Table C.4
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 | ||||
|
|
|||||||||
| LSQ14mo | |||||||||
| 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 | ||||
|
|
|||||||||
| Host galaxy | |||||||||
| 2015 Jan.-Feb. | 57 065.58 | 293.5 | |||||||
| A | 0.57 | 0.33 | 0.21 | ||||||
| B | 0.44 | 0.35 | 0.15 | ||||||
| C | 0.58 | 0.37 | 0.19 | ||||||
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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