Michael V. Maseda

12.2k total citations · 3 hit papers
84 papers, 1.8k citations indexed

About

Michael V. Maseda is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, Michael V. Maseda has authored 84 papers receiving a total of 1.8k indexed citations (citations by other indexed papers that have themselves been cited), including 79 papers in Astronomy and Astrophysics, 46 papers in Instrumentation and 11 papers in Nuclear and High Energy Physics. Recurrent topics in Michael V. Maseda's work include Galaxies: Formation, Evolution, Phenomena (74 papers), Astronomy and Astrophysical Research (46 papers) and Stellar, planetary, and galactic studies (33 papers). Michael V. Maseda is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (74 papers), Astronomy and Astrophysical Research (46 papers) and Stellar, planetary, and galactic studies (33 papers). Michael V. Maseda collaborates with scholars based in Netherlands, Germany and United States. Michael V. Maseda's 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 and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

Michael V. Maseda

80 papers receiving 1.6k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Metal-poor star formation at z > 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales

2024 72 citations Michael W. Topping, Daniel P. Stark et al. Monthly Notices of the Royal Astronomical Society profile →
The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus

2024 50 citations Pieter van Dokkum, Gabriel Brammer et al. profile →
Deep Rest-UV JWST/NIRSpec Spectroscopy of Early Galaxies: The Demographics of C iv and N-emitters in the Reionization Era

2025 22 citations Michael W. Topping, Dan Stark et al. The Astrophysical Journal profile →

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
Michael V. Maseda Netherlands	25	1.7k	790	262	75	75	84	1.8k
Hanae Inami United States	25	1.5k 0.9×	671 0.8×	272 1.0×	81 1.1×	70 0.9×	55	1.6k
Jacopo Chevallard France	24	2.0k 1.2×	953 1.2×	187 0.7×	79 1.1×	96 1.3×	52	2.1k
Renske Smit United Kingdom	23	2.1k 1.3×	990 1.3×	317 1.2×	105 1.4×	86 1.1×	50	2.2k
Takatoshi Shibuya Japan	18	1.5k 0.9×	655 0.8×	287 1.1×	81 1.1×	65 0.9×	36	1.5k
Nimish P. Hathi United States	23	1.8k 1.1×	961 1.2×	197 0.8×	92 1.2×	90 1.2×	72	1.8k
Alaina Henry United States	21	1.7k 1.0×	779 1.0×	229 0.9×	53 0.7×	82 1.1×	59	1.8k
Fuyan Bian United States	25	2.3k 1.4×	698 0.9×	470 1.8×	75 1.0×	79 1.1×	85	2.4k
Fergus Cullen United Kingdom	23	1.7k 1.0×	867 1.1×	165 0.6×	69 0.9×	45 0.6×	62	1.7k
Marc Rafelski United States	25	1.7k 1.0×	613 0.8×	319 1.2×	59 0.8×	39 0.5×	91	1.8k
Göran Östlin Sweden	25	2.1k 1.2×	758 1.0×	300 1.1×	81 1.1×	80 1.1×	99	2.1k

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

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Schindler, Jan–Torge, Joseph F. Hennawi, Frederick B. Davies, et al.. (2025). A little red dot at z = 7.3 within a large galaxy overdensity. Nature Astronomy. 9(11). 1732–1744. 1 indexed citations

Wang, Weichen, Sebastiano Cantalupo, Antonio Pensabene, et al.. (2025). A giant disk galaxy two billion years after the Big Bang. Nature Astronomy. 9(5). 710–719. 4 indexed citations

Topping, Michael W., Dan Stark, Peter Senchyna, et al.. (2025). Deep Rest-UV JWST/NIRSpec Spectroscopy of Early Galaxies: The Demographics of C iv and N-emitters in the Reionization Era. The Astrophysical Journal. 980(2). 225–225. 22 indexed citations breakdown →

Ormerod, Katherine, Joris Witstok, Renske Smit, et al.. (2025). Detection of the 2175 Å UV bump at z > 7: evidence for rapid dust evolution in a merging reionization-era galaxy. Monthly Notices of the Royal Astronomical Society. 542(2). 1136–1154.

