◍wovepaper
SearchResearchersInstitutions
Sign in
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 2018Show all

3 papers · 1 filter

astro-ph.GA2018★ 222 cited

MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II - Star Formation Histories and Galaxy Quenching

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

We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5 < z < 2.5 using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates…

astro-ph.GA2018★ 92 cited

Resolving Quiescent Galaxies at z≳2: II. Direct Measures of Rotational Support

Andrew B. Newman, Sirio Belli, Richard S. Ellis +1

Stellar kinematics provide insights into the masses and formation histories of galaxies. At high redshifts, spatially resolving the stellar kinematics of quiescent galaxies is chal…

astro-ph.GA2018★ 62 cited

Resolving Quiescent Galaxies at z≳2: I. Search for Gravitationally Lensed Sources and Characterization of their Structure, Stellar Populations, and Line Emission

Andrew B. Newman, Sirio Belli, Richard S. Ellis +1

Quiescent galaxies at z≳2 are compact and have weak or absent emission lines, making it difficult to spatially resolve their kinematics and stellar populations using grou…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.