output
20072026
most citedA Survey on Deep Learning for Skin Lesion Segmentation

192 citations

31 papers

cs.SE2026

Characterizing the Usefulness of Code Review Comments in Scientific Software for Software Quality and Scientific Rigor

Sharif Ahmed, Nasir U. Eisty

Context: Innovation thrives on scientific software, with useful code review feedback enhancing its correctness and impact. However, unlike general-purpose commercial and open-sourc…

astro-ph.SR2025

Citizen CATE 2024: Extending Totality During the 8 April 2024 Total Solar Eclipse with a Distributed Network of Community Participants

Sarah A. Kovac, Amir Caspi, Daniel B. Seaton +240

The Citizen CATE 2024 next-generation experiment placed 43 identical telescope and camera setups along the path of totality during the total solar eclipse (TSE) on 8 April 2024 to…

astro-ph.EP2024★ 5 cited

Properties of outer solar system pebbles during planetesimal formation from meteor observations

Peter Jenniskens, Paul R. Estrada, Stuart Pilorz +42

In the late stages of accretion leading up to the formation of planetesimals, particles grew to pebbles the size of 1-mm to tens of cm. That is the same size range that dominates t…

cs.PL2023★ 1 cited

Disco: A Functional Programming Language for Discrete Mathematics

Brent A. Yorgey

Disco is a pure, strict, statically typed functional programming language designed to be used in the setting of a discrete mathematics course. The goals of the language are to intr…

astro-ph.HE2023★ 6 cited

Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts

R. Jain, E. F. Brown, H. Schatz +11

The observation of X-rays during quiescence from transiently accreting neutron stars provides unique clues about the nature of dense matter. This, however, requires extensive model…

astro-ph.GA2022★ 7 cited

Evidence for an interaction between the Galactic Center clouds M0.10-0.08 and M0.11-0.11

Natalie O. Butterfield, Cornelia C. Lang, Adam Ginsburg +3

We present high-resolution (~2-3"; ~0.1 pc) radio observations of the Galactic center cloud M0.10-0.08 using the Very Large Array at K and Ka band (~25 and 36 GHz). The M0.10-0.08…