VizieR Online Data Catalog: UV-NIR LCs of the energetic H-stripped SN2016coi (Terreran+, 2019)

SN 2016coi was discovered on 2016 May 27.55 UT (MJD57535.55; Holoien+ 2016ATel.9086....1H) by the All Sky Automated Survey for SuperNovae (ASAS-SN; Shappee+ 2014, J/ApJ/788/48) in the irregular galaxy UGC 11868.

Our photometric data have been obtained from several different telescopes and instruments, see Table 3. Our UV-to-NIR campaign densely samples the evolution of SN 2016coi in its first ~400 days post explosion, with more than 1100 observations distributed over 166 nights (the gap around 200-300 days corresponds to when SN 2016coi was behind to the Sun). See Section 2.

We obtained optical spectroscopy of SN 2016coi from a few days until t>400days post explosion with a variety of instruments on different telescopes. The spectroscopic log can be found in Table 9. See Section 3.

We present in Figure 8 multiband observations of SN 2016coi taken up to 278 days post explosion with the Karl G. Jansky Very Large Array (VLA; projects 16A-447 and 17A-167). The details of these data are given in Table 10. See Section 4.

The X-Ray Telescope (XRT), on board the Neil Gehrels Swift Observatory, started observing SN 2016coi on 2016 May 27 (δt~2days post explosion) until 2017 April 17 (δt~326days), for a total exposure time of 94.4ks. See Section 5.

(6 data files).