S. Husa

100.5k total citations · 7 hit papers
91 papers, 8.0k citations indexed

About

S. Husa is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, S. Husa has authored 91 papers receiving a total of 8.0k indexed citations (citations by other indexed papers that have themselves been cited), including 87 papers in Astronomy and Astrophysics, 38 papers in Nuclear and High Energy Physics and 13 papers in Geophysics. Recurrent topics in S. Husa's work include Pulsars and Gravitational Waves Research (77 papers), Astrophysical Phenomena and Observations (52 papers) and Black Holes and Theoretical Physics (36 papers). S. Husa is often cited by papers focused on Pulsars and Gravitational Waves Research (77 papers), Astrophysical Phenomena and Observations (52 papers) and Black Holes and Theoretical Physics (36 papers). S. Husa collaborates with scholars based in Germany, Spain and United Kingdom. S. Husa's co-authors include M. D. Hannam, Bernd Brügmann, F. Ohme, Ulrich Sperhake, José A. González, M. Pürrer, A. Bohé, S. Khan, Mark Hannam and Xisco Jiménez Forteza and has published in prestigious journals such as Physical Review Letters, The Astrophysical Journal and Journal of Computational Physics.

In The Last Decade

S. Husa

90 papers receiving 7.7k citations

Hit Papers

align trajectories sort by overperformance

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.

Frequency-domain gravitational waves from nonprecessing black-hole binaries. II. A phenomenological model for the advanced detector era

2016 724 citations S. Khan, S. Husa et al. Physical review. D profile →
Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. New numerical waveforms and anatomy of the signal

2016 535 citations S. Husa, S. Khan et al. Physical review. D profile →
Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms

2014 468 citations M. D. Hannam, P. Schmidt et al. Physical Review Letters profile →
Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins

2011 406 citations P. Ajith, M Hannam et al. Physical Review Letters profile →
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 →

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author						Papers	Cites
S. Husa	7.8k	2.1k	1.2k	830	639	91	8.0k
Larry Kidder	8.3k 1.1×	2.6k 1.2×	1.1k 1.0×	818 1.0×	621 1.0×	156	8.7k
Mark Scheel	8.9k 1.1×	3.2k 1.5×	1.2k 1.0×	807 1.0×	624 1.0×	171	9.3k
Bernd Brügmann	7.6k 1.0×	3.0k 1.4×	903 0.8×	685 0.8×	431 0.7×	121	8.0k
Curt Cutler	6.6k 0.8×	1.5k 0.7×	1.1k 1.0×	939 1.1×	533 0.8×	67	6.8k
Luc Blanchet	8.9k 1.1×	3.2k 1.5×	1.2k 1.0×	1.1k 1.3×	595 0.9×	120	9.1k
D. R. Lorimer	9.3k 1.2×	2.6k 1.3×	1.2k 1.0×	1.6k 2.0×	387 0.6×	208	9.6k
Alessandra Buonanno	10.5k 1.4×	3.1k 1.5×	1.5k 1.3×	1.2k 1.4×	1.0k 1.6×	136	11.0k
J. M. Cordes	7.3k 0.9×	2.6k 1.2×	848 0.7×	966 1.2×	336 0.5×	199	7.6k
B. W. Stappers	7.2k 0.9×	2.1k 1.0×	1.2k 1.0×	1.2k 1.4×	306 0.5×	278	7.5k
I. H. Stairs	7.7k 1.0×	2.2k 1.1×	1.3k 1.1×	1.6k 2.0×	327 0.5×	141	7.9k

Countries citing papers authored by S. Husa

Since Specialization

Citations

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

Fields of papers citing papers by S. Husa

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Husa

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Husa, S., et al.. (2025). First Eccentric Inspiral–Merger–Ringdown Analysis of Neutron Star–Black Hole Mergers. The Astrophysical Journal. 995(1). 47–47. 2 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

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

García-Quirós, C., et al.. (2020). Accelerating the evaluation of inspiral–merger–ringdown waveforms with adapted grids. Classical and Quantum Gravity. 38(1). 15006–15006. 28 indexed citations

Vañó-Viñuales, Alex & S. Husa. (2018). Spherical symmetry as a test case for unconstrained hyperboloidal evolution II: gauge conditions. Classical and Quantum Gravity. 35(4). 45014–45014. 16 indexed citations

London, L. T., S. Khan, Edward Fauchon-Jones, et al.. (2018). First Higher-Multipole Model of Gravitational Waves from Spinning and Coalescing Black-Hole Binaries. Physical Review Letters. 120(16). 161102–161102. 178 indexed citations

Hannam, M. D., P. Schmidt, A. Bohé, et al.. (2014). Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms. Physical Review Letters. 113(15). 151101–151101. 468 indexed citations breakdown →

10.

Hannam, Mark, P. Schmidt, A. Bohé, et al.. (2013). Twist and shout: A simple model of complete precessing black-hole-binary gravitational waveforms. arXiv (Cornell University). 3 indexed citations

11.

Schmidt, P., M. D. Hannam, & S. Husa. (2012). Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and nonprecessing inspiral signals. Physical review. D. Particles, fields, gravitation, and cosmology. 86(10). 155 indexed citations

12.

Ajith, P., M Hannam, S. Husa, et al.. (2011). Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins. Physical Review Letters. 106(24). 241101–241101. 406 indexed citations breakdown →

13.

Reisswig, Christian, S. Husa, Luciano Rezzolla, et al.. (2009). Gravitational-wave detectability of equal-mass black-hole binaries with aligned spins. Physical review. D. Particles, fields, gravitation, and cosmology. 80(12). 54 indexed citations

14.

Husa, S., et al.. (2008). Discretization of the Cauchy problem for second order in space, first order in time systems using high order finite difference operators. arXiv (Cornell University). 2 indexed citations

15.

Sperhake, Ulrich, et al.. (2007). SUPERMASSIVE KICKS FOR SPINNING BLACK HOLES. arXiv (Cornell University). 7 indexed citations

16.

Hannam, M. D., S. Husa, Denis Pollney, Bernd Brügmann, & Niall Ó Murchadha. (2007). Geometry and Regularity of Moving Punctures. Physical Review Letters. 99(24). 241102–241102. 107 indexed citations

17.

González, José A., Ulrich Sperhake, Bernd Brügmann, M. D. Hannam, & S. Husa. (2007). Maximum Kick from Nonspinning Black-Hole Binary Inspiral. Physical Review Letters. 98(9). 91101–91101. 307 indexed citations

18.

González, José A., M. D. Hannam, Ulrich Sperhake, Bernd Brügmann, & S. Husa. (2007). Supermassive Recoil Velocities for Binary Black-Hole Mergers with Antialigned Spins. Physical Review Letters. 98(23). 231101–231101. 247 indexed citations

19.

Husa, S.. (2002). 12. Problems and Successes in the Numerical Approach to the Conformal Field Equations. Lecture notes in physics. 604. 239–259. 7 indexed citations

20.

Husa, S. & Jeffrey Winicour. (1999). Asymmetric merger of black holes. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 60(8). 35 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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