activity
19992026
most citedObservation of electron-antineutrino disappearance at Daya Bay

2.2k citations · 9.5k across the 137 of their papers we have counts for

collaborators

138 papers

astro-ph.GA2026

Rapid quenching and early gas depletion in the core of a galaxy protocluster at z=2.2

C. D'Eugenio, H. Dannerbauer, A. Naufal +6

Understanding how galaxy evolution is affected in forming high-z overdensities is a major open question in modern astrophysics. Here, we present the average properties of the quies…

astro-ph.GA2026

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster

J. Nadolny, J. M. Pérez-Martínez, H. Dannerbauer +8

We investigate how the environment affects galaxy structure in the Spiderweb protocluster at using JWST/NIRCam F115W, F182M, and F410M imaging (rest-frame Å to…

astro-ph.CO2026

KiDS-Legacy: Joint analysis of second- and third-order cosmic shear

L. Linke, L. Porth, P. Burger +21

Weak lensing by large-scale structure is a powerful cosmological probe. While most analyses rely on second-order correlations, these are primarily sensitive to the parameter combin…

astro-ph.GA2025★ 3 cited

JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster

Y. H. Zhang, H. Dannerbauer, J. M. Pérez-Martínez +14

We present JWST/NIRCam imaging of dusty star-forming galaxies (DSFGs) detected by Atacama Large Millimeter/submillimeter Array (ALMA) in the Spiderweb protocluster at . We…

astro-ph.GA2025

Euclid Quick Data Release (Q1): Euclid spectroscopy of quasars. 1. Identification and redshift determination of 3500 bright quasars

Euclid Collaboration, Y. Fu, R. Bouwens +354

The slitless spectroscopy mode of the NISP onboard Euclid has enabled efficient spectroscopy of objects within a large FoV. We present a large and homogeneous sample of bright quas…

nucl-ex2025★ 1 cited

Half-life determination of heavy ions in a storage ring considering feeding and depleting background processes

R. J. Chen, G. Leckenby, R. S. Sidhu +49

Heavy-ion storage rings have relatively large momentum acceptance which allows for multiple ion species to circulate at the same time. This needs to be considered in radioactive de…

astro-ph.HE2025★ 3 cited

An extremely soft and weak fast X-ray transient associated with a luminous supernova

W. -X. Li, Z. -P. Zhu, X. -Z. Zou +101

Long gamma-ray bursts (LGRBs), including their subclasses of low-luminosity GRBs (LL-GRBs) and X-ray flashes (XRFs) characterized by low spectral peak energies, are known to be ass…

nucl-th2025

Effective proton-neutron interaction in mirror nuclei

Y. M. Xing, Y. F. Luo, K. H. Li +9

Effective proton-neutron interactions, , in mirror nuclei are systematically analyzed using the ground-state atomic masses. A mirror symmetry of is found for bound…

nucl-ex2025

Magicity Revealed by the Mass of the Proton Dripline Nucleus Si

Y. M. Xing, Y. F. Luo, Y. H. Zhang +36

Using the -defined isochronous mass spectrometry technique, we conducted the first mass measurement of the proton dripline nucleus Si. We confirm that Si is bound…

astro-ph.HE2025★ 1 cited

An Intermediate-mass Black Hole Lurking in A Galactic Halo Caught Alive during Outburst

C. -C. Jin, D. -Y. Li, N. Jiang +137

Stellar-mass and supermassive black holes abound in the Universe, whereas intermediate-mass black holes (IMBHs) of ~10^2-10^5 solar masses in between are largely missing observatio…

nucl-ex2025★ 10 cited

Bound-State Beta Decay of Ions and the LOREX Project

R. S. Sidhu, G. Leckenby, R. J. Chen +55

Stable Tl ions have the lowest known energy threshold for capturing electron neutrinos () of \,keV. The Lorandite Experiment (LOREX), proposed in th…

astro-ph.GA2024★ 11 cited

ASWDF: Census of the obscured star formation in a galaxy cluster in formation at

Y. H. Zhang, H. Dannerbauer, J. M. Pérez-Martínez +13

We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm mapping of the Spiderweb protocluster at . The observations were divid…

astro-ph.HE2024★ 30 cited

A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova

H. Sun, W. -X. Li, L. -D. Liu +163

Massive stars end their lives as core-collapse supernovae, amongst which some extremes are broad-lined type Ic supernovae from Wolf-Rayet stars associated with long-duration gamma-…

nucl-th2024★ 5 cited

Exploring isospin-nonconserving effects in the upper shell with new mass measurements

