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.
Stellar Orbits around the Galactic Center Black Hole
2005428 citationsA. M. Ghez, Jessica R. Lu et al.The Astrophysical Journalprofile →
High Proper‐Motion Stars in the Vicinity of Sagittarius A*: Evidence for a Supermassive Black Hole at the Center of Our Galaxy
1998423 citationsA. M. Ghez, M. Morris et al.The Astrophysical Journalprofile →
The First Measurement of Spectral Lines in a Short-Period Star Bound to the Galaxy’s Central Black Hole: A Paradox of Youth
2003413 citationsA. M. Ghez, Gaspard Duchêne et al.The Astrophysical Journalprofile →
Observational Constraints on the Formation and Evolution of Binary Stars
2001329 citationsR. J. White, A. M. GhezThe Astrophysical Journalprofile →
The multiplicity of T Tauri stars in the star forming regions Taurus-Auriga and Ophiuchus-Scorpius: A 2.2 micron speckle imaging survey
1993321 citationsA. M. Ghez, K. Matthews et al.The Astronomical Journalprofile →
Measuring Distance And Properties Of The Milky Way's Central Supermassive Black Hole With Stellar Orbits
This map shows the geographic impact of A. M. Ghez'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 A. M. Ghez with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. M. Ghez more than expected).
This network shows the impact of papers produced by A. M. Ghez. 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 A. M. Ghez. The network helps show where A. M. Ghez may publish in the future.
Co-authorship network of co-authors of A. M. Ghez
This figure shows the co-authorship network connecting the top 25 collaborators of A. M. Ghez.
A scholar is included among the top collaborators of A. M. Ghez 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 A. M. Ghez. A. M. Ghez is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Witzel, Gunther, Breann Sitarski, A. M. Ghez, et al.. (2017). The Post-periapsis Evolution of Galactic Center Source G1: The Second Case of a Resolved Tidal Interaction with a Supermassive Black Hole. eScholarship (California Digital Library).29 indexed citations
11.
Chappell, Samantha, A. M. Ghez, Tuan Do, et al.. (2016). The late-type stellar density profile in the Galactic Center: A statistical approach. eScholarship (California Digital Library).1 indexed citations
12.
Sitarski, Breann, A. M. Ghez, M. Morris, et al.. (2015). Galactic Center Source G1 and other G2-like Sources. AAS. 225.1 indexed citations
13.
Sitarski, Breann, Tuan Do, Gunther Witzel, et al.. (2014). Is G2 Alone? Other Infrared Sources in the Central 0.04 Parsecs of the Galactic Center. 223.1 indexed citations
Macintosh, Bruce, James R. Graham, A. M. Ghez, et al.. (2002). Extreme Adaptive Optics Planet Imager. AAS. 201.1 indexed citations
18.
Cotera, A., M. Morris, A. M. Ghez, et al.. (1999). Mid-Infrared Imaging of the Central Parsec with Keck. ASPC. 186. 240.3 indexed citations
19.
Larkin, James, et al.. (1998). GRB980329 Keck K-band observations. GRB Coordinates Network. 51. 1.1 indexed citations
20.
Patience, J., A. M. Ghez, R. J. White, et al.. (1998). A High-Resolution Search for Stellar Companions to Stars with Planets. AAS. 193.1 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.