2004IAUC.8362....1A

Three apparent supernovae have been discovered on unfiltered CCD images – 2004cv by M. Armstrong (Rolvenden, U.K., 0.35-m reflector), 2004cw by C. Jacques (Belo Horizonte, Brazil), and 2004cx by L. A. G. Monard (Pretoria, South Africa, 0.30-m reflector). SN 2004 UT R.A. (2000.0) Decl. Mag. Offset 2004cv June 24.97 16 06 14.45 +18 24 54.0 16.8 1" W, 2" N 2004cw June 13.24 19 30 57.45 -53 32 28.7 16.6 11".4 W, 8".3 N 2004cx June 26.06 23 47 52.86 -30 31 32.6 17.0 14" E, 17" S Additional magnitudes by the respective discoverers: SN 2004cv in MCG +03-41-120, May 18 UT, [19.0; June 8, [19.0; 25.921, 16.6. SN 2004cw in ESO 184-75, 2002 Apr. 2.27, [17.8; 2003 Apr. 4.41, [18.7; June 19.18, 17.0; 25.03, 17.2. SN 2004cx in NGC 7755, May 29.1, [17.7; June 27.08, 16.8. Nothing is visible at the location of SN 2004cv on red Palomar Sky Survey images from 1987 and 1991 (limiting mag about 20.0-20.8) and a blue POSS image from 1992. There appears to be a strong H II region at the location of SN 2004cw. Nothing is visible at the location of SN 2004cx on the Digitized Sky Survey (limiting red mag 20.5).