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Fig. C.1
Short wavelength (1200–1700 Å) late time spectra of ONe novae observed at high resolution with IUE and HST (GHRS and STIS); time after maximum is noted. See Sect. 4 for discussion. Note that the designation of epoch for Nova Mon 2012 in both figures is relative to the Fermi/LAT observation and not the visual maximum.
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