SN 2016frp
RA/DEC (2000)
00:21:32.54 -05:57:24.29
5.385583 -5.956747
SN Ib-pec
Source Group
Zhijian Xu, Wenxiong Li (THU), Bin Li (PMO), Zesheng Yang (THU), Hanjie Tan (CCU), Xiaofeng Wang (THU), Haibin Zhao (PMO), Lifan Wang (PMO), Jujia Zhang(YNAO)
Discovery Date
2016-08-27 18:36:59
Host Name
GALEXASC J002132.53-055728.4
Discovery Mag
Discovery Mag Filter
 2016-09-05 16:47:59 BAO-2.16m / Phot-spec (PTSS)
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   Binning factor: (rounded to nearest integer >1)
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See separate spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
3932016-09-05 16:47:59BAO-2.16m / Phot-spec3600Junjun JiaLiming RuiPTSS tns_2016frp_2016-09-05.70_BAO-2.16m_Phot-spec_PTSS.txtObjectPTSS
Light Curves
FilterTel / InstObs-date rangePhotometry
r-SloanCNEOST_STA16002016-08-27 18:36:59 - 2016-08-27 18:36:591
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
65922016-08-27 18:36:5918.50.1VegaMagr-SloanCNEOST_STA160060Bin Li
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
48592016-09-04 05:35:04M51Zhijian Xu, Wenxiong Li (THU), Bin Li (PMO), Zesheng Yang (THU), Hanjie Tan (CCU), Xiaofeng Wang (THU), Haibin Zhao (PMO), Lifan Wang (PMO), Jujia Zhang(YNAO)PTSS00:21:32.54-05:57:24.292016-08-27 18:36:5918.5r-SloanPSNPTSS-16mvzPTSSThis possible supernova was discovered by the 1.04-m schmidt telescope at Xuyi Observatory during the PMO-Tsinghua Supernova Survey (PTSS). The transient is located 1" east and 5” north of the center of GALEXASC J002132.53-055728.4
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
3852016-09-06 17:25:19xwangL. Rui, X. Wang, W. Li, Z.Yang (THU), Z. Xu, B. Li, H. Zhao, L. Wang (PMO), J. Jia, H. Wu, T. Zhang (NAOC), and J. Zhang (YNAO)PTSSSN Ib-pec0.027PTSSA spectrum taken on UT Sep. 05.7 with the Xinglong 2.16m telescope of NAOC shows that this transient is consistent with a peculiar type Ib supernova a few days before the maximum light.