| Wednesday, 23 October |
|
| 09:30 | Registration, and welcome coffee |
Session 1: PoET and related instrumentation – Chair: Bachar Wehbe |
|
| 10:00 | Nuno C. Santos PoET: an overview |
| 10:20 | Alexandre Cabral PoET design |
| 10:40 | André Silva PoET Observations |
| 11:00 | Maddalena Bugatti/Francesco Pepe nuAncestor, a wavelength calibration satellite of interest to PoET and ESPRESSO? |
| 11:20 | Lilly Zhao Integration times for solar observations |
| 11:35 | Gaspare lo Curto Operations of HELIOS |
| 11:50 | Alain Smette Molecfit: Recent results relevant for PoET |
| 12:10 | General discussion |
| 12:45 | Lunch Break |
Session 2: Radial velocities – Chair: Eduardo Cristo |
|
| 14:00 | André Silva Observing strategies and their role in the improvement of RV analysis |
| 14:20 | Carmen San Nicolás Martinéz Refining the radial velocity method to uncover other Earths |
| 14:40 | Alba Barka Modelling stellar noise in precise radial velocities: using the Sun as a proxy |
| 15:00 | Andrew Collier Cameron Mapping granulation velocities versus depth with MURaM simulations of PoET disc-centre intensities |
| 15:20 | Coffee Break |
| 15:40 | Michael Palumbo Probing Line-by-Line Variability from Granulation with PoET |
| 16:00 | Cretignier Michael How PoET could deliver the ingredients for the ultimate stellar activity correction |
| 16:20 | Eric Ford Line shape variations from the NEID Solar Telescope |
| 16:40 | Xavier Dumusque Solar RV in the VIS and NIR |
| 17:00 | General discussion |
| 18:00 | End of day 1 |
| 19:00 | Social program (gathering for drinks and dinner) |
| Thursday, 24 October |
|
Session 2: Radial velocities – Chair: André Silva |
|
| 09:30 | Annelies Mortier ABORAS: A polarising Sun-as-a-star telescope coupled to HARPS3 |
| 09:50 | Khaled Al Moulla Small-scale magnetic field proxies in the optical and near-infrared using solar observations from HARPS-N, HARPS, and NIRPS |
| 10:10 | Nadege Meunier Confrontation between modelled and direct observation of the convective blueshift inhibition |
| 10:30 | Ignasi Ribas Physical modelling of solar and stellar activity (TBC) |
| 10:50 | Federica Rescigno Re-calibration and analysis of the BiSON data and its impact on PoET observational plan |
| 11:10 | Coffee Break |
| 11:30 | General discussion |
| 12:30 | Lunch Break |
Session 3: Atmospheres – Chair: Olivier Demangeon |
|
| 14:00 | William Dethier Stellar contaminations in high-resolution transit spectroscopy |
| 14:20 | Julia Seidel Time-resolved exoplanet atmospheric retrievals - stellar impact and the role of the Sun |
| 14:40 | Eduardo Cristo Bridging PoET Observations with Simulations with SOAP |
| 15:00 | Jennifer Peralta Detecting exoplanet atmospheres in the presence of stellar activity |
| 15:20 | Coffee Break |
| 15:50 | Vincent Bourrier Optimal extraction of spatially-resolved stellar spectra with high-resolution transit spectroscopy |
| 16:10 | Heather Cegla Granulation at different limb angles through 3D simulations |
| 16:30 | General discussion |
Session 4: Solar and stellar physics – Chair: Ricardo Gafeira |
|
| 17:30 | Ângela Santos Stochastic solar phenomena: insights into granulation and oscillation properties |
| 17:50 | Sowmya Krishnamurthy Sensitivity of spectral lines to solar granulation |
| 18:10 | End of day 2 |
| Friday, 25 October |
|
Session 4: Solar and stellar physics – Chair: Ângela Santos |
|
| 09:00 | Alex Pietrow Sun as a star flare observations with HARPS-N |
| 09:20 | Jean Costes New stellar activity indicators and how PoET could help us understand the physics of astrophysical noise |
| 09:40 | Momo Ellwarth Varying Convective Motions in High-Resolution IAG Solar Observations |
| 10:00 | Sasha Shapiro Modeling magnetic features on surfaces of cool stars |
| 10:20 | Coffee Break |
| 10:50 | Dainis Dravins Solar photospheric spectrum microvariability |
| 11:10 | Hans Peter Doerr The Tautenburg Solar Laboratory - A Pathfinder for a Next-Generation Network of Ground-Based Synoptic Solar Observatories |
| 11:30 | Ricardo Gafeira Influence of spatial resolution in the diagnostic capabilities of spectropolarimetric observations |
| 11:50 | General discussion |
| 12:30 | End of meeting |
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