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.
BATSE observations of gamma-ray burst spectra. I - Spectral diversity
19931.2k citationsD. L. Band, J. L. Matteson et al.The Astrophysical Journalprofile →
Identification of two classes of gamma-ray bursts
19931.0k citationsC. Kouveliotou, Charles A. Meegan et al.The Astrophysical Journalprofile →
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 ·
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Countries citing papers authored by W. S. Pačiesas
Since
Specialization
Citations
This map shows the geographic impact of W. S. Pačiesas'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 W. S. Pačiesas with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. S. Pačiesas more than expected).
This network shows the impact of papers produced by W. S. Pačiesas. 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 W. S. Pačiesas. The network helps show where W. S. Pačiesas may publish in the future.
Co-authorship network of co-authors of W. S. Pačiesas
This figure shows the co-authorship network connecting the top 25 collaborators of W. S. Pačiesas.
A scholar is included among the top collaborators of W. S. Pačiesas 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 W. S. Pačiesas. W. S. Pačiesas is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Bhat, P. N., W. S. Pačiesas, & A. J. van der Horst. (2008). GRB 080905B: Fermi gamma-ray burst monitor detection.. GCN. 8205. 1.1 indexed citations
3.
Cherry, M. L., G. L. Case, J. Cravens, et al.. (2004). CASTER: A Scintillator-Based Black Hole Finder Probe. 8.1 indexed citations
4.
Briggs, M. S., D. L. Band, R. D. Preece, W. S. Pačiesas, & G. N. Pendleton. (1999). Analysis of Line Candidates in Gamma-Ray Bursts Observed by BATSE. CERN Bulletin. 39. 237.1 indexed citations
5.
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
6.
Harmon, B. A., W. S. Pačiesas, G. J. Fishman, et al.. (1996). Periodic transient hard X-ray emission from GRO 1849-03.. 120. 227–230.2 indexed citations
7.
Harmon, B. A., et al.. (1996). Deep search for celestial hard X-ray emission by earth occultation with BATSE/CGRO.. Astronomy & Astrophysics Supplement Series. 120. 137–140.1 indexed citations
8.
Vikhlinin, A., R. Sunyaev, E. Churazov, et al.. (1996). Cygnus X-1. International Astronomical Union Circular. 5576. 1.1 indexed citations
9.
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
10.
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
11.
Band, D. L., J. L. Matteson, W. S. Pačiesas, et al.. (1996). BATSE Observations of Gamma-Ray Burst Spectra. The Astrophysical Journal. 473(1).55 indexed citations
12.
Митрофанов, И. Г., et al.. (1995). Statistical analysis of flux variability and energy spectra of cosmic gamma-ray bursts observed with the BATSE Experiment of the Compton Observatory. AZh. 72. 344.1 indexed citations
13.
Koshut, T. M., W. S. Pačiesas, C. Kouveliotou, et al.. (1995). T 90 as a Measurment of the Duration of GRBs. AAS. 186.1 indexed citations
14.
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
15.
Hurley, K., M. Sommer, M. Boër, et al.. (1993). Ulysses precise localizations of gamma-ray bursts. Astronomy & Astrophysics Supplement Series. 97(1). 39–41.2 indexed citations
16.
Bhat, P. N., G. J. Fishman, C. Meegan, et al.. (1992). Evidence of sub-millisecond structure in a gamma-ray burst. Nature. 359(6392).1 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.
Pačiesas, W. S., et al.. (1988). Observations of Hard X-ray Continuum Emission from SN1987A. Bulletin of the American Astronomical Society. 20. 726.
20.
Matteson, J. L., R. F. Mushotzky, W. S. Pačiesas, & J. G. Laros. (1976). Intensity and Spectral Variations of Cyg X-1 Observed from Balloons. Bulletin of the American Astronomical Society. 389. 407–424.
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.