SN 2017hk
RA/DEC (2000)
12:45:15.31 +26:05:07.10
191.313792 26.085306
Type
SN IIP
Redshift
0.059
Source Group
TNTS
Discoverer
Hanjie Tan(CCU), Wenxiong Li (THU),Tianmeng Zhang (NAOC), Zesheng Yang(THU), Zhijian Xu, Hao Song(THU), Xiaofeng Wang(THU), Jun Mo(THU), Xu Zhou(NAOC) on behalf of the TNTS
Discovery Date
2017-01-08 21:07:12
TNS AT
Y
Public
Y
Host Name
KUG 1242+263
Host Redshift
0.059
Discovery Mag
17.9
Discovery Mag Filter
Clear-
 2017-01-20 21:07:12 LJT / YFOSC (TNTS)
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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
7382017-01-20 21:07:12LJT / YFOSC2200Chuanjun WangJujia ZhangTNTS tns_2017hk_2017-01-20.88_LJT_YFOSC_TNTS.datObjectTNTS
Light Curves
FilterTel / InstObs-date rangePhotometry
Clear-BAO-0.6m_BATC2017-01-08 21:07:12 - 2017-01-08 21:07:121
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
116292017-01-08 21:07:1217.9VegaMagClear-BAO-0.6m_BATC
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
78852017-01-09 06:19:09M51Hanjie Tan(CCU), Wenxiong Li (THU),Tianmeng Zhang (NAOC), Zesheng Yang(THU), Zhijian Xu, Hao Song(THU), Xiaofeng Wang(THU), Jun Mo(THU), Xu Zhou(NAOC) on behalf of the TNTSTNTS12:45:15.31+26:05:07.102017-01-08 21:07:1217.9Clear-PSNTNTSThis possible supernova was discovered by the 0.6 m schmidt telescope at Xinglong Observatory during the Tsinghua-NAOC Transient Survey (TNTS). The transient is located 4" west and 4" north of the center of KUG 1242+263
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
7282017-01-21 06:02:53xwangJ. Zhang, C. Wang (YNAO), X. Wang, W. Li, Z. Yang, J. Mo (THU), H. Tang (CCU), Z. Xu, T. Zhang, X. Zhou (NAOC)TNTSSN IIP0.059TNTSA spectrum taken on Jan. 20.9 2017 with the Lijiang 2.4-m telescope indicates that this transient is consistent with a type IIP supernova a few days after the maximum light.

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