2285 20160701171702.0 10.1007/s10509-009-0219-z DOI ASTROimport-442 Maisonneuve, F. 2010 Spectroscopic mode identification of main-sequence non-radially pulsating stars We are undertaking an extensive observational campaign of a number of non-radially pulsating stars using the high-resolution HERCULES spectrograph on the 1.0-m telescope at the Mt John University Observatory. This is part of a large world-wide multi-site campaign to improve mode-identification techniques in non-radially pulsating stars, particularly for g-mode pulsators. This paper outlines our campaign and presents preliminary results for one γ Doradus star, HD 40745, and one β Cephei star, HD 61068. We have used a representative cross-correlation line-profile technique presented by Wright in 2008 to extract line profiles and these have then been analyzed using the FAMIAS package due to Zima published in 2006 to derive a spectroscopic mode identification. Pollard, K. R. Cottrell, P. L. Kilmartin, P. M. Wright, D. J. De Cat, P. Astrophysics and Space Science 328 1-2 2010 105-108 http://esoads.eso.org/abs/2010Ap%26SS.328..105M published in REFERD