SN 2017boa
RA/DEC (2000)
14:30:31.63 +52:42:15.57
217.631785826 52.7043249401
Médéric Boquien, Dalya Baron, Lluís Galbany, Dovi Poznanski
Discovery Date
2017-01-18 15:00:00
End Prop. Period
Host Name
SDSS J143031.19+524225.8
Host Redshift
Discovery Mag
Discovery Mag Filter
 2016-03-15 09:30:00 Other / Other
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IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
8362016-03-15 09:30:00Other / OtherMaNGA team tns_2017boa_2016-03-15_09-30-00_Other_Other.datObjectSpectrum of the transient observed at the 2.5m APO telescope with the MaNGA IFU spectrum in plate 8547 IFU 12701. The initial cube was processed with the following software versions of the pipeline: VERSDRP2= 'v2_0_1  '           / MaNGA DRP version (2d processing) VERSDRP3= 'v2_0_1  '           / MaNGA DRP Version (3d processing) VERSPLDS= 'v2_52   '           / Platedesign Version VERSFLAT= 'v1_26   '           / Specflat Version VERSCORE= 'v1_3_1  '           / MaNGAcore Version VERSPRIM= 'v2_2    '           / MaNGA Preimaging Version VERSUTIL= 'v5_5_25 '           / Version of idlutils VERSIDL = 'x86_64 linux unix linux 7.1.1 Aug 21 2009 64 64 ' / Version of IDL VERSPY  = '3.5.1   '           / Python version VERSNP  = '1.11.0  '           / Numpy version VERSSCI = '0.17.1  '           / Scipy version VERSAST = '1.1.2   '           / Astropy version VERSPYDL= '0.5.0   '           / pydl version VERSDAP = '2.0.2   '           / MaNGA DAP version Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatório Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.
Light Curves
FilterTel / InstObs-date rangePhotometry
r-SloanOther_Other2016-03-15 09:30:00 - 2016-03-15 09:30:001
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
141372016-03-15 09:30:0019ABMagr-SloanOther_OtherObserved at the APO 2.5m with the MaNGA IFU spectrograph.
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
96072017-02-28 12:15:50mboquienMédéric Boquien, Dalya Baron, Lluís Galbany, Dovi Poznanski14:30:31.63+52:42:15.572017-01-18 15:00:0019r-SloanOther2017-03-01SNIa discovered in an SDSS-IV/MaNGA spectra (Bundy et al. 2015; ​ found by the algorithm of Baron & Poznanski (2017).
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
8262017-03-03 20:03:20mboquienMédéric Boquien, Dalya Baron, Lluís Galbany, Dovi PoznanskiSN IaWe fitted the spectrum to a library of template spectra using SNID (Blondin & Tonry, 2007, ApJ, 666, 1024). We find a best match to the Type Ia SN 2001G at +66d past maximum. Accounting for a rise time of about 20 days, this dates the explosion to the 2nd half of December 2015.