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.
An Overview of the Performance and Scientific Results from theChandra X‐Ray Observatory
2002458 citationsG. P. Garmire, S. S. Murray et al.profile →
The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source Catalogs
2003447 citationsW. N. Brandt, G. P. Garmire et al.profile →
Advanced CCD imaging spectrometer (ACIS) instrument on the Chandra X-ray Observatory
2003440 citationsG. P. Garmire, J. A. Nousek et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
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).
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.
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
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.