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C. Williams

216 papers hereh-index 509k citations269 works total

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

author position
  • first author10
  • middle author156
  • last author28

Across the 194 of 216 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA201
  • astro-ph.CO6
  • astro-ph.IM3
  • astro-ph.SR3
  • astro-ph.HE2
  • astro-ph1
same name
  • C. Williams — 55 papers, h 35
  • C. Williams — 32 papers, h 35
  • C. Williams — 22 papers, h 3
  • C. Williams — 13 papers, h 10
  • C. Williams — 10 papers, h 8
  • C. Williams — 9 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
20042026
most citedNear-Infrared Photometry and Spectroscopy of L and T Dwarfs: the Effects of Temperature, Clouds, and Gravity

543 citations · 8.3k across the 210 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.CO2013★ 132 cited

The Progenitors of the Compact Early-Type Galaxies at High-Redshift

Christina C. Williams, Mauro Giavalisco, Paolo Cassata +19

We use GOODS and CANDELS images to identify progenitors of massive (log M > 10 Msun) compact "early-type" galaxies (ETGs) at z~1.6. Since merging and accretion increase the size of…

astro-ph.GA2013★ 82 cited

CANDELS: The correlation between galaxy morphology and star formation activity at z~2

Bomee Lee, Mauro Giavalisco, Christina C. Williams +13

We discuss the state of the assembly of the Hubble Sequence in the mix of bright galaxies at redshift 1.4< z \le 2.5 with a large sample of 1,671 galaxies down to H_{AB}~26, select…

astro-ph.GA2013★ 27 cited

X-ray Detections of Sub-millimetre Galaxies: Active Galactic Nuclei Versus Starburst Contribution

Seth P. Johnson, Grant W. Wilson, Danial Q. Wang +14

We present a large-scale study of the X-ray properties and near-IR-to-radio SEDs of submillimetre galaxies (SMGs) detected at 1.1mm with the AzTEC instrument across a ~1.2 square d…

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