Michael V. Maseda

80 papers receiving 1.6k citations

Hit Papers

Metal-poor star formation at z > 6 with JWST: new insi...202420262025202420242025204060

Peers

Michael V. Maseda
Comparison fields: 5 of 49
  • Astronomy and Astrophysics 1.7k
  • Instrumentation 790
  • Nuclear and High Energy Physics 262
  • Atomic and Molecular Physics, and Optics 75
  • Electrical and Electronic Engineering 75
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Hanae Inami United States
Gergö Popping Germany
Jacopo Chevallard France
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Citations per year

Countries citing papers authored by Michael V. Maseda

Since Specialization
Citations

This map shows the geographic impact of Michael V. Maseda'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 Michael V. Maseda with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Michael V. Maseda more than expected).

Fields of papers citing papers by Michael V. Maseda

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Michael V. Maseda. 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 Michael V. Maseda. The network helps show where Michael V. Maseda may publish in the future.

Co-authorship network of co-authors of Michael V. Maseda

This figure shows the co-authorship network connecting the top 25 collaborators of Michael V. Maseda. A scholar is included among the top collaborators of Michael V. Maseda based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Michael V. Maseda. Michael V. Maseda is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
#WorkIndexed citations
1 1
2 4
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Deep Rest-UV JWST/NIRSpec Spectroscopy of Early Galaxies: The Demographics of C iv and N-emitters in the Reionization Erabreakdown →
22
4 0
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Metal-poor star formation at z > 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scalesbreakdown →
72
6 4
7 2
8 7
9 3
10 8
11 7
12 18
13 21
14 9
15 12
16 43
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Dust Attenuation Curves at z ~ 0.8 from LEGA-C : Precise Constraints on the Slope and 2175Å Bump Strength
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18 58
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Rejuvenation in z ∼ 0.8 Quiescent Galaxies in LEGA-C
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20 52

About Michael V. Maseda

Michael V. Maseda is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 84 papers that have together received 1.8k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (74 papers), Astronomy and Astrophysical Research (46 papers) and Stellar, planetary, and galactic studies (33 papers). The work is most often cited by research in Instrumentation (790 citations), Astronomy and Astrophysics (1.7k citations) and Nuclear and High Energy Physics (262 citations). Michael V. Maseda has collaborated with scholars based in Netherlands, Germany and United States. Frequent co-authors include L. Wisotzki, J. Brinchmann, Johan Richard, Joop Schaye, R. A. Marino, Roland Bacon, T. Contini, Marijn Franx, Anne Verhamme and Arjen van der Wel. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

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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