SIMBAD references

Kazuyoshi Imamura, Okayama University of Science (OUS) team, writes that he obtained a low-dispersion spectrum (R about 400) of PNV J17395600-2447420 on May 22.697 UT using a 0.28-m Schmidt-Cassegrain telescope (+ DSS-7 spectrometer) at the OUS observatory. Broad and prominent emission lines of the Balmer series, Fe II (multiplets 42, 48, 49, 74), O I (747.7- and 777.3-nm), and Mg II (823.2-nm ) can be seen in the spectrum. The FWHM of H-alpha is approximately 2900 km/s. This suggests that the object is a classical nova. The spectrogram has been posted at the following website URL: http://blog-imgs-44.fc2.com/t/n/b/tnblab/pnOPH_20120522.png.