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Jiayin Gu

43 papers hereh-index 222.1k citations70 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author15
  • middle author19
  • last author5

Across the 39 of 43 papers where every author was matched, so the position is known.

fields
  • hep-ph26
  • cond-mat.stat-mech7
  • astro-ph.GA4
  • hep-ex2
  • physics.acc-ph2
  • astro-ph.IM1
same name
  • Jiayin Gu — 4 papers, h 1
  • Jiayin Gu — 4 papers, h 1
  • Jiayin Gu — 3 papers, h 2
  • Jiayin Gu — 2 papers, h 2
  • Jiayin Gu — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20112023
most citedPrecision Higgs Physics at CEPC

168 citations · 1.1k across the 42 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

hep-ph2016★ 5 cited

Exploring the nearly degenerate stop region with sbottom decays

Haipeng An, Jiayin Gu, Lian-Tao Wang

A light stop with mass almost degenerate with the lightest neutralino has important connections with both naturalness and dark matter relic abundance. This region is also very hard…

astro-ph.GA2016★ 14 cited

Kinematics of the Galactic disk from LAMOST Dwarf sample

Yingjie Jing, Cuihua Du, Jiayin Gu +10

Based on the LAMOST survey and Sloan Digital Sky Survey (SDSS), we use low-resolution spectra of 130,043 F/G-type dwarf stars to study the kinematics and metallicity properties of…

astro-ph.IM2016★ 1 cited

A Monte-Carlo Method for Making SDSS u-Band Magnitude more accurate

Jiayin Gu, Cuihua Du, Wenbo Zuo +4

We develop a new Monte-Carlo-based method to convert the SDSS (Sloan Digital Sky Survey) u-band magnitude to the SCUSS (South Galactic Cap of u-band Sky Survey) u-band magnit…

astro-ph.GA2016★ 5 cited

A Monte-Carlo Method for Estimating Stellar Photometric Metallicity Distributions

Jiayin Gu, Cuihua Du, Yingjie jing +1

Based on the Sloan Digital Sky Survey (SDSS), we develop a new monte-carlo based method to estimate the photometric metallicity distribution function (MDF) for stars in the Milky W…

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