1991 20160701171656.0 10.1553/cia_153s54 DOI ASTROimport-148 Lampens, P. 2008 A three-year photometric study of the oscillating Algol-type binary CT Her We present the first results of a multi-site photometric campaign carried out in 2004-2006 on the Algol-type eclipsing binary system CT Her, the primary component of which is a δ Scuti-type pulsator. Our observations include (almost complete) binary light curves in the filters B and V which have been analysed following the principles of the Wilson-Devinney method. After removal of the best-matching light curve solution, the residual B and V light curves have been investigated for their pulsational content. Strigachev, A. Kim, S.-L. Rodríguez, E. López-González, M. J. Vidal-Saínz, J. Mkrtichian, D. Litvinenko, D. van Cauteren, P. Wils, P. Gómez Forellad, J. M. Communications in Asteroseismology 153 2008 54-62 http://esoads.eso.org/abs/2008CoAst.153...54L published in REFERD