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.
Identification of two classes of gamma-ray bursts
19931.0k citationsC. Kouveliotou, Charles A. Meegan et al.profile →
An X-ray pulsar with a superstrong magnetic field in the soft γ-ray repeater SGR1806 − 20
1998613 citationsC. Kouveliotou, S. Dieters et al.Natureprofile →
Discovery of Intense Gamma-Ray Flashes of Atmospheric Origin
1994576 citationsG. J. Fishman, P. N. Bhat et al.profile →
Spatial distribution of γ-ray bursts observed by BATSE
1992283 citationsC. Meegan, G. J. Fishman et al.Natureprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
hero ref
This map shows the geographic impact of G. J. Fishman'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 G. J. Fishman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. J. Fishman more than expected).
This network shows the impact of papers produced by G. J. Fishman. 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 G. J. Fishman. The network helps show where G. J. Fishman may publish in the future.
Co-authorship network of co-authors of G. J. Fishman
This figure shows the co-authorship network connecting the top 25 collaborators of G. J. Fishman.
A scholar is included among the top collaborators of G. J. Fishman 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 G. J. Fishman. G. J. Fishman 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.
Briggs, M. S., V. Connaughton, M. Stanbro, et al.. (2015). The First Fermi Gamma-ray Burst Monitor (GBM) Terrestrial Gamma-ray Flash (TGF) Catalog. EGUGA. 9961.2 indexed citations
2.
Kouveliotou, C., C. Kouveliotou, R. W. Klebesadel, et al.. (2012). Gamma-ray Bursts. Cambridge University Press eBooks.18 indexed citations
Fishman, G. J., S. McBreen, M. S. Briggs, et al.. (2008). SGR 0501+4516: Fermi GBM (formerly GLAST burst monitor) observations of three exceptionally intense outbursts.. GRB Coordinates Network. 8139. 1.1 indexed citations
Kippen, R. M., Robert S. Mallozzi, & G. J. Fishman. (2000). Gamma-ray bursts : 5th Huntsville Symposium, Huntsville, Alabama, 18-22 October 1999. American Institute of Physics eBooks.3 indexed citations
7.
Fishman, G. J.. (1998). Gamma-Ray Bursts. 115.2 indexed citations
8.
Kouveliotou, C., S. Dieters, Tod E. Strohmayer, et al.. (1998). An X-ray pulsar with a superstrong magnetic field in the soft γ-ray repeater SGR1806 − 20. Nature. 393(6682). 235–237.613 indexed citations breakdown →
9.
Hartmann, D. H., M. S. Briggs, W. S. Pačiesas, et al.. (1996). Testing the Dipole and Quadrupole Moments of Galactic Models. TigerPrints (Clemson University).1 indexed citations
10.
Vikhlinin, A., R. Sunyaev, E. Churazov, et al.. (1996). Cygnus X-1. International Astronomical Union Circular. 5576. 1.1 indexed citations
11.
Harmon, B. A., W. S. Pačiesas, G. J. Fishman, et al.. (1996). Low state hard X-ray outburst from the X-ray burster 4U 1608-522 observed by BATSE/CGRO.. 120. 279–282.1 indexed citations
12.
Rubin, B. C., F. Lei, G. J. Fishman, et al.. (1996). A model of the gamma-ray background on the BATSE experiment.. 120. 687–690.1 indexed citations
13.
Pendleton, Geoffrey N., W. S. Pačiesas, Robert S. Mallozzi, et al.. (1995). The detector response matrices of the burst and transient source experiment (BATSE) on the Compton Gamma Ray Observatory. Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment.2 indexed citations
14.
Fishman, G. J.. (1994). Gamma-ray bursts : second workshop, Huntsville, AL, October 1993. American Institute of Physics eBooks.1 indexed citations
15.
Kouveliotou, C., W. S. Pačiesas, G. J. Fishman, C. Meegan, & Robert Wilson. (1993). Gamma-ray burst color-color diagrams.. Astronomy & Astrophysics Supplement Series. 97(1). 55–57.
16.
Pačiesas, W. S., B. A. Harmon, G. N. Pendleton, et al.. (1993). Studies of hard X-ray source variability using BATSE.. Astronomy & Astrophysics Supplement Series. 97(1). 253–255.2 indexed citations
17.
Pačiesas, W. S. & G. J. Fishman. (1992). Gamma-ray bursts, Huntsville, AL 1991. American Institute of Physics eBooks.7 indexed citations
18.
Meegan, C., G. J. Fishman, Robert Wilson, et al.. (1992). Gamma-Ray Bursts. International Astronomical Union Circular. 3025. 1.12 indexed citations
19.
Pendleton, G. N., W. S. Pačiesas, R. B. Wilson, G. J. Fishman, & C. Meegan. (1989). Hard X-Ray Continuum Spectra of SN1987A. Bulletin of the American Astronomical Society. 21. 1214.1 indexed citations
20.
Pačiesas, W. S., et al.. (1988). Observations of Hard X-ray Continuum Emission from SN1987A. Bulletin of the American Astronomical Society. 20. 726.
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.