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Jian Wang

Researcher at University of Florida

Publications -  537
Citations -  25657

Jian Wang is an academic researcher from University of Florida. The author has contributed to research in topics: Large Hadron Collider & Standard Model. The author has an hindex of 73, co-authored 483 publications receiving 21301 citations. Previous affiliations of Jian Wang include Petersburg Nuclear Physics Institute & Shandong University.

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Particle-flow reconstruction and global event description with the CMS detector

Albert M. Sirunyan, +2215 more
- 06 Oct 2017 - 
TL;DR: A fully-fledged particle-flow reconstruction algorithm tuned to the CMS detector was developed and has been consistently used in physics analyses for the first time at a hadron collider as mentioned in this paper.
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Event generator tunes obtained from underlying event and multiparton scattering measurements

Vardan Khachatryan, +2286 more
- 17 Mar 2016 - 
TL;DR: Combined fits to CMS UE proton–proton data at 7TeV and to UEProton–antiproton data from the CDF experiment at lower s, are used to study the UE models and constrain their parameters, providing thereby improved predictions for proton-proton collisions at 13.
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The CMS trigger system

U. Bhawandeep, +2292 more
- 24 Jan 2017 - 
TL;DR: In this paper, the trigger system consists of two levels designed to select events of potential physics interest from a GHz (MHz) interaction rate of proton-proton (heavy ion) collisions.
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Jet energy scale and resolution in the CMS experiment in pp collisions at 8 TeV

Khachatryan, +2288 more
- 22 Feb 2017 - 
TL;DR: In this paper, an improved jet energy scale corrections, based on a data sample corresponding to an integrated luminosity of 19.7 fb^(-1) collected by the CMS experiment in proton-proton collisions at a center-of-mass energy of 8 TeV, are presented.
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The First Data Release (DR1) of the LAMOST general survey

A-Li Luo, +142 more
- 07 May 2015 - 
TL;DR: The Large sky Area Multi-Object Spectroscopic Telescope (LAMOST) General Survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs.