A. Ibarra

2.8k total citations
26 papers, 221 citations indexed

About

A. Ibarra is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Nuclear and High Energy Physics. According to data from OpenAlex, A. Ibarra has authored 26 papers receiving a total of 221 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 8 papers in Computational Mechanics and 7 papers in Nuclear and High Energy Physics. Recurrent topics in A. Ibarra's work include Astrophysical Phenomena and Observations (15 papers), Astronomical Observations and Instrumentation (8 papers) and Gamma-ray bursts and supernovae (6 papers). A. Ibarra is often cited by papers focused on Astrophysical Phenomena and Observations (15 papers), Astronomical Observations and Instrumentation (8 papers) and Gamma-ray bursts and supernovae (6 papers). A. Ibarra collaborates with scholars based in Spain, United Kingdom and United States. A. Ibarra's co-authors include E. Kuulkers, Jan‐Uwe Ness, A. M. T. Pollock, C. Gabriel, K. L. Page, P. A. Evans, J. P. Osborne, R. D. Saxton, J. Chenevez and A. J. van der Horst and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Annals of Nuclear Energy.

In The Last Decade

A. Ibarra

23 papers receiving 215 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. Ibarra Spain 8 195 70 23 21 15 26 221
C. Bartolini Italy 8 201 1.0× 41 0.6× 17 0.7× 19 0.9× 20 1.3× 40 219
Ole König Germany 9 195 1.0× 62 0.9× 24 1.0× 11 0.5× 13 0.9× 20 203
M. Tripiciano Italy 4 216 1.1× 78 1.1× 23 1.0× 40 1.9× 15 1.0× 5 233
A. Belinski Russia 10 266 1.4× 50 0.7× 8 0.3× 14 0.7× 41 2.7× 50 287
Sebastian Falkner United States 10 265 1.4× 88 1.3× 20 0.9× 87 4.1× 38 2.5× 15 271
Shri Kulkarni United States 8 230 1.2× 23 0.3× 5 0.2× 18 0.9× 23 1.5× 17 254
C. Graziani United States 8 229 1.2× 81 1.2× 3 0.1× 11 0.5× 8 0.5× 17 249
Kwan-Lok Li Taiwan 11 256 1.3× 125 1.8× 7 0.3× 43 2.0× 9 0.6× 37 272
R. M. Bandyopadhyay United States 9 259 1.3× 85 1.2× 25 1.1× 24 1.1× 25 1.7× 15 268
А. В. Додин Russia 11 301 1.5× 45 0.6× 6 0.3× 8 0.4× 24 1.6× 51 325

Countries citing papers authored by A. Ibarra

Since Specialization
Citations

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

Fields of papers citing papers by A. Ibarra

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. Ibarra

This figure shows the co-authorship network connecting the top 25 collaborators of A. Ibarra. A scholar is included among the top collaborators of A. Ibarra 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 A. Ibarra. A. Ibarra 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.
Mao, Junjie, J. S. Kaastra, M. Guainazzi, et al.. (2019). CIELO-RGS: a catalog of soft X-ray ionized emission lines. Springer Link (Chiba Institute of Technology). 3 indexed citations
2.
Ness, Jan‐Uwe, A. Ibarra, R. D. Saxton, et al.. (2019). Towards a better coordination of multimessenger observations.. Memorie della Societa Astronomica Italiana. 90. 110. 1 indexed citations
3.
Arviset, C., et al.. (2015). Long-term Preservation of Data Analysis Capabilities. ASPC. 495. 245. 1 indexed citations
4.
Vries, C. P. de, J. W. den Herder, C. Gabriel, et al.. (2014). Calibration and in-orbit performance of the reflection grating spectrometer onboardXMM-Newton. Astronomy and Astrophysics. 573. A128–A128. 19 indexed citations
5.
Kuulkers, E., Jan‐Uwe Ness, A. Ibarra, et al.. (2013). XMM-Newton X-ray pre-nova detection and current Swift non-detection of PNV J13544700-5909080 (= Nova Cen 2013). The astronomer's telegram. 5628. 1. 1 indexed citations
6.
Kuulkers, E., C. Kouveliotou, T. Belloni, et al.. (2013). MAXI J1659−152: the shortest orbital period black-hole transient in outburst. Astronomy and Astrophysics. 552. A32–A32. 61 indexed citations
7.
Martín-Carrillo, A., Marcus Kirsch, I. Caballero, et al.. (2012). The relative and absolute timing accuracy of the EPIC-pn camera onXMM-Newton, from X-ray pulsations of the Crab and other pulsars. Astronomy and Astrophysics. 545. A126–A126. 17 indexed citations
8.
Bel, M. Cadolle, E. Kuulkers, A. Ibarra, et al.. (2010). Simultaneous INTEGRAL, RXTE, Swift and FT South observations of the transition of GX 339-4. The astronomer's telegram. 2573. 1.
9.
Ibarra, A., E. Kuulkers, J. P. Osborne, et al.. (2009). Pre-nova X-ray observations of V2491 Cygni (Nova Cyg 2008b). Astronomy and Astrophysics. 497(1). L5–L8. 15 indexed citations
10.
Ibarra, A. & E. Kuulkers. (2008). X-ray identification of the prenova of V2491 Cyg. The astronomer's telegram. 1473. 1. 1 indexed citations
11.
Osborne, J. P., K. L. Page, P. A. Evans, et al.. (2008). Nova V2491 Cyg has become a bright super-soft source. ATel. 1542. 1. 2 indexed citations
12.
Page, K. L., J. P. Osborne, P. A. Evans, et al.. (2008). Swift X-ray and UV evolution of nova V2491 Cyg 7-34 days after eruption. ATel. 1523. 1. 1 indexed citations
13.
Ibarra, A., E. Kuulkers, A. P. Beardmore, et al.. (2008). The persistent, spectral variable pre-nova X-ray source in V2491 Cyg: Swift J194302.1+321913. The astronomer's telegram. 1478. 1. 1 indexed citations
14.
Kuulkers, E., A. Ibarra, K. L. Page, et al.. (2008). Swift and MERLIN observations of Swift J194302.1+321913 during the nova outburst of V2491 Cyg. Research Explorer (The University of Manchester). 1480. 1. 1 indexed citations
15.
Read, A. M., R. D. Saxton, J. P. Osborne, et al.. (2007). XMM-Newton and Swift-XRT see declining X-ray flux from the nova XMMSL1 J070542.7-381442 (V598 Pup). The astronomer's telegram. 1301. 1. 1 indexed citations
16.
Ibarra, A., G. Matt, M. Guainazzi, et al.. (2006). The XMM-Newton/INTEGRAL monitoring campaign of IGR J16318-4848. Springer Link (Chiba Institute of Technology). 9 indexed citations
17.
Ibarra, A., et al.. (2006). Optimizing SAS tasks for Grid Architectures. 351. 520. 1 indexed citations
18.
Gabriel, C., et al.. (2004). The XMM-Newton SAS - Distributed Development and Maintenance of a Large Science Analysis System: A Critical Analysis. ASPC. 314. 759. 17 indexed citations
19.
Queral, César, et al.. (2004). Simulation of Accident Sequences Including Emergency Operating Procedures. OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information). 1 indexed citations
20.
Hidalgo, J. Ignacio, Juan Lanchares, A. Ibarra, & R. Hermida. (2003). A hybrid evolutionary algorithm for Multi-FPGA systems design. 60–67. 5 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