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).
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.
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
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
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.
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
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
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.