SN 2016jdj
RA/DEC (2000)
13:26:01.99 +02:17:00.80
201.508292 +2.283556
Type
SN Ia
Redshift
0.137
Source Group
XOSS
Discovery Date
2016-12-28 23:24:57
TNS AT
Y
Public
Y
Host Name
PGC 1221823
Discovery Mag
18.4
Filter
Clear-
Discoverer/s
Wei Gao,Xing Gao
 2016-12-29 22:04:48 Lijiang-2.4m / YFOSC
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
6902016-12-29 22:04:48Lijiang-2.4m / YFOSC2000Xiaoguang YuJujia Zhang tns_2016jdj_2016-12-29.92_LJT_YFOSC.datObjectPTSS
Light Curves
FilterTel / InstObs-date rangePhotometry
Clear-Other_Other2016-12-28 23:24:57 - 2016-12-28 23:24:571
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
110342016-12-28 23:24:5718.419.9VegaMagClear-Other_Other90X.GaoUsing 0.5-m f/4 reflector + CCD
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
75392016-12-29 01:43:38gaoweiWei Gao,Xing GaoXOSS13:26:01.99+02:17:00.802016-12-28 23:24:5718.4Clear-PSNXOSSWei Gao (Nong'an, Jilin, China) and Xing Gao (Urumqi, Xinjiang, China), report the discovery of a possible supernova (mag approximately 18.4) on a 3x90s stack image (limiting mag about 19.9) taken by Xing Gao in Xingming Observatory Sky Survey (C42) around Dec. 28.97566 UT using a unfilled CCD ( + 0.5-m f/4 reflector + CCD ). The new object approximately located at R.A.=13h26m01s.99 Decl.=+02°17'00".8 (equinox 2000.0).Which is about 1.6" west and 10.8" north of the center of the PGC 1221823.
Related files
FileFile TypeCommentsLast Modified (UT)Modified By
tns_2016jdj_atrep_7539_XOSS.jpgGraphics2016-12-29 01:43:38gaowei
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
6802016-12-30 11:01:29xwangJujia Zhang, Xiaoguang Yu (YNAO), Xiaofeng Wang (Tsinghua University)SN Ia0.137PTSSA spectrum taken on UT Dec. 29.9 2016 with the Lijiang 2.4-m telescope indicates that this transient is a type Ia supernova at around the maximum light.

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