SN 2016ccs
RA/DEC (2000)
14:45:20.100 +03:50:16.00
221.33375 +3.837778
Type
SN Ia
Redshift
0.062
Source Group
TNTS
Discovery Date
2016-05-09 17:31:12
TNS AT
Y
Public
Y
Host Name
SDSS J144519.89+035017.5
Host Redshift
0.062
Discovery Mag
18
Filter
Clear-
Discoverer/s
Zhijian Xu, Wenxiong Li (THU), Zesheng Yang (THU), Tianmeng Zhang (NAOC), Xiaofeng Wang (THU), on behalf of the TNTS

Spectra

 SN_2016ccs - 2016-05-11 17:02:24 Lijiang-2.4m / YFOSC (TNTS)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
2242016-05-11 17:02:24Lijiang-2.4m / YFOSC1800Chuanjun WangJujia ZhangTNTS tns_2016ccs_2016-05-11.71_LJT_YFOSC_TNTS.datObjectTNTS
Light Curves
FilterTel / InstObs-date rangePhotometry
Clear-BAO-0.6m_BATC2016-05-09 17:31:12 - 2016-05-09 17:31:121
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
25182016-05-09 17:31:1218VegaMagClear-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
22352016-05-11 02:41:05M51Zhijian Xu, Wenxiong Li (THU), Zesheng Yang (THU), Tianmeng Zhang (NAOC), Xiaofeng Wang (THU), on behalf of the TNTSTNTS14:45:20.100+03:50:16.002016-05-09 17:31:1218Clear-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 3" east and 2" south of the center of SDSS J144519.89+035017.5
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
2172016-05-12 02:32:38xwangJ. Zhang, C. Wang (YNAO), Z. Xu, W. Li, Z. Yang, X. Wang (THU), T. Zhang (NAOC)TNTSSN Ia0.062TNTSA spectrum taken with the Lijiang 2.4-m telescope (+YFOSC) shows that this transient is consistent with a type Ia supernova around the maximum light.