SN 2018aii
RA/DEC ()
12:22:10.413 +26:59:40.44
185.543387333 +26.994566
Type
SN I
Redshift
0.0792
Source Group
ATLAS
Discovery Date
2018-01-15 16:07:40
TNS AT
Y
Public
Y
Discovery Mag
-20.303
Filter
orange-ATLAS
Discoverer/s
J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K. W. Smith, S. J. Smartt, D. R. Young, M. Fulton, O. McBrien, D. O'Neill, P. Clark (Queen's University Belfast)

Spectra

 SN_2018aii - 2018-03-25 05:32:37 ESO-NTT / EFOSC2-NTT (ePESSTO)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
18022018-03-25 05:32:37ESO-NTT / EFOSC2-NTT900Christian Vogl, Andreas Flörs, Stefan TaubenbergerStefano BenettiePESSTO tns_2018aii_2018-03-25_05-32-37_ESO-NTT_EFOSC2-NTT_ePESSTO.asci tns_2018aii_2018-03-25_05-32-37_ESO-NTT_EFOSC2-NTT_ePESSTO.fitsObjectePESSTO
Light Curves
FilterTel / InstObs-date rangePhotometry
orange-ATLASATLAS1_ACAM12018-01-15 15:48:57 - 2018-01-15 16:07:402
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
262822018-01-15 16:07:40-20.3030.27218.26ABMagorange-ATLASATLAS1_ACAM130Robot
262812018-01-15 15:48:5719.4ABMagorange-ATLASATLAS1_ACAM130Robot[Last non detection]
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
173872018-03-18 00:00:05ATLAS_Bot1J. Tonry, B. Stalder, L. Denneau, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI), K. W. Smith, S. J. Smartt, D. R. Young, M. Fulton, O. McBrien, D. O'Neill, P. Clark (Queen's University Belfast)ATLAS12:22:10.413+26:59:40.442018-01-15 16:07:40-20.303orange-ATLASPSNATLAS18mmuATLAS
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
17972018-03-26 13:21:41ePESSTO_Bot1Christian Vogl, Andreas Flörs, Stefan Taubenberger, Stefano Benetti, O. Yaron, N. Knezevic on behalf of ePESSTOePESSTOSN I0.0792ePESSTOThe spectrum resembles that of the Type Ic SN 2004aw (Taubenberger et al. 2006) at the light curve peak, but also shares some similarity with the spectra of 1991T-like SNe slightly before the maximum light.