SIMBAD references

P. Challis, R. Foley, G. H. Marion, and R. Kirshner, Harvard-Smithsonian Center for Astrophysics (CfA); and J. Ruel, Physics Department, Harvard University, on behalf of the CfA Supernova Group, report on spectroscopic observations that were obtained of 2010db (cf. CBET 2290) by P. Berlind on June 7 UT with the F. L. Whipple Observatory 1.5-m telescope (+ FAST; range 360-760 nm). The spectrum of 2010db appears to be that of an M-type star with significant proper motion. The star was at R.A. = 18:26:12.958, Decl. = +30:14:26.34 (equinox 2000.0, FK5) in a red Digitized Sky Survey (DSS) image from 1989 May 3, and at position end figures 11s.808, 21".05 in a DSS infrared image from 1995 Sept. 12. W. Brown, CfA, notes that this star was designated LSR J1826+3014 = LSPM J1826+3014 when reported by Lepine et al. (2002, Ap.J. 581, L47; 2005, A.J. 129, 1483) with magnitudes V = 19.4, I = 14.4, and K = 10.8 and proper motion of 2.382 arcsec/yr.