Abstract Submission

Our splinter session will have up to 6 contributed talks from the community. We thus welcome the submission of abstracts suitable for this session. We encourage students and early-career scientists to submit an abstract.

The splinter session will focus on the spectroscopic manifestation of stellar variability, covering a large range of spectral types (F-M stars), where similar processes are present but with different relative impacts on radial velocities. We will also focus on attempting to significantly improve our understanding of RV variability to enable the detection of very low-mass planets. We have therefore two main objectives:

1. Improve exchanges between communities (techniques, characterisation of stellar activity) to get a more complete view of the processes, focusing here on main sequence stars.
2. Improve a better community effort to identify the next steps and define what we need to improve our understanding of RV stellar variability (theoretical works, other techniques, simultaneous observations…).

We encourage attendees to develop collaborations across the various observational and theoretical techniques. There is much to be gained from further exploring those synergies and comparing the Sun to other stars.

Submission process and deadline

Deadline : May 1st 2022

Submit you title and abstract on this form