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researcher

A. Newman

38 papers hereh-index 282.7k citations58 works total

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

author position
  • first author14
  • middle author22
  • last author1

Across the 37 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph.CO15
  • astro-ph.HE1
same name
  • A. Newman — 20 papers, h 7
  • A. Newman — 5 papers, h 4
  • A. Newman — 4 papers, h 3
  • A. Newman — 2 papers, h 4
  • A. Newman — 2 papers, h 1
  • A. Newman — 2 papers, h 2

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
20092024
most citedCan Minor Merging Account for the Size Growth of Quiescent Galaxies? New Results from the CANDELS Survey

459 citations · 3.6k across the 37 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 65 cited

The Initial Mass Function in the Nearest Strong Lenses from SNELLS: Assessing the Consistency of Lensing, Dynamical, and Spectroscopic Constraints

Andrew B. Newman, Russell J. Smith, Charlie Conroy +2

We present new observations of the three nearest early-type galaxy (ETG) strong lenses discovered in the SINFONI Nearby Elliptical Lens Locator Survey (SNELLS). Based on their lens…

astro-ph.GA2016★ 125 cited

Evidence for a Hard Ionizing Spectrum from a z=6.11 Stellar Population

Ramesh Mainali, Juna A. Kollmeier, Daniel P. Stark +4

We present the Magellan/FIRE detection of highly-ionized CIV 1550 and OIII] 1666 in a deep infrared spectrum of the z=6.11 gravitationally lensed low-mass galaxy RXC J2248.7-4431-I…

astro-ph.GA2016★ 102 cited

MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I - Evolution of Structural and Dynamical Properties

Sirio Belli, Andrew B. Newman, Richard S. Ellis

We present deep near-infrared spectra for a sample of 24 quiescent galaxies in the redshift range 1.5 < z < 2.5 obtained with the MOSFIRE spectrograph at the W. M. Keck Observatory…

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