most citedHadronic "flow" in p--Pb collisions at the Large Hadron Collider?

6 citations · 6 across the 1 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202114 cited

A cautionary tale in fitting galaxy rotation curves with Bayesian techniques: does Newton's constant vary from galaxy to galaxy?

Pengfei Li, Federico Lelli, Stacy McGaugh +2

The application of Bayesian techniques to astronomical data is generally non-trivial because the fitting parameters can be strongly degenerated and the formal uncertainties are the…

astro-ph.GA2020

Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters

Yong Tian, Po-Chieh Yu, Pengfei Li +2

We investigate the mass-velocity dispersion relation (MVDR) in 29 galaxy clusters in the HIghest X-ray FLUx Galaxy Cluster Sample (HIFLUGCS). We measure the spatially resolved, lin…

astro-ph.GA2020

Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies

Kyu-Hyun Chae, Federico Lelli, Harry Desmond +3

The strong equivalence principle (SEP) distinguishes General Relativity from other viable theories of gravity. The SEP demands that the internal dynamics of a self-gravitating syst…

astro-ph.GA2020

Characteristic mass in galaxy quenching: environmental versus internal effects

Pengfei Li, Huiyuan Wang, H. J. Mo +2

A clear transition feature of galaxy quenching is identified in the multi-parameter space of stellar mass (), bulge to total mass ratio (), halo mass (

astro-ph.GA2020

A comprehensive catalog of dark matter halo models for SPARC galaxies

Pengfei Li, Federico Lelli, Stacy McGaugh +1

We present rotation curve fits to 175 late-type galaxies from the Spitzer Photometry & Accurate Rotation Curves (SPARC) database using seven dark matter (DM) halo profiles: pseudo-…

astro-ph.GA201923 cited

The halo mass function of late-type galaxies from HI kinematics

Pengfei Li, Federico Lelli, Stacy McGaugh +3

We present an empirical method to measure the halo mass function (HMF) of galaxies. We determine the relation between the \hi\ line-width from single-dish observations and the dark…