000006684 001__ 6684
000006684 005__ 20240126151541.0
000006684 037__ $$aSCART-2024-0052
000006684 100__ $$aDe Cat, Peter
000006684 245__ $$aThe prospects of pulsating stars studies with the International Liquid Mirror Telescope
000006684 260__ $$c2024
000006684 520__ $$aThe Hertzsprung-Russell diagram is populated with pulsating stars of many different kinds and flavours. Asteroseismology uses the pulsations of these stars to gain information about their interior, which is needed to improve our understanding of stellar evolution. During the last decade, asteroseismic studies have greatly boosted thanks to space missions like Microvariability and Oscillations of Stars (Walker et al., 2003), COnvection ROtation and Planetary Transits (CoRoT; Auvergne et al. 2009), Kepler/K2 (Borucki et al., 2010), and Transiting Exoplanet Survey Satellite (TESS; Ricker et al. 2015). These missions have collected nearly uninterrupted photometric time series with a precision down to a few µmag and a total time base of up to 4 years. TESS is the only one of these missions that is still collecting data and that is covering the largest part of the sky and hence will have targets in common with the strip of the sky that is monitored by the 4-m International Liquid Mirror Telescope from the Devasthal Observatory in northern India. In this paper, we try to find out for which types of pulsating stars the ILMT observations are expected to be most appropriate for asteroseismic studies.
000006684 536__ $$aBL/$$c33/$$fIN12 (BINA)
000006684 594__ $$aNO
000006684 6531_ $$aTelescopes
000006684 6531_ $$aSurveys
000006684 6531_ $$aStars: oscillations
000006684 700__ $$aDe Becker, Michaël
000006684 700__ $$aKumar, Brajesh
000006684 773__ $$pBulletin de la Société Royale des Sciences de Liège$$v93$$y2024
000006684 8560_ $$fpeter.decat@ksb-orb.be
000006684 8564_ $$s1430025$$uhttp://publi2-as.oma.be/record/6684/files/S11-P05_DeCatP.pdf
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000006684 905__ $$ain press to
000006684 980__ $$aREFERD