D. M. Faes

598 total citations
27 papers, 357 citations indexed

About

D. M. Faes is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, D. M. Faes has authored 27 papers receiving a total of 357 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 12 papers in Instrumentation and 6 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in D. M. Faes's work include Stellar, planetary, and galactic studies (23 papers), Astrophysics and Star Formation Studies (18 papers) and Astronomy and Astrophysical Research (12 papers). D. M. Faes is often cited by papers focused on Stellar, planetary, and galactic studies (23 papers), Astrophysics and Star Formation Studies (18 papers) and Astronomy and Astrophysical Research (12 papers). D. M. Faes collaborates with scholars based in Brazil, United States and Chile. D. M. Faes's co-authors include Th. Rivinius, A. C. Carciofi, R. G. Vieira, K. S. Bjorkman, D. Baade, D. Panoglou, Aulus Cavalieri Carciofí, Robert Klement, M. Curé and C. Georgy and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

D. M. Faes

24 papers receiving 328 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. M. Faes Brazil 11 336 98 25 21 18 27 357
D. Panoglou Brazil 9 269 0.8× 52 0.5× 15 0.6× 17 0.8× 13 0.7× 15 279
S. Štefl Germany 14 533 1.6× 113 1.2× 24 1.0× 23 1.1× 7 0.4× 29 547
Robert Klement United States 10 299 0.9× 100 1.0× 19 0.8× 22 1.0× 10 0.6× 25 326
K. Dsilva Belgium 9 310 0.9× 109 1.1× 25 1.0× 19 0.9× 4 0.2× 13 332
Steve Gunnels United States 7 231 0.7× 93 0.9× 19 0.8× 31 1.5× 10 0.6× 10 263
G. Banyard Belgium 9 344 1.0× 147 1.5× 20 0.8× 22 1.0× 3 0.2× 12 364
Soumen Mondal India 10 310 0.9× 69 0.7× 13 0.5× 14 0.7× 8 0.4× 76 342
Deepak Raghavan United States 8 262 0.8× 112 1.1× 24 1.0× 31 1.5× 3 0.2× 10 268
M. Abdul-Masih Belgium 11 469 1.4× 204 2.1× 41 1.6× 24 1.1× 3 0.2× 22 501
D. Chochol Slovakia 9 275 0.8× 73 0.7× 27 1.1× 17 0.8× 4 0.2× 76 280

Countries citing papers authored by D. M. Faes

Since Specialization
Citations

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

Fields of papers citing papers by D. M. Faes

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. M. Faes

This figure shows the co-authorship network connecting the top 25 collaborators of D. M. Faes. A scholar is included among the top collaborators of D. M. Faes 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 D. M. Faes. D. M. Faes 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.
Carciofi, A. C., P. Santos, R. G. Vieira, et al.. (2023). Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of α Eri and β CMi. Monthly Notices of the Royal Astronomical Society. 526(2). 3007–3036. 13 indexed citations
2.
Kervella, P., S. Borgniet, A. Mérand, et al.. (2022). The binary system of the spinning-top Be star Achernar. Astronomy and Astrophysics. 667. A111–A111. 6 indexed citations
3.
Carciofi, A. C., et al.. (2021). A Multi–Observing Technique Study of the Dynamical Evolution of the Viscous Disk around the Be Star ω CMa. The Astrophysical Journal. 909(2). 149–149. 17 indexed citations
4.
Pak, Soojong, D. L. DePoy, J. L. Marshall, et al.. (2020). Giant Magellan Telescope Multi-object Astronomical and Cosmological Spectrograph (GMACS): conceptual design. 6–6. 1 indexed citations
5.
Panoglou, D., M. Borges Fernandes, D. Baade, et al.. (2019). Modelling the periodical variations in multiband polarization and photometry for discs of binary Be stars. Monthly Notices of the Royal Astronomical Society. 486(4). 5139–5157. 6 indexed citations
6.
Rivinius, Th., A. Mehner, Christophe Martayan, et al.. (2018). Stellar parameters of Be stars observed with X-shooter. Springer Link (Chiba Institute of Technology). 18 indexed citations
7.
Froning, Cynthia S., D. Bortoletto, D. L. DePoy, et al.. (2018). GMACS: a wide-field, moderate-resolution spectrograph for the Giant Magellan Telescope. Ground-based and Airborne Instrumentation for Astronomy VII. 69–69. 4 indexed citations
8.
9.
Carciofí, Aulus Cavalieri, R. G. Vieira, Th. Rivinius, et al.. (2018). The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars. Monthly Notices of the Royal Astronomical Society. 476(3). 3555–3579. 58 indexed citations
10.
Panoglou, D., D. M. Faes, & A. C. Carciofi. (2017). Variability of the decretion disc of Be stars in binary systems. Redalyc (Universidad Autónoma del Estado de México). 49. 94–94. 1 indexed citations
11.
Millour, F., A. Domiciano de Souza, R. Petrov, et al.. (2017). VLTI/PIONIER images the Achernar disk swell. HAL (Le Centre pour la Communication Scientifique Directe). 1 indexed citations
12.
Klement, Robert, Aulus Cavalieri Carciofí, Th. Rivinius, et al.. (2017). Revealing the structure of the outer disks of Be stars. Astronomy and Astrophysics. 601. A74–A74. 39 indexed citations
13.
Klement, Robert, A. C. Carciofi, Th. Rivinius, et al.. (2015). Multitechnique testing of the viscous decretion disk model. Astronomy and Astrophysics. 584. A85–A85. 28 indexed citations
14.
Klement, Robert, A. C. Carciofi, Th. Rivinius, et al.. (2015). Multitechnique testing of the viscous decretion disk model I. The stable and tenuous disk of the late-type Be star $β$ CMi. arXiv (Cornell University). 13 indexed citations
15.
Kervella, P., D. M. Faes, A. Mérand, et al.. (2014). The environment of the fast rotating star Achernar. Astronomy and Astrophysics. 569. A10–A10. 44 indexed citations
16.
Faes, D. M., A. C. Carciofi, Th. Rivinius, et al.. (2013). Differential interferometric phases at high spectral resolution as a sensitive physical diagnostic of circumstellar disks. Astronomy and Astrophysics. 555. A76–A76. 7 indexed citations
17.
Souza, A. Domiciano de, F. Vakili, Philippe Bendjoya, et al.. (2012). Beyond the diffraction limit of optical/IR interferometers. Astronomy and Astrophysics. 545. A130–A130. 21 indexed citations
18.
Rivinius, Th., A. C. Carciofi, J. Grunhut, et al.. (2012). The interferometric signature of the rapidly corotating magnetosphere of HR 59071. AIP conference proceedings. 102–105. 1 indexed citations
19.
Faes, D. M.. (2012). Use of Python programming language in astronomy and science. arXiv (Cornell University). 3(3). 3 indexed citations
20.
Faes, D. M., R. D. D. Costa, & C. Morisset. (2011). MAPPING AND MODELING THE PROPERTIES OF BIPOLAR PLANETARY NEBULAE. Redalyc (Universidad Autónoma del Estado de México). 40. 233–234. 2 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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