Marcos P. Diaz

964 total citations
50 papers, 634 citations indexed

About

Marcos P. Diaz is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics. According to data from OpenAlex, Marcos P. Diaz has authored 50 papers receiving a total of 634 indexed citations (citations by other indexed papers that have themselves been cited), including 48 papers in Astronomy and Astrophysics, 9 papers in Geophysics and 9 papers in Nuclear and High Energy Physics. Recurrent topics in Marcos P. Diaz's work include Astrophysical Phenomena and Observations (35 papers), Astrophysics and Star Formation Studies (23 papers) and Stellar, planetary, and galactic studies (22 papers). Marcos P. Diaz is often cited by papers focused on Astrophysical Phenomena and Observations (35 papers), Astrophysics and Star Formation Studies (23 papers) and Stellar, planetary, and galactic studies (22 papers). Marcos P. Diaz collaborates with scholars based in Brazil, United States and Chile. Marcos P. Diaz's co-authors include J. E. Steiner, R. E. Mennickent, I. Hubený, R. E. Williams, George W. Preston, E. Mason, T. Bensby, A. Bruch, Manoel Odorico de Moraes and G. Pietrzyński 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

Marcos P. Diaz

46 papers receiving 608 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Marcos P. Diaz Brazil 16 627 92 66 56 51 50 634
A. F. Valeev Russia 11 370 0.6× 73 0.8× 56 0.8× 32 0.6× 17 0.3× 68 380
R. Zamanov Bulgaria 13 659 1.1× 97 1.1× 128 1.9× 39 0.7× 60 1.2× 59 670
Tom Marsh United Kingdom 9 336 0.5× 50 0.5× 33 0.5× 20 0.4× 36 0.7× 28 358
J. Smak Poland 10 397 0.6× 50 0.5× 41 0.6× 54 1.0× 45 0.9× 63 410
F. A. Ringwald United States 13 603 1.0× 25 0.3× 124 1.9× 56 1.0× 117 2.3× 47 617
V. P. Goranskij Russia 11 316 0.5× 65 0.7× 24 0.4× 45 0.8× 18 0.4× 58 327
K. O. Mason United Kingdom 13 290 0.5× 29 0.3× 74 1.1× 25 0.4× 33 0.6× 31 307
S. M. Caballero‐Nieves United States 10 512 0.8× 161 1.8× 78 1.2× 25 0.4× 9 0.2× 19 524
M. Kotze South Africa 11 388 0.6× 70 0.8× 53 0.8× 41 0.7× 56 1.1× 22 403
W. Huang United States 11 414 0.7× 113 1.2× 69 1.0× 22 0.4× 19 0.4× 15 425

Countries citing papers authored by Marcos P. Diaz

Since Specialization
Citations

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

Fields of papers citing papers by Marcos P. Diaz

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Marcos P. Diaz. 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 Marcos P. Diaz. The network helps show where Marcos P. Diaz may publish in the future.

