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20102026
most citedDetection of lensing substructure using ALMA observations of the dusty galaxy SDP.81

327 citations · 4.5k across the 98 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

math.CO2026

On the sum of eccentric subgraph numbers of the vertices of a connected graph

Akash De, Kamal Lochan Patra

Let be a connected graph. The eccentric subgraph number of a vertex of is defined as , where is the number of connec…

astro-ph.CO2026

Observation-driven simulations of strong lensing galaxy clusters

L. Leuzzi, M. Meneghetti, A. Adam +9

Galaxy clusters are the most powerful strong lenses: they greatly magnify the flux of distant and faint sources. Strong lensing also allows for the reconstruction of their mass dis…

astro-ph.EP2026

POSTELLAR: Posterior Stellar Spectrum Sampling - An Alternative to Approximate Stellar Spectra for Exoplanetary Analysis

Dhvani Doshi, Nicolas B. Cowan, Yashar Hezaveh +2

We present a novel approach to perform posterior sampling of the underlying stellar spectrum in high-resolution spectroscopic observations. Our method, postellar, coherently combin…

cs.LG2026

Do Tabular Foundation Models Know Physics? Contamination, Units, and the Deterministic Limit

Wassim Tenachi, Yashar Hezaveh, Laurence Perreault Levasseur +1

Tabular foundation models (TFMs) learn to fill in tables the way language models fill in text --- and tables are arguably the format in which most physical measurement arrives. Did…

astro-ph.IM2026

Microlensing Detection and Inference via Learned Bayes Factors

Nolan Smyth, Laurence Perreault-Levasseur, Yashar Hezaveh

We present a unified framework for gravitational microlensing event detection and parameter inference. Traditional pipelines use deterministic hard cuts on photometric statistics,…

astro-ph.IM2026

Strong Gravitational Lensing Posterior Sampling in Pixel-Space Using Diffusion Models and Recurrent Inference Machines

Guillaume Payeur, Laurence Perreault-Levasseur, Gabriel Missael Barco +1

Modeling galaxy-galaxy strong gravitational lenses to infer the brightness of the source galaxy and the mass distribution of the foreground galaxy is computationally challenging, p…