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T. Jiang

4 papers hereh-index 373 citations4 works total

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

author position
  • first author1
  • last author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM2
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • T. Jiang — 135 papers, h 10
  • T. Jiang — 55 papers, h 3
  • T. Jiang — 35 papers, h 4
  • T. Jiang — 32 papers, h 22
  • T. Jiang — 30 papers
  • T. Jiang — 10 papers, h 43

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
20112018
most citedThe Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?

60 citations · 89 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2018★ 16 cited

Testing General Relativity with geodetic VLBI: what profit from a single, specially designed experiment?

Oleg Titov, Anastasiia Girdiuk, Sebastien Lambert +15

Context. We highlight the capabilities of the geodetic VLBI technique to test General relativity in the classical astrometric style, i.e., measuring the deflection of light in the…

astro-ph.IM2017★ 1 cited

Testing of General Relativity with Geodetic VLBI

O. Titov

The geodetic VLBI technique is capable of measuring the Sun's gravity light deflection from distant radio sources around the whole sky. This light deflection is equivalent to the c…

astro-ph.CO2011★ 60 cited

The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?

Douglas F. Watson, Andreas A. Berlind, Cameron K. McBride +2

We investigate the radial distribution of galaxies within their host dark matter halos by modeling their small-scale clustering, as measured in the Sloan Digital Sky Survey. Specif…

astro-ph.GA2011★ 12 cited

Galaxy growth by merging in the nearby universe

Tao Jiang, David W. Hogg, Michael R. Blanton

We measure the mass growth rate by merging for a wide range of galaxy types. We present the small-scale (0.014 < r < 11 h70^{-1} Mpc) projected cross-correlation functions w(rp) of…

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