◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

G. Martin

30 papers hereh-index 18983 citations40 works total

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

author position
  • first author7
  • middle author20
  • last author2

Across the 29 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA28
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • G. Martin — 62 papers, h 17
  • G. Martin — 40 papers, h 31
  • G. Martin — 30 papers, h 20
  • G. Martin — 25 papers, h 22
  • G. Martin — 21 papers, h 15
  • G. Martin — 18 papers, h 9

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
20172023
most citedIntroducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time

229 citations · 1.5k across the 30 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 61 cited

Introducing the LBT Imaging of Galactic Halos and Tidal Structures (LIGHTS) survey. A preview of the low surface brightness Universe to be unveiled by LSST

Ignacio Trujillo, Mauro D'Onofrio, Dennis Zaritsky +10

We present the first results of the LBT Imaging of Galaxy Haloes and Tidal Structures (LIGHTS) survey. LIGHTS is an ongoing observational campaign with the 2x8.4m Large Binocular T…

astro-ph.GA2021★ 4 cited

The Star Formation Rates of Elliptical Galaxies from Core-Collapse Supernovae

Thomas M. Sedgwick, Ivan K. Baldry, Philip A. James +2

The level of star formation in elliptical galaxies is poorly constrained, due to difficulties in quantifying the contamination of flux-based estimates of star formation from unrela…

astro-ph.GA2021★ 1 cited

The NewHorizon Simulation -- To Bar Or Not To Bar

J. Reddish, K. Kraljic, M. S. Petersen +12

We use the NewHorizon simulation to study the redshift evolution of bar properties and fractions within galaxies in the stellar masses range $M_{\star} = 10^{7.25} - 10^{11.4} \ \r…

◍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.