H. Estellés

22.0k total citations · 4 hit papers
21 papers, 1.2k citations indexed

About

H. Estellés is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics. According to data from OpenAlex, H. Estellés has authored 21 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 18 papers in Astronomy and Astrophysics, 9 papers in Geophysics and 5 papers in Nuclear and High Energy Physics. Recurrent topics in H. Estellés's work include Pulsars and Gravitational Waves Research (18 papers), Astrophysical Phenomena and Observations (7 papers) and High-pressure geophysics and materials (6 papers). H. Estellés is often cited by papers focused on Pulsars and Gravitational Waves Research (18 papers), Astrophysical Phenomena and Observations (7 papers) and High-pressure geophysics and materials (6 papers). H. Estellés collaborates with scholars based in Spain, Germany and United Kingdom. H. Estellés's co-authors include A. Ramos-Buades, C. García-Quirós, S. Husa, M. Colleoni, R. Jaume, G. Pratten, M. Mateu-Lucena, D. Keitel, M. Haney and Jonathan E. Thompson and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Physical review. D.

In The Last Decade

H. Estellés

20 papers receiving 1.2k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes

2021 351 citations G. Pratten, C. García-Quirós et al. Physical review. D profile →
Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries

2020 194 citations C. García-Quirós, M. Colleoni et al. Physical review. D profile →
Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes

2020 179 citations G. Pratten, S. Husa et al. Physical review. D profile →
Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes

2023 87 citations A. Ramos-Buades, Alessandra Buonanno et al. Physical review. D profile →

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
H. Estellés Spain	13	1.2k	240	239	171	84	21	1.2k
C. García-Quirós Spain	12	1.2k 1.1×	249 1.0×	259 1.1×	175 1.0×	87 1.0×	16	1.3k
A. Ramos-Buades Germany	19	1.5k 1.3×	305 1.3×	292 1.2×	216 1.3×	99 1.2×	29	1.5k
Serguei Ossokine United States	17	1.6k 1.4×	377 1.6×	319 1.3×	200 1.2×	112 1.3×	21	1.7k
R. Jaume Spain	6	820 0.7×	172 0.7×	164 0.7×	113 0.7×	58 0.7×	6	840
M. Mateu-Lucena Spain	10	813 0.7×	179 0.7×	165 0.7×	111 0.6×	56 0.7×	10	835
M. Favata United States	14	1.1k 0.9×	251 1.0×	160 0.7×	127 0.7×	56 0.7×	21	1.1k
Sean T. McWilliams United States	21	1.4k 1.2×	367 1.5×	176 0.7×	111 0.6×	114 1.4×	38	1.4k
M. Haney Switzerland	13	936 0.8×	182 0.8×	181 0.8×	123 0.7×	55 0.7×	21	951
Nathan K. Johnson-McDaniel United States	15	882 0.8×	194 0.8×	200 0.8×	145 0.8×	63 0.8×	27	904
Nils Dorband Germany	7	1.2k 1.1×	312 1.3×	185 0.8×	140 0.8×	112 1.3×	7	1.3k

Countries citing papers authored by H. Estellés

Since Specialization

Citations

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

Fields of papers citing papers by H. Estellés

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of H. Estellés. A scholar is included among the top collaborators of H. Estellés 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. Estellés. H. Estellés is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Buonanno, Alessandra, Mohammed Khalil, A. Ramos-Buades, et al.. (2025). Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model seobnrv5ehm. Physical review. D. 112(4). 18 indexed citations

Mihaylov, Deyan P., Serguei Ossokine, Alessandra Buonanno, et al.. (2025). pySEOBNR: A software package for the next generation of effective-one-body multipolar waveform models. SoftwareX. 30. 102080–102080. 1 indexed citations

Ramos-Buades, A., et al.. (2025). Reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures. Physical review. D. 112(12). 3 indexed citations

Xu, Yumeng, Shubhanshu Tiwari, M. Ebersold, et al.. (2024). Enhancing gravitational wave parameter estimation with nonlinear memory: Breaking the distance-inclination degeneracy. Physical review. D. 109(12). 10 indexed citations

Khalil, Mohammed, Alessandra Buonanno, H. Estellés, et al.. (2023). Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5. Physical review. D. 108(12). 40 indexed citations

Ramos-Buades, A., Alessandra Buonanno, H. Estellés, et al.. (2023). Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes. Physical review. D. 108(12). 87 indexed citations breakdown →

Estellés, H., S. Husa, M. Colleoni, et al.. (2022). Time-domain phenomenological model of gravitational-wave subdominant harmonics for quasicircular nonprecessing binary black hole coalescences. Physical review. D. 105(8). 46 indexed citations

Estellés, H., S. Husa, M. Colleoni, et al.. (2022). A Detailed Analysis of GW190521 with Phenomenological Waveform Models. The Astrophysical Journal. 924(2). 79–79. 45 indexed citations

Mateu-Lucena, M., S. Husa, M. Colleoni, et al.. (2022). Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1. Monthly Notices of the Royal Astronomical Society. 517(2). 2403–2425. 10 indexed citations

10.

Estellés, H., M. Colleoni, C. García-Quirós, et al.. (2022). New twists in compact binary waveform modeling: A fast time-domain model for precession. Physical review. D. 105(8). 65 indexed citations

11.

Estellés, H., A. Ramos-Buades, S. Husa, et al.. (2021). Phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes. Physical review. D. 103(12). 50 indexed citations

12.

Pratten, G., C. García-Quirós, M. Colleoni, et al.. (2021). Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes. Physical review. D. 103(10). 351 indexed citations breakdown →

13.

Colleoni, M., M. Mateu-Lucena, H. Estellés, et al.. (2021). Towards the routine use of subdominant harmonics in gravitational-wave inference: Reanalysis of GW190412 with generation X waveform models. Physical review. D. 103(2). 30 indexed citations

14.

García-Quirós, C., M. Colleoni, S. Husa, et al.. (2020). Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries. Physical review. D. 102(6). 194 indexed citations breakdown →

15.

Pratten, G., C. García-Quirós, M. Colleoni, et al.. (2020). Let's twist again: computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes. 16 indexed citations

16.

Pratten, G., S. Husa, C. García-Quirós, et al.. (2020). Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes. Physical review. D. 102(6). 179 indexed citations breakdown →

17.

Oliver, M., D. Keitel, A. L. Miller, H. Estellés, & A. M. Sintes. (2019). Matched-filter study and energy budget suggest no detectable gravitational-wave ‘extended emission’ from GW170817. Monthly Notices of the Royal Astronomical Society. 485(1). 843–850. 3 indexed citations

18.

Cervera, Francisco, Francisco Belmar, & H. Estellés. (1994). A Low Cost Robot for Acoustic Intensity Measurements. Noise Control Engineering Journal. 42(1). 31–31.

19.

Estellés, H., et al.. (1987). SEL for electrically hauled trains. Applied Acoustics. 22(1). 15–23. 1 indexed citations

20.

Estellés, H., et al.. (1984). COMMUNITY RESPONSE TO TRAFFIC NOISE IN VALENCIA CITY ---INTERNOISE 84. INTERNATIONAL COOPERATION FOR NOISE CONTROL. PROCEEDINGS 1984 INTERNATIONAL CONFERENCE ON NOISE CONTROL ENGINEERING, HONOLULU, HAWAII, 3-5 DECEMBER 1984, VOLUMES 1 AND 2.. 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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