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20022025
most citedObservation of electron-antineutrino disappearance at Daya Bay

2.2k citations

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6 papers · 1 filter

hep-ex20252 cited

First Search for Neutral Current Coherent Single-Photon Production in MicroBooNE

MicroBooNE Collaboration, P. Abratenko, D. Andrade Aldana +177

This article presents the first search for neutrino-induced neutral current coherent single-photon production (NC coherent 1). The search makes use of data from the MicroBooNE 8…

cs.HC202519 cited

Users' Mental Models of Generative AI Chatbot Ecosystems

Xingyi Wang, Xiaozheng Wang, Sunyup Park +1

The capability of GenAI-based chatbots, such as ChatGPT and Gemini, has expanded quickly in recent years, turning them into GenAI Chatbot Ecosystems. Yet, users' understanding of h…

astro-ph.GA20255 cited

Physical characterization of the FeLoBAL outflow in SDSS J0932+0840: Analysis of VLT/UVES observations

Mayank Sharma, Nahum Arav, Kirk T. Korista +5

Context: The study of quasar outflows is essential in understanding the connection between active galactic nuclei (AGN) and their host galaxies. We analyze the VLT/UVES spectrum of…

quant-ph2025

Masking Countermeasures Against Side-Channel Attacks on Quantum Computers

Jason T. LeGrow, Travis Morrison, Jamie Sikora +1

We propose a modification to the transpiler of a quantum computer to safeguard against side-channel attacks aimed at learning information about a quantum circuit. We demonstrate th…

hep-ex2025

Design and Implementation of the Cosmic Ray Tagger System for the ICARUS detector at FNAL

A. Aduszkiewicz, L. Bagby, B. Behera +50

The ICARUS-T600 Liquid Argon Time Projection Chamber is operating at Fermilab at shallow depth and thus exposed to a high flux of cosmic rays that can fake neutrino interactions. A…

astro-ph.HE202515 cited

SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases

R. Dastidar, K. Misra, S. Valenti +31

We present a comprehensive photometric and spectroscopic study of the Type IIP SN 2018is. The -band luminosity and the expansion velocity at 50 days post-explosion are 15.1$\…