SIMBAD references

U. Munari and A. Siviero, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory; A. Henden, AAVSO; and S. Dallaporta and G. Cherini, ANS ("Asiago Novae and Symbiotic stars") Collaboration, report that V2362 Cyg (= N Cyg 2006) has apparently concluded its re-brightening phase (cf. CBET 739), which began in July, and has turned toward a new decline (perhaps its final decline). The peak in the re-brightening was apparently reached around Nov. 30.2 UT, when the nova showed B = 10.46, B-V = +0.48, V-I_c = +1.14, and R_c–Ic = +0.54. The latest magnitude data for Dec. 5.7 give B = 10.63, B-V = +0.45, V-I_c = +1.17, and R_c–Ic = +0.53.