SN 2016bpq
RA/DEC ()
18:53:29.295 +30:40:45.12
283.372062031 +30.6792011047
Type
SN II
Redshift
Source Group
Pan-STARRS1
Discovery Date
2016-03-30 15:23:47
TNS AT
Y
Public
Y
Discovery Mag
16.77
Filter
z-Sloan
Discoverer/s
K. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, N. Primak, A. Schultz, (IfA, University of Hawaii), S. J. Smartt, K. W. Smith, (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright, D. R. Young (Queen's University Belfast)

Spectra

 SN_2016bpq - 2016-04-18 10:17:12 MDM-2.4 / OSMOS (None)z=
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   Binning factor: (rounded to nearest integer >1)
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Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
2112016-04-18 10:17:12MDM-2.4 / OSMOSD. Godoy-RiveraNone tns_2016bpq_2457496.92862_MDM-2.4_OSMOS.txt tns_2016bpq_2457496.92862_MDM-2.4_OSMOS.fitsObject
Light Curves
FilterTel / InstObs-date rangePhotometry
z-SloanPS1_GPC12016-03-30 15:23:47 - 2016-03-30 15:23:471
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
21242016-03-30 15:23:4716.77ABMagz-SloanPS1_GPC1
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
18822016-04-15 18:05:59David YoungK. C. Chambers, M. E. Huber, H. Flewelling, E. A. Magnier, N. Primak, A. Schultz, (IfA, University of Hawaii), S. J. Smartt, K. W. Smith, (Queen's University Belfast), J. Tonry, C. Waters, (IfA, University of Hawaii) D. E. Wright, D. R. Young (Queen's University Belfast)Pan-STARRS118:53:29.295+30:40:45.122016-03-30 15:23:4716.77z-SloanPSNPS16bosPan-STARRS1
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
2042016-04-20 00:59:19jlprietoD. Godoy-Rivera, J. Prieto, S. DongNoneSN IIThe spectrum of PS16bos/AT2016bpq shows a blue continuum and broad Balmer P-Cygni profiles, consistent with a Type II SN. After cross-correlation with a library of SN spectra using SNID (Blondin & Tonry 2007, ApJ, 666, 1024), the best match is the spectrum of the Type IIP SN 2004et at peak.