(Monty Python and the) HoliGRALE: A Hybrid GRALE Lens Inversion Methodology Diagnostically Evaluated with Synthetic and Real Data

arXiv:2610.09014 · astro-ph.GA · Submitted 2026-10-06 · Read on arXiv

astro-ph.GA

Submitted: 2026-10-06

Updated: 2026-10-06

Terminology

• Core — 27× in this paper · explained in 2 episodes
• Accuracy — 23× in this paper · explained in 1 episode
• Gravitational Lensing — 9× in this paper · explained in 2 episodes
• Velocity Dispersion — 9× in this paper · explained in 2 episodes
• Consistency — 4× in this paper · explained in 3 episodes
• Failure Modes — 4× in this paper · explained in 3 episodes
• Hybrid Models — 4× in this paper · explained in 2 episodes
• Hubble Frontier Fields — 2× in this paper
• Adam — 1× in this paper · explained in 2 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Fidelity — 1× in this paper · explained in 2 episodes
• Hubble Space Telescope — 1× in this paper
• Hybrid Approach — 1× in this paper · explained in 4 episodes
• James Webb Space Telescope — 1× in this paper
• Microlensing — 1× in this paper · explained in 2 episodes
• Quantifying Uncertainty — 1× in this paper · explained in 5 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Systematic Bias — 1× in this paper · explained in 3 episodes
• Trace — 1× in this paper · explained in 2 episodes
• Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

• JWST's GLIMPSE: an overview of the deepest probe of early galaxy formation and cosmic reionization
• A new H 0 measurement with SNe Requiem and Encore using Gravity.jl
• Hedorah, the first yellow supergiant Kaiju star candidate at z=3.7 revealed by JWST behind AS1063
• Where is the matter in the Merging Cluster Abell 2218?
• Flashlights: More than A Dozen High-Significance Microlensing Events of Extremely Magnified Stars in Galaxies at Redshifts z=0.7-1.5
• A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones
• Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters

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