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By-product of the V1162 Ori multisite campaign: the new Scuti star GSC 4778 00324

    P. Lampens, P. van Cauteren, P. Niarchos, K. Gazeas, V. Manimanis, T. Arentoft, P. Wils, A. Bruch, R. Garrido, R. Shobbrook

Communications in Asteroseismology 141, pp. 65-71, 2007/07/19

January, 2002

doi: 10.1553/cia141s65

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doi:10.1553/cia141



doi:10.1553/cia141s65


The satellite photometry of the _ Scuti star 0² Tau obtained with the Wide- Field Infrared Explorer (WIRE) led to the detection of 12 frequencies of pulsation (Poretti et al. 2002). We examine the available ground-based photometry in the literature to check whether these frequencies are also present. The re-analysis of the 1986 Delta Scuti Network data leads to 10 statistically significant frequencies (amplitude signal/noise ratio greater than 4.0). 9 of these 10 frequencies are in excellent agreement with those detected from space, while the 10th frequency is seen as a peak in the WIRE residuals, though not at a statistically significant level. Previous reports on amplitude variability are confirmed.