3950 20190128152925.0 10.1093/mnras/sty034 DOI SCART-2019-0083 Brunsden, E. Frequency and mode identification of γ Doradus from photometric and spectroscopic observations 2018 The prototype star for the γ Doradus class of pulsating variables was studied employing photometric and spectroscopic observations to determine the frequencies and modes of pulsation. The four frequencies found are self-consistent between the observation types and almost identical to those found in previous studies (1.3641 d-1, 1.8783 d-1, 1.4742 d-1, and 1.3209 d-1). Three of the frequencies are classified as l, m = (1, 1) pulsations and the other is ambiguous between l, m = (2, 0) and (2, -2) modes. Two frequencies are shown to be stable over 20 yr since their first identification. The agreement in ground-based work makes this star an excellent calibrator between high-precision photometry and spectroscopy with the upcoming TESS observations and a potential standard for continued asteroseismic modelling. NO line: profiles techniques: spectroscopic stars: oscillations stars: variables: general Pollard, K. R. Wright, D. J. De Cat, P. Cottrell, P. L. Monthly Notices of the Royal Astronomical Society 475 2018 3 3813-3822 peter.decat@observatoire.be https://academic.oup.com/mnras/article/475/3/3813/4795324 published in REFERD