G. P. Garmire

22.0k total citations · 3 hit papers
281 papers, 10.0k citations indexed

About

G. P. Garmire is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Radiation. According to data from OpenAlex, G. P. Garmire has authored 281 papers receiving a total of 10.0k indexed citations (citations by other indexed papers that have themselves been cited), including 234 papers in Astronomy and Astrophysics, 113 papers in Nuclear and High Energy Physics and 33 papers in Radiation. Recurrent topics in G. P. Garmire's work include Astrophysical Phenomena and Observations (156 papers), Astrophysics and Cosmic Phenomena (99 papers) and Gamma-ray bursts and supernovae (68 papers). G. P. Garmire is often cited by papers focused on Astrophysical Phenomena and Observations (156 papers), Astrophysics and Cosmic Phenomena (99 papers) and Gamma-ray bursts and supernovae (68 papers). G. P. Garmire collaborates with scholars based in United States, United Kingdom and Netherlands. G. P. Garmire's co-authors include W. N. Brandt, Eric D. Feigelson, Patrick S. Broos, Leisa K. Townsley, G. Chartas, J. A. Nousek, A. E. Hornschemeier, G. Ricker, F. E. Bauer and M. W. Bautz and has published in prestigious journals such as Nature, Science and Journal of Geophysical Research Atmospheres.

In The Last Decade

G. P. Garmire

267 papers receiving 9.7k citations

Hit Papers

An Overview of the Performance and Scientific Results fro... 2002 2026 2010 2018 2002 2003 2003 100 200 300 400

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
G. P. Garmire United States 55 9.5k 3.6k 899 457 423 281 10.0k
K. Nandra United States 52 10.0k 1.1× 3.7k 1.0× 1.3k 1.5× 274 0.6× 517 1.2× 239 10.4k
J. C. Raymond United States 57 12.7k 1.3× 4.0k 1.1× 279 0.3× 505 1.1× 845 2.0× 459 13.4k
Julian H. Krolik United States 56 10.0k 1.0× 3.4k 0.9× 857 1.0× 477 1.0× 404 1.0× 197 10.4k
R. F. Mushotzky United States 65 14.5k 1.5× 5.9k 1.6× 1.6k 1.8× 225 0.5× 554 1.3× 396 14.9k
J. S. Kaastra Netherlands 51 8.2k 0.9× 2.8k 0.8× 551 0.6× 259 0.6× 975 2.3× 331 8.8k
J. E. Grindlay United States 44 6.5k 0.7× 2.0k 0.5× 373 0.4× 1.2k 2.5× 357 0.8× 418 7.3k
J. Greiner Germany 44 5.8k 0.6× 1.9k 0.5× 403 0.4× 333 0.7× 263 0.6× 388 6.2k
M. Elvis United States 57 11.8k 1.2× 4.7k 1.3× 1.4k 1.5× 137 0.3× 417 1.0× 351 12.1k
W. N. Brandt United States 68 16.5k 1.7× 5.6k 1.6× 3.1k 3.5× 294 0.6× 573 1.4× 406 16.8k
E. Churazov Germany 52 8.5k 0.9× 3.3k 0.9× 904 1.0× 437 1.0× 254 0.6× 343 8.8k

Countries citing papers authored by G. P. Garmire

Since Specialization
Citations

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

Fields of papers citing papers by G. P. Garmire

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. P. Garmire. 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. P. Garmire. The network helps show where G. P. Garmire may publish in the future.

