COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2526 Konkoly Observatory Budapest 28 May 1984 HU ISSN 0374-0676 OBSERVATIONS OF AT Cnc IN THE SEASON 1983/84 The star which is probably of cataclysmic type was inspected on 24 blue- sensitive plates (ORWO-ZU21 + GG13 + BG12) obtained in the B system with the Schmidt camera 50/70/172 cm of Sonneberg Observatory covering the time interval between 1983 December 3 and 1984 March 23; the sequence of comparison stars given in I.B.V.S. No. 2363 was used. These observations are listed in Table I. Table I J.D.244... mB J.D.244... mB 5672.522 13m00 5680.515 15m83 5672.549 12.79 5683.633 12.79 5672.576 12.79 5684.627 13.34 5672.603 12.66 5750.323 12.66 5672.660 12.66 5752.420 14.57 5673.511 13.21 5761.319 13.07 5673.533 13.34 5763.359 15.25 5673.558 13.34 5779.347 15.98 5674.530 14.57 5780.344 15.11 5674.553 14.16 5781.339 12.52 5676.547 15.98 5782.335 12.66 5679.507 >15.0 5783.331 12.59 The light curve of the star shows variations over the whole amplitude between mB = 12.5m and mB = 16.0m. A remarkable increase of brightness with Delta mB = -3.46m within 1.992d was stated between 1984 March 19 and March 21. On the other hand on the series of plates from 1983 December 3 and December 4 only small variations can be seen. W. GOTZ Akademie der Wissenschaften der DDR, Zentralinstitut fur Astrophysik, Sternwarte Sonneberg CORRIGENDA (to I.B.V.S. No. 2477) On p.1. The observed time of Min. II is J.D. 2444679.6663. (The J.D. of this minimum is correctly stated in Table I.) On p.2. Table I. The O-C value given for the last two minima is +0.0097 and not +0.0079. (These residuals are correctly plotted in Fig.1.)