D. Magee

9.1k citations
67 papers · 6.6k · 9 hit papers · h-index 42

Impact in

    • Astronomy and Astrophysical Research
    • Galaxies: Formation, Evolution, Phenomena
    • Stellar, planetary, and galactic studies
    • Gamma-ray bursts and supernovae
    • Astrophysics and Star Formation Studies
    • Astrophysical Phenomena and Observations
    • Cosmology and Gravitation Theories

Papers in

    • Astronomy and Astrophysical Research 44
    • Galaxies: Formation, Evolution, Phenomena 58
    • Gamma-ray bursts and supernovae 29
    • Stellar, planetary, and galactic studies 15
    • Astrophysical Phenomena and Observations 7
    • Astrophysics and Star Formation Studies 5

D. Magee

67 papers receiving 5.9k citations

D. Magee's Hit Papers

JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe 2025 · 71 citations
710+6+12Years since publication100200300400

Peers

D. Magee
Comparison fields: 5 of 61
  • Instrumentation 3.5k
  • Astronomy and Astrophysics 6.2k
  • Nuclear and High Energy Physics 813
  • Atomic and Molecular Physics, and Optics 330
  • Statistical and Nonlinear Physics 130
Replace Hanae Inami with:
Hanae Inami United States
Tadayuki Kodama Japan
Mauro Stefanon United States
Brian C. Lemaux United States
Michele Cirasuolo United Kingdom
G. R. Meurer United States
David Sobral United Kingdom
G. W. Wilson United States
N. Arimoto Japan
M. Pannella Germany
D. Magee relative to Hanae Inami United States Hanae Inami's profile →
Citations per field
00.5×1.6×
Hanae Inami · 1×
Citations per year

Countries citing papers authored by D. Magee

Since Specialization
Citations

This map shows the geographic impact of D. Magee's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by D. Magee with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Magee more than expected).

Fields of papers citing papers by D. Magee

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by D. Magee. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by D. Magee. The network helps show where D. Magee may publish in the future.

Co-authors

The 25 scholars most cited alongside D. Magee, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with D. Magee Line = papers co-authored together D. Magee links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown

Showing the 20 most-cited of 67 papers — load more, or switch the sort, to bring in the rest.

#Work
1
Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse
Hit paper breakdown →
2008476
2
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging
Hit paper breakdown →
2022380
3
Two Remarkably Luminous Galaxy Candidates at z ≈ 10–12 Revealed by JWST
Hit paper breakdown →
2022378
4
A REMARKABLY LUMINOUS GALAXY AT Z = 11.1 MEASURED WITH HUBBLE SPACE TELESCOPE GRISM SPECTROSCOPY
Hit paper breakdown →
2016371
5 2012342
6 1999260
7
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 Grism Spectra, Redshifts, and Emission Line Measurements for ~ 100,000 Galaxies
2016229
8 2013228
9 2013201
10 2011193
11
A massive quiescent galaxy at redshift 4.658
Hit paper breakdown →
2023190
12
The JWST FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields
Hit paper breakdown →
2023189
13 2018173
14 2015167
15 2009161
16 2004156
17
The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields
Hit paper breakdown →
2025141
18
JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z ≃ 9 – 15
Hit paper breakdown →
2024132
19 2023124
20 2023118

About D. Magee

D. Magee is a scholar working on Instrumentation, Astronomy and Astrophysics, Nuclear and High Energy Physics, Atomic and Molecular Physics, and Optics and Electrical and Electronic Engineering, having authored 67 papers that have together received 6.6k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (58 papers), Astronomy and Astrophysical Research (44 papers), Gamma-ray bursts and supernovae (29 papers), Stellar, planetary, and galactic studies (15 papers), Astrophysical Phenomena and Observations (7 papers), Adaptive optics and wavefront sensing (7 papers), CCD and CMOS Imaging Sensors (5 papers) and Astrophysics and Star Formation Studies (5 papers). The work is most often cited by research in Instrumentation (3.5k citations), Astronomy and Astrophysics (6.2k citations), Nuclear and High Energy Physics (813 citations), Atomic and Molecular Physics, and Optics (330 citations) and Statistical and Nonlinear Physics (130 citations). D. Magee has collaborated with scholars based in United States, Netherlands and United Kingdom. Frequent co-authors include Garth D. Illingworth, Marijn Franx, Rychard Bouwens, Pieter van Dokkum, Pascal Oesch, Ivo Labbé, Michele Trenti, Valentino González, C. M. Carollo and Bradford P. Holden. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Letters, Nature and Astronomy and Astrophysics.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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