activity
19962026
most citedHigher Charmonia

809 citations · 28.2k across the 927 of their papers we have counts for

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124 papers · 1 filter

cs.LG2026

One Temperature to Rule Them All?

Aviv Orly, Ori Shem-Ur, Yaron Oz

Inference-time sampling is a central mechanism for improving large language models, with temperature controlling the tradeoff between reliability and diversity. While recent work s…

astro-ph.GA2026

A combined PRIMER+MINERVA study of the evolution of $\mathbf{[O\mbox{III}]+Hβ}$ equivalent width from to

Isaac J. B. Holst, Ross J. McLure, Ryan Begley +15

We present an analysis of the evolution of equivalent width () over the redshift range to , based on combining the JWST NIRCam PRIMER and M…

astro-ph.GA2026

Euclid Quick Data Release (Q1). Refining the strong lens sample with Space Warps crowd-sourced science

Euclid Collaboration, P. Holloway, A. Verma +315

We demonstrate the efficacy of crowd-sourced refinement of strong gravitational lens candidate samples by citizen scientists. Binary (lens/non-lens) classification by citizen scien…

astro-ph.GA2026

EMU/GAMA: Understanding the link between dust geometry and star formation rate in galaxies

U. T. Ahmed, A. M. Hopkins, B. Farley +10

We investigate the link between dust obscuration and star formation rate (SFR) estimators using Halpha luminosities, L_Halpha and radio luminosities, L_radio. While the Balmer Decr…

astro-ph.GA2026

Euclid Quick Data Release (Q1). Mass-to-light ratio of elliptical galaxies: constraints from strong lensing

Euclid Collaboration, A. Sonnenfeld, A. Nersesian +312

Mass is among the most fundamental properties describing a galaxy. The relation between the luminosity and the total mass of a galaxy contains information on the efficiency of the…

cond-mat.quant-gas2026

Multidimensional revival dynamics in a bosonic many-body system

Denis Ullmo, Steven Tomsovic, Gabriel M. Lando +1

The collapse and revival of localized states in many-body systems is a quintessential example of a quantum interference phenomenon that cannot be explained purely within mean-field…

astro-ph.GA2026

Detection of HNCOH+ in the interstellar medium

M. Rey-Montejo, I. Jimenez-Serra, M. Sanz-Novo +12

Only five out of the 350 molecules detected in the interstellar medium (ISM) carry the isocyanate functional group (NCO), the essential substructure of peptide bonds in prote…

astro-ph.EP2026

Discovery of activity on Main Belt Asteroid 6993 (1995 BJ4)

Erin M. Clark, David E. Trilling, Revanth Munugala +9

We report the discovery of activity on asteroid 6993 (1995 BJ4) in the Zwicky Transient Facility (ZTF) alert stream data on UT 2026 August 5, with the help of machine learning. Vis…

hep-ph2026

Gauge Field Fluctuations Protect the Higgs Vacuum When a Small Universe Begins

Alan Zhang

The Standard Model Higgs quartic coupling turns negative at high energies. We show that in a small periodic box with antiperiodic fermions, zero-point fluctuations of the const…

cond-mat.str-el2026

Chiral magnetic excitations in the RMn6Sn6 kagome metals (R=Tb, Ho, Er, and Y)

Christopher J. Ranlett, Tianxiong Han, S. X. M. Riberolles +9

Recent inelastic neutron scattering (INS) investigations of the kagome metal TbMn6Sn6 reveal novel chiral magnetic excitations associated with the kagome layer. These excitations a…

cs.GT2026

k-Submodular Cover Problem with a Matroid Constraint

Xinru Li, Donglei Du, Qian Liu +2

We investigate k-submodular cover problem with a matroid constraint on an n-element ground set V , which seeks k disjoint subsets of V with minimal cost, where their union is an in…

astro-ph.SR2026

On the Nature of the BeWD System Nova FQ Circinus

Shatakshi Chamoli, Philip A. Charles, Judhajeet Basu +3

The classical nova FQ Cir (Schaefer et al. 2026) has recently been shown to have a Be star donor, and has been identified as a High Mass Cataclysmic Variable (HMCV), with an orbita…

astro-ph.HE2026

Supermassive Black Hole Winds in X-rays -- SUBWAYS. VI. Interplay between the soft X-ray excess and ultra-fast outflows

