160 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of Wisconsin–MadisonUS25 papers
- University of Maryland, College ParkUS10 papers
- Pennsylvania State UniversityUS9 papers
- University of UtahUS9 papers
- Sungkyunkwan UniversityKR8 papers
- Columbia UniversityUS7 papers
- SLAC National Accelerator LaboratoryUS7 papers
- Stanford UniversityUS7 papers
- Friedrich-Alexander-Universität Erlangen-NürnbergDE6 papers
- Georgia Institute of TechnologyUS6 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS6 papers
- The Ohio State UniversityUS6 papers
28 papers
The Vera C. Rubin Observatory Data Preview 1
Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325
We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…
The first 10years of the HAWC Gamma-Ray Observatory: science results
Anna Lia Longinotti, HAWC Collaboration
The High-Altitude Water Cherenkov (HAWC) Observatory, located on the slopes of the Sierra Negra volcano in Mexico, began operations in March 2015. Over the past decade, HAWC has en…
Design and Performance of the Upgraded Prototype Schwarzschild-Couder Telescope Camera Module
Giovanni Ambrosi, Carla Aramo, Mattia Barbanera +54
The Cherenkov Telescope Array Observatory (CTAO) is a ground-based observatory that will improve upon the sensitivities of the current generation of very-high-energy gamma-ray inst…
Particle Astrophysics with High and Ultrahigh Energy Neutrinos
Ke Fang, Kohta Murase
We summarize recent results of the observations of high (1 TeV-100 PeV) and ultrahigh ( PeV) energy neutrinos, including the detection of a diffuse cosmic high-energy neu…
Background Measurements and Simulations of the ComPair Balloon Flight
Zachary Metzler, Nicholas Kirschner, Lucas Smith +31
ComPair, a prototype of the All-sky Medium Energy Gamma-ray Observatory (AMEGO), completed a short-duration high-altitude balloon campaign on August 27, 2023 from Fort Sumner, New…
GollumFit: An IceCube Open-Source Framework for Binned-Likelihood Neutrino Telescope Analyses
IceCube Collaboration
We present GollumFit, a framework designed for performing binned-likelihood analyses on neutrino telescope data. GollumFit incorporates model parameters common to any neutrino tele…
Absence of TeV halos around millisecond pulsars
A. U. Abeysekara, R. Alfaro, C. Alvarez +82
TeV halos are extended very-high-energy (VHE; 0.1-100 TeV) gamma-ray emission around middle-aged pulsars. So far they have only been found around isolated pulsars, but it has been…
Resilient Stellarator Divertor Characteristics in the Helically Symmetric eXperiment
K. A. Garcia, A. Bader, D. Boeyaert +5
Resilient divertor features connected to open chaotic edge structures in the Helically Symmetric Experiment (HSX) are investigated. For the first time, an expanded vessel wall was…
CTC and CT5TEA: an advanced multi-channel digitizer and trigger ASIC for imaging atmospheric Cherenkov telescopes
Benjamin Schwab, Adrian Zink, Davide Depaoli +12
We have developed a new set of Application-Specific Integrated Circuits (ASICs) of the TARGET family (CTC and CT5TEA), designed for the readout of signals from photosensors in came…
Search for Continuous and Transient Neutrino Emission Associated with IceCube's Highest-Energy Tracks: An 11-Year Analysis
R. Abbasi, M. Ackermann, J. Adams +406
IceCube alert events are neutrinos with a moderate-to-high probability of having astrophysical origin. In this study, we analyze 11 years of IceCube data and investigate 122 alert…
Exploration of Non-Resonant Divertor Features on the Compact Toroidal Hybrid
K. A. Garcia, A. Bader, H. Frerichs +4
Non-resonant divertors (NRDs) separate the confined plasma from the surrounding plasma facing components (PFCs). The resulting striking field line intersection pattern on these PFC…
Multimessenger Potential of the Radio Neutrino Observatory in Greenland
Marco Stein Muzio
The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ~PeV) neutrino monitor of the Northern sky and will soon be the world's most sen…
Kinetic-Ballooning-Limited Pedestals in Spherical Tokamak Plasmas
J. F. Parisi, W. Guttenfelder, A. O. Nelson +12
A theoretical model is presented that for the first time matches experimental measurements of the pedestal width-height Diallo scaling in the low-aspect-ratio high- tokamak NSTX…
Search for inelastic WIMP-iodine scattering with COSINE-100
G. Adhikari, N. Carlin, J. J. Choi +56
We report the results of a search for inelastic scattering of weakly interacting massive particles (WIMPs) off I nuclei using NaI(Tl) crystals with a data exposure of 97.7…
Constraints on the origins of the Galactic neutrino flux
Abhishek Desai, Justin Vandenbroucke, Samalka Anandagoda +2
Galactic and extragalactic objects in the universe are sources of high-energy neutrinos {that may contribute to the astrophysical neutrino signal seen by IceCube.} Recently, a stud…
Milky Way as a Neutrino Desert Revealed by IceCube Galactic Plane Observation
Ke Fang, John S. Gallagher, Francis Halzen
The Galactic diffuse emission (GDE) is formed when cosmic rays leave the sources where they were accelerated, diffusively propagate in the Galactic magnetic field, and interact wit…
Prometheus: An Open-Source Neutrino Telescope Simulation
Jeffrey Lazar, Stephan Meighen-Berger, Christian Haack +3
Neutrino telescopes are gigaton-scale neutrino detectors comprised of individual light-detection units. Though constructed from simple building blocks, they have opened a new windo…
IceCat-1: the IceCube Event Catalog of Alert Tracks
R. Abbasi, M. Ackermann, J. Adams +390
We present a catalog of likely astrophysical neutrino track-like events from the IceCube Neutrino Observatory. IceCube began reporting likely astrophysical neutrinos in 2016 and th…
Development of the ComPair gamma-ray telescope prototype
Daniel Shy, Carolyn Kierans, Nicolas Cannady +22
There is a growing interest in the science uniquely enabled by observations in the MeV range, particularly in light of multi-messenger astrophysics. The Compton Pair (ComPair) tele…
Three-year annual modulation search with COSINE-100
100 Collaboration, G. Adhikari, E. Barbosa de Souza +55
COSINE-100 is a direct detection dark matter experiment that aims to test DAMA/LIBRA's claim of dark matter discovery by searching for a dark matter-induced annual modulation signa…
Searching for low-mass dark matter via Migdal effect in COSINE-100
G. Adhikari, N. Carlin, J. J. Choi +53
We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 exp…
Multi-messenger Implications of Sub-PeV Diffuse Galactic Gamma-Ray Emission
Ke Fang, Kohta Murase
The diffuse Galactic gamma-ray flux between 0.1 and 1 PeV has recently been measured by the Tibet AS Collaboration. The flux and spectrum are consistent with the decay of neutra…
Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification
K. M. Stringer, J. P. Long, L. M. Macri +75
Many studies have shown that RR Lyrae variable stars (RRL) are powerful stellar tracers of Galactic halo structure and satellite galaxies. The Dark Energy Survey (DES), with its de…
Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data
J. Etherington, D. Thomas, C. Maraston +61
Measurements of the galaxy stellar mass function are crucial to understand the formation of galaxies in the Universe. In a hierarchical clustering paradigm it is plausible that the…