activity
19962026
most citedHigher Charmonia

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

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40 papers · 1 filter

physics.acc-ph2022

The ECFA Early Career Researcher's Panel: composition, structure, and activities, 2021 -- 2022

ECFA Early-Career Researcher Panel, :, Andrei Alexandru Geanta +74

The European Committee for Future Accelerators (ECFA) Early Career Researcher's (ECR) panel, which represents the interests of the ECR community to ECFA, officially began its activ…

astro-ph.GA2022★ 21 cited

Fraction of Stars in Clusters for the LEGUS Dwarf Galaxies

D. O. Cook, J. C. Lee, A. Adamo +20

We study the young star cluster populations in 23 dwarf and irregular galaxies observed by the HST Legacy ExtraGalactic Ultraviolet Survey (LEGUS), and examine relationships betwee…

astro-ph.GA2022★ 31 cited

PHANGS-JWST First Results: The 21 m Compact Source Population

Hamid Hassani, Erik Rosolowsky, Adam K. Leroy +24

We use PHANGS-JWST data to identify and classify 1271 compact 21 m sources in four nearby galaxies using MIRI F2100W data. We identify sources using a dendrogram-based algorithm…

nucl-ex2022

Isoscalar giant monopole strength in Ni, Zr, Sn and Pb

A. Bahini, R. Neveling, P. von Neumann-Cosel +22

Inelastic -particle scattering at energies of a few hundred MeV and very-forward scattering angles including has been established as a tool for the study of the isosca…

astro-ph.CO2022

Euclid preparation. XXVII. Covariance model validation for the 2-point correlation function of galaxy clusters

Euclid Collaboration, A. Fumagalli, A. Saro +191

Aims. We validate a semi-analytical model for the covariance of real-space 2-point correlation function of galaxy clusters. Methods. Using 1000 PINOCCHIO light cones mimicking the…

astro-ph.HE2022★ 3 cited

Image plane detection of FRB121102 with the MeerKAT radio telescope

J. C. Andrianjafy, N. Heeralall-Issur, A. A. Deshpande +9

We present the analysis of radio interferometric 2-s images from a MeerKAT observation of the repeating fast radio burst FRB121102 on September 2019, during which 11 distinct pulse…

hep-ph2022

Probing a 96 GeV Higgs Boson in the Di-Photon Channel at the LHC

Rachid Benbrik, Mohammed Boukidi, Stefano Moretti +1

Recently the CMS collaboration reported a local excess in the di-photon spectrum at 96 GeV. The same mass range concurs with a local excess in the i…

cond-mat.mtrl-sci2022

Magnetism and phase diagrams of Na and Ag substituted EuCdAs

Brinda Kuthanazhi, Kamal R. Joshi, Sunil Ghimire +7

EuCdAs is an antiferromagnetic semimetal, that can host non-trivial topological properties, depending upon its magnetic state and excitations. Here, we report the synthesis…

nucl-ex2022★ 14 cited

Isoscaling in central Sn+Sn collisions at 270 MeV/u

J. W. Lee, M. B. Tsang, C. Y. Tsang +61

Experimental information on fragment emissions is important in understanding the dynamics of nuclear collisions and in the development of transport model simulating heavy-ion colli…

astro-ph.HE2022★ 3 cited

Magnetically driven coupling in relativistic radiation-mediated shocks

J. F. Mahlmann, A. Vanthieghem, A. A. Philippov +3

The radiation drag in photon-rich environments of cosmic explosions can seed kinetic instabilities by inducing velocity spreads between relativistically streaming plasma components…

astro-ph.GA2022★ 15 cited

On the Use of Field RR Lyrae as Galactic Probes. VI. Mixed mode RR Lyrae variables in Fornax and in nearby dwarf galaxies

V. F. Braga, G. Fiorentino, G. Bono +11

We investigate the properties of the mixed-mode (RRd) RR Lyrae (RRL) variables in the Fornax dwarf spheroidal (dSph) galaxy by using - and -band time series collected over tw…

astro-ph.GA2022★ 14 cited

ALMA uncovers highly filamentary structure towards the Sgr E region

J. Wallace, C. Battersby, E. A. C. Mills +7

We report on the discovery of linear filaments observed in CO(1-0) emission for a field of view toward the Sgr E star forming region centered at (l,b)=(358.720, 0.…

astro-ph.HE2022★ 15 cited

Radio observations of the Black Hole X-ray Binary EXO 1846-031 re-awakening from a 34-year slumber

