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We present new transit light curves for planets in six extrasolar planetarysystems. They were acquired with 0.4-2.2 m telescopes located in west Asia,Europe, and South America. When combined with literature data, they allowed usto redetermine system parameters in a homogeneous way. Our results forindividual systems are in agreement with values reported in previous studies.We refined transit ephemerides and reduced uncertainties of orbital periods bya factor between 2 and 7. No sign of any variations in transit times wasdetected for the planets studied.

New transit observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b, and WASP-39 b