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researcher

E. Bell

19 papers hereh-index 6169 citations21 works total

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

author position
  • first author2
  • middle author16

Across the 18 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA16
  • astro-ph2
  • astro-ph.IM1
same name
  • E. Bell — 326 papers, h 87
  • E. Bell — 22 papers, h 16
  • E. Bell — 7 papers, h 6
  • E. Bell — 2 papers, h 1
  • E. Bell — 1 paper, h 6
  • E. Bell — 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
19982026
most citedTwo Ultra-Faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey

95 citations · 189 across the 18 of their papers we have counts for

collaborators
Showing 2026 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2026

Discovery, Characterization, and Potential Origins of a Stream in the Stellar Halo of Nearby LMC-Mass Galaxy NGC 55

Benjamin N. Velguth, Burçin Mutlu-Pakdil, Erik Tollerud +33

We present a previously undetected stellar stream in the halo of the LMC-mass dwarf galaxy NGC 55 (2 Mpc), as part of an ongoing effort to characterize the stellar halos of LMC/SMC…

astro-ph.GA2026★ 1 cited

The role of mass loss in constraining quenching time in dwarf galaxies from AGB and RGB star counts

Paolo Ventura, Richard D'Souza, Flavia Dell'Agli +4

The capability of reconstructing the past star formation history of dwarf elliptical galaxies out of the Local Volume relies on modelling bright stellar populations currently evolv…

astro-ph.GA2026

A Chemodynamical Census of the Milky Way's Ultra-Faint Compact Satellites. I. A First Population-Level Look at the Internal Kinematics and Metallicities of 19 Extremely-Low-Mass Halo Stellar Systems

William Cerny, Ting S. Li, Andrew B. Pace +13

Deep, wide-area photometric surveys have uncovered a population of compact (r1/2​≈ 1-15 pc), extremely-low-mass (M∗​≈ 20-4000 M⊙​) stellar systems in th…

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