SN 2016jab
RA/DEC (2000)
07:05:26.71 -76:00:33.48
106.36128 -76.0093
Type
SN Ia
Redshift
0.0215
Source Group
ASAS-SN
Discovery Date
2016-12-23 05:16:48
TNS AT
Y
Public
Y
Discovery Mag
16.3
Filter
V-Johnson
Discoverer/s
K. Z. Stanek, for the ASAS-SN team
 2016-12-24 05:47:27 LCO-duPont / WFCCD (ASAS-SN)
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Spectra
IDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
7182016-12-24 05:47:27LCO-duPont / WFCCDN. MorrellASAS-SN tns_2016jab_2457746.74129404_LCO-duPont_WFCCD_ASAS-SN.txt tns_2016jab_2457746.74129404_LCO-duPont_WFCCD_ASAS-SN.fitsObjectASAS-SN
Light Curves
FilterTel / InstObs-date rangePhotometry
V-JohnsonASASSN-2_Cassius2016-12-17 06:28:48 - 2016-12-23 05:16:483
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
108852016-12-23 05:16:4816.30.117.2VegaMagV-JohnsonASASSN-2_Cassius
108862016-12-20 06:14:2416.60.1217.2VegaMagV-JohnsonASASSN-2_Cassius
108842016-12-17 06:28:4817.2VegaMagV-JohnsonASASSN-2_Cassius[Last non detection]
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
74432016-12-23 19:50:44KZStanekK. Z. Stanek, for the ASAS-SN teamASAS-SN07:05:26.71-76:00:33.482016-12-23 05:16:4816.3V-JohnsonPSNASASSN-16pdASAS-SNIn several epochs and two chips, blue uncatalogued DSS galaxy nearby
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
7082017-01-11 03:52:19jlprietoN. Morrell, B. ShappeeASAS-SNSN Ia0.0215ASAS-SNWe report optical spectroscopic observation of supernova candidate ASASSN-16pd/2016jab (ATel #9898) using the du Pont 2.5-m telescope (+ WFCCD) at Las Campanas Observatory on UT 2016-12-24.24. The target was discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014, ApJ, 788, 48). We used SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) to identify the type and phase of the SN spectra. The spectrum matches normal SN Ia, few days before maximum light. Narrow Halpha emission is visible at z=0.0215. The SNID estimated redshift (z=0.022) is consistent with this value.