H. Quintana

1.8k total citations · 1 hit paper
26 papers, 903 citations indexed

About

H. Quintana is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, H. Quintana has authored 26 papers receiving a total of 903 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 18 papers in Instrumentation and 6 papers in Nuclear and High Energy Physics. Recurrent topics in H. Quintana's work include Galaxies: Formation, Evolution, Phenomena (19 papers), Astronomy and Astrophysical Research (18 papers) and Astrophysical Phenomena and Observations (10 papers). H. Quintana is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (19 papers), Astronomy and Astrophysical Research (18 papers) and Astrophysical Phenomena and Observations (10 papers). H. Quintana collaborates with scholars based in Chile, Germany and United States. H. Quintana's co-authors include S. S. Murray, A. Vikhlinin, Alexey Voevodkin, H. Ebeling, Andrey V. Kravtsov, W. Forman, Daisuke Nagai, C. Jones, R. Burenin and A. Hornstrup and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

H. Quintana

24 papers receiving 878 citations

Hit Papers

CHANDRACLUSTER COSMOLOGY ... 2009 2026 2014 2020 2009 100 200 300 400

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
H. Quintana Chile 13 853 332 302 37 36 26 903
Michael J. Ledlow United States 20 1.2k 1.4× 349 1.1× 497 1.6× 39 1.1× 24 0.7× 40 1.2k
Neil H. M. Crighton United Kingdom 20 883 1.0× 256 0.8× 306 1.0× 32 0.9× 27 0.8× 30 907
Russell Cannon Australia 15 659 0.8× 271 0.8× 150 0.5× 23 0.6× 41 1.1× 52 710
George Rhee United States 10 1.1k 1.2× 416 1.3× 303 1.0× 61 1.6× 36 1.0× 30 1.1k
Sambit Roychowdhury Australia 14 917 1.1× 272 0.8× 221 0.7× 32 0.9× 24 0.7× 25 949
A. Streblyanska Spain 13 1.1k 1.2× 310 0.9× 280 0.9× 16 0.4× 39 1.1× 33 1.1k
Eric Wilcots United States 18 1.1k 1.3× 390 1.2× 201 0.7× 20 0.5× 23 0.6× 86 1.1k
P. R. Burchat United States 8 611 0.7× 265 0.8× 233 0.8× 16 0.4× 53 1.5× 15 714
Renato A. Dupke United States 17 787 0.9× 315 0.9× 153 0.5× 33 0.9× 54 1.5× 48 817
R. Burenin Russia 14 1.1k 1.3× 296 0.9× 412 1.4× 18 0.5× 25 0.7× 108 1.1k

Countries citing papers authored by H. Quintana

Since Specialization
Citations

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

Fields of papers citing papers by H. Quintana

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of H. Quintana

This figure shows the co-authorship network connecting the top 25 collaborators of H. Quintana. A scholar is included among the top collaborators of H. Quintana 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 H. Quintana. H. Quintana 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.
Nastasi, A., R. Fassbender, H. Böhringer, et al.. (2011). Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 atz= 1.49. Astronomy and Astrophysics. 532. L6–L6. 11 indexed citations
2.
Fassbender, R., A. Nastasi, H. Böhringer, et al.. (2011). The X-ray luminous galaxy cluster XMMU J1007.4+1237 atz= 1.56. Astronomy and Astrophysics. 527. L10–L10. 44 indexed citations
3.
Fassbender, R., A. Nastasi, H. Böhringer, et al.. (2011). The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z=1.56 - The dawn of starburst activity in cluster cores. arXiv (Cornell University). 527. 1–6. 35 indexed citations
4.
Schwope, A., G. Lamer, A. de Hoon, et al.. (2010). XMMU J100750.5+125818: a strong lensing cluster atz= 1.082. Astronomy and Astrophysics. 513. L10–L10. 16 indexed citations
5.
Fassbender, R., H. Böhringer, Joana Santos, et al.. (2010). A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 atz= 0.975. Astronomy and Astrophysics. 527. A78–A78. 11 indexed citations
6.
Quintana, H., et al.. (2009). High relative velocity central dumbbells in poor clusters. Astronomische Nachrichten. 330(9-10). 924–927.
7.
Vikhlinin, A., R. Burenin, H. Ebeling, et al.. (2009). CHANDRACLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION. The Astrophysical Journal. 692(2). 1033–1059. 416 indexed citations breakdown →
8.
Cappelluti, N., M. Ajello, P. Rebusco, et al.. (2009). A candidate tidal disruption event in the Galaxy cluster Abell 3571. Astronomy and Astrophysics. 495(2). L9–L12. 47 indexed citations
9.
Nakos, Theodoros, J. P. Willis, S. Andreon, et al.. (2008). A multi-wavelength survey of AGN in the XMM-LSS field: I. Quasar selection via the KX technique. ArXiv.org. 5 indexed citations
10.
Willis, J. P., F. Pacaud, I. Valtchanov, et al.. (2005). The XMM Large-Scale Structure survey: an initial sample of galaxy groups and clusters to a redshift z < 0.6. Monthly Notices of the Royal Astronomical Society. 363(2). 675–691. 38 indexed citations
11.
Alloin, D., B. Altieri, M. N. Bremer, et al.. (2001). The XMM large scale structure survey and its multi-λ follow-up. Explore Bristol Research. 105. 32–36. 5 indexed citations
12.
Aharonian, F., et al.. (2001). 5@5 – a 5 GeV energy threshold array of imaging atmospheric Cherenkov telescopes at 5 km altitude. Astroparticle Physics. 15(4). 335–356. 39 indexed citations
13.
Drinkwater, M. J., et al.. (1999). New Structure in the Shapley Supercluster. Publications of the Astronomical Society of Australia. 16(2). 113–123. 12 indexed citations
14.
Quintana, H., A. Ramírez, & M. J. Way. (1996). Dynamics of the Cluster of Galaxies A3266 (Sersic 40/60). I. Spectroscopic Data. The Astronomical Journal. 112. 36–36. 30 indexed citations
15.
Quintana, H. & A. Ramírez. (1995). Redshifts of 165 Abell and southern rich clusters of galaxies. The Astrophysical Journal Supplement Series. 96. 343–343. 34 indexed citations
16.
Quintana, H. & R. A. White. (1990). A partial list of southern clusters of galaxies. Astrophysics and Space Science. 173(2). 265–292. 1 indexed citations
17.
Infante, L., et al.. (1986). Galaxy counts and colors in a South Galactic Pole field. The Astronomical Journal. 91. 217–217. 18 indexed citations
18.
Quintana, H.. (1979). Core radii and mass segregation in clusters of galaxies. The Astronomical Journal. 84. 15–15. 14 indexed citations
19.
Steigman, Gary, H. Quintana, Craig L. Sarazin, & J. S. Faulkner. (1978). Dynamical interactions and astrophysical effects of stable heavy neutrinos. The Astronomical Journal. 83. 1050–1050. 73 indexed citations
20.
Quintana, H.. (1976). The structure equations of a slowly rotating, fully relativistic solid star. The Astrophysical Journal. 207. 279–279. 12 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026