J. Echevarría

612 total citations
33 papers, 175 citations indexed

About

J. Echevarría is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Geophysics. According to data from OpenAlex, J. Echevarría has authored 33 papers receiving a total of 175 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 8 papers in Computational Mechanics and 4 papers in Geophysics. Recurrent topics in J. Echevarría's work include Astrophysical Phenomena and Observations (23 papers), Gamma-ray bursts and supernovae (11 papers) and Stellar, planetary, and galactic studies (10 papers). J. Echevarría is often cited by papers focused on Astrophysical Phenomena and Observations (23 papers), Gamma-ray bursts and supernovae (11 papers) and Stellar, planetary, and galactic studies (10 papers). J. Echevarría collaborates with scholars based in Mexico, United Kingdom and Netherlands. J. Echevarría's co-authors include R. Costero, R. Michel, S. V. Zharikov, G. Tovmassian, E. De la Fuente, J V Hernández Santisteban, M. G. Richer, Ariel Ramírez‐Torres, J. León-Tavares and T. J. O’Brien 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

J. Echevarría

33 papers receiving 167 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
J. Echevarría Mexico 8 165 30 17 13 9 33 175
V. N. Komarova Russia 10 185 1.1× 44 1.5× 10 0.6× 25 1.9× 11 1.2× 19 191
Т. И. Ларченкова Russia 5 76 0.5× 23 0.8× 10 0.6× 18 1.4× 9 1.0× 25 86
Noel Castro Segura United Kingdom 6 113 0.7× 42 1.4× 12 0.7× 10 0.8× 6 0.7× 29 127
I. Traulsen Germany 8 162 1.0× 52 1.7× 22 1.3× 13 1.0× 9 1.0× 17 171
Ashish Raj India 8 147 0.9× 54 1.8× 12 0.7× 17 1.3× 10 1.1× 28 157
D. M. Hewitt Netherlands 7 127 0.8× 28 0.9× 8 0.5× 18 1.4× 6 0.7× 9 134
H. Khandrika United States 4 133 0.8× 28 0.9× 4 0.2× 11 0.8× 16 1.8× 16 139
F. Rantakyrö Chile 6 116 0.7× 24 0.8× 5 0.3× 6 0.5× 11 1.2× 8 123
A. Burtovoi Italy 6 68 0.4× 32 1.1× 7 0.4× 9 0.7× 8 0.9× 18 84
Sumin Tang United States 7 143 0.9× 18 0.6× 18 1.1× 18 1.4× 26 2.9× 15 155

Countries citing papers authored by J. Echevarría

Since Specialization
Citations

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

Fields of papers citing papers by J. Echevarría

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of J. Echevarría

This figure shows the co-authorship network connecting the top 25 collaborators of J. Echevarría. A scholar is included among the top collaborators of J. Echevarría 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 J. Echevarría. J. Echevarría 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.
Scaringi, Simone, Colin Littlefield, D. de Martino, et al.. (2025). DW Cnc: a micronova with a negative superhump and a flickering spin. Monthly Notices of the Royal Astronomical Society. 539(3). 2424–2434. 2 indexed citations
2.
Herrera, Joel, et al.. (2023). OPTICAM triple-channel astronomical image acquisition control software and external triggering synchronization system. Astronomy and Computing. 46. 100773–100773. 1 indexed citations
3.
Echevarría, J., et al.. (2023). The period bouncer system SDSS J105754.25+275947.5: first radial velocity study. Monthly Notices of the Royal Astronomical Society. 526(4). 5110–5117. 2 indexed citations
4.
Michel, R., J. Echevarría, & J V Hernández Santisteban. (2013). Photometry of the eclipsing cataclysmic variable SDSS J152419.33+220920.0. Springer Link (Chiba Institute of Technology). 1 indexed citations
5.
González–Buitrago, D., G. Tovmassian, S. V. Zharikov, et al.. (2013). Multiwavelength observations of V479 Andromedae: a close compact binary with an identity crisis. Springer Link (Chiba Institute of Technology). 6 indexed citations
6.
Zharikov, S. V., G. Tovmassian, V. Neustroev, et al.. (2008). Cyclic brightening in the short-period WZ Sge-type cataclysmic variable SDSS J080434.20+510349.2. Astronomy and Astrophysics. 486(2). 505–509. 13 indexed citations
7.
Echevarría, J. & R. Michel. (2007). Radial velocity study of uz serpentis. Redalyc (Universidad Autónoma del Estado de México). 43(2). 291–296. 2 indexed citations
8.
Echevarría, J., R. Michel, R. Costero, & S. V. Zharikov. (2006). Determination of the basic parameters of the dwarf nova EY Cygni. Astronomy and Astrophysics. 462(3). 1069–1080. 12 indexed citations
9.
Richer, M. G., J. A. López, W. Steffen, et al.. (2003). The kinematics of the most oxygen-poor\n planetary nebula PN G 135.9+55.9. Springer Link (Chiba Institute of Technology). 7 indexed citations
10.
Michel, R., et al.. (2003). Seeing Measurements at San Pedro Mártir Observatory using the DIMM Method. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 39(2). 291–301. 1 indexed citations
11.
Echevarría, J., et al.. (2003). DOPPLER TOMOGRAPHY OF CATACLYSMIC VARIABLES: WHAT CAN WE DO WITH THE GTC?. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 16. 154–157. 1 indexed citations
12.
Tovmassian, G., J. Greiner, S. V. Zharikov, J. Echevarría, & A. Y. Kniazev. (2001). The new cataclysmic variable RX J1554.2+2721 in the period gap. Springer Link (Chiba Institute of Technology). 7 indexed citations
13.
Zharikov, S. V., et al.. (2001). The orbital period of intermediate polar 1WGA J1958.2+3232. Astronomy and Astrophysics. 366(3). 834–839. 3 indexed citations
14.
Echevarría, J., et al.. (1999). Radial velocity study of the dwarf novae KT Per and Tz Per. 35(2). 135–141. 1 indexed citations
15.
Echevarría, J., M. Tapia, R. Costero, et al.. (1998). Site testing at Observatorio Astronómico Nacional in San Pedro Mártir. 34(1). 47–60. 4 indexed citations
16.
Echevarría, J.. (1988). Photometry of the faint dwarf nova UZ Serpentis: detection of the orbital period.. 16(1). 37–39. 1 indexed citations
17.
Echevarría, J.. (1987). Multi-wavelength observations of dwarf novae during outburst. Astrophysics and Space Science. 130(1-2). 103–109. 2 indexed citations
18.
Costero, R., et al.. (1986). Observations and models of the eclipse of the central star of ngc 2346. 13(2). 149–158. 6 indexed citations
19.
Echevarría, J., et al.. (1983). Elementos traza en leches de lactancia españolas: III.- Determinación de nitratos. Alimentaria: Revista de tecnología e higiene de los alimentos. 51–57. 1 indexed citations
20.
Echevarría, J., et al.. (1978). Photometric Study of Trapezium-Type Systems. Bulletin of the American Astronomical Society. 10(3). 287–296. 3 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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