COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1309 Konkoly Observatory Budapest 1977 July 27 PHOTOELECTRIC MOMENTS OF MAXIMA OF SZ Lyn According to the programme of investigations of dwarf cepheids photoelectric observations of the variable SZ Lyn were carried out in the years 1974-76. Within 12 nights over 500 photoelectric observations have been obtained in the system close to BV which made it possible to determine 10 maxima of light variations in SZ Lyn in each colour. The epochs E and deviations (O-C) are estimated relative to the ephemeris D3, GCVS, 1968: Max. J.D. = 2438124.3977 + 0.12053487 E. The moments of maxima and the deviations (O-C) observed relative to the above elements are tabulated below: Table Max. J.D. E (O-C) 2442129.5391 B 33228 +0.0087d .5394 V 33228 +0.0090 136.2887 B 33284 +0.0084 .2893 V 33284 +0.0090 .4091 B 33285 +0.0083 .4112 V 33285 +0.0104 .5294 B 33286 +0.080 .5298 V 33286 +0.0084 162.4450 B 33501 +0.0086 .4440 V 33501 +0.0076 871.4218 B 39383 -0.0007 .4232 V 39383 +0.0007 872.3861 B 39391 -0.0007 .3854 V 39391 -0.0014 874.3152 B 39407 -0.0001 .3161 V 39407 +0.0008 .4352 B 39408 -0.0006 .4367 V 39408 +0.0009 Deviations (O-C) confirm the conclusions made on the variability of the period of light variations in SZ Lyn with a cycle of the order of 1146 days. V.G. KARETNIKOV Yu.A. MEDVEDEV Astronomical Observatory of the Odessa University, USSR