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Siyi Xu

37 papers hereh-index 17985 citations50 works total

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

author position
  • first author7
  • middle author20
  • last author5

Across the 32 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP18
  • astro-ph.SR15
  • astro-ph.IM3
  • astro-ph.GA1
same name
  • Siyi Xu — 11 papers, h 10
  • Siyi Xu — 10 papers, h 3
  • Siyi Xu — 10 papers, h 3
  • Siyi Xu — 8 papers, h 4
  • Siyi Xu — 3 papers, h 4
  • Siyi Xu — 2 papers

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
20102026
most citedA Giant Planet Candidate Transiting a White Dwarf

183 citations · 1.4k across the 36 of their papers we have counts for

collaborators
Showing 2018Show all

4 papers · 1 filter

astro-ph.SR2018★ 24 cited

Distant White Dwarfs in the US Naval Observatory Flagstaff Station Parallax Sample

S. K. Leggett, P. Bergeron, John P. Subasavage +18

This paper presents new trigonometric parallaxes and proper motions for 214 stars. The measurements were made at the US Naval Observatory Flagstaff Station (NOFS) between 1989 and…

astro-ph.EP2018★ 48 cited

Dust Production and Depletion in Evolved Planetary Systems

J. Farihi, R. van Lieshout, P. W. Cauley +15

The infrared dust emission from the white dwarf GD 56 is found to rise and fall by 20% peak-to-peak over 11.2 yr, and is consistent with ongoing dust production and depletion. It i…

astro-ph.EP2018★ 43 cited

Infrared Variability of Two Dusty White Dwarfs

Siyi Xu, Kate Y. L. Su, Laura Rogers +11

The most heavily polluted white dwarfs often show excess infrared radiation from circumstellar dust disks, which are modeled as a result of tidal disruption of extrasolar minor pla…

astro-ph.EP2018★ 47 cited

The Excited Spin State of 1I/2017 U1 `Oumuamua

Michael J. S. Belton, Olivier R. Hainaut, Karen J. Meech +15

We show that `Oumuamua's excited spin could be in a high energy LAM state, which implies that its shape could be far from the highly elongated shape found in previous studies. CLEA…

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