; Orig Type=IIb ]
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 ]
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.
5707SN 2011ef23:30:57.019+15:29:24.29SN IIUGC 12640 NY17.72011-07-18 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2772; PositionRef=CBET 2772; Orig Type=II ]
5706SN 2011ee23:27:57.341+08:46:38.10SN IcNGC 7674 NY18.62011-06-27 00:00:00[Discoverer=Miluzio, Benetti, et al.; DiscoveryRef=CBET 2773; PositionRef=CBET 2773; Orig Type=Ic ]
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 ]
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 ]
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 ]
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 ]
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.
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 ]
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 ]
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? ]
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.
5695SN 2011du18:56:42.060+36:38:10.72SN IIAnon. NY18.82011-06-23 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2753; PositionRef=CBET 2753; Orig Type=II ]
5694SN 2011dt14:24:36.120+35:16:38.71SN IIUGC 9233 NY18.62011-06-08 00:00:00[Discoverer=Cenko et al. (LOSS); DiscoveryRef=CBET 2752; PositionRef=CBET 2752; 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 ]
5692SN 2011dr20:06:20.261-42:45:58.10SN IIPAnon. NY17.82011-05-25 00:00:00[Discoverer=Howerton, Drake et al. (Siding Spring Survey); DiscoveryRef=CBET 2750; PositionRef=CBET 2750; Orig Type=IIP ]
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 ]
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 ]
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 ]
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 ]
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 ]
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 ]
5685SN 2011dk21:00:42.199+17:48:22.00SN IINGC 7003 NY16.52011-06-12 00:00:00[Discoverer=Ciabattari et al.; DiscoveryRef=CBET 2741; PositionRef=CBET 2741; Orig Type=II ]
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 ]
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 ]
5682SN 2011dh13:30:05.119+47:10:10.81SN IIPNGC 5194 NY142011-06-01 00:00:00[Discoverer=Reiland; Griga; Riou; Lamotte Bailey; DiscoveryRef=CBET 2736; PositionRef=CBET 2736; Orig Type=IIP ]
5681SN 2011dg15:05:09.101-43:30:46.19SN IIPIC 4523 NY172011-05-18 00:00:00[Discoverer=Pignata et al. (CHASE); DiscoveryRef=CBET 2732; PositionRef=CBET 2732; Orig Type=IIP ]
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 reportings
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.
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 reportings
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.
5678SN 2011dd10:16:09.650-15:47:35.09SN IIPNGC 3178 NY15.82011-05-15 00:00:00[Discoverer=Pignata et al. (CHASE); DiscoveryRef=CBET 2727; PositionRef=CBET 2727; Orig Type=IIP ]
5677SN 2011dc14:58:56.510+65:54:08.32SN IAnon. NY172011-05-14 00:00:00[Discoverer=Drake et al. (Catalina Sky Survey); DiscoveryRef=CBET 2726; PositionRef=CBET 2726; Orig Type=I? ]
5676SN 2011db13:49:05.899+17:14:00.49SN IIAnon. NY17.42011-05-12 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2725; PositionRef=CBET 2725; Orig Type=II ]
5675SN 2011da12:22:27.910+37:49:39.50SN IIPAnon. NY19.22011-05-04 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2733; PositionRef=CBET 2733; Orig Type=IIP ]
5673SN 2011cz12:11:24.091+37:25:52.50SN IIPAnon. NY19.22011-05-04 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2733; PositionRef=CBET 2733; Orig Type=IIP ]
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 ]
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 ]
5670SN 2011cw14:47:39.550+51:41:04.70SN IInAnon. NY18.32011-05-01 00:00:00[Discoverer=Drake et al. (Catalina Real-Time Transient Survey); DiscoveryRef=CBET 2733; PositionRef=CBET 2733; Orig Type=IIn ]

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