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- H. Kjeldsen3 profiles69 · h 77
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- Centre National de la Recherche ScientifiqueFR185 papers
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126 papers · 1 filter
Fragility of the Dirac Cone Splitting in Topological Crystalline Insulator Heterostructures
Craig M. Polley, Ryszard Buczko, Alexander Forsman +11
The 'double Dirac cone' 2D topological interface states found on the (001) faces of topological crystalline insulators such as PbSnSe feature degeneracies located awa…
Why So Many Published Sensitivity Analyses Are False. A Systematic Review of Sensitivity Analysis Practices
Andrea Saltelli, Ksenia Aleksankina, William Becker +5
Sensitivity analysis (SA) has much to offer for a very large class of applications, such as model selection, calibration, optimization, quality assurance and many others. Sensitivi…
Using the phase shift to asymptotically characterize the dipolar mixed modes in post-main-sequence stars
C. Jiang, J. Christensen-Dalsgaard, M. Cunha
Mixed modes have been extensively observed in post-main-sequence stars by the Kepler and CoRoT space missions. The mixture of the p and g modes can be measured by the dimensionless…
Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology
Tanda Li, Timothy R. Bedding, Daniel Huber +4
Stellar models rely on a number of free parameters. High-quality observations of eclipsing binary stars observed by Kepler offer a great opportunity to calibrate model parameters f…
Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries
Simon J. Murphy, Maxwell Moe, Donald W. Kurtz +3
The orbital parameters of binaries at intermediate periods (-- d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new s…
Constraints on the Obliquities of Kepler Planet-Hosting Stars
Joshua N. Winn, Erik A. Petigura, Timothy D. Morton +8
Stars with hot Jupiters have obliquities ranging from 0-180 degrees, but relatively little is known about the obliquities of stars with smaller planets. Using data from the Califor…