J. B. Stephen

7.3k total citations
180 papers, 2.5k citations indexed

About

J. B. Stephen is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Radiation. According to data from OpenAlex, J. B. Stephen has authored 180 papers receiving a total of 2.5k indexed citations (citations by other indexed papers that have themselves been cited), including 111 papers in Astronomy and Astrophysics, 101 papers in Nuclear and High Energy Physics and 66 papers in Radiation. Recurrent topics in J. B. Stephen's work include Astrophysical Phenomena and Observations (90 papers), Particle Detector Development and Performance (58 papers) and Advanced Semiconductor Detectors and Materials (57 papers). J. B. Stephen is often cited by papers focused on Astrophysical Phenomena and Observations (90 papers), Particle Detector Development and Performance (58 papers) and Advanced Semiconductor Detectors and Materials (57 papers). J. B. Stephen collaborates with scholars based in Italy, United Kingdom and France. J. B. Stephen's co-authors include L. Bassani, A. Malizia, A. Bazzano, P. Ubertini, A. J. Bird, E. Caroli, G. Di Cocco, A. Spizzichino, L. Natalucci and A. J. Dean and has published in prestigious journals such as Nature, Science and Journal of Applied Physics.

In The Last Decade

J. B. Stephen

167 papers receiving 2.4k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
J. B. Stephen Italy 25 1.9k 1.1k 515 370 227 180 2.5k
G. Di Cocco Italy 18 1.9k 1.0× 1.2k 1.1× 368 0.7× 139 0.4× 160 0.7× 100 2.4k
E. Costa Italy 25 3.0k 1.6× 1.5k 1.3× 487 0.9× 180 0.5× 128 0.6× 228 3.5k
W. N. Johnson United States 26 1.9k 1.0× 1.3k 1.2× 540 1.0× 148 0.4× 200 0.9× 140 2.5k
G. K. Skinner United Kingdom 21 1.2k 0.6× 510 0.5× 266 0.5× 79 0.2× 155 0.7× 112 1.5k
R. Willingale United Kingdom 31 2.5k 1.3× 1.1k 1.0× 230 0.4× 90 0.2× 101 0.4× 155 2.8k
D. Stutman United States 25 652 0.3× 1.6k 1.4× 418 0.8× 199 0.5× 421 1.9× 147 2.0k
Stephen L. O’Dell United States 24 2.1k 1.1× 1.2k 1.1× 387 0.8× 270 0.7× 139 0.6× 202 2.6k
G. A. Wurden United States 27 884 0.5× 1.8k 1.6× 177 0.3× 439 1.2× 212 0.9× 152 2.2k
L. Natalucci Italy 19 1.1k 0.6× 381 0.3× 221 0.4× 82 0.2× 215 0.9× 114 1.4k
L. Piro Italy 30 4.1k 2.2× 1.5k 1.4× 167 0.3× 115 0.3× 149 0.7× 241 4.3k

Countries citing papers authored by J. B. Stephen

Since Specialization
Citations

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

Fields of papers citing papers by J. B. Stephen

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by J. B. Stephen. 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 J. B. Stephen. The network helps show where J. B. Stephen may publish in the future.