H. F. Li, X. Xu, Y. Sun +8

Nuclear mass measurements have recently been extended conspicuously to proton-rich region in the upper shell. The new data are utilized to study isospin symmetry breaking phen…

astro-ph.HE2024★ 2 cited

Soft X-ray prompt emission from a high-redshift gamma-ray burst EP240315a

Y. Liu, H. Sun, D. Xu +191

Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early un…

nucl-ex2024

Neutron radius determination of 133Cs and its impact on the interpretation of CEvNS-CsI measurement

Y. Huang, S. Y. Xia, Y. F. Li +16

Proton-Cs elastic scattering at low momentum transfer is performed using an in-ring reaction technique at the Cooler Storage Ring at the Heavy Ion Research Facility in Lanz…

astro-ph.HE2024

Pulsed Iron line Emission from the First Galactic Ultraluminous X-ray Pulsar Swift J0243.6+6124

Y. X. Xiao, Y. J. Xu, M. Y. Ge +14

We report the phase-resolved spectral results of the first Galactic Pulsating Ultra-Luminous X-ray source (PULX) Swift J0243.6+6124, modeling at its 2017-2018 outburst peak using d…

astro-ph.HE2023★ 11 cited

Magnetar emergence in a peculiar gamma-ray burst from a compact star merger

H. Sun, C. -W. Wang, J. Yang +42

The central engine that powers gamma-ray bursts (GRBs), the most powerful explosions in the universe, is still not identified. Besides hyper-accreting black holes, rapidly spinning…

nucl-th2023

Investigation of isospin-symmetry-breaking in mirror energy difference and nuclear mass with ab initio calculations

H. H. Li, Q. Yuan, J. G. Li +7

Isospin-symmetry breaking is responsible for the energy difference of excited states in mirror nuclei. It also influences the coefficient of the isobaric multiplet mass equation. I…

nucl-th2023★ 18 cited

Ab initio descriptions of mirror nuclei with resonance and continuum coupling

S. Zhang, F. R. Xu, J. G. Li +6

We have used an {\it ab initio} Gamow shell model to study the isospin symmetry breaking in the mirror nuclei of F, N, Ne and C. Starting from a…

nucl-th2021★ 18 cited

Systematic trends of neutron skin thickness versus relative neutron excess

J. T. Zhang, X. L. Tu, P. Sarriguren +7

Available experimental neutron skin thicknesses of even-even stable Ca, Ni, Sn, Pb, and Cd isotopes are evaluated, and separate trends of neutron skin thickness versus relative neu…

hep-ex2021★ 14 cited

Measurement of the branching fraction of leptonic decay via

M. Ablikim, M. N. Achasov, P. Adlarson +503

By analyzing of annihilation data collected at the center-of-mass energies between 4.178 and 4.226\,GeV with the BESIII detector, we determine the…

hep-ex2021★ 13 cited

Measurements of the branching fractions of and

BESIII Collaboration, M. Ablikim, M. N. Achasov +505

Based on events collected with the BESIII detector at BEPCII, the branching fraction of the isospin violating decay …

nucl-th2020★ 20 cited

Probing the nature of the conjectured low-spin wobbling bands in atomic nuclei

S. Guo, X. H. Zhou, C. M. Petrache +28

Precession is a unique motion in which the orientation of the rotational axis of a rotating body is not fixed but moving, and it generally exists in the Universe from giant stars t…