Publications (7)
The PLATO Mission
Heike Rauer, Conny Aerts, Juan Cabrera +842
PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…
What CoRoT tells us about δ Scuti stars existence of a regular pattern and seismic indices to characterize stars
Eric Michel, Marc-Antoine Dupret, Daniel Reese +8
Inspired by the so appealing example of red giants, where going from a handful of stars to thousands revealed the structure of the eigenspectrum, we inspected a large homogeneous s…
The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission
Matthew Raymond Gent, Maria Bergemann, Aldo Serenelli +25
We introduce the SAPP (Stellar Abundances and atmospheric Parameters Pipeline), the prototype of the code that will be used to determine parameters of stars observed within the cor…
Linear approximation of seismic inversions: new kernels and structural effects
Gaël Buldgen, Daniel Reese, Marc-Antoine Dupret
Thanks to the space-based photometry missions CoRoT and Kepler, we now benefit from a wealth of seismic data for stars other than the sun. In the future, K2, Tess and Plato will pr…
Asteroseismic inversions in the Kepler era: application to the Kepler Legacy sample
Gaël Buldgen, Daniel Reese, Marc-Antoine Dupret
In the past few years, the CoRoT and Kepler missions have carried out what is now called the space photometry revolution. This revolution is still ongoing thanks to K2 and will be…
Pulsations of rapidly rotating stars: I. The ACOR numerical code
Rhita-Maria Ouazzani, Marc-Antoine Dupret, Daniel Reese
Very high precision seismic space missions such as CoRoT and Kepler provide the means of testing the modeling of transport processes in stellar interiors. For some stars, such as s…
Five young Scuti stars in the Pleiades seen with Kepler/K2
Simon J. Murphy, Timothy R. Bedding, Timothy R. White +4
We perform mode identification for five Scuti stars in the Pleiades star cluster, using custom light curves from K2 photometry. By creating échelle diagrams, we identify radi…