This map shows the geographic impact of O. G. Franz'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 O. G. Franz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. G. Franz more than expected).
This network shows the impact of papers produced by O. G. Franz. 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 O. G. Franz. The network helps show where O. G. Franz may publish in the future.
Co-authorship network of co-authors of O. G. Franz
This figure shows the co-authorship network connecting the top 25 collaborators of O. G. Franz.
A scholar is included among the top collaborators of O. G. Franz 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 O. G. Franz. O. G. Franz is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Benedict, G. F., B. McArthur, A. L. Whipple, et al.. (1997). Proxima Centauri and Barnard's Star: Low-mass Companion Astrometric Detection Limits and High-Precision Photometry with HST. Bulletin of the American Astronomical Society. 28. 1103.2 indexed citations
6.
Altena, W. F. van, X. Guo, B. McArthur, et al.. (1997). The Distance to the Hyades Cluster Based on HST FGS3 Parallaxes. Bulletin of the American Astronomical Society. 28. 1102.2 indexed citations
7.
Franz, O. G., L. H. Wasserman, A. J. Bradley, et al.. (1994). Astrometric Companions Detected at Visible Wavelengths with the Hubble Space Telescope Fine Guidance Sensors. American Astronomical Society Meeting Abstracts. 185.1 indexed citations
Benedict, G. F., B. McArthur, Edmund Nelan, et al.. (1993). The Search for Planets around Proxima Centauri using Hubble Space Telescope Fine Guidance Sensor #3: A Progress Report. 182. 137–138.1 indexed citations
10.
Millis, R. L., L. H. Wasserman, O. G. Franz, et al.. (1993). The Size and Bulk Density of Pluto. DPS. 25.1 indexed citations
11.
Benedict, G. F., E. Nelan, D. Story, et al.. (1992). Astrometric performance characteristics of the Hubble Space Telescope fine guidance sensors. 180.
12.
Millis, R. L., O. G. Franz, L. H. Wasserman, et al.. (1989). Constraints on the size, shape, and density of (4) Vesta.. Bulletin of the American Astronomical Society. 21(4). 1247.5 indexed citations
13.
Wasserman, L. H., R. L. Millis, & O. G. Franz. (1986). The Occultation of AG + 20° 1138 by 129 Antigone on 11 April 1985. Bulletin of the American Astronomical Society. 18. 797.3 indexed citations
14.
McAlister, H. A., William I. Hartkopf, D. J. Hutter, & O. G. Franz. (1985). Interferometric Measurements of Binary Stars with the GSU ICCD Speckle Camera. Bulletin of the American Astronomical Society. 17. 551.1 indexed citations
Franz, O. G.. (1978). UBV Photometry of Triton.. Bulletin of the American Astronomical Society. 10. 585.3 indexed citations
17.
Franz, O. G.. (1975). A Photoelectric Color and Magnitude of Mimas. Bulletin of the American Astronomical Society. 7. 388.5 indexed citations
18.
Franz, O. G. & R. L. Millis. (1973). UBV Photometry of Enceladus, Tethys, and Dione. Bulletin of the American Astronomical Society. 5. 304.3 indexed citations
19.
Franz, O. G., et al.. (1969). A Search for an Anomalous Brightening of Io After Eclipse. Bulletin of the American Astronomical Society. 1. 344.6 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.