activity
20202026
most citedThe white dwarf binary pathways survey V. The Gaia white dwarf plus AFGK binary sample and the identification of 23 close binaries

28 citations · 55 across the 7 of their papers we have counts for

collaborators

7 papers

hep-ex2026

Observation of and Threshold Enhancements in the System

BESIII Collaboration, M. Ablikim, M. N. Achasov +716

Using million events collected with the BESIII detector, the system produced in radiative decays is studied. A model-independent part…

hep-ex2026

Search for the isospin-violating decays and

BESIII Collaboration, M. Ablikim, M. N. Achasov +701

Using a sample of ~ events collected with the BESIII detector, we perform a search for the isospin-violating decays $χ_{cJ}\toΛ\barΣ^{0}+c.c.~…

hep-ex2025

Search for a dark baryon in the decay

BESIII Collaboration, M. Ablikim, M. N. Achasov +689

A search for a dark baryon is performed for the first time in the two-body decay using events collected at…

hep-ex2025

Observation of the -annihilation process and measurement of in decays

BESIII Collaboration, M. Ablikim, M. N. Achasov +650

We present the first amplitude analysis and branching fraction measurement of the decay , using collision data collected with the BESIII detector…

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 …

astro-ph.SR2020★ 28 cited

The white dwarf binary pathways survey V. The Gaia white dwarf plus AFGK binary sample and the identification of 23 close binaries

J. -J. Ren, R. Raddi, A. Rebassa-Mansergas +22

Close white dwarf binaries consisting of a white dwarf and an A, F, G or K type main sequence star, henceforth close WD+AFGK binaries, are ideal systems to understand the nature of…