output
20042026
most citedDeep learning guided image-based droplet sorting for on-demand selection and analysis of single cells and 3D cell cultures

112 citations

27 papers

astro-ph.EP2026

Exploration of Exoplanet Atmospheres with the James Webb Space Telescope

Sasha Hinkley, David K. Sing

The James Webb Space Telescope (JWST) is providing transformative characterization capabilities for the study of both transiting and directly imaged extrasolar planets. Observation…

astro-ph.SR2026

Interferometric Images of the Starspot Evolution of Andromedae

Rachael M. Roettenbacher, John D. Monnier, Heidi Korhonen +21

The evolution of starspots of the giant primaries of RS CVn systems is typically detected indirectly with photometric and spectroscopic monitoring. These observations suggest slowl…

astro-ph.HE2025★ 5 cited

Cosmic-ray transport in inhomogeneous media

Robert J. Ewart, Patrick Reichherzer, Shuzhe Ren +6

A theory of cosmic-ray transport in multi-phase diffusive media is developed, with the specific application to cases in which the cosmic-ray diffusion coefficient has large spatial…

quant-ph2024★ 1 cited

Minimum Synthesis Cost of CNOT Circuits

Alan Bu, Evan Fan, Robert Sanghyeon Joo

Optimizing the size and depth of CNOT circuits is an active area of research in quantum computing and is particularly relevant for circuits synthesized from the Clifford + T univer…

astro-ph.IM2024

Planet Formation Imager (PFI): Project update and future directions

John D. Monnier, Stefan Kraus, Michael J. Ireland

The Planet Formation Imager (PFI) Project is dedicated to defining a next-generation facility that can answer fundamental questions about how planets form, including detection of y…

astro-ph.SR2024

Orbits and Dynamical Masses for Six Binary Systems in the Hyades Cluster

Guillermo Torres, Gail H. Schaefer, Robert P. Stefanik +8

We report long baseline interferometric observations with the CHARA Array that resolve six previously known double-lined spectroscopic binary systems in the Hyades cluster, with or…