Mauro Stefanon

9.6k total citations · 3 hit papers
69 papers, 3.0k citations indexed

About

Mauro Stefanon is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, Mauro Stefanon has authored 69 papers receiving a total of 3.0k indexed citations (citations by other indexed papers that have themselves been cited), including 67 papers in Astronomy and Astrophysics, 48 papers in Instrumentation and 4 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in Mauro Stefanon's work include Galaxies: Formation, Evolution, Phenomena (61 papers), Astronomy and Astrophysical Research (48 papers) and Gamma-ray bursts and supernovae (30 papers). Mauro Stefanon is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (61 papers), Astronomy and Astrophysical Research (48 papers) and Gamma-ray bursts and supernovae (30 papers). Mauro Stefanon collaborates with scholars based in United States, Netherlands and Denmark. Mauro Stefanon's co-authors include Ivo Labbé, Pascal A. Oesch, G. D. Illingworth, Pieter van Dokkum, R. J. Bouwens, Danilo Marchesini, Gabriel Brammer, Adam Muzzin, Marijn Franx and B. Milvang‐Jensen and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Mauro Stefanon

66 papers receiving 2.7k citations

Hit Papers

THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMI... 2013 2026 2017 2021 2013 2023 2023 100 200 300 400 500
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.

  1. THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMING AND QUIESCENT GALAXIES TOz= 4 FROM THE COSMOS/UltraVISTA SURVEY
    2013 522 citations Adam Muzzin, Danilo Marchesini et al. The Astrophysical Journal profile →
  2. A population of red candidate massive galaxies ~600 Myr after the Big Bang
    2023 281 citations Ivo Labbé, Pieter van Dokkum et al. Nature profile →
  3. Evolution of the UV LF from z ∼ 15 to z ∼ 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
    2023 86 citations R. J. Bouwens, Mauro Stefanon et al. Monthly Notices of the Royal Astronomical Society profile →

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Mauro Stefanon United States 29 2.9k 1.8k 385 124 87 69 3.0k
D. Magee United States 30 3.2k 1.1× 1.9k 1.1× 417 1.1× 153 1.2× 120 1.4× 47 3.2k
Eric Gawiser United States 33 3.0k 1.0× 1.2k 0.7× 572 1.5× 97 0.8× 112 1.3× 90 3.1k
R. A. A. Bowler United Kingdom 28 2.8k 1.0× 1.5k 0.8× 395 1.0× 147 1.2× 136 1.6× 54 2.9k
Michele Cirasuolo United Kingdom 23 2.2k 0.8× 1.2k 0.7× 318 0.8× 95 0.8× 118 1.4× 34 2.2k
Ivelina Momcheva United States 24 2.4k 0.8× 1.4k 0.8× 237 0.6× 115 0.9× 76 0.9× 53 2.5k
M. Pannella Germany 29 2.7k 0.9× 1.5k 0.8× 374 1.0× 77 0.6× 47 0.5× 60 2.7k
Fabio Fontanot Italy 30 2.6k 0.9× 1.6k 0.9× 294 0.8× 57 0.5× 77 0.9× 86 2.6k
Kristian Finlator United States 28 2.8k 1.0× 1.3k 0.7× 458 1.2× 68 0.5× 90 1.0× 54 2.9k
K. I. Caputi Netherlands 27 2.1k 0.7× 1.1k 0.6× 304 0.8× 118 1.0× 80 0.9× 61 2.2k
N. Arimoto Japan 35 3.5k 1.2× 1.9k 1.1× 324 0.8× 149 1.2× 61 0.7× 119 3.6k

Countries citing papers authored by Mauro Stefanon

Since Specialization
Citations

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

Fields of papers citing papers by Mauro Stefanon

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Mauro Stefanon. 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 Mauro Stefanon. The network helps show where Mauro Stefanon may publish in the future.

