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Found 9 papers, 4 papers with code
Laboratory Experiments of Model-based Reinforcement Learning for Adaptive Optics Control
RL is an active branch of the machine learning research field, where control of a system is learned through interaction with the environment.
Model-based Reinforcement Learning
reinforcement-learning
+1
Inferring Atmospheric Properties of Exoplanets with Flow Matching and Neural Importance Sampling
Atmospheric retrievals (AR) characterize exoplanets by estimating atmospheric parameters from observed light spectra, typically by framing the task as a Bayesian inference problem.
Parameterizing pressure-temperature profiles of exoplanet atmospheres with neural networks
When training and evaluating our method on two publicly available datasets of self-consistent PT profiles, we find that our method achieves, on average, better fit quality than existing baseline methods, despite using fewer parameters.
Half-sibling regression meets exoplanet imaging: PSF modeling and subtraction using a flexible, domain knowledge-driven, causal framework
Our HSR-based method provides an alternative, flexible and promising approach to the challenge of modeling and subtracting the stellar PSF and systematic noise in exoplanet imaging data.
High contrast imaging for the enhanced resolution imager and spectrometer (ERIS)
ERIS is a diffraction limited thermal infrared imager and spectrograph for the Very Large Telescope UT4.
Instrumentation and Methods for Astrophysics
Physically constrained causal noise models for high-contrast imaging of exoplanets
The detection of exoplanets in high-contrast imaging (HCI) data hinges on post-processing methods to remove spurious light from the host star.
MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 micron. I. Photometric analysis of $β$ Pic b, HIP 65426 b, PZ Tel B and HD 206893 B
The $L'$-NB4. 05 and $L'$-$M'$ colors of the studied sample are all red while the NB4. 05-$M'$ color is blue for $\beta$ Pic b, gray for PZ Tel B, and red for HIP 65426 b and HD 206893 B (although typically with low significance).
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
PynPoint: a modular pipeline architecture for processing and analysis of high-contrast imaging data
The architecture of PynPoint has been redesigned with the core functionalities decoupled from the pipeline modules.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics
The formation of Jupiter by hybrid pebble-planetesimal accretion
The evidence that Jupiter slowed down its growth after reaching 20 Earth masses for at least 2 Myr is puzzling because a planet of this mass is expected to trigger fast runaway gas accretion.
Earth and Planetary Astrophysics
