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Dear colleagues, I examined VRI photometry of the rest of the fields measured during 2002 with 40cm telescope at Brno observatory in 2002 (some data were taken together with Petr Sobotka and Jan Skalicky). The images were processed automatically. The field photometry was searched for new variable stars using algorithm described e.g. in Pojmanski, 2000 (astro-ph/0005236), and implemented in VARFIND by Lukas Kral (http://kral.astronomy.cz/soft/varfind/). Three new variables were detected. Pej 018 = GSC 2137:222 in the field of BF Cyg RA = 19:23:57.6, Dec = 29:37:13 (J2000) The light curve suggests short period variable star. USNO A2.0 gives b-r = 1.9 mag, but the star is of neutral colour on my images (2 Cyg some 2 arcmin to the east might spoil USNO A2.0 photometry). As it is probably short period star, I give raw measurements (R and I band measurements are differentials against GSC 2136:27, V band are absolute): 20020603.9461 1.43Ic 20020705.9650 1.73Ic 20020705.9652 1.84Ic 20020705.9655 1.68Ic 20020720.8858 1.42Ic 20020720.8860 1.42Ic 20020727.9579 1.56Ic 20020727.9588 1.54Ic 20020727.9597 1.62Ic 20020819.9546 1.58Ic 20020830.8771 1.53Ic 20020830.8780 1.57Ic 20020830.8789 1.50Ic 20021026.8507 1.78Ic 20021026.8517 1.74Ic 20021026.8526 1.83Ic 20030105.6895 1.49Ic 20030105.6913 1.57Ic 20020518.9204 1.17Rc 20020518.9214 1.14Rc 20020603.9472 1.33Rc 20020603.9474 1.29Rc 20020603.9477 1.34Rc 20020705.9662 1.55Rc 20020705.9664 1.64Rc 20020705.9668 1.59Rc 20020720.8868 1.34Rc 20020720.8871 1.35Rc 20020720.8873 1.33Rc 20020727.9577 1.48Rc 20020727.9586 1.47Rc 20020727.9595 1.43Rc 20020819.9525 1.45Rc 20020819.9535 1.41Rc 20020819.9544 1.41Rc 20020830.8769 1.68Rc 20020830.8778 1.51Rc 20020830.8788 1.48Rc 20021026.8506 1.65Rc 20021026.8515 1.62Rc 20021026.8524 1.72Rc 20021231.7514 1.27Rc 20021231.7523 1.03Rc 20030105.6893 1.43Rc 20030105.6902 1.40Rc 20030105.6911 1.49Rc 20020518.9226 13.32V 20020518.9231 13.29V 20020518.9236 13.28V 20020518.9242 13.29V 20020518.9247 13.30V 20020603.9489 13.43V 20020603.9494 13.38V 20020603.9500 13.38V 20020705.9678 13.92V 20020705.9682 13.82V 20020705.9687 13.84V 20020720.8887 13.46V 20020720.8892 13.55V 20020720.8896 13.50V 20020727.9575 13.52V 20020727.9584 13.55V 20020727.9593 13.57V 20020819.9523 13.78V 20020819.9533 13.66V 20020819.9542 13.59V 20020830.8767 13.67V 20020830.8777 13.61V 20020830.8786 13.65V 20021026.8504 13.77V 20021026.8513 13.79V 20021026.8522 13.84V 20021231.7521 13.44V 20030105.6892 13.40V 20030105.6901 13.41V 20030105.6910 13.47V Pej 019 in the field of BF Cyg RA = 19:24:10.5, Dec = +29:42:48 (J2000), USNO A2.0 gives b-r = 2.2 mag The star is red on my images and perhaps another low amplitude SR. Nightly averages (concerning the comparison stars see description of Pej 018, V filter isn't included due to low S/N): 20020603.9461 0.78Ic 20020705.9652 0.75Ic 20020720.8860 0.66Ic 20020727.9588 0.70Ic 20020819.9546 0.79Ic 20020830.8780 0.79Ic 20021026.8517 0.64Ic 20021231.7510 0.81Ic 20030105.6905 0.82Ic 20020518.9204 2.04Rc 20020603.9474 2.13Rc 20020705.9665 2.15Rc 20020720.8871 1.89Rc 20020727.9586 1.85Rc 20020819.9535 2.04Rc 20020830.8778 2.15Rc 20021026.8515 1.87Rc 20030105.6902 2.11Rc Pej 020 in the field of V1016 Cyg RA = 19:57:14.9, Dec = +39:49:55 (J2000), USNO A2.0 gives b-r = 1.8 mag, although the USNO A2.0 star is slightly (several arcsec) off the position. Perhaps another low amplitude SR. Nightly averages (differentials against GSC 3141:577): 20020604.0601 1.59Ic 20020706.0585 1.54Ic 20020720.8751 1.67Ic 20020727.9762 1.69Ic 20020819.9714 1.77Ic 20020830.8958 1.79Ic 20021026.8694 1.51Ic 20021231.7693 1.60Ic 20030105.7072 1.60Ic 20020604.0609 3.05Rc 20020706.0596 3.12Rc 20020720.8762 3.14Rc 20020727.9760 3.18Rc 20020819.9708 3.33Rc 20021026.8692 3.03Rc 20030105.7071 3.14Rc V1116 Cyg in the same field was also observed. Best regards, Ondrej Pejcha
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