Using Arne Henden's recent field photometry [vsnet-chat 2144] I have derived the following sequence for N. Aql 1999. As Arne mentioned the photometry can be considered as reliable down to V=14, which explains why this sequence stops at that magnitude. A fainter extension will hopefully be available at a later date. Bruce Sumner ---------------------------------------------------------------- 144 N. AQUILAE 1999 (N) Range: 8.8 - ? Position: 19 07 36.88 +12 31 26.7 (J2000, from .dat file) Magnitude: V=11.567 BV=1.247 (from .dat file) ID RA (2000) DEC X Y N V ERR BV ERR 1 19 07 24.9 +12 37 25 175 358 3 8.381 0.060 0.285 0.045 2 19 07 14.2 +12 32 22 332 55 3 10.391 0.006 1.159 0.010 3 19 07 47.4 +12 36 25 154 298 3 11.688 0.008 0.509 0.011 4 19 07 32.7 +12 28 27 62 180 3 12.004 0.006 1.334 0.013 5 19 07 43.6 +12 33 25 98 118 3 12.811 0.008 0.844 0.004 6 19 07 42.6 +12 32 49 84 82 2 13.195 0.006 0.767 0.002 7 19 07 50.8 +12 31 07 203 20 3 13.379 0.005 0.538 0.016 8 19 07 40.2 +12 32 46 48 79 1 14.228 9.999 0.612 9.999