SIMBAD references

Kazuyoshi Imamura, Okayama University of Science (OUS), reports that a low-dispersion spectrum (R about 400) of PNV J17260708-2551454 was obtained on Mar. 27.836 UT using the 0.28-m Schmidt-Cassegrain telescope (+ DSS-7 spectrometer) at the OUS observatory, suggesting that the variable is a classical nova. An H-alpha emission line can be seen in the spectrum (FWHM < 800 km/s). The spectrum is posted at the following website URL: http://blog-imgs-32-origin.fc2.com/t/n/b/tnblab/pnv_inOph_20120327.png.