SN 2016frp
RA/DEC (2000)
00:21:32.54 -05:57:24.29
5.385583 -5.956747
Type
SN Ib-pec
Redshift
0.027
Source Group
PTSS
Discovery Date
2016-08-27 18:36:59
TNS AT
Y
Public
Y
Host Name
GALEXASC J002132.53-055728.4
Discovery Mag
18.5
Filter
r-Sloan
Discoverer/s
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)
 2016-09-05 16:47:59 BAO-2.16m / Phot-spec (PTSS)
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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
Photometry
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), 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.

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