Search
Degrees (0..360, with decimal point) or sexagesimal: HH:MM:SS.SS / HH MM SS.SS
Degrees (-90..+90, with decimal point) or sexagesimal: ±DD:MM:SS.SS / ±DD MM SS.SS
E.g., 2024-03-28
to
E.g., 2024-03-28
Download as CSVDownload as TSV
Showing results 1 to 1 out of 1
IDNameRepsClassRADECObj. TypeRedshiftHost NameHost RedshiftReporting Group/sDiscovery Data Source/sClassifying Group/sAssociated Group/sDisc. Internal NameDisc. Instrument/sClass. Instrument/sTNS ATPublicEnd Prop. Periodsort descendingObject SpectraDiscovery Mag/FluxDiscovery FilterDiscovery Date (UT)SenderRemarksSourcesBibcodeExt. catalog/s
33673SN 2019qb3109:35:27.777+53:46:12.49SN Ia0.061ZTF, ATLAS, Pan-STARRSZTF, ATLAS, Pan-STARRSSCATATLAS, Pan-STARRS, ZTFZTF19aacijieATLAS-HKO - ATLAS-02, ATLAS-MLO - ATLAS-01, P48 - ZTF-Cam, PS1 - GPC1UH88 - SNIFSYY120.02g-ZTF2019-01-08 10:47:05.000ZTF_AMPEL_NEW2019TNSTR..74....1N
AT reports
IDTime Received (UT)SenderReporter/s (Discoverer/s)Reporting GroupDisc. Data SourceRADECDiscovery Date (UT)Discovery Mag.FilterPhotometryRelated FilesAT TypeHost NameHost RedshiftInternal NameAssoc. GroupsEnd Prop. PeriodRemarksBibcode
398342019-07-01 08:35:35PS1_Bot1K. C. Chambers, T. de Boer, J. Bulger, J. Fairlamb, M. Huber, C.-C. Lin, T. Lowe, E. Magnier, A. Schultz, R. J. Wainscoat, M. Willman (IfA, University of Hawaii), K. W. Smith, D. R. Young, O. McBrien, J. Gillanders. S. Srivastav, S. J. Smartt, D. O'Neil, P. Clark, S. Sim (Queen's University Belfast), D. E. Wright (University of Minnesota)Pan-STARRSPan-STARRS09:35:27.777+53:46:12.492019-01-09 11:34:04.00019.34w-P11PSNPS19cslPan-STARRS
Photometry
IDObs-date (UT)Mag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserverRemarks
751762019-01-09 11:34:0419.340.0222ABMagw-P1PS1_GPC145Robot
288652019-01-16 11:36:13ATLAS_Bot1J. Tonry, L. Denneau, A. Heinze, H. Weiland, H. Flewelling (IfA, University of Hawaii), B. Stalder (LSST), A. Rest (STScI), C. Stubbs (Harvard University), K. W. Smith, S. J. Smartt, D. R. Young, K. Maguire, S. J. Prentice, O. McBrien, D. O'Neill, P. Clark, M. Magee, M. Fulton, A. McCormack (Queen's University Belfast), D. E. Wright (University of Minnesota)ATLASATLAS09:35:27.772+53:46:12.602019-01-15 12:27:21.00018.355orange-ATLAS2PSNATLAS19bksATLAS
Photometry
IDObs-date (UT)Mag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserverRemarks
515622019-01-15 12:27:2118.3550.15419.37ABMagorange-ATLASATLAS-MLO_ATLAS-0130Robot
515612019-01-13 14:35:3119.62ABMagorange-ATLASATLAS-HKO_ATLAS-0230Robot[Last non detection]
287152019-01-11 14:09:28ZTF_AMPEL_NEWJ. Nordin, V. Brinnel, M. Giomi, J. van Santen (HU Berlin), A. Gal-Yam, O. Yaron, S. Schulze (Weizmann) on behalf of ZTFZTFZTF09:35:27.768+53:46:12.712019-01-08 10:47:05.00020.02g-ZTF3PSNZTF19aacijieZTF2019TNSTR..74....1N
Photometry
IDObs-date (UT)Mag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserverRemarks
512232019-01-11 11:22:3118.790.0720.85ABMagg-ZTFP48_ZTF-Cam30
512222019-01-08 10:47:0520.020.2419.77ABMagg-ZTFP48_ZTF-Cam30
512212019-01-03 11:08:0920.43ABMagr-ZTFP48_ZTF-Cam30[Last non detection]
Classification reports
IDTime Received (UT)SenderClassifier/sGroupClassificationRedshiftSpectraRelated FilesAssoc. GroupsEnd Prop. PeriodRemarksADS Bibcode
34052019-01-13 13:38:55avpayneAnna V Payne, Michael A Tucker, Aaron Do, Benjamin J Shappee, Mark E HuberSCATSN Ia0.0611SCATType Ia supernova before maximum light. SNID phase: -0.6(4.5) days, redshift 0.0612019TNSCR..80....1P
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
34122019-01-13 00:24:54UH88_SNIFS1800PayneSCAT tns_2019qb_2458496.5173_UH88_SNIFS_SCAT.datObjectSCATReduced with summit-based quick reduction pipeline. Care should be taken before using this spectrum for further science.
Spectra
IDObs-date (UT)Tel / InstExp-timeObserver/sReducer/sGroupSpectrum ascii FileSpectrum fits FileSpec. TypeAssoc. GroupsEnd Prop. PeriodRemarks
34122019-01-13 00:24:54UH88 / SNIFS1800PayneSCAT tns_2019qb_2458496.5173_UH88_SNIFS_SCAT.datObjectSCATReduced with summit-based quick reduction pipeline. Care should be taken before using this spectrum for further science.