Table 1
Log of spectral observations.
| Date | Phase | Telescope + Instrument | Range | Resolution |
| (y/m/d) | (d) | (Å) | (Å) | |
|
|
||||
| 2014/11/15 | +2.6 | NTT + EFOSC2 grism 13 | 3661–8815 | 18.2 |
| 2014/11/16 | +3.5 | NTT + EFOSC2 grism 16 | 6006–9786 | 13.4 |
| 2014/11/29 | +15.4 | VLT + FORS2 grism 300I | 6150–9261 | 13.0 |
| 2014/12/14 | +29.3 | NTT + EFOSC2 grism 11 | 3582–7463 | 13.8 |
Notes. A slit width of 1.̋0 was used for every observation. Phases are rest frame days measured from JD of I-band maximum, JD 2 456 973.9. Resolution is the standard value of the given instrumental configuration for a 1.̋0 slit at the central wavelength. The range reflects the useful range plotted in Fig. 2.
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