Eduardo Bravo

2.9k total citations · 1 hit paper
75 papers, 1.7k citations indexed

About

Eduardo Bravo is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Radiation. According to data from OpenAlex, Eduardo Bravo has authored 75 papers receiving a total of 1.7k indexed citations (citations by other indexed papers that have themselves been cited), including 65 papers in Astronomy and Astrophysics, 34 papers in Nuclear and High Energy Physics and 5 papers in Radiation. Recurrent topics in Eduardo Bravo's work include Gamma-ray bursts and supernovae (59 papers), Astro and Planetary Science (24 papers) and Astrophysics and Cosmic Phenomena (19 papers). Eduardo Bravo is often cited by papers focused on Gamma-ray bursts and supernovae (59 papers), Astro and Planetary Science (24 papers) and Astrophysics and Cosmic Phenomena (19 papers). Eduardo Bravo collaborates with scholars based in Spain, United States and Japan. Eduardo Bravo's co-authors include Carles Badenes, G. Martı́nez-Pinedo, Domingo Garcı́a-Senz, John P. Hughes, W. R. Hix, K. Langanke, N. T. Zinner, Carla Fröhlich, F.‐K. Thielemann and M. Liebendörfer and has published in prestigious journals such as Nature, Physical Review Letters and The Astrophysical Journal.

In The Last Decade

Eduardo Bravo

68 papers receiving 1.6k 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.

Neutrino-Induced Nucleosynthesis ofA>64Nuclei: TheνpProcess

2006 379 citations Carla Fröhlich, G. Martı́nez-Pinedo et al. profile →

Peers

Eduardo Bravo

AA

NHEP

RADIA

AMPO

INSTR

Aimee Hungerford United States

V. Tatischeff France

S. Palmerini Italy

Jennifer Barnes United States

I. V. Panov Russia

Y.‐Z. Qian United States

Z. Meisel United States

K. D. Küntz United States

P. M. Rodriguez‐Pascual Spain

K. Farouqi Germany

Aimee Hungerford United States

Eduardo Bravo

840 ×0.6

AA

423 ×0.4

NHEP

49 ×0.5

RADIA

75 ×1.0

AMPO

38 ×0.7

INSTR

Citations per year, relative to Eduardo Bravo Eduardo Bravo (= 1×) peers Aimee Hungerford

Countries citing papers authored by Eduardo Bravo

Since Specialization

Citations

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

Fields of papers citing papers by Eduardo Bravo

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Eduardo Bravo

This figure shows the co-authorship network connecting the top 25 collaborators of Eduardo Bravo. A scholar is included among the top collaborators of Eduardo Bravo 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 Eduardo Bravo. Eduardo Bravo 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

1.

Bravo, Eduardo, et al.. (2024). Birdwatching as an Alternative for Forest Conservation. Revista de Gestão Social e Ambiental. 18(12). e010396–e010396.

2.

Badenes, Carles, et al.. (2024). SNR 0519−69.0 as a Type Ia Explosion in a Planetary Nebula Cocoon. Research Notes of the AAS. 8(12). 309–309. 1 indexed citations

3.

Badenes, Carles, et al.. (2024). Do Type Ia Supernovae Explode inside Planetary Nebulae?. The Astrophysical Journal. 962(1). 63–63. 5 indexed citations

4.

Piersanti, L., L. R. Yungelson, & Eduardo Bravo. (2024). Expected evolution of the binary system PTF J2238+743015.1. Astronomy and Astrophysics. 689. A287–A287. 3 indexed citations

5.

Bravo, Eduardo, J. Isern, & L. Piersanti. (2024). Type Ia supernovae from chemically segregated white dwarfs. Astronomy and Astrophysics. 683. A237–A237. 1 indexed citations

6.

Blondin, S., Eduardo Bravo, F. X. Timmes, Luc Dessart, & D. J. Hillier. (2022). Stable nickel production in type Ia supernovae: A smoking gun for the progenitor mass?. Astronomy and Astrophysics. 660. A96–A96. 13 indexed citations

7.

Piersanti, L., Eduardo Bravo, O. Straniero, S. Cristallo, & I. Domı́nguez. (2022). Pre-explosive Accretion and Simmering Phases of SNe Ia. The Astrophysical Journal. 926(1). 103–103. 7 indexed citations

8.

Bravo, Eduardo, L. Piersanti, S. Blondin, et al.. (2022). Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints. Monthly Notices of the Royal Astronomical Society Letters. 517(1). L31–L35. 6 indexed citations

9.

McWilliam, Andrew, Anthony L. Piro, Carles Badenes, & Eduardo Bravo. (2018). Evidence for a Sub-Chandrasekhar-mass Type Ia Supernova in the Ursa Minor Dwarf Galaxy. The Astrophysical Journal. 857(2). 97–97. 23 indexed citations

10.

Yamaguchi, Hiroya, John P. Hughes, Carles Badenes, et al.. (2017). THE ORIGIN OF THE IRON-RICH KNOT IN TYCHO’S SUPERNOVA REMNANT. The Astrophysical Journal. 834(2). 124–124. 22 indexed citations

11.

Yamaguchi, Hiroya, Carles Badenes, Adam Foster, et al.. (2015). A CHANDRASEKHAR MASS PROGENITOR FOR THE TYPE Ia SUPERNOVA REMNANT 3C 397 FROM THE ENHANCED ABUNDANCES OF NICKEL AND MANGANESE. The Astrophysical Journal Letters. 801(2). L31–L31. 64 indexed citations

12.

Churazov, E., R. Sunyaev, J. Isern, et al.. (2015). GAMMA RAYS FROM TYPE Ia SUPERNOVA SN 2014J. The Astrophysical Journal. 812(1). 62–62. 24 indexed citations

13.

Churazov, E., R. Sunyaev, J. Isern, et al.. (2014). Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J. Nature. 512(7515). 406–408. 83 indexed citations

14.

Bravo, Eduardo. (2012). Benjamin Lacombe: ilustración para aprender a ser adultos. 40–45.

15.

Isern, J., P. Jean, Eduardo Bravo, et al.. (2011). Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI. ATel. 3683. 1. 1 indexed citations

16.

Bravo, Eduardo, et al.. (2007). A three-dimensional picture of the delayed-detonation model of type Ia supernovae. Springer Link (Chiba Institute of Technology). 18 indexed citations

17.

Bravo, Eduardo, et al.. (2007). Photons and Positrons in Type Ia Supernovae. ASPC. 372. 407.

18.

Bravo, Eduardo, et al.. (2005). Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants .. Memorie della Societa Astronomica Italiana. 76(3). 555–559.

19.

Fröhlich, Carla, Peter C. Hauser, G. Martı́nez-Pinedo, et al.. (2004). Composition of the Innermost Supernova Ejecta. arXiv (Cornell University). 1 indexed citations

20.

Bravo, Eduardo, J. Isern, R. Canal, & J. Labay. (1992). On the contribution of Ne-22 to the synthesis of Fe-54 and Ni-58 in thermonuclear supernovae. A&A. 257(2). 534–538. 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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