Co-authorship network of co-authors of G. P. Garmire

This figure shows the co-authorship network connecting the top 25 collaborators of G. P. Garmire. A scholar is included among the top collaborators of G. P. Garmire 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. P. Garmire. G. P. Garmire 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.
McDonald, M., B. A. Benson, L. E. Bleem, et al.. (2024). The SPT-Chandra BCG Spectroscopic Survey. I. Evolution of the Entropy Threshold for ICM Cooling and AGN Feedback in Galaxy Clusters over the Last 10 Gyr. The Astrophysical Journal. 976(2). 169–169. 1 indexed citations
2.
Hare, Jeremy, George G. Pavlov, Oleg Kargaltsev, & G. P. Garmire. (2023). First Ejection from the PSR B1259-63/LS 2883 High Mass Gamma-Ray Binary Detected During the 2021–2024 Binary Cycle. Research Notes of the AAS. 7(3). 52–52. 1 indexed citations
3.
Ruppin, F., M. McDonald, Julie Hlavacek-Larrondo, et al.. (2023). Redshift Evolution of the Feedback–Cooling Equilibrium in the Core of 48 SPT Galaxy Clusters: A Joint Chandra–SPT–ATCA Analysis. The Astrophysical Journal. 948(1). 49–49. 4 indexed citations
4.
McDonald, M., Eric D. Miller, B. A. Benson, et al.. (2018). THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 <. DSpace@MIT (Massachusetts Institute of Technology). 43 indexed citations
5.
Nurgaliev, D., M. McDonald, B. A. Benson, et al.. (2017). Testing for X-Ray–SZ Differences and Redshift Evolution in the X-Ray Morphology of Galaxy Clusters. The Astrophysical Journal. 841(1). 5–5. 29 indexed citations
6.
McDonald, M., S. W. Allen, Matthew Bayliss, et al.. (2017). The Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.9. The Astrophysical Journal. 843(1). 28–28. 78 indexed citations
7.
Pavlov, G. G., et al.. (2011). Chandra and XMM-Newton Observations of the Gamma-ray Binary 1FGL J1018.6-5856. ATel. 3228. 1. 1 indexed citations
8.
Burrows, D. N., J. L. Racusin, Svetozar A. Zhekov, et al.. (2009). SNR 1987A: Ten Years of Chandra Monitoring. 22. 1 indexed citations
9.
Burrows, D. N., G. P. Garmire, G. Ricker, et al.. (2009). Chandra Searches for Late-Time Jet Breaks in GRB X-ray Afterglows. 23.
10.
Eckart, A., F. K. Baganoff, M. Morris, et al.. (2009). Modeling mm- to X-ray flare emission from Sagittarius A*. Springer Link (Chiba Institute of Technology). 32 indexed citations
11.
Hughes, John P., et al.. (2006). Chandra Observation of Galactic SNR G299.2-2.9. AAS. 214. 1 indexed citations
12.
Sanwal, D., et al.. (2002). Accreting Compact Object at the Center of the Supernova Remnant RCW 103.. 200. 1 indexed citations
13.
Hurley, Kevin, et al.. (2001). The Proper Motion of SGR1900+14. American Astronomical Society Meeting Abstracts. 199. 1 indexed citations
14.
Burrows, D. N., Yoshitomo Maeda, G. P. Garmire, et al.. (2001). Early Results from Chandra Observations of Supernova Remnants. ASPC. 234. 189. 1 indexed citations
15.
Mori, Koji, et al.. (2001). Improvement of the Chandra ACIS Spatial Resolution by Selecting the Split Pixel Events. 251. 576. 1 indexed citations
16.
Pavlov, George G., D. Sanwal, G. P. Garmire, et al.. (2000). Observations of the Vela Pulsar and its Compact Nebula with the Chandra High Resolution Camera. AAS. 196. 1 indexed citations
17.
Chartas, G., et al.. (1996). Measuring the X-ray transmission function of the ACIS UV/Optical blocking filters at the National Synchrotron Light Source.. 188.
18.
Garmire, G. P., et al.. (1981). Possible Detection of a Galactic Wind. Bulletin of the American Astronomical Society. 13. 786. 2 indexed citations
19.
Rothschild, R. E., E. A. Boldt, S. Holt, et al.. (1978). The cosmic X-ray experiment aboard HEAO-1. NASA STI/Recon Technical Report N. 4. 269–301. 6 indexed citations
20.
Kraushaar, W. L., et al.. (1963). COSMIC GAMMA-RAY RESULTS FROM EXPLORER XI. ICRC. 3. 184. 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.

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