The programme will include 30 min (20+10) talks as well as longer tutorials and discussion sessions.
The recorded talks, discussion and tutorials will be uploaded to our YouTube channel, where you can already find talks from the first GRPV workshop in 2022.
All sessions will take place in the Old Library, unless otherwise stated.
* Please note that the tutorial sessions on Day 2 and Day 3 will take place in parallel. For each parallel session, one will be held in the Old Library and the other in the Hovenden Room.
12:00 - Arrival + registration + lunch
13:30 - Welcome
Suzanne Aigrain
Chair: Baptiste Klein
13:45 - A Model Selection Criterion for Multidimensional Gaussian Processes applied to RVs
Oscar Barragán
14:15 - A physics-based model of stellar activity
Nathan Hara
14:30 - Incorporating Stellar Magnetic Cycles into Gaussian Process Modelling to Improve Earth-Analogue Sensitivity
Valentina Tardugno
14:45 - Poster talks
15:30 - Tea break
16:00 - A scalable approach for likelihood-based coherence modeling in many-variate GPs with applications to RV planet detection
Chris Geoga
16:30 - CALM periodogram method enables simultaneous fitting of any RV noise tracer within your planet search
Zoë de Beurs
17:00 - Discussion 1: When should we use GPs?
David Hogg
17:30 - End of Day 1
Chair: Suzanne Aigrain
09:30 - Measuring Sub-Kelvin Variations in Stellar Temperature: the dTemp indicator
Charles Cadieux
10:00 - Chromatic signatures of stellar activity in near-infrared radial velocities
Salome Grouffal
10:30 - CANSTAR: Mitigating stellar radial velocity jitter using orthogonal activity indices and a time-aware neural network
Jordi Blanco Pozo
11:00 - Coffee break
11:30 - Tutorial 1: dTemp *
Charles Cadieux
11:30 - Tutorial 2: Pyaneti *
Oscar Barragán
12:30 - Lunch
Chair: Valentina Tardugno
14:00 - The Extreme Stellar Signals Project IV: Results with Concurrent Solar Data
Lily Zhao
14:30 - Visible Versus Near-Infrared Solar-type Activity Patterns
Khaled Al Moulla
15:00 - Tracing the Spectral Fingerprints of Magnetically Active Regions Across the Optical Spectrum
Katlyn Hobbs
15:30 - Tea break
16:00 - Isolating astrophysical from instrumental variability at the pixel level in EPRV solar spectra
Ryan Rubenzahl
16:15 - An Exposure-averaged Gaussian Process Framework to Recover Stellar Variability in Combined Radial Velocity Data Sets
Jacob Luhn
16:30 - Tutorial 3: smolgp *
Soichiro Hattori & Ryan Rubenzahl
16:30 - Tutorial 4: SNAKY / YARARA *
Michael Cretignier
17:30 - End of Day 2
Chair: Oscar Barragán
10:00 - From Solar to Stellar: Investigating the Spectral Impact of Supergranulation
Niamh O'Sullivan
10:30 - Using structure functions to study supergranulation and granulation in stars other than the Sun
Jay Fitzpatrick
11:00 - Coffee break
11:30 - Tutorial 5: Learning from the Loudest: What active stars can teach us about detecting Earth 2.0 *
Louise Nielsen
11:30 - Tutorial 6: S+LEAF/FENRIR *
Jean-Baptiste Delisle & Nathan Hara
12:30 - Lunch break
Chair: Niamh O'Sullivan
14:00 - Stellar granulation-induced variability across the optical spectrum
Cis Lagae
14:30 - Measuring Granulation Jitter in 3D and Probing Depth-dependent Variability
Michael Palumbo
15:00 - Granulation signatures in line-by-line precise RVs from first disk-resolved PoET observations
Carmen San Nicolas Martinez
15:30 - Tea break
Chair: Niamh O'Sullivan
16:00 - Modeling the vertical velocity gradient to disentangle stellar activity from exoplanet signal
Varghese Reji
16:30 - Beating solar radial velocity jitter below 50cm/s with physics-based modeling
Sophie Stucki
17:00 - Reproducing HARPS-N solar RVs with disc-integrated MURaM_MPS-ATLAS spectra and SDO activity maps
Ryan Corzo
17:30 - End of Day 3
09:30 - Discussion 2: Instrumental limiting factors
Michael Cretignier
10:15 - Discussion 3: Benchmark datasets and standards
Jennifer Burt
11:00 - Coffee Break
11:30 - Discussion 4: EPRV in the PLATO era
12:15 - Concluding remarks
Suzanne Aigrain
12:30 - Lunch
14:00 - End of Day 4