000006691 001__ 6691
000006691 005__ 20240126170736.0
000006691 037__ $$aPOSTER-2024-0017
000006691 100__ $$aDe Cat, Peter
000006691 245__ $$aThe prospects of pulsating stars studies with the International Liquid Mirror Telescope
000006691 260__ $$c2023
000006691 269__ $$c2023-03-22
000006691 520__ $$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.
000006691 536__ $$aBL/$$c33/$$fIN12 (BINA)
000006691 594__ $$aNO
000006691 6531_ $$aTelescopes; Surveys
000006691 6531_ $$aStars: oscillations
000006691 700__ $$aDe Becker, Michaël
000006691 700__ $$aKumar, Brajesh
000006691 773__ $$t3rd BINA Workshop "Scientific Potential of Indo-Belgian Co-operation", Bhimtal, India
000006691 8560_ $$fpeter.decat@ksb-orb.be
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000006691 980__ $$aCPOSTER