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(FCAPT) are presented for the mCP stars HD 142070, HR 6967, and HR 8434 and the CP star HR 5341. The latter star is found to be constant. Improved periods were derived for HD 142070, 3.37189 d, HR 6967, 3.91227 d, and HR 8434, 1.43237 d. Further observations of HD 142070 are needed to phase the magnetic data with the photometry, of HR 6967 to settle minor discrepancies between y and scaled GenevaV photometry, and of HR 8434 to resolve small discrepancies between two uvby photometric data sets.

$\vec{uvby}$ photometry of the CP stars HR 5341, HD 142070, HR 6967, and HR 8434