SN 2018lei
RA/DEC (2000)
02:33:34.402 -39:02:45.24
38.39334 -39.0459
Type
SN Ic
Redshift
0.006
Source Group
ASAS-SN
Discovery Date
2018-12-31 03:36:00
TNS AT
Y
Public
Y
Host Name
NGC 0986
Host Redshift
0.006585
Discovery Mag
16.8
Filter
g-Sloan
Discoverer/s
K. Z. Stanek, for the ASAS-SN team

Spectra

 SN_2018lei - 2018-12-31 05:36:40 UH88 / SNIFS (SCAT)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
34012018-12-31 05:36:40UH88 / SNIFS1200M E HuberSCAT tns_2018lei_2458483.7338_UH88_SNIFS_SCAT.txtObjectSCATReduced with a summit quick-reduction pipeline, care should be taken before re-using this data for further science.
Light Curves
FilterTel / InstObs-date rangePhotometry
g-SloanASASSN-2_Cassius2018-12-31 03:36:00 - 2018-12-31 03:36:001
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
490752018-12-31 03:36:0016.8ABMagg-SloanASASSN-2_Cassius
g-SloanASASSN-5_Payne-Gaposchkin2018-12-26 20:09:36 - 2018-12-26 20:09:361
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
490742018-12-26 20:09:3618.7ABMagg-SloanASASSN-5_Payne-Gaposchkin[Last non detection]
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
276492018-12-31 20:52:43KZStanekK. Z. Stanek, for the ASAS-SN teamASAS-SN02:33:34.402-39:02:45.242018-12-31 03:36:0016.8g-SloanPSNASASSN-18aclASAS-SNPresent in several epochs, on the rise, close to the nucleus
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
33942019-01-09 00:31:08tuckermaM A Tucker, M E Huber (IfA), J Strader (MSU), K Z Stakek (OSU), B J Shappee (IfA)SCATSN Ic0.006SCATSpectrum heavily contaminated by host emission, notably the Balmer series, OIII, and NII. After clipping host emission, spectrum provides a good match to a few Ic-norm SNID templates near maximum light. (SNID phase: -1 +/- 5, redshift from host)

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