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Liang Yu

29 papers hereh-index 211.9k citations49 works total

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

author position
  • first author5
  • middle author13
  • last author7

Across the 25 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP25
  • astro-ph.SR2
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • Liang Yu — 19 papers
  • Liang Yu — 9 papers, h 22
  • Liang Yu — 8 papers, h 13
  • Liang Yu — 5 papers, h 26
  • Liang Yu — 4 papers, h 3
  • Liang Yu — 3 papers, h 8

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
20152021
most citedThe clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2

413 citations · 2.2k across the 29 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.CO2017★ 413 cited

The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2

Metin Ata, Falk Baumgarten, Julian Bautista +60

We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space using the clustering of quasars. We consider a sample of 147,000 quasars from the extended…

astro-ph.EP2017★ 183 cited

The Apparently Decaying Orbit of WASP-12

Kishore C. Patra, Joshua N. Winn, Matthew J. Holman +3

We present new transit and occultation times for the hot Jupiter WASP-12b. The data are compatible with a constant period derivative: P˙=−29±3 ms yr−1 and $P/\dot{P…

astro-ph.EP2017★ 12 cited

The K2-ESPRINT Project VI: K2-105 b, a Hot-Neptune around a Metal-rich G-dwarf

Norio Narita, Teruyuki Hirano, Akihiko Fukui +16

We report on the confirmation that the candidate transits observed for the star EPIC 211525389 are due to a short-period Neptune-sized planet. The host star, located in K2 campaign…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.