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researcher

M. Girard

3 papers hereh-index 4160 citations11 works total

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

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
same name
  • M. Girard — 44 papers, h 70
  • M. Girard — 41 papers, h 56
  • M. Girard — 25 papers
  • M. Girard — 15 papers, h 43
  • M. Girard — 8 papers, h 9
  • M. Girard — 3 papers, h 1

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

most citedThe DUVET Survey: Resolved Maps of Star Formation Driven Outflows in a Compact, Starbursting Disk Galaxy

36 citations · 55 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2022★ 12 cited

Stellar Masses of Clumps in Gas-rich, Turbulent Disk Galaxies

Liyualem Ambachew, Deanne B. Fisher, Karl Glazebrook +6

In this paper we use HST/WFC3 observations of 6 galaxies from the DYNAMO survey, combined with stellar population modelling of the SED, to determine the stellar masses of DYNAMO cl…

astro-ph.GA2022★ 36 cited

The DUVET Survey: Resolved Maps of Star Formation Driven Outflows in a Compact, Starbursting Disk Galaxy

Bronwyn Reichardt Chu, Deanne B. Fisher, Nikole M. Nielsen +9

We study star formation driven outflows in a z∼0.02 starbursting disk galaxy, IRAS08339+6517, using spatially resolved measurements from the Keck Cosmic Web Imager (KCWI). We…

astro-ph.GA2020★ 7 cited

The KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics and clumpiness of low-mass galaxies at cosmic noon

M. Girard, C. A. Mason, A. Fontana +9

We present results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS), an ESO Very Large Telescope (VLT) large program using gravitational lensing to study the spatially res…

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