M. Benacquista

9.4k total citations
10 papers, 184 citations indexed

About

M. Benacquista is a scholar working on Astronomy and Astrophysics, Oceanography and Molecular Biology. According to data from OpenAlex, M. Benacquista has authored 10 papers receiving a total of 184 indexed citations (citations by other indexed papers that have themselves been cited), including 10 papers in Astronomy and Astrophysics, 4 papers in Oceanography and 1 paper in Molecular Biology. Recurrent topics in M. Benacquista's work include Pulsars and Gravitational Waves Research (9 papers), Gamma-ray bursts and supernovae (5 papers) and Geophysics and Gravity Measurements (4 papers). M. Benacquista is often cited by papers focused on Pulsars and Gravitational Waves Research (9 papers), Gamma-ray bursts and supernovae (5 papers) and Geophysics and Gravity Measurements (4 papers). M. Benacquista collaborates with scholars based in United States, Germany and Armenia. M. Benacquista's co-authors include Manuel Arca Sedda, Kelly Holley‐Bockelmann, Krzysztof Belczyński, Martina Donnari, Mirek Giersz, Rainer Spurzem, Dafei Jin, Diogo Belloni, Grzegorz Wiktorowicz and Abbas Askar 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. Benacquista

9 papers receiving 172 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
M. Benacquista United States	7	183	22	17	10	6	10	184
H. Thankful Cromartie United States	4	90 0.5×	16 0.7×	18 1.1×	12 1.2×	3 0.5×	8	99
Michele Vallisneri Netherlands	2	107 0.6×	14 0.6×	11 0.6×	4 0.4×	4 0.7×	2	109
Nihan S. Pol United States	6	149 0.8×	25 1.1×	24 1.4×	10 1.0×	11 1.8×	12	154
Kaitlyn Shin United States	3	188 1.0×	21 1.0×	7 0.4×	8 0.8×	3 0.5×	5	189
Z. L. Yang China	5	105 0.6×	14 0.6×	18 1.1×	12 1.2×	7 1.2×	12	112
Phrudth Jaroenjittichai Thailand	4	80 0.4×	20 0.9×	13 0.8×	6 0.6×	4 0.7×	17	86
Megan E. DeCesar United States	8	137 0.7×	51 2.3×	17 1.0×	20 2.0×	7 1.2×	14	140
Ü. Kızıloğlu Türkiye	6	114 0.6×	28 1.3×	7 0.4×	18 1.8×	8 1.3×	21	118
Mouza Almualla United States	6	149 0.8×	47 2.1×	8 0.5×	7 0.7×	4 0.7×	7	162
A. Yu. Kirichenko Russia	7	128 0.7×	23 1.0×	14 0.8×	17 1.7×	2 0.3×	18	130

Countries citing papers authored by M. Benacquista

Since Specialization

Citations

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

Fields of papers citing papers by M. Benacquista

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Benacquista

This figure shows the co-authorship network connecting the top 25 collaborators of M. Benacquista. A scholar is included among the top collaborators of M. Benacquista 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. Benacquista. M. Benacquista 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:

10 of 10 papers shown

1.

Belczyński, Krzysztof, Abbas Askar, Manuel Arca Sedda, et al.. (2018). The origin of the first neutron star – neutron star merger. Astronomy and Astrophysics. 615. A91–A91. 72 indexed citations

2.

Sedda, Manuel Arca & M. Benacquista. (2018). Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources. Monthly Notices of the Royal Astronomical Society. 36 indexed citations

3.

Grudzińska, M., Krzysztof Belczyński, J. Casares, et al.. (2015). On the formation and evolution of the first Be star in a black hole binary MWC 656. Monthly Notices of the Royal Astronomical Society. 452(3). 2773–2787. 21 indexed citations

4.

Benacquista, M., Krzysztof Belczyński, M. Beroiz, et al.. (2014). A program for optical observations of advanced LIGO early triggers in the southern hemisphere. EAS Publications Series. 67-68. 357–358.

5.

Benacquista, M. & Kelly Holley‐Bockelmann. (2006). Consequences of Disk Scale Height onLISAConfusion Noise from Close White Dwarf Binaries. The Astrophysical Journal. 645(1). 589–596. 23 indexed citations

6.

Benacquista, M., et al.. (2004). Gravitational Radiation from Pulsating Magnetic White Dwarfs. Astrophysics. 47(3). 324–334. 2 indexed citations

7.

Benacquista, M., et al.. (2003). Gravitational Radiation from Pulsating White Dwarfs. The Astrophysical Journal. 596(2). L223–L226. 8 indexed citations

8.

Седракян, Д. М., et al.. (2003). Gravitational Radiation from Fluctuations in Rotating Neutron Stars. Astrophysics. 46(4). 445–454. 8 indexed citations

9.

Benacquista, M.. (2001). Detecting eccentric globular cluster binaries with LISA. AIP conference proceedings. 586. 793–795. 5 indexed citations

10.

Benacquista, M. & Kenneth Nordtvedt. (1988). A many-body Lagrangian for celestial body dynamics to second post-Newtonian linear field order. The Astrophysical Journal. 328. 588–588. 9 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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