M. Figueira

417 total citations
20 papers, 195 citations indexed

About

M. Figueira is a scholar working on Astronomy and Astrophysics, Spectroscopy and Statistical and Nonlinear Physics. According to data from OpenAlex, M. Figueira has authored 20 papers receiving a total of 195 indexed citations (citations by other indexed papers that have themselves been cited), including 18 papers in Astronomy and Astrophysics, 7 papers in Spectroscopy and 2 papers in Statistical and Nonlinear Physics. Recurrent topics in M. Figueira's work include Astrophysics and Star Formation Studies (13 papers), Stellar, planetary, and galactic studies (13 papers) and Galaxies: Formation, Evolution, Phenomena (6 papers). M. Figueira is often cited by papers focused on Astrophysics and Star Formation Studies (13 papers), Stellar, planetary, and galactic studies (13 papers) and Galaxies: Formation, Evolution, Phenomena (6 papers). M. Figueira collaborates with scholars based in France, Poland and Italy. M. Figueira's co-authors include A. Zavagno, D. Russeil, N. Schneider, A. Men’shchikov, D. Vergani, K. Małek, A. Pollo, L. Bronfman, F. Louvet and T. Hill and has published in prestigious journals such as SHILAP Revista de lepidopterología, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

M. Figueira

19 papers receiving 177 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
M. Figueira France	9	186	33	25	17	14	20	195
Drew Brisbin United States	8	196 1.1×	18 0.5×	43 1.7×	10 0.6×	5 0.4×	14	202
Sarah Jeffreson United States	10	268 1.4×	17 0.5×	37 1.5×	15 0.9×	13 0.9×	16	275
Th. Henning Germany	9	175 0.9×	32 1.0×	19 0.8×	22 1.3×	24 1.7×	10	187
Christopher M. Faesi United States	6	169 0.9×	20 0.6×	26 1.0×	9 0.5×	6 0.4×	9	173
Ana-Maria Piso United States	3	256 1.4×	29 0.9×	15 0.6×	17 1.0×	7 0.5×	3	264
B. Ocaña Flaquer Spain	5	230 1.2×	38 1.2×	38 1.5×	24 1.4×	13 0.9×	9	249
Sarah Jaffa United Kingdom	7	189 1.0×	53 1.6×	9 0.4×	35 2.1×	8 0.6×	12	203
Chakali Eswaraiah India	12	293 1.6×	28 0.8×	50 2.0×	21 1.2×	4 0.3×	30	302
Nalin Vutisalchavakul United States	5	272 1.5×	39 1.2×	33 1.3×	20 1.2×	4 0.3×	5	273
P. Didelon France	7	138 0.7×	23 0.7×	21 0.8×	24 1.4×	13 0.9×	13	149

Countries citing papers authored by M. Figueira

Since Specialization

Citations

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

Fields of papers citing papers by M. Figueira

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Figueira

This figure shows the co-authorship network connecting the top 25 collaborators of M. Figueira. A scholar is included among the top collaborators of M. Figueira 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 M. Figueira. M. Figueira 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

Karska, A., M. Figueira, Christian Fischer, et al.. (2025). SOFIA FIFI-LS spectroscopy of DR21 Main: Energetics of the spatially resolved outflow from a high-mass protostar. Astronomy and Astrophysics. 697. A186–A186.

Figueira, M., M. Siudek, A. Pollo, et al.. (2024). The quiescent population at 0.5 ≤ z ≤ 0.9: Environmental impact on the mass–size relation. Astronomy and Astrophysics. 687. A117–A117. 4 indexed citations

Pollo, A., M. Figueira, D. Vergani, et al.. (2024). A comparative study of the fundamental metallicity relation. Astronomy and Astrophysics. 683. A203–A203. 8 indexed citations

Balogh, Michael L., Katherine Alatalo, Asa F. L. Bluck, et al.. (2024). RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution. SHILAP Revista de lepidopterología. 7. 4 indexed citations

Pearson, William, M. Figueira, K. Małek, et al.. (2023). Influence of star-forming galaxy selection on the galaxy main sequence. Astronomy and Astrophysics. 679. A35–A35. 4 indexed citations

Urquhart, J. S., C. König, Dario Colombo, et al.. (2023). OGHReS: star formation in the outer galaxy (ℓ = 250°–280°). Monthly Notices of the Royal Astronomical Society. 528(3). 4746–4759. 6 indexed citations

Figueira, M., K. Małek, A. Nanni, et al.. (2023). Decoding the IRX–β dust attenuation relation in star-forming galaxies at intermediate redshift. Astronomy and Astrophysics. 679. A26–A26. 3 indexed citations

Figueira, M., A. Pollo, K. Małek, et al.. (2022). SFR estimations from z = 0 to z = 0.9. Astronomy and Astrophysics. 667. A29–A29. 15 indexed citations

Pollo, A., M. Scodeggio, M. Figueira, et al.. (2022). The fundamental metallicity relation from SDSS (z ∼ 0) to VIPERS (z ∼ 0.7). Astronomy and Astrophysics. 663. A162–A162. 8 indexed citations

10.

Figueira, M. & Nuno Horta. (2022). Machine Learning-Based Pairs Trading Strategy with Multivariate. SSRN Electronic Journal. 1 indexed citations

11.

Karska, A., Marcin Gronowski, L. E. Kristensen, et al.. (2021). Signatures of UV radiation in low-mass protostars. Astronomy and Astrophysics. 656. A146–A146. 6 indexed citations

12.

Figueira, M., A. Zavagno, L. Bronfman, et al.. (2020). APEX CO observations towards the photodissociation region of RCW 120. Springer Link (Chiba Institute of Technology). 8 indexed citations

13.

Russeil, D., et al.. (2020). OB stars and YSO populations in the region of NGC 6334–NGC 6357 as seen withGaiaDR2. Astronomy and Astrophysics. 642. A21–A21. 4 indexed citations

14.

Zhang, Siju, A. Zavagno, A. López-Sepulcre, et al.. (2020). H II regions and high-mass starless clump candidates. Astronomy and Astrophysics. 646. A25–A25. 19 indexed citations

15.

Zavagno, A., Ph. André, F. Schüller, et al.. (2020). The role of Galactic H II regions in the formation of filaments. Astronomy and Astrophysics. 638. A7–A7. 22 indexed citations

16.

Figueira, M., et al.. (2019). Multiwavelength study of the G345.5+1.5 region. Springer Link (Chiba Institute of Technology). 4 indexed citations

17.

Figueira, M., L. Bronfman, A. Zavagno, et al.. (2018). ALMA observations of RCW 120 Fragmentation at 0.01 pc scale. Astronomy and Astrophysics. 616. L10–L10. 14 indexed citations

18.

Liu, Hongli, M. Figueira, A. Zavagno, et al.. (2017). Herschelobservations of the Galactic H ii region RCW 79. Astronomy and Astrophysics. 602. A95–A95. 17 indexed citations

19.

Figueira, M., A. Zavagno, L. Deharveng, et al.. (2017). Star formation towards the Galactic H II region RCW 120 Herschel observations of compact sources. Kölner Universitäts PublikationsServer (Universität zu Köln). 19 indexed citations

20.

Figueira, M., A. Zavagno, L. Deharveng, et al.. (2017). Star formation towards the Galactic H II region RCW 120. Astronomy and Astrophysics. 600. A93–A93. 29 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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