SN 2017aap
RA/DEC (2000)
11:36:18.31 +38:07:09.20
174.076292 38.119222
Type
SN Ia
Redshift
0.11
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
2017-02-01 19:34:19
TNS AT
Y
Public
Y
Host Name
SDSS J113618.34+380706.8
Discovery Mag
19.6
Discovery Mag Filter
r-Sloan
 2017-02-02 15:36:00 LJT / YFOSC (PTSS)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
7752017-02-02 15:36:00LJT / YFOSC2400Yuxin XinJujia ZhangPTSS tns_2017aap_2017-02-02.65_LJT_YFOSC_PTSS.datObjectPTSS
Light Curves
FilterTel / InstObs-date rangePhotometry
r-SloanCNEOST_STA16002017-02-01 19:34:19 - 2017-02-01 19:34:191
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
125832017-02-01 19:34:1919.6VegaMagr-SloanCNEOST_STA1600Bin Li
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
84682017-02-02 09:41:16M51Zhijian 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)PTSS11:36:18.31+38:07:09.202017-02-01 19:34:1919.6r-SloanPSNPTSS-17diePTSSThis 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 0" east and 2" north of the center of SDSS J113618.34+380706.8.
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
7652017-02-04 07:22:31xwangJ. Zhang, Y. Xin (YNAO), Z. Xu, W. Li, X., Wang (THU), B. Li, H. Zhao, L. Wang (PMO), H. Tan (CCU), L. Rui, Z. Yang (THU)PTSSSN Ia0.11PTSSA spectrum taken on Feb. 02.86 with the Lijiang 2.4-m telescope indicates that this transient is consisten with overluminous peculiar type Ia supernova like SN 1991T at a few days after the maximum light.

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