Topping, Michael W., Daniel P. Stark, Peter Senchyna, et al.. (2024). Metal-poor star formation at z > 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales. Monthly Notices of the Royal Astronomical Society. 529(4). 3301–3322. 72 indexed citations breakdown →

Verhamme, Anne, Pascale Hibon, Belén Alcalde Pampliega, et al.. (2024). The MUSE eXtremely Deep Field. Astronomy and Astrophysics. 694. A100–A100. 4 indexed citations

Kusakabe, Haruka, Valentin Mauerhofer, Anne Verhamme, et al.. (2024). The MUSE eXtremely Deep Field: Detections of circumgalactic Si II* emission at z ≳ 2. Astronomy and Astrophysics. 691. A255–A255. 2 indexed citations

Wu, Po-Feng, Rachel Bezanson, Francesco D’Eugenio, et al.. (2023). Stars, Gas, and Star Formation of Distant Post-starburst Galaxies. The Astrophysical Journal. 955(1). 75–75. 7 indexed citations

Monreal‐Ibero, A., Peter M. Weilbacher, Genoveva Micheva, W. Kollatschny, & Michael V. Maseda. (2023). UM 462, a local green pea galaxy analogue under the MUSE magnifying glass. Astronomy and Astrophysics. 674. A210–A210. 3 indexed citations

10.

Nersesian, Angelos, Arjen van der Wel, Anna Gallazzi, et al.. (2023). Less is less: Photometry alone cannot predict the observed spectral indices of z ~ 1 galaxies from the LEGA-C spectroscopic survey. Astronomy and Astrophysics. 681. A94–A94. 8 indexed citations

11.

Schouws, Sander, R. J. Bouwens, Renske Smit, et al.. (2023). ALMA as a Redshift Machine: Using [C ii] to Efficiently Confirm Galaxies in the Epoch of Reionization. The Astrophysical Journal. 954(1). 103–103. 7 indexed citations

12.

Kusakabe, Haruka, Anne Verhamme, J. Blaizot, et al.. (2022). The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z ≃ 2.9–4.4. Astronomy and Astrophysics. 660. A44–A44. 18 indexed citations

13.

Kerutt, Josephine, L. Wisotzki, Anne Verhamme, et al.. (2022). Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep. Astronomy and Astrophysics. 659. A183–A183. 21 indexed citations

14.

Sobral, David, Arjen van der Wel, Rachel Bezanson, et al.. (2022). The LEGA-C of Nature and Nurture in Stellar Populations at z ∼ 0.6–1.0: D_n4000 and Hδ Reveal Different Assembly Histories for Quiescent Galaxies in Different Environments. The Astrophysical Journal. 926(2). 117–117. 9 indexed citations

15.

Kerutt, Josephine, L. Wisotzki, T. Urrutia, et al.. (2021). Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 <z< 6.4. Astronomy and Astrophysics. 654. A80–A80. 12 indexed citations

16.

Muzahid, Sowgat, Joop Schaye, R. A. Marino, et al.. (2020). MUSEQuBES: calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles. Monthly Notices of the Royal Astronomical Society. 496(2). 1013–1022. 43 indexed citations

17.

Barišić, Ivana, Camilla Pacifici, Arjen van der Wel, et al.. (2020). Dust Attenuation Curves at z ~ 0.8 from LEGA-C : Precise Constraints on the Slope and 2175Å Bump Strength. Lancaster EPrints (Lancaster University). 6 indexed citations

18.

Urrutia, T., L. Wisotzki, Josephine Kerutt, et al.. (2019). The MUSE-Wide Survey: survey description and first data release. Springer Link (Chiba Institute of Technology). 58 indexed citations

19.

Chauké, Priscilla, Arjen van der Wel, Camilla Pacifici, et al.. (2019). Rejuvenation in z ∼ 0.8 Quiescent Galaxies in LEGA-C. Lancaster EPrints (Lancaster University). 39 indexed citations

20.

Herenz, E. C., T. Urrutia, L. Wisotzki, et al.. (2017). The MUSE-Wide survey: A first catalogue of 831 emission line galaxies. Springer Link (Chiba Institute of Technology). 52 indexed citations

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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