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Tao An

7 papers hereh-index 3118 citations5 works total

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

author position
  • first author2
  • middle author2
  • last author2

Across the 6 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
  • astro-ph.HE2
  • astro-ph1
same name
  • Tao An — 14 papers, h 4
  • Tao An — 13 papers, h 1
  • Tao An — 8 papers, h 2
  • Tao An — 4 papers, h 2
  • Tao An — 2 papers, h 5
  • Tao An — 2 papers, h 5

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
20042025
most citedThe Submillimeter Array 1.3 mm line survey of Arp 220

96 citations · 208 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

4 papers · 1 filter

astro-ph.CO2011★ 30 cited

Radio structure of the blazar 1156+295 with sub-pc resolution

W. Zhao, X. -Y. Hong, T. An +4

1156+295 is a flat-spectrum quasar which is loud at radio and gamma-ray. Previous observations of the source revealed a radio morphology on pc to kpc scales consistent with a helic…

astro-ph.CO2010★ 96 cited

The Submillimeter Array 1.3 mm line survey of Arp 220

S. Martin, M. Krips, J. Martin-Pintado +7

We present the first aperture synthesis unbiased spectral line survey toward an extragalactic object. The survey covered the 40 GHz frequency range between 202 and 242 GHz of the 1…

astro-ph.CO2009★ 5 cited

Metal Enrichment via Ram Pressure Stripping in the IGM of the Compact Galaxy Group RGH 80

Haijuan Cui, Haiguang Xu, Junhua Gu +4

By creating and analyzing the two dimensional gas temperature and abundance maps of the RGH 80 compact galaxy group with the high-quality Chandra data, we detect a high-abundance (…

astro-ph.CO2009★ 46 cited

Kinematics of the parsec-scale radio jet in 3C48

T. An, X. Y. Hong, M. J. Hardcastle +6

We present results on the compact steep-spectrum quasar 3C 48 from observations with the VLBA, MERLIN and EVN at multiple radio frequencies. In the 1.5-GHz VLBI images, the radio j…

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