Updated 2025 January 4

BAA meetings

Variations on an Exoplanet Theme – Part 2. On-line webinar

Provisional agenda

10:30 – 11:00 Introduction to morning session and TTVs – Roger Dymock

11:00 – 12:00 Analysis of TTVs using Exoplanetpie – Peter Vuylsteke

12:00 – 12:30 Exoplanets orbiting non-eclipsing binaries, simulator demo – Paul Dooley

12:30 – 13:30 Lunch break

13:30 – 13:50 Introduction to afternoon session – Rodney Buckland

13:50 – 14:20 Stellar variability and the PLATO mission – Karen Burgess

14:20 – 14:30 Break

14:30 – 15:00 Reducing effects of stellar variability using Lomb-Scargle techniques – Daniel
Barbos

15:00 – 15:30 The Kepler 88 exoplanetary system – Roger Dymock

15:30 – 16:00 Q and A and close of mtg – Rodney Buckland and Roger Dymock

Other organisations’ meetings

Know they star, know thy planet 2 conference, 2025 February 3-7. Caltech Caampus, Pasadena, Californaia, USA
Over the past seven years since the first conference, the limits of exoplanet discovery and the field of exoplanet characterization have changed dramatically, with great strides made in the community to understand and account for, at any even more precise and complex levels, the characteristics and effects of the stellar hosts

Exoclimes VII Montreal (Canada) from July 7 to 11, 2025.
Exoclimes VII conference will be organized by the Trottier Institute for Research in Exoplanets (https://exoplanetes.umontreal.ca/en/) and held in Montreal (Canada) from July 7 to 11, 2025. To maintain the collaborative spirit of Exoclimes, the number of participants will be limited to 200 Exoclimes is a conference series devoted to the atmosphere, climate, and evolution of sub-stellar bodies from solar system worlds to exoplanets and brown dwarfs.

Detection and Dynamics of Exoplanets (DDE): Interplay between theory and observations University of Coimbra, Portugal, 7 to 11 July 2025
Detecting and characterizing planets in multiple systems is not an easy task, because the traces of each body overlap, and the observations can be reproduced by different orbital configurations. Additionally, in many systems, planets are involved in mean motion resonances or resonant chains,