Co-authorship network of co-authors of Marcos P. Diaz

This figure shows the co-authorship network connecting the top 25 collaborators of Marcos P. Diaz. A scholar is included among the top collaborators of Marcos P. Diaz 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 Marcos P. Diaz. Marcos P. Diaz 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.
Jablonski, F., et al.. (2023). Revised ephemeris and orbital period derivative of the supersoft X-ray source CAL 87 based on 34 yr of observations. Monthly Notices of the Royal Astronomical Society. 527(3). 8991–8995.
2.
Cruz, P., et al.. (2022). Detached eclipsing binaries from the Kepler field: radii and photometric masses of components in short-period systems. Monthly Notices of the Royal Astronomical Society. 515(1). 1416–1429. 3 indexed citations
3.
Levenhagen, R. S., Marcos P. Diaz, E. B. Amôres, & N. V. Leister. (2020). The Hα line emission of the Be star β Psc: the last 40 yr. Monthly Notices of the Royal Astronomical Society. 501(1). 747–755. 3 indexed citations
4.
Oliveira, A. S., et al.. (2019). Optical observations and cyclops post-shock region modelling of the polar V348 Pav. Monthly Notices of the Royal Astronomical Society. 489(3). 4032–4042. 5 indexed citations
5.
Diaz, Marcos P., et al.. (2018). The structure of a recent nova shell as observed by ALMA. Monthly Notices of the Royal Astronomical Society Letters. 480(1). L54–L57. 9 indexed citations
6.
Diaz, Marcos P., et al.. (2017). 3D photoionization models of nova V723 Cas. Monthly Notices of the Royal Astronomical Society. 473(1). 355–365. 5 indexed citations
7.
8.
Mason, E., Marcos P. Diaz, R. E. Williams, George W. Preston, & T. Bensby. (2012). The peculiar nova V1309 Scorpii/nova Scorpii 2008 A candidate twin of V838 Monocerotis. Scientific Electronic Library Online (São Paulo Research Foundation, Latin American and Caribbean Center on Health Sciences Information, Conselho Nacional de Desenvolvimento Científico e Tecnológico). 40 indexed citations
9.
Mennickent, R. E., Z. Kołaczkowski, G. Djurašević, et al.. (2012). A cyclic bipolar wind in the interacting binary V 393 Scorpii. Monthly Notices of the Royal Astronomical Society. 427(1). 607–624. 28 indexed citations
10.
Diaz, Marcos P., et al.. (2011). A METHOD FOR THE STUDY OF ACCRETION DISK EMISSION IN CATACLYSMIC VARIABLES. I. THE MODEL. The Astrophysical Journal. 736(1). 17–17. 16 indexed citations
11.
Moraes, Manoel Odorico de & Marcos P. Diaz. (2009). HR Del REMNANT ANATOMY USING TWO-DIMENSIONAL SPECTRAL DATA AND THREE-DIMENSIONAL PHOTOIONIZATION SHELL MODELS. The Astronomical Journal. 138(6). 1541–1556. 17 indexed citations
12.
Diaz, Marcos P., et al.. (2007). A Statistical Study of Accretion Disk Model Spectra for Cataclysmic Variables. The Astronomical Journal. 134(5). 1923–1933. 37 indexed citations
13.
Diaz, Marcos P., et al.. (2007). Emission-Line Flickering from the Secondary Star in Cataclysmic Variables? A Study of V3885 Sagittarii. The Astronomical Journal. 133(6). 2659–2668. 7 indexed citations
14.
Mennickent, R. E., Marcos P. Diaz, & C. Tappert. (2004). A search for brown dwarf like secondaries in cataclysmic variables - II. Monthly Notices of the Royal Astronomical Society. 347(4). 1180–1186. 10 indexed citations
15.
Mennickent, R. E., G. Pietrzyński, Marcos P. Diaz, & W. Gieren. (2003). Double-periodic blue variables in the Magellanic Clouds. Springer Link (Chiba Institute of Technology). 31 indexed citations
16.
Augusto, Alessandra & Marcos P. Diaz. (2003). The Spectral Evolution of V382 Velorum (Nova Vela 1999). The Astronomical Journal. 125(6). 3349–3358. 6 indexed citations
17.
Diaz, Marcos P.. (2002). Physical and Chemical Diagnostic of Structured Nova Shells. AIP conference proceedings. 637. 538–542. 1 indexed citations
18.
Mennickent, R. E., Marcos P. Diaz, Warren Skidmore, & C. Sterken. (2001). Discovery of a cataclysmic variable with a sub-stellar companion. Springer Link (Chiba Institute of Technology). 13 indexed citations
19.
Diaz, Marcos P., et al.. (1999). A Spectroscopic Study of V617 Sagittarii. The Astronomical Journal. 117(1). 534–540. 14 indexed citations
20.
Diaz, Marcos P., R. E. Williams, M. M. Phillips, & M. Hamuy. (1995). Recent observations of nova GQ Mus 1983. Monthly Notices of the Royal Astronomical Society. 277(3). 959–964. 9 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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