K-corrections for LSQ14mo and its host galaxy system derived from the spectroscopic observations using snake (Inserra et al. 2017).
|Date||MJD||Phase||K g → u||K r → g||K i → r|
|2014 Jan. 31||56 688.16||–7.0||0.20||0.26||0.29|
|2014 Feb. 6||56 694.19||–2.2||0.22||0.24||0.28|
|2014 Feb. 20||56 708.06||8.8||0.28||0.27||0.26|
|2014 Feb. 28||56 716.13||15.2||0.37||0.34||0.26|
|2014 Mar. 8||56 724.26||21.7||0.41||0.38||0.25|
|2014 Apr. 21||56 768.04||56.5||0.38||0.32||0.31|
|2015 Jan.-Feb.||57 065.58||293.5|
Notes. The phase (day) has been corrected for time dilation (z = 0.256) and is relative to the SN r-band maximum on MJD 56 697. The MJD and phase of the host galaxy was adopted from the middle time of three VLT observations.
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