Showing 1–20 of 90 results
/ Date/ Name
Oct 27, 2021Study of Chemically Peculiar Stars-I : High-resolution Spectroscopy and K2 Photometry of Am Stars in the Region of M44Mar 21, 2022The near-core rotation of HD 112429: a gamma Doradus star with TESS photometry and legacy spectroscopyJan 21, 2009New magnetic field measurements of beta Cephei stars and Slowly Pulsating B starsDec 31, 2009Kepler Asteroseismology Program: Introduction and First ResultsMar 31, 2010Ground-based follow-up in relation to Kepler Asteroseismic InvestigationOct 1, 2022Transfer Learning for Individual Treatment Effect EstimationMay 19, 2023Mode-Aware Continual Learning for Conditional Generative Adversarial NetworksJan 31, 2023Improving Open-Domain Dialogue Evaluation with a Causal Inference ModelMar 3, 2011Kepler observations of variability in B-type starsJul 1, 2011The Kepler characterization of the variability among A- and F-type stars. I. General overviewJul 1, 2014MOST light-curve analysis of the gamma Dor pulsator HR 8799, showing resonances and amplitude variationsSep 26, 2012Spectroscopic Pulsational Frequency Identification and Mode Determination of γ Doradus Star HD 12901Jan 14, 2014Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giantsMay 31, 2007Search for pulsation among suspected A-type binaries and the new multiperiodic Delta Scuti star HD217860Sep 20, 2011The excitation of solar-like oscillations in a delta Scuti star by efficient envelope convectionMar 31, 2009An asteroseismic study of the beta Cephei star 12 Lacertae: multisite spectroscopic observations, mode identification and seismic modellingJun 19, 2009Ground-based observations of the beta Cephei CoRoT main target HD 180642: abundance analysis and mode identificationSep 22, 2010Spectral analysis of Kepler SPB and Beta Cep candidate starsJan 11, 2023Comprehensive spectroscopic and photometric study of pulsating eclipsing binary star AI HyaMay 10, 2022Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT