output
20042026
most citedGalaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey

708 citations

146 papers

cs.CR2026★ 7 cited

PrivDNN: A Secure Multi-Party Computation Framework for Deep Learning using Partial DNN Encryption

Liangqin Ren, Zeyan Liu, Fengjun Li +3

In the past decade, we have witnessed an exponential growth of deep learning models, platforms, and applications. While existing DL applications and Machine Learning as a service (…

astro-ph.GA2026

Specific Star Formation Rate Enhancement across the Galaxy Merger Sequence: Insights from Citizen Science Classifications

Jacob Lee, Alexandra Le Reste, Claudia Scarlata +1

We present an analysis of specific star formation rates (sSFR) across the galaxy merger sequence using visual classifications from the Zooniverse citizen science project "Cosmic Di…

astro-ph.GA2026

4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < < 7) selected with SED fitting

T. Mkrtchyan, C. Mazzucchelli, R. J. Assef +12

The identification of high-redshift quasars () is critical for studying the early Universe, supermassive black hole growth, and cosmic reionization. Most known high-redshi…

physics.chem-ph2025★ 1 cited

Real-time dynamics with bead-Fourier path integrals I: Bead-Fourier CMD

Nathan London, Mohammad R. Momeni

Developing new methods for the accurate and efficient calculations of real-time quantum correlation functions is deemed one of the most challenging problems of modern condensed mat…

physics.chem-ph2025★ 1 cited

Elucidating Ion Capture and Transport Mechanisms of Preyssler Anions in Aqueous Solutions Using Biased MACE-Accelerated MD Simulations

Quadri O. Adewuyi, Suchona Akter, Md Omar Faruque +4

Equilibrium and biased MACE accelerated MD simulations in aqueous solutions are performed to investigate the ion capture and transport mechanisms of the {P5W30} Preyssler anion (PA…

astro-ph.GA2025★ 5 cited

Directly Imaging the Cooling Flow in the Phoenix Cluster

Michael Reefe, Michael McDonald, Marios Chatzikos +14

In the centers of many galaxy clusters, the hot (10 K) intracluster medium (ICM) can become dense enough that it should cool on short timescales. However, the low measure…