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researcher

T. Hamilton

18 papers hereh-index 12826 citations47 works total

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

author position
  • sole author1
  • first author3
  • middle author10

Across the 14 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA8
  • astro-ph4
  • astro-ph.CO4
  • astro-ph.HE2
same name
  • T. Hamilton — 15 papers, h 24
  • T. Hamilton — 2 papers, h 35
  • T. Hamilton — 2 papers, h 14
  • T. Hamilton — 1 paper, h 4
  • T. Hamilton — 1 paper, h 6
  • T. Hamilton — 1 paper, h 3

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
20002022
most citedA Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

350 citations · 1.2k across the 18 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.CO2014★ 12 cited

Thirty-six New, High-Probability, Damped Ly-alpha Absorbers at Redshift 0.42 < z < 0.70

David A. Turnshek, Eric M. Monier, Sandhya M. Rao +3

Quasar damped Ly-alpha (DLA) absorption line systems with redshifts z<1.65 are used to trace neutral gas over approximately 70 per cent of the most recent history of the Universe.…

astro-ph.GA2014★ 50 cited

SDSSJ143244.91+301435.3: a link between radio-loud narrow-line Seyfert 1 galaxies and compact steep-spectrum radio sources?

A. Caccianiga, S. Antón, L. Ballo +12

We present SDSSJ143244.91+301435.3, a new case of radio-loud narrow line Seyfert 1 (RL NLS1) with a relatively high radio power (P1.4GHz=2.1x10^25 W Hz^-1) and large radioloudness…

astro-ph.GA2014★ 172 cited

Morphologies of z~0.7 AGN Host Galaxies in CANDELS: No trend of merger incidence with AGN luminosity

C. Villforth, F. Hamann, D. J. Rosario +24

The processes that trigger Active Galactic Nuclei (AGN) remain poorly understood. While lower luminosity AGN may be triggered by minor disturbances to the host galaxy, stronger dis…

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