Co-authorship network of co-authors of J. B. Stephen

This figure shows the co-authorship network connecting the top 25 collaborators of J. B. Stephen. A scholar is included among the top collaborators of J. B. Stephen 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 J. B. Stephen. J. B. Stephen 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.
Silva, R. M. Curado da, J.M. Maia, E. Caroli, et al.. (2021). Polarimetry With a Multilayer CdTe Prototype for Soft Gamma-Ray Astrophysics. IEEE Transactions on Nuclear Science. 68(11). 2655–2660. 2 indexed citations
2.
Malizia, A., L. Bassani, J. B. Stephen, A. Bazzano, & P. Ubertini. (2020). X-ray absorption in INTEGRAL active galactic nuclei. Springer Link (Chiba Institute of Technology). 6 indexed citations
3.
Ursini, F., L. Bassani, A. Malizia, et al.. (2019). The coronal temperature of NGC 4388 and NGC 2110 measured with INTEGRAL. Springer Link (Chiba Institute of Technology). 6 indexed citations
4.
Masetti, N., P. Parisi, E. Jiménez‐Bailón, et al.. (2012). Unveiling the nature of INTEGRAL objects through optical spectroscopy IX. Twenty two more identifications, and a glance into the far hard X-ray Universe. Americanae (AECID Library). 23 indexed citations
5.
Molina, M., R. Landi, L. Bassani, et al.. (2012). Flat-spectrum radio sources as likely counterparts of unidentified INTEGRAL sources. Springer Link (Chiba Institute of Technology). 4 indexed citations
6.
Parisi, P., N. Masetti, E. Jiménez‐Bailón, et al.. (2009). Accurate classification of 17 AGNs detected with\nSwift/BAT. Springer Link (Chiba Institute of Technology). 16 indexed citations
7.
Frontera, F., G. Loffredo, V. Carassiti, et al.. (2008). A gamma-ray Laue lens focusing telescope aboard a balloon experiment. Institutional Research Information System University of Ferrara (University of Ferrara). 79. 807. 4 indexed citations
8.
Masetti, N., S. A. Cellone, R. Landi, et al.. (2007). Identification of 2 INTEGRAL sources via Swift/XRT plus CASLEO followup. The astronomer's telegram. 1034. 1. 3 indexed citations
9.
Masetti, N., L. Bassani, A. Bazzano, et al.. (2006). Emission-line early-type stars as possible optical counterparts of INTEGRAL hard X-ray sources IGR J08408-4503 and IGR J15539-6142. ATel. 815. 1. 4 indexed citations
10.
Stephen, J. B., et al.. (2005). Photo Mosaics In Shallow Water Environments:Challenges And Results. WIT transactions on the built environment. 79. 1 indexed citations
11.
Malizia, A., L. Bassani, J. B. Stephen, et al.. (2005). The INTEGRAL/IBIS source AXJ1838.0-0655: a soft X-ray to TeV γ-ray broad band emitter. 1. 16 indexed citations
12.
Sguera, V., A. Malizia, L. Bassani, J. B. Stephen, & G. Di Cocco. (2004). 3EG J2027+3429: Another blazar behind the Galactic Plane. Springer Link (Chiba Institute of Technology). 5 indexed citations
13.
Malizia, A., L. Bassani, G. Di Cocco, et al.. (2004). IGR J16393-4643 a possible X-ray counterpart to 3EG J1639-4702 discovered by INTEGRAL.. The astronomer's telegram. 227(227). 1. 1 indexed citations
14.
Sordo, S. Del, G. Agnetta, B. Biondo, et al.. (2004). Spectroscopic performances of 16 × 16 pixel CZT imaging hard-X-ray detectors. 119(3). 257–270. 15 indexed citations
15.
Bassani, L., A. Malizia, J. B. Stephen, et al.. (2004). 17 New Identified INTEGRAL Sources. ATel. 232. 1. 1 indexed citations
16.
Cocco, G. Di, E. Caroli, L. Foschini, et al.. (2003). IBIS/PICsIT in-flight performances. Springer Link (Chiba Institute of Technology). 38 indexed citations
17.
Malaguti, G., A. Bazzano, A. J. Bird, et al.. (2003). In-flight calibrations of IBIS/PICsIT. Springer Link (Chiba Institute of Technology). 4 indexed citations
18.
Foschini, L., G. Di Cocco, Luis C. Ho, et al.. (2002). XMM–Newton observations of ultraluminous X–ray sources in nearby galaxies. Springer Link (Chiba Institute of Technology). 39 indexed citations
19.
Foschini, L., Luis C. Ho, N. Masetti, et al.. (2002). BL Lac identification for the ultraluminous X-ray source observed inthe direction of NGC 4698. Springer Link (Chiba Institute of Technology). 17 indexed citations
20.
O’Brien, P. T., J. N. Reeves, Martin Turner, et al.. (2001). XMM-Newton detection of a Comptonized accretion disc in the quasar PKS 0558-504. Springer Link (Chiba Institute of Technology). 21 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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