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Q

Q. Feng

Researcher at Columbia University

Publications -  180
Citations -  5116

Q. Feng is an academic researcher from Columbia University. The author has contributed to research in topics: Blazar & Telescope. The author has an hindex of 38, co-authored 172 publications receiving 4421 citations. Previous affiliations of Q. Feng include Purdue University & McGill University.

Papers
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Constraints on cosmic rays, magnetic fields, and dark matter from gamma-ray observations of the coma cluster of galaxies with veritas and fermi

T. Arlen, +83 more
TL;DR: In this paper, the gamma-ray upper limits of the Coma galaxy cluster with the VERITAS array of imaging Cerenkov telescopes, with complementing Fermi Large Area Telescope observations at GeV energies, were investigated.
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VERITAS deep observations of the dwarf spheroidal galaxy Segue 1

E. Aliu, +92 more
- 05 Mar 2012 - 
TL;DR: In this paper, the VERITAS array of Cherenkov telescopes has carried out a deep observational program on the nearby dwarf spheroidal galaxy Segue 1, and upper limits on the integrated flux are derived.
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Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010

Jelena Aleksić, +259 more
TL;DR: In this paper, the day-scale SEDs with one-zone and two-zone synchrotron self-Compton (SSC) models were investigated, and the observed broadband SED variability can be associated to variations in the relativistic particle population.
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Dark matter constraints from a joint analysis of dwarf Spheroidal galaxy observations with VERITAS

S. Archambault, +73 more
- 05 Apr 2017 - 
TL;DR: In this article, the authors present constraints on the annihilation cross section of weakly interacting massive particles dark matter based on the joint statistical analysis of four dwarf galaxies with VERITAS.
Journal ArticleDOI

Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010

Jelena Aleksić, +259 more
TL;DR: In this paper, the authors modeled the day-scale SED with one-zone and two-zone synchrotron self-Compton (SSC) models, investigated the physical parameters, and evaluated whether the observed broadband SED variability can be associated with variations in the relativistic particle population.