EXTREMELY RARE OUTBURST OF CI GEM Last evening I found on a CCD image taken upon my request by Mark Parker with the UC Santa Barbara ROT (Celestron-14 telescope) on Feb. 18.185 UT a 'new' object of mag 15-16 slightly south of the cataloged position of CI Gem. As comparison image I used one taken with the same instrument on Feb. 11.161 UT. Shortly after my detection I made a phone call to the Isaac Newton Group (ING) at La Palma. Few hours later Pepe Vilchez and Peter Sorensen took three 150 sec images with the Wide Field Camera (WFC) attached to the Issac Newton Telescope (INT). The 'new' object is clearly visible on these images. A candidate object for CI Gem in quiescence is marked both in Duerbeck's nova catalog and in the CV catalog by Downes and Shara. The coordinates according to D/S are: R.A. 06h30m05.75s Decl. +22d18'57.7" (J2000.0) The USNO-A2.0 catalog gives the following coordinates for this star: R.A. 06h30m05.745s Decl. +22d18'58.18" (J2000.0) r= 18.4, b= 19.0 Vilchez and Sorensen mention the very blue color of the 'new' object and a magnitude difference of R= -2.6 and B= -3.9 between the 'new' object and Duerbeck's CI Gem candidate. Using the USNO magnitudes I get R= 15.8 and B= 15.1 for the 'new' object. Using the first INT image I computed the following coordinates for the 'new' object: R.A. 06h30m05.90s Decl. +22d18'50.8" (J2000.0) Nothing is visible at this position on the POSS image reproduced in Duerbeck's catalog. So I would suggest a magnitude range for ('the true') CI Gem of 15 - [21. CI Gem = 101.1943 Gem = S 3428 was discovered in 1943 by C. Hoffmeister on Sonneberg plates taken in 1940 January (MVS 30). The star reached a maximum of mpg= 14.7 on JD 2429632.5 (Jan. 4) and was brighter than mpg= 16.0 between JD 2429630.5 (Jan. 2) and JD 2429646.6 (Jan. 18) (P. Ahnert et al., VSS 1, 107). W. Wenzel (IBVS 3440) found three additional outbursts on Sonneberg plates: 1963 Oct. 15 = JD 2438318.5: mpg= 16.5 (2 plates) 1966 Feb. 23 = JD 2439180.4: mpg= 16.5 1986 Dec. 3 = JD 2446768.6: mpg= 14.5 Spectroscopy and high-speed photometry are strongly recommended for the current rare outburst of CI Gem (a SU UMa-type dwarf nova candidate). My warmest thanks to Mark Parker and Tom Fuller (both UCSB) and Pepe Vilchez and Peter Sorensen (both ING). Regards, Patrick