B. Paul

25.5k total citations
36 papers, 436 citations indexed

About

B. Paul is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, B. Paul has authored 36 papers receiving a total of 436 indexed citations (citations by other indexed papers that have themselves been cited), including 27 papers in Astronomy and Astrophysics, 14 papers in Nuclear and High Energy Physics and 12 papers in Geophysics. Recurrent topics in B. Paul's work include Astrophysical Phenomena and Observations (26 papers), Pulsars and Gravitational Waves Research (13 papers) and High-pressure geophysics and materials (12 papers). B. Paul is often cited by papers focused on Astrophysical Phenomena and Observations (26 papers), Pulsars and Gravitational Waves Research (13 papers) and High-pressure geophysics and materials (12 papers). B. Paul collaborates with scholars based in India, Japan and Italy. B. Paul's co-authors include P. C. Agrawal, A. R. Rao, Sachindra Naik, J. S. Yadav, S. Seetha, Shunji Kitamoto, K. Kasturirangan, Ranjeev Misra, R. Manchanda and H. M. Antia 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

B. Paul

33 papers receiving 417 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
B. Paul India 14 403 122 110 42 30 36 436
Jonathan Woo United States 13 375 0.9× 118 1.0× 127 1.2× 46 1.1× 25 0.8× 23 427
K. Makishima Japan 13 326 0.8× 100 0.8× 71 0.6× 27 0.6× 20 0.7× 40 354
H. Huckle United Kingdom 8 522 1.3× 172 1.4× 74 0.7× 34 0.8× 32 1.1× 11 549
Adrienne M. Juett United States 14 548 1.4× 96 0.8× 132 1.2× 50 1.2× 17 0.6× 16 565
Biswajit Paul India 13 343 0.9× 92 0.8× 124 1.1× 32 0.8× 36 1.2× 43 366
M. Bałucińska‐Church United Kingdom 16 501 1.2× 141 1.2× 89 0.8× 100 2.4× 31 1.0× 39 505
D. Pandel United States 9 595 1.5× 216 1.8× 98 0.9× 30 0.7× 21 0.7× 12 613
Sachindra Naik India 16 715 1.8× 237 1.9× 167 1.5× 60 1.4× 30 1.0× 86 755
T. Kennedy United Kingdom 5 480 1.2× 160 1.3× 56 0.5× 34 0.8× 19 0.6× 10 503
K. Mitsuda Japan 11 601 1.5× 167 1.4× 131 1.2× 107 2.5× 30 1.0× 24 627

Countries citing papers authored by B. Paul

Since Specialization
Citations

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

Fields of papers citing papers by B. Paul

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of B. Paul

This figure shows the co-authorship network connecting the top 25 collaborators of B. Paul. A scholar is included among the top collaborators of B. Paul 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 B. Paul. B. Paul 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.
Bhaduri, Partha Pratim, et al.. (2025). A systematic study of initial state quark energy loss in fixed target proton nucleus collisions. The European Physical Journal C. 85(3). 1 indexed citations
2.
Paul, B.. (2022). $\psi$(2S) production and nuclear modification factor in nucleus-nucleus collisions with ALICE. Proceedings of 41st International Conference on High Energy physics — PoS(ICHEP2022). 445–445. 1 indexed citations
3.
Paul, B.. (2017). Charmonium production in Pb-Pb collisions at and 5.02 TeV with ALICE. Journal of Physics Conference Series. 779. 12037–12037. 2 indexed citations
4.
Bozzo, E., et al.. (2017). Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind?. Astronomy and Astrophysics. 610. A50–A50. 14 indexed citations
5.
Yadav, J. S., P. C. Agrawal, H. M. Antia, et al.. (2017). Large Area X-Ray Proportional Counter Instrument on AstroSat. Current Science. 113(4). 591–591. 13 indexed citations
6.
Yadav, J. S., P. C. Agrawal, H. M. Antia, et al.. (2016). Large Area X-ray Proportional Counter (LAXPC) instrument onboard ASTROSAT. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 9905. 99051D–99051D. 69 indexed citations
7.
Jain, Chetana, et al.. (2014). Torque reversals and pulse profile of the pulsar 4U 1626-67. Monthly Notices of the Royal Astronomical Society. 439(2). 1940–1947. 19 indexed citations
8.
Naik, Sachindra, Mousumi Das, Chetana Jain, & B. Paul. (2010). An X-ray bright nucleus in the low-surface-brightness galaxy UGC 6614. Monthly Notices of the Royal Astronomical Society. 7 indexed citations
9.
Naik, Sachindra, et al.. (2008). Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion. Advances in Space Research. 43(6). 900–904. 5 indexed citations
10.
Paul, B., et al.. (2006). Variable Quasi Periodic Oscillations during an outburst of the transient X-ray pulsar XTE J1858 + 034. Journal of Astrophysics and Astronomy. 27(1). 25–35. 6 indexed citations
11.
Paul, B., et al.. (2005). X-ray properties of the transient pulsar 3A 0535+262 in quiescence. Springer Link (Chiba Institute of Technology). 21 indexed citations
12.
Paul, B., Sachindra Naik, & N. Bhatt. (2004). Soft excess and orbital evolution studies of X-ray pulsars with BeppoSAX. Nuclear Physics B - Proceedings Supplements. 132. 548–553. 5 indexed citations
13.
Bhatt, N., et al.. (2003). Orbital Evolution of the Binary X-ray Pulsar Her X-1. Bulletin of the Astronomical Society of India. 31. 367–368. 1 indexed citations
14.
Naik, Sachindra, et al.. (2002). New measurements of orbital period change in Cygnus X-3. Springer Link (Chiba Institute of Technology). 34 indexed citations
15.
Naik, Sachindra, P. C. Agrawal, A. R. Rao, & B. Paul. (2002). X-ray properties of the microquasar GRS 1915105 during a variability class transition. Monthly Notices of the Royal Astronomical Society. 330(2). 487–496. 13 indexed citations
16.
Mukerjee, K., P. C. Agrawal, B. Paul, et al.. (2001). Pulse Characteristics of the X‐Ray Pulsar 4U 1907+09. The Astrophysical Journal. 548(1). 368–376. 18 indexed citations
17.
Paul, B., Shunji Kitamoto, & Fumiaki Makino. (2000). Changes in the Long‐Term Intensity Variations in Cygnus X‐2 and LMC X‐3. The Astrophysical Journal. 528(1). 410–417. 25 indexed citations
18.
Rao, A. R., P. C. Agrawal, & B. Paul. (1997). Observations of Cygnus X-1 during the two spectral states with the Indian X-ray Astronomy Experiment (IXAE). arXiv (Cornell University). 330(1). 181–188. 1 indexed citations
19.
Agrawal, P. C., B. Paul, A. R. Rao, et al.. (1996). X-Ray Astronomy Experiment on the Indian Satellite IRS-P3. Journal of The Korean Astronomical Society. 29. 429–432. 3 indexed citations
20.
Rao, A. R., B. Paul, V. R. Chitnis, P. C. Agrawal, & R. Manchanda. (1994). Detection of a very low hard X-ray pulse fraction in the bright state of GX 1+4.. A&A. 289.

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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