The lack of any past observations of this UGZ: variable, together with recent observations by Gary Poyner of a varying star near the nominal position of EV Aqr, imply that EV Aqr has been misidentified as a CV. To assist observers monitor this variable, here is presented a comparison star sequence based on field photometry obtained by Arne Henden. The position given here for EV Aqr is of the varying red star star observed by Poyner. This star is identical with GSC 0526-01562 and is the star identified by Tsesevich and Kazanasmas (1971) as EV Aqr. Kato [vsnet-id 86] mentions that the VSNET chart of EV Aqr (Nov 1995) gave V=13.57 for this star and marks it as var?. This magnitude appears to be accurate, as the magnitudes on the VSNET chart have negligible zero point offset when compared to the sequence presented here. Additionally the field photometry (three nights) used to derive this sequence also confirms that the star here identified as EV Aqr is indeed a red variable. It is quite possibly a SR variable. Bruce Sumner ------------------------------------------------------------------- EV AQUARII (?) Range: 12.3-14v Position: 21 06 17.86 +00 52 44.3 (J2000, from .dat file) Magnitude: V=12.444 B-V=1.483 (from .dat file) ID RA (2000) DEC X Y N V ERR B-V ERR 1 21 06 20.0 +00 50 59 31 -105 3 12.439 0.017 0.790 0.012 2 21 06 06.3 +00 48 19 -174 -265 3 12.629 0.026 0.603 0.016 3 21 06 27.1 +00 55 50 138 186 3 13.064 0.013 1.135 0.006 4 21 06 39.2 +00 54 09 320 85 3 13.309 0.020 0.713 0.007 5 21 06 14.4 +00 55 19 -52 155 3 14.040 0.020 0.690 0.012 6 21 06 10.8 +00 52 04 -106 -40 3 14.479 0.019 0.732 0.018 7 21 06 15.8 +00 54 02 -32 78 3 15.209 0.022 0.802 0.013 8 21 06 12.4 +00 52 56 -83 12 3 15.909 0.020 0.834 0.017 9 21 06 17.4 +00 51 43 -7 -61 3 16.227 0.084 0.952 0.015 10 21 06 17.2 +00 53 11 -10 27 3 16.268 0.000 1.148 0.004 11 21 06 20.1 +00 52 51 33 7 3 17.042 0.023 0.959 0.009