NGC/IC Project Restoration Effort

===== NGC 447 = IC 1656. This is misnamed "NGC 449" in CGCG, and that has unfortunately carried over into several other catalogues. The galaxy was found by d'Arrest who observed it on four different nights, each time measuring its position with a micrometer. His position is good, as is his description, especially concerning an 11th magnitude star 9.2 seconds of time east and 110 arcseconds north of the nebula -- the star is there, so the identification is secure. IC 1656 was found about 40 years later by Barnard. Since this is one of the nebulae which he "published" in a private communication to Dreyer, we have only the position and description in the second IC to guide us. His RA is good, but the declination is about 1.4 arcmin north of the galaxy. His description is similarly confused, "Neb, S * close sf, *9 sf 3 arcmin." The "S * close sf" is indeed superposed on the southeastern edge side of the galaxy (the GSC position is a blend of this and the galaxy), but the "* 9 sf 3 arcmin" is actually northwest by three minutes. It is the same star that d'Arrest called 11th magnitude. Still, the are no other galaxies in the area with quite that arrangement of stars around them, so Barnard's object is certainly the same one that d'Arrest had seen earlier. See NGC 451 = IC 1661 for more about Barnard's observations in the area.

===== NGC 447 17.5" (9/19/87): very faint, very small, round. A mag 15 star is involved at the southeast end. In a group with NGC 449 and NGC 451. Incorrectly identified as NGC 449 in the RNGC, CGCG, UGC.