M. Jaque Arancibia

558 total citations
27 papers, 221 citations indexed

About

M. Jaque Arancibia is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, M. Jaque Arancibia has authored 27 papers receiving a total of 221 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 3 papers in Instrumentation and 3 papers in Nuclear and High Energy Physics. Recurrent topics in M. Jaque Arancibia's work include Stellar, planetary, and galactic studies (17 papers), Astro and Planetary Science (15 papers) and Astrophysics and Star Formation Studies (9 papers). M. Jaque Arancibia is often cited by papers focused on Stellar, planetary, and galactic studies (17 papers), Astro and Planetary Science (15 papers) and Astrophysics and Star Formation Studies (9 papers). M. Jaque Arancibia collaborates with scholars based in Chile, Argentina and United States. M. Jaque Arancibia's co-authors include C. Saffe, E. Jofré, R. Petrucci, G. Damke, Mauricio Solar, J. L. Sokoloski, J. F. González, A. Segreto, K. Mukai and G. J. M. Luna 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

M. Jaque Arancibia

22 papers receiving 185 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. Jaque Arancibia Chile 9 194 41 22 19 12 27 221
Maayane T. Soumagnac United States 7 189 1.0× 34 0.8× 21 1.0× 18 0.9× 5 0.4× 13 215
A. Scaife United Kingdom 6 105 0.5× 19 0.5× 46 2.1× 16 0.8× 5 0.4× 11 130
David G. Whelan United States 9 219 1.1× 79 1.9× 9 0.4× 13 0.7× 3 0.3× 14 257
Jundan Nie China 9 308 1.6× 151 3.7× 15 0.7× 29 1.5× 2 0.2× 31 323
K. G. Strassméier Germany 11 278 1.4× 96 2.3× 19 0.9× 19 1.0× 5 0.4× 38 308
Emily C. Martin United States 8 251 1.3× 106 2.6× 7 0.3× 17 0.9× 2 0.2× 27 282
R. H. McNaught Australia 7 201 1.0× 62 1.5× 13 0.6× 19 1.0× 4 0.3× 29 222
Thomas Madura United States 13 413 2.1× 40 1.0× 30 1.4× 24 1.3× 11 0.9× 32 423
Wen Hou China 9 186 1.0× 109 2.7× 8 0.4× 40 2.1× 3 0.3× 17 211
S. T. Holfeltz United States 8 291 1.5× 126 3.1× 15 0.7× 9 0.5× 3 0.3× 21 310

Countries citing papers authored by M. Jaque Arancibia

Since Specialization
Citations

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

Fields of papers citing papers by M. Jaque Arancibia

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Jaque Arancibia

This figure shows the co-authorship network connecting the top 25 collaborators of M. Jaque Arancibia. A scholar is included among the top collaborators of M. Jaque Arancibia 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. Jaque Arancibia. M. Jaque Arancibia 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.
Saffe, C., et al.. (2025). Discovery of λ Boo stars in open clusters. Astronomy and Astrophysics. 698. A137–A137.
2.
Saffe, C., et al.. (2025). Searching for λ Boo stars in binary systems. Astronomy and Astrophysics. 696. A123–A123. 1 indexed citations
3.
4.
Saffe, C., et al.. (2024). The largest metallicity difference in twin systems: High-precision abundance analysis of the benchmark pair Krios and Kronos. Astronomy and Astrophysics. 688. A73–A73. 6 indexed citations
5.
Galarza, Jhon Yana, Henrique Reggiani, Diego Lorenzo-Oliveira, et al.. (2024). Detailed Abundances of the Planet-hosting TOI-1173 A/B System: Possible Evidence of Planet Engulfment in a Very Wide Binary. The Astrophysical Journal. 974(1). 122–122. 1 indexed citations
6.
Saffe, C., Eder Martioli, M. Jaque Arancibia, et al.. (2024). Disentangling the origin of chemical differences using GHOST. Astronomy and Astrophysics. 682. L23–L23. 8 indexed citations
7.
Arancibia, M. Jaque, et al.. (2024). Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves. Astronomy and Astrophysics. 691. A106–A106. 3 indexed citations
8.
Saffe, C., et al.. (2023). Elemental abundance differences in the massive planet-hosting wide binary HD 196067−68. Monthly Notices of the Royal Astronomical Society. 527(4). 10016–10024. 8 indexed citations
9.
Saffe, C., et al.. (2022). Testing the accretion scenario of λ Boo stars. Astronomy and Astrophysics. 660. A98–A98. 4 indexed citations
10.
Saffe, C., et al.. (2022). Are Am stars and hot-Jupiter planets related?. Astronomy and Astrophysics. 668. A157–A157. 2 indexed citations
11.
Luna, G. J. M., K. Mukai, J. L. Sokoloski, et al.. (2022). Taking a break: Paused accretion in the symbiotic binary RT Cru. Astronomy and Astrophysics. 670. A32–A32. 8 indexed citations
12.
Saffe, C., et al.. (2021). Chemical analysis of early-type stars with planets. Astronomy and Astrophysics. 647. A49–A49. 17 indexed citations
13.
Saffe, C., et al.. (2020). KELT-17: a chemically peculiar Am star and a hot-Jupiter planet. Springer Link (Chiba Institute of Technology). 7 indexed citations
14.
Arancibia, M. Jaque, et al.. (2020). Detecting prolonged activity minima in binary stars. Astronomy and Astrophysics. 645. L6–L6. 1 indexed citations
15.
Saffe, C., et al.. (2019). High-precision analysis of binary stars with planets. Astronomy and Astrophysics. 625. A39–A39. 17 indexed citations
16.
Luna, G. J. M., K. Mukai, J. L. Sokoloski, et al.. (2018). X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Crucis. Springer Link (Chiba Institute of Technology). 14 indexed citations
17.
Saffe, C., et al.. (2018). Using non-solar-scaled opacities to derive stellar parameters. Astronomy and Astrophysics. 620. A54–A54. 12 indexed citations
18.
González, J. F., et al.. (2018). HD 38858: A solar-Type star with an activity cycle of ∼10.8 yr: Searching for variations in the Balmer and metallic lines. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 6 indexed citations
19.
González, J. F., et al.. (2018). HD 38858: a solar-type star with an activity cycle of ∼10.8 yr. Astronomy and Astrophysics. 620. A34–A34. 14 indexed citations
20.
González, J. F., et al.. (2016). Discovery of an activity cycle in the solar-analog HD 45184. Exploring Balmer and metallic lines as activity proxy candidates. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 1 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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