Fig. 2.
Sample fluxed spectra (ergs/cm2 s−1/Å) from the spectroscopic observations in Table 1. The UT date of each observing run is indicated in the figure itself. The dashed vertical lines in the top panel delimit the wavelength range of the time series from 27 October. The emission lines in the November 2008 spectrum (bottom panel) redward of 7000 Å are due to second-order overlap (see text).
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