SN 2014dz
RA/DEC (2000)
03:28:14.191 +38:01:11.10
52.05913 +38.01975
Discovery Date
2014-12-20 00:00:00.000
Host Name
[Discoverer=Gagliano, Newton, Pattishall, Post, Puckett; DiscoveryRef=CBET 4052; PositionRef=CBET 4052; Orig Type=Ia]
Discovery Mag
IAU name


 SN_2014dz - 2014-12-31 03:27:29 Other / Other (None)z=
 SN_2014dz - 2014-12-31 03:27:28 Plaskett / Plaskett (DAO_OTS)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
162014-12-31 03:27:29Other / Other3418BalamBalamNone None_2014dz_2014-12-31_03:27:29_Other_Other.txtObjectspectrum via 1.82-m Plaskett Telescope, Dominion Astrophysical Observatory (National Research Council of Canada)
482014-12-31 03:27:28Plaskett / Plaskett3418BalamBalamDAO_OTS DAO_OTS_2014dz_2014-12-31_03:27:28_Plaskett_Telescope_Plaskett.txt DAO_OTS_2014dz_2014-12-31_03:27:28_Plaskett_Telescope_Plaskett.fitsObjectDAO_OTS
Light Curves
No Data
AT Reports
No Data
Classification Reports
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarksADS Bibcode
432016-01-21 22:32:00DAO_OTSDave Balam on behalf of DAO_OTSDAO_OTSSN Ia0.018DAO_OTSif the host is 2MASS J03281358+3800587 then the redshift is z=0.018. Our best SNid fit is to SN 2003du at T about 1 week post-maximum. If the host is valid then the expansion velocity of the ejected material, as inferred from the position of the absorption of the Si II 635.5-nm line, is about 8300 km/s.2016TNSCR1115....1B
142016-01-17 00:15:36DAO_OTSDave Balam on behalf of DAO_OTSDAO_OTSSN IaCross-correlation with a library of supernova spectra using the "Supernova Identification" code (Blondin and Tonry 2007, Ap.J. 666,1024) indicates that 2014dz is most similar to the type-Ia supernova 2003du at 9 days past maximum light. The photospheric velocity estimated from the Si II 635.5-nm feature is about 8700 km/s.2016TNSCR..28....1B