D. R. A. Williams, S. E. Motta, R. Fender +15

We present radio [1.3 GHz MeerKAT, 4-8 GHz Karl G. Jansky Very Large Array (VLA) and 15.5 GHz Arcminute Microkelvin Imager Large Array (AMI-LA)] and X-ray (Swift and MAXI) data fro…

astro-ph.EP2022★ 28 cited

Variability due to climate and chemistry in observations of oxygenated Earth-analogue exoplanets

Gregory Cooke, Dan Marsh, Catherine Walsh +2

The Great Oxidation Event was a period during which Earth's atmospheric oxygen (O) concentrations increased from times its present atmospheric level (PAL) to nea…

astro-ph.GA2022★ 16 cited

Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion

Eric F. Bell, Adam Smercina, Paul A. Price +8

The faint and ultrafaint dwarf galaxies in the Local Group form the observational bedrock upon which our understanding of small-scale cosmology rests. In order to understand whethe…

astro-ph.GA2022★ 25 cited

Characterizing Compact 15-33 GHz Radio Continuum Sources in Local U/LIRGs

Y. Song, S. T. Linden, A. S. Evans +23

We present the analysis of pc-scale compact radio continuum sources detected in 63 local (Ultra) Luminous Infrared Galaxies (U/LIRGs; ), u…

astro-ph.GA2022★ 15 cited

WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49

Federico Lelli, Timothy A. Davis, Martin Bureau +5

The mm-Wave Interferometric Survey of Dark Object Masses (WISDOM) is probing supermassive black holes (SMBHs) in galaxies across the Hubble sequence via molecular gas dynamics. We…

astro-ph.GA2022★ 5 cited

Radio Dichotomy in Quasars with H FWHM greater than km\,s

A. Chakraborty, A. Bhattacharjee, M. S. Brotherton +3

It has been inferred from large unbiased samples that - of all quasars are radio-loud (RL). Using the quasar catalog from the Sloan Digital Sky Survey, we show that the…

astro-ph.GA2022★ 25 cited

On the rotation curve of disk galaxies in General Relativity

Luca Ciotti

Recently, it has been suggested that the phenomenology of flat rotation curves observed at large radii in the equatorial plane of disk galaxies can be explained as a manifestation…

physics.acc-ph2022★ 2 cited

The Development of Energy-Recovery Linacs

Chris Adolphsen, Kevin Andre, Deepa Angal-Kalinin +46

Energy-recovery linacs (ERLs) have been emphasised by the recent (2020) update of the European Strategy for Particle Physics as one of the most promising technologies for the accel…

hep-ph2022

Search for charged Higgs boson in channel within 2HDM type-III

Rachid Benbrik, Mohammed Boukidi, Bouzid Manaut +3

We discus the muonic decay of light charged Higgs boson for in the context of the generic two Higgs doublet model (2HDM) type-III. We show that for both alig…

cond-mat.str-el2022★ 21 cited

Identifying the octupole Antiferromagnetic domain orientation in MnNiN by scanning Anomalous Nernst Effect microscopy

F. Johnson, J. Kimák, J. Zemen +9

The intrinsic anomalous Nernst effect in a magnetic material is governed by the Berry curvature at the Fermi energy and can be realized in non-collinear antiferromagnets with vanis…

astro-ph.IM2022★ 2 cited

A Method for Quantifying Position Reconstruction Uncertainty in Astroparticle Physics using Bayesian Networks

Christina Peters, Aaron Higuera, Shixiao Liang +4

Robust position reconstruction is paramount for enabling discoveries in astroparticle physics as backgrounds are significantly reduced by only considering interactions within the f…

astro-ph.GA2022★ 11 cited

Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven H Filaments

Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais +5

The hot intracluster medium (ICM) is thought to be quiescent with low observed velocity dispersions. Surface brightness fluctuations of the ICM also suggest that its turbulence is…