A. Cibinel

1.9k total citations
19 papers, 842 citations indexed

About

A. Cibinel is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, A. Cibinel has authored 19 papers receiving a total of 842 indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 13 papers in Instrumentation and 4 papers in Nuclear and High Energy Physics. Recurrent topics in A. Cibinel's work include Galaxies: Formation, Evolution, Phenomena (18 papers), Astronomy and Astrophysical Research (13 papers) and Astrophysics and Star Formation Studies (5 papers). A. Cibinel is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (18 papers), Astronomy and Astrophysical Research (13 papers) and Astrophysics and Star Formation Studies (5 papers). A. Cibinel collaborates with scholars based in Switzerland, United Kingdom and United States. A. Cibinel's co-authors include C. M. Carollo, Masato Onodera, S. J. Lilly, Ewan Cameron, F. Bournaud, E. Daddi, Pascal A. Oesch, A. Renzini, R. Gobat and B. Holden and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

A. Cibinel

19 papers receiving 808 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. Cibinel Switzerland 16 830 467 74 37 29 19 842
J. C. Muñoz-Mateos Spain 9 963 1.2× 546 1.2× 64 0.9× 34 0.9× 25 0.9× 11 978
Caroline M. S. Straatman United States 17 852 1.0× 551 1.2× 74 1.0× 23 0.6× 23 0.8× 39 866
A. Cimatti Italy 5 923 1.1× 523 1.1× 100 1.4× 24 0.6× 21 0.7× 5 949
Silvia Fabello United States 9 820 1.0× 404 0.9× 85 1.1× 21 0.6× 22 0.8× 10 834
R. Gobat France 19 1.0k 1.2× 588 1.3× 107 1.4× 28 0.8× 19 0.7× 32 1.0k
Mattia Fumagalli Netherlands 10 891 1.1× 519 1.1× 72 1.0× 25 0.7× 22 0.8× 12 904
Ivo Labbé United States 8 775 0.9× 466 1.0× 71 1.0× 18 0.5× 20 0.7× 10 798
David V. Stark United States 17 681 0.8× 370 0.8× 55 0.7× 21 0.6× 21 0.7× 42 714
G. Bergond Spain 17 727 0.9× 408 0.9× 91 1.2× 48 1.3× 19 0.7× 24 739
É. Giovannoli France 6 725 0.9× 360 0.8× 53 0.7× 37 1.0× 30 1.0× 10 741

Countries citing papers authored by A. Cibinel

Since Specialization
Citations

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

Fields of papers citing papers by A. Cibinel

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. Cibinel

This figure shows the co-authorship network connecting the top 25 collaborators of A. Cibinel. A scholar is included among the top collaborators of A. Cibinel 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 A. Cibinel. A. Cibinel is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

19 of 19 papers shown
1.
Coogan, R. T., M. Sargent, A. Cibinel, et al.. (2023). Looking ahead to the sky with the Square Kilometre Array: simulating flux densities and resolved radio morphologies of 0 < z < 2.5 star-forming galaxies. Monthly Notices of the Royal Astronomical Society. 525(3). 3413–3438. 1 indexed citations
2.
Cibinel, A., E. Daddi, M. Sargent, et al.. (2019). Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 ≤ z ≤ 2. Monthly Notices of the Royal Astronomical Society. 485(4). 5631–5651. 43 indexed citations
3.
Zanella, Anita, E. Le Floc’h, C. M. Harrison, et al.. (2019). A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies. Monthly Notices of the Royal Astronomical Society. 489(2). 2792–2818. 47 indexed citations
4.
Erroz-Ferrer, Santiago, C. M. Carollo, Mark den Brok, et al.. (2019). The MUSE Atlas of Disks (MAD): resolving star formation rates and gas metallicities on <100 pc scales†. Monthly Notices of the Royal Astronomical Society. 484(4). 5009–5027. 70 indexed citations
5.
Morselli, L., P. Popesso, A. Cibinel, et al.. (2019). Spatial distribution of stellar mass and star formation activity at 0.2 < z < 1.2 across and along the main sequence. Astronomy and Astrophysics. 626. A61–A61. 23 indexed citations
6.
Reddy, Naveen A., Pascal A. Oesch, R. J. Bouwens, et al.. (2018). The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies. The Astrophysical Journal. 853(1). 56–56. 125 indexed citations
7.
Oesch, Pascal A., Mireia Montes, Naveen A. Reddy, et al.. (2018). HDUV: The Hubble Deep UV Legacy Survey. Figshare. 16 indexed citations
8.
Naidu, Rohan P., Pascal A. Oesch, Naveen A. Reddy, et al.. (2017). The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ∼ 2 Revealed by HST UV Imaging*. The Astrophysical Journal. 847(1). 12–12. 26 indexed citations
9.
Tacchella, Sandro, C. M. Carollo, S. M. Faber, et al.. (2017). On the Evolution of the Central Density of Quiescent Galaxies. The Astrophysical Journal Letters. 844(1). L1–L1. 19 indexed citations
10.
Cibinel, A., E. Daddi, F. Bournaud, et al.. (2017). ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5−4) emission from UV-bright clumps. Monthly Notices of the Royal Astronomical Society. 469(4). 4683–4704. 16 indexed citations
11.
Carollo, C. M., A. Cibinel, S. J. Lilly, et al.. (2016). ZENS. IV. Similar morphological changes associated with mass quenching and environment quenching and the relative importance of bulge growth versus the fading of disks. Figshare. 16 indexed citations
12.
Daddi, E., H. Dannerbauer, Daizhong Liu, et al.. (2015). CO excitation of normal star-forming galaxies out toz= 1.5 as regulated by the properties of their interstellar medium. Astronomy and Astrophysics. 577. A46–A46. 143 indexed citations
13.
Zanella, Anita, E. Daddi, E. Le Floc’h, et al.. (2015). An extremely young massive clump forming by gravitational collapse in a primordial galaxy. Nature. 521(7550). 54–56. 45 indexed citations
14.
Silverman, J. D., Francesco Miniati, A. Finoguenov, et al.. (2014). The X-Ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton observations of active galactic nuclei in galaxies in nearby groups. Figshare. 4 indexed citations
15.
Pipino, A., A. Cibinel, Sandro Tacchella, et al.. (2014). THE ZURICH ENVIRONMENTAL STUDY (ZENS) OF GALAXIES IN GROUPS ALONG THE COSMIC WEB. V. PROPERTIES AND FREQUENCY OF MERGING SATELLITES AND CENTRALS IN DIFFERENT ENVIRONMENTS. The Astrophysical Journal. 797(2). 127–127. 9 indexed citations
17.
Carollo, C. M., A. Renzini, S. J. Lilly, et al.. (2013). NEWLY QUENCHED GALAXIES AS THE CAUSE FOR THE APPARENT EVOLUTION IN AVERAGE SIZE OF THE POPULATION. The Astrophysical Journal. 773(2). 112–112. 154 indexed citations
19.
Carollo, C. M., A. Cibinel, S. J. Lilly, et al.. (2013). THE ZURICH ENVIRONMENTAL STUDY OF GALAXIES IN GROUPS ALONG THE COSMIC WEB. I. WHICH ENVIRONMENT AFFECTS GALAXY EVOLUTION?. The Astrophysical Journal. 776(2). 71–71. 39 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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