1973 20160701171656.0 ASTROimport-130 Lampens, P. 2008 Frequency analysis of the δ Scuti type pulsations in the semi-detachedeclipsing binary CT Her We present the latest results of a multisite photometric campaign carried out in 2004-2007 on the Algol-type eclipsing binary system CT Her, the primary component of which is a δ Scuti- type pulsator with a main pulsation period of only 27 min. CT Her belongs to the new class of oscillating Algol-type binary systems. We collected enough data in two passbands to perform a modelling of the light curves using PHOEBE and detected up to 7 significant pulsation frequencies in the frequency range between 45-53 d-1 in the B-residual data (independent of the adopted solution for the binary model). The remaining standard deviation of the ca. 7500 B-residuals spread over 4 years is 5.0 mmag. Strigachev, A. Kim, S.-L. Rodriguez, E. Lopez-Gonzales, M. J. Vidal-Sainz, J. Mkrtichian, D. Litvinenko, D. van Cauteren, P. Wils, P. Communications in Asteroseismology 157 2008 328-329 http://esoads.eso.org/abs/2008CoAst.157..328L published in REFERD