Co-authorship network of co-authors of Mauro Stefanon

This figure shows the co-authorship network connecting the top 25 collaborators of Mauro Stefanon. A scholar is included among the top collaborators of Mauro Stefanon 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 Mauro Stefanon. Mauro Stefanon 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
1.
Gottumukkala, Rashmi, Laia Barrufet, Pascal A. Oesch, et al.. (2024). Unveiling the hidden Universe with JWST: the contribution of dust-obscured galaxies to the stellar mass function at z ~ 3 – 8. Monthly Notices of the Royal Astronomical Society. 530(1). 966–983. 11 indexed citations
2.
Palla, Marco, Ilse De Looze, M. Relaño, et al.. (2024). Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations. Monthly Notices of the Royal Astronomical Society. 528(2). 2407–2427. 6 indexed citations
3.
Labbé, Ivo, Pieter van Dokkum, Erica J. Nelson, et al.. (2023). A population of red candidate massive galaxies ~600 Myr after the Big Bang. Nature. 616(7956). 266–269. 281 indexed citations breakdown →
4.
Bouwens, R. J., Mauro Stefanon, Gabriel Brammer, et al.. (2023). Evolution of the UV LF from z ∼ 15 to z ∼ 8 using new JWST NIRCam medium-band observations over the HUDF/XDF. Monthly Notices of the Royal Astronomical Society. 523(1). 1036–1055. 86 indexed citations breakdown →
5.
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
6.
Algera, Hiddo, Hanae Inami, Laura Sommovigo, et al.. (2023). Cold dust and low [O iii]/[C ii] ratios: an evolved star-forming population at redshift 7. Monthly Notices of the Royal Astronomical Society. 527(3). 6867–6887. 20 indexed citations
7.
González, Valentino, Mauro Stefanon, Pascal A. Oesch, et al.. (2023). The Hα Luminosity Function of Galaxies at z ∼ 4.5 . The Astrophysical Journal. 946(2). 117–117. 2 indexed citations
8.
Barrufet, Laia, Pascal A. Oesch, Andrea Weibel, et al.. (2023). Unveiling the nature of infrared bright, optically dark galaxies with early JWST data. Monthly Notices of the Royal Astronomical Society. 522(1). 449–456. 41 indexed citations
9.
Schouws, Sander, Mauro Stefanon, R. J. Bouwens, et al.. (2022). Significant Dust-obscured Star Formation in Luminous Lyman-break Galaxies at z ∼ 7–8. The Astrophysical Journal. 928(1). 31–31. 33 indexed citations
10.
Witstok, Joris, Renske Smit, R. Maiolino, et al.. (2022). Dual constraints with ALMA: new [O iii] 88-μm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z ∼ 7. Monthly Notices of the Royal Astronomical Society. 515(2). 1751–1773. 41 indexed citations
11.
Bouwens, R. J., Pascal A. Oesch, Mauro Stefanon, et al.. (2021). New determinations of the UV luminosity functions from z ~ 9 to 2 show a remarkable consistency with halo growth and a constant star formation efficiency. Figshare. 5 indexed citations
12.
Forrest, Ben, Marianna Annunziatella, Gillian Wilson, et al.. (2020). An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models*. The Astrophysical Journal Letters. 890(1). L1–L1. 57 indexed citations
13.
Matthee, Jorryt, David Sobral, Max Grönke, et al.. (2018). Confirmation of double peaked Lyα emission at z = 6.593. Astronomy and Astrophysics. 619. A136–A136. 58 indexed citations
14.
Kado-Fong, Erin, Danilo Marchesini, Z. Cemile Marsan, et al.. (2017). Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7. OakTrust (Texas A&M University Libraries). 5 indexed citations
15.
Ellis, Richard S., et al.. (2017). The z ~ 6 Luminosity Function Fainter than −15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties. UCL Discovery (University College London). 164 indexed citations
16.
Stefanon, Mauro, R. J. Bouwens, Ivo Labbé, et al.. (2017). The Rest-frame Optical (900 nm) Galaxy Luminosity Function at z ~ 4-7: Abundance Matching Points to Limited Evolution in the M_STAR/M_HALO Ratio at z >= 4. Leiden Repository (Leiden University). 42 indexed citations
17.
Muzzin, Adam, Marijn Franx, C. Schreiber, et al.. (2017). The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5. The Astrophysical Journal. 837(2). 147–147. 37 indexed citations
18.
Roberts-Borsani, Guido, R. J. Bouwens, Pascal A. Oesch, et al.. (2016). z? 7 galazies with red spitzer/IRAC [3.6]–[4.5] colors in the full CANDELS data set: the brightest-known galaxies at z~ 7–9 and a probable spectroscopic confirmation atz= 7.48. Figshare. 140 indexed citations
19.
Bouwens, R. J., Pascal A. Oesch, Ivo Labbé, et al.. (2016). THE BRIGHT END OF THE z ∼ 9 AND z ∼ 10 UV LUMINOSITY FUNCTIONS USING ALL FIVE CANDELS FIELDS∗. The Astrophysical Journal. 830(2). 67–67. 81 indexed citations
20.
Vulcani, Benedetta, Danilo Marchesini, G. De Lucia, et al.. (2016). MERGERS AND STAR FORMATION: THE ENVIRONMENT AND STELLAR MASS GROWTH OF THE PROGENITORS OF ULTRA-MASSIVE GALAXIES SINCE Z = 2. The Astrophysical Journal. 816(2). 86–86. 23 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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