SIMBAD references

H. Yamaoka, Kyushu University, reports that – using CCD images taken by K. Nakajima (Kumano, Mie, Japan, Apr. 5.76 UT), H. Naito (Nishi-Harima Astronomical Observatory, Apr. 5.79), and H. Maehara (University of Tokyo, Apr. 5.81) – he has measured the following averaged precise position of V2362 Cyg (IAUC 8697, 8698) using UCAC2-catalogue stars: R.A. = 21h11m32s.346 ± 0s.010, Decl. = +44d48'03".66 ± 0".14 (equinox 2000.0). The nearby "red" star mentioned on IAUC 8697 has UCAC2 position end figures 31s.884, 3".23 (with negligible proper motion), placing it about 4".9 away from the nova's position. The 2MASS images (1998 Oct. 13) and the Digitized Sky Survey I image (1994 Sept. 13) do not show any other object. The DSS blue (1993 June 27) and red (1990 Sept. 10) images show a dimmer object (red mag about 18) near the nova's position; if it is a true progenitor, the amplitude of nova outburst is about 10 magnitudes.