VizieR Online Data Catalog: UV to visible-light observations of SN 2018fif (Soumagnac+, 2020)

SN 2018fif was first detected on 2018 August 21 at 8:46 UT by the ZTF wide-field camera mounted on the 1.2m Samuel Oschin Telescope (P48) at Palomar Observatory. Previous ZTF observations were obtained in the months prior to the SN explosion and the most recent nondetection was on 2018 August 20 at 9:37:26.40 UT, i.e., less than 24hr before the first detection. SN 2018fif was photometrically followed in multiple bands for ~5 months. The photometry is reported in Table 2.

Swift observations of the SN 2018fif field started on 2018 August 21 and 11 observations were obtained with a cadence of ~1 day.

Observations from P48 were obtained using the ZTF mosaic camera through r-band and g-band filters of the SDSS.

Observations from the robotic 1.52m telescope at Palomar (P60) were obtained using the rainbow camera arm of the SED Machine spectrograph, equipped with a 2048x2048 pixel CCD camera and with g', r', and i' SDSS filters.

(1 data file).