SN 2017cff
RA/DEC (2000)
13:39:17.00 +35:08:39.03
204.820833 35.144175
Type
SN IIP
Redshift
0.019
Source Group
PTSS
Discoverer
Zhijian Xu, Wenxiong Li (THU), Bin Li (PMO), Zesheng Yang (THU), Hanjie Tan(CCU), Xiaofeng Wang (THU), Haibin Zhao (PMO), Lifan Wang (PMO), and Jujia Zhang(YNAO)
Discovery Date
2017-03-16 20:00:05
TNS AT
Y
Public
Y
Host Name
GALEXASC J133917.08+350841.1
Discovery Mag
17.4
Discovery Mag Filter
r-Sloan
 2017-03-19 18:14:24 LJT / YFOSC (PTSS)
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   Binning factor: (rounded to nearest integer >1)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
8602017-03-19 18:14:24LJT / YFOSC1800Yuxin Xin (YNAO)Jujia Zhang (YNAO)PTSS tns_2017cff_2017-03-19.76_LJT_YFOSC_PTSS.datObjectPTSS
Light Curves
FilterTel / InstObs-date rangePhotometry
r-SloanCNEOST_STA16002017-03-16 20:00:05 - 2017-03-16 20:00:051
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
149882017-03-16 20:00:0517.4VegaMagr-SloanCNEOST_STA1600Bin Li
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
100962017-03-17 08:19:38M51Zhijian Xu, Wenxiong Li (THU), Bin Li (PMO), Zesheng Yang (THU), Hanjie Tan(CCU), Xiaofeng Wang (THU), Haibin Zhao (PMO), Lifan Wang (PMO), and Jujia Zhang(YNAO)PTSS13:39:17.00+35:08:39.032017-03-16 20:00:0517.4r-SloanPSNPTSS-17nemPTSSThis possible supernova was discovered by the 1.04 m schmidt telescope at Xuyi Observatory during the PMO-Tsinghua Transient Survey (PTSS). The transient is located 1" west and 2" south of the center of GALEXASC J133917.08+350841.1
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
8502017-03-20 02:58:29xwangJ. Zhang, Y. Xin (YNAO), Z. Xu, W. Li, X Wang (THU), B. Li, H. Zhao, L. Wang (PMO), H. Tan(CCU), L. Rui, D. Xiang (THU)PTSSSN IIP0.019PTSSA spectrum taken on UT Mar. 19.76 2017 with the Lijiang 2.4-m telescope indicates that this transient is consistent with a young type IIP supernova. The redshift is obtained from the SNID fit to the observed

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