V. E. Gianolli, P-O. Petrucci, S. Bianchi +42

We present a broadband, multiwavelength study of the interplay between the soft X-ray excess (SE), ultra-fast outflows (UFOs), and warm absorbers (WAs) in 21 active galactic nuclei…

astro-ph.IM2026

The LSST Science Pipelines Software: Optical Survey Pipeline Reduction and Analysis Environment

Rubin Observatory Science Pipelines Developers, Yusra AlSayyad, Robert Armstrong +83

The NSF-DOE Vera C. Rubin Observatory is executing the Legacy Survey of Space and Time (LSST) as its prime mission, producing a series of data releases over the ten-year survey. Th…

astro-ph.IM2026

Chemistry on solar system scales

Catherine Walsh, Maria Drozdovskaya, Dmitry Semenov +33

The initial chemical composition of planets, primitive bodies in our solar system, and exoplanets is ultimately set by their nascent protoplanetary disks. Yet observing key carbon-…

nucl-ex2026

Double-differential neutron-induced cross sections on Fe-nat at GANIL-NFS

L. de Arruda, D. Tarrío, X. Ledoux +8

An experimental campaign to measure double-differential cross sections (DDXS) for light-charged particles (LCPs) emitted from Fe was carried out in 2023 at the Neutrons…

astro-ph.SR2026

Ensemble pulsational characteristics of eclipsing binaries containing Cep stars observed by the TESS mission

C. I. Eze, G. Handler, M. Vanrespaille +4

Massive pulsators in eclipsing binaries provide precise, model-independent stellar parameters that, combined with asteroseismic constraints, provide powerful probes of interior pro…

physics.optics2026

A Mid-Infrared Absorber Inspired by the Wing-Scale Photonic Structure of Troides magellanus

Amandine Marchand, Kevin Delmote, Olivier Deparis +1

Growing environmental and energy-related challenges have intensified the search for technologies capable of improving energy recovery and resource efficiency. Bioinspired photonic…

astro-ph.GA2026

Chemical complexity in feedback from supernova remnants: first detection of PO+ in IC443 and W44

G. Cosentino, F. Priestley, S. Scibelli +1

Supernova remnant (SNR) may shape the physical and chemical properties of star formation. By releasing refractory elements into the gas phase, they inject material of pre-biotic re…

astro-ph.SR2026

ALMA's sharpest view of IRAS 08544-4431: Unveiling the dust distribution asymmetries in the circumbinary disk

Maksym Mohorian, Devika Kamath, Elizabeth Cappellazzo +10

The interactions between post-asymptotic giant branch (post-AGB) binaries and their circumbinary disks play a central role in shaping the evolution of these systems. Circumbinary d…

hep-ph2026

Precise QCD Predictions for the Scotogenic Model at Colliders

Mohammed Boukidi, Camila Ramos, Richard Ruiz

Motivated by the anticipated data rates of the high-luminosity phase of the Large Hadron Collider, we report the first predictions up to next-to-leading order in quantum chromodyna…

astro-ph.IM2026

Probing Millisecond Optical Timescales with Continuous-Readout Mode Observations from ZTF

Shar Daniels, Federica Bianco, Igor Andreoni +6

The subminute-timescale phase space is an underexplored regime of the optical sky. Sub-second optical observations are difficult to accomplish with traditional CCD exposure-readout…

astro-ph.HE2026

Euclid: Quick Data Release (Q1) -- Optical hotspots in powerful radio galaxies

M. J. Hardcastle, L. Bisigello, M. Bondi +154

The hotspots of powerful radio galaxies are the sites of high-energy particle acceleration, but radio observations give us limited information on the electron energy distributions…

astro-ph.SR2026

Orbital and stellar parameter determination of eclipsing Cep pulsators

C. I. Eze, G. Handler, F. Kahraman Aliçavuş +2

Eclipsing binaries provide precise constraints on stellar properties and evolution, making those hosting Cep pulsators particularly valuable for characterising massive pulsatin…