Summary: SOFI spectra reduced with PESSTO pipeline version 2.4.0. The final SOFI reductions resulted in 30 reduced near-IR science spectra of which 16 in GB, and 14 in GR. Notes on the reductions below. 2016-10-04: Hip6206 telluric standard observed before and after the spectra of SN2016gkg. The PESSTO pipeline produces an artifact when using the first set of GB observations: SOFI.2016-10-05T02:16:53.155.fits SOFI.2016-10-05T02:17:05.808.fits Therefore, the second set of observations used both for GB and GR: SOFI.2016-10-05T05:12:57.182.fits SOFI.2016-10-05T05:13:09.834.fits SOFI.2016-10-05T05:14:28.486.fits SOFI.2016-10-05T05:14:43.138.fits 2016-10-21: The PESSTO pipeline produces *_sc.fits files of HIP108375 in GB and GR, even if these are not science observations but a telluric standard. HIP108375_20161021_GB_merge_58757_2_sc.fits HIP108375_20161021_GR_merge_58757_1_sc.fits 2016-11-26: SN2016ije GB and GR spectra have a very low signal-to-noise ratio. 2017-02-05: SN2016gkg GB data does not have any signal. The observations were aborted after two frames and problems with a guide star were reported by the observers in the night report. Data not useful. 2017-02-05: The PESSTO pipeline produces *_sc.fits files of Hip7584 in GB and GR, even if these are not science observations but a telluric standard. Hip7584_20170205_GB_merge_58759_1_sc.fits Hip7584_20170205_GR_merge_58759_1_sc.fits 2017-03-25: SN2017cbv GB and GR observations did not include accompanying spectroscpic standard star observations during the same night. EG274 2017-03-07 spectrum was used for calibration. Notes on the most prominent noise spikes in the reduced spectra: 2016-12-23: A prominent noise spike around the telluric contamination region of the GB spectrum of AT2016ezh. 2017-01-18: Prominent noise spikes around the telluric contamination region of the GB spectrum of SN2016ija. 2017-03-24: Prominent noise spikes around the telluric contamination region of the GB spectrum of SN2017cbv. 2016-12-28: A prominent noise spike at the red end of the GR spectrum of SN2016ezh. 2017-01-18: A prominent noise spike at the red end of the GR spectrum of SN2016ija. 2017-02-05: A prominent noise spike at the red end of the GR spectrum of SN2016ija. 2017-03-24: A prominent noise spike at the red end of the GR spectrum of SN2017cbv. 2019-03-27: A prominent noise spike at the red end of the GR spectrum of SN2017ijn. |