SN 2016ije
RA/DEC (2000)
01:58:30.33 +12:55:27.90
29.626375 12.924417
Type
SN Ia-91bg-like
Redshift
0.04
Source Group
TNTS
Discoverer
Tianmeng Zhang (NAOC), Wenxiong Li (THU),,Hanjie Tan(CCU), Zhijian Xu, Xiaofeng Wang(THU), Jun Mo(THU), Xu Zhou(NAOC) on behalf of the TNTS
Discovery Date
2016-11-22 17:02:24
TNS AT
Y
Public
Y
Host Name
SDSS J015830.25+125528.1
Discovery Mag
17.8
Discovery Mag Filter
Clear-
 2016-11-23 18:00:00 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
5942016-11-23 18:00:00LJT / YFOSC2100Jianguo WangJujia ZhangTNTS tns_2016ije_2016-11-23.75_LJT_YFOSC_TNTS.datObjectTNTS
Light Curves
FilterTel / InstObs-date rangePhotometry
Clear-BAO-0.6m_BATC2016-11-22 17:02:24 - 2016-11-22 17:02:241
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
100112016-11-22 17:02:2417.8VegaMagClear-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
69442016-11-23 04:12:59M51Tianmeng Zhang (NAOC), Wenxiong Li (THU),,Hanjie Tan(CCU), Zhijian Xu, Xiaofeng Wang(THU), Jun Mo(THU), Xu Zhou(NAOC) on behalf of the TNTSTNTS01:58:30.33+12:55:27.902016-11-22 17:02:2417.8Clear-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 1" east and 0" north of the center of SDSS J015830.25+125528.1
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
5852016-11-24 10:12:25xwangJ.-J. Zhang, J.-G. Wang(YNAO), X.-F. Wang, W.-X. Li, L.-M. Rui, D.-F. Xiang (THU), T.-M. Zhang (NAOC), Z.-J. Xu, H.-J. Tan (CCU)TNTSSN Ia-91bg-like0.04TNTSA spectrum taken with the Lijiang 2.4-m telescope indicates that this transient discovered during the Tsinghua-NAOC Transient Survey is a subluminous, 91bg-like type Ia supernova at a relatively young phase.

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