SN 2016grz
RA/DEC (2000)
01:55:32.95 +33:49:22.70
28.887292 +33.822972
Type
SN Ia
Redshift
0.087
Source Group
TNTS
Discovery Date
2016-09-28 19:12:00
TNS AT
Y
Public
Y
Host Name
SDSS J015533.01+334921.3
Discovery Mag
19.1
Filter
Clear-
Discoverer/s
Zhijian Xu, Wenxiong Li (THU), Hanjie Tan (CCU), Tianmeng Zhang (NAOC), Zesheng Yang (THU), Xiaofeng Wang (THU), on behalf of the TNTS
 2016-10-01 21:36:00 Lijiang-2.4m / YFOSC (TNTS)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
4772016-10-01 21:36:00Lijiang-2.4m / YFOSC2400Yuxin XinJujia ZhangTNTS tns_2016grz_2016-10-01.90_LJT_YFOSC_TNTS.datObjectTNTS
Light Curves
FilterTel / InstObs-date rangePhotometry
Clear-BAO-0.6m_BATC2016-09-28 19:12:00 - 2016-09-28 19:12:001
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
77922016-09-28 19:12:0019.1VegaMagClear-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
56012016-09-29 14:18:32M51Zhijian Xu, Wenxiong Li (THU), Hanjie Tan (CCU), Tianmeng Zhang (NAOC), Zesheng Yang (THU), Xiaofeng Wang (THU), on behalf of the TNTSTNTS01:55:32.95+33:49:22.702016-09-28 19:12:0019.1Clear-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" west and 1" north of the center of SDSS J015533.01+334921.3
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
4692016-10-02 05:36:58xwangJ.-J. Zhang, Y.-X. Xing (YNAO), X.-F. Wang, W.-X. Li, Z.-S. Yang (THU), Z.-J. Xu, H. J. Tan (CCNU), T. Zhang (NAOC)TNTSSN Ia0.087TNTSA spectrum taken on Oct. 01.90 2016 with the Lijiang 2.4-m telescope indicates that AT 2016grz is a type Ia supernova at about one week before the maximum light.

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