SN 2017ckc
RA/DEC (2000)
14:28:36.17 +16:41:04.42
217.150708 +16.684561
Type
SN Ia
Redshift
0.054
Source Group
PTSS
Discovery Date
2017-03-25 19:56:00
TNS AT
Y
Public
Y
Host Name
SDSS J142836.23+164104.6
Discovery Mag
18.3
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)
 2017-04-06 19:40:48 LJT / YFOSC (PTSS)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
9002017-04-06 19:40:48LJT / YFOSC2400Jujia ZhangJujia ZhangPTSS tns_2017ckc_2017-04-06.82_LJT_YFOSC_PTSS.datObjectPTSS
Light Curves
FilterTel / InstObs-date rangePhotometry
r-SloanCNEOST_STA16002017-03-25 19:56:00 - 2017-03-25 19:56:001
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
152392017-03-25 19:56:0018.3VegaMagr-SloanCNEOST_STA1600Bin Li
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
102342017-03-26 11:00:42M51Zhijian 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)PTSS14:28:36.17+16:41:04.422017-03-25 19:56:0018.3r-SloanPSNPTSS-17nipPTSSThis 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 0" south of the center of SDSS J142836.23+164104.6
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
8902017-04-07 00:34:11xwangJ. Zhang (YNAO), X. Wang, Z. Xu, W. Li (THU), B. Li (PMO), Z. Yang (THU), H. Tan(CCU), H. Zhao, L. Wang (PMO) PTSSSN Ia0.054PTSSA spectrum taken on April 06.82 2017 with the Lijiang 2.4-m telescope indicates that this transient is consistent with a type Ia supernova at around the maximum light.

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