Arthur M. Wolfe

14.1k total citations · 3 hit papers
135 papers, 9.0k citations indexed

About

Arthur M. Wolfe is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, Arthur M. Wolfe has authored 135 papers receiving a total of 9.0k indexed citations (citations by other indexed papers that have themselves been cited), including 115 papers in Astronomy and Astrophysics, 37 papers in Instrumentation and 22 papers in Nuclear and High Energy Physics. Recurrent topics in Arthur M. Wolfe's work include Galaxies: Formation, Evolution, Phenomena (78 papers), Astrophysics and Star Formation Studies (58 papers) and Stellar, planetary, and galactic studies (55 papers). Arthur M. Wolfe is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (78 papers), Astrophysics and Star Formation Studies (58 papers) and Stellar, planetary, and galactic studies (55 papers). Arthur M. Wolfe collaborates with scholars based in United States, United Kingdom and Chile. Arthur M. Wolfe's co-authors include J. X. Prochaska, Rainer K. Sachs, Eric Gawiser, David A. Turnshek, Kenneth M. Lanzetta, M. T. Murphy, John K. Webb, Lisa J. Storrie‐Lombardi, S. Herbert-Fort and V. A. Dzuba and has published in prestigious journals such as Nature, Science and Physical Review Letters.

In The Last Decade

Arthur M. Wolfe

134 papers receiving 8.8k citations

Hit Papers

Perturbations of a Cosmological Model and Angular Variati... 1967 2026 1986 2006 1967 2001 2005 250 500 750 1000

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Arthur M. Wolfe United States 48 8.5k 2.5k 1.6k 541 372 135 9.0k
Barry F. Madore United States 50 9.6k 1.1× 1.4k 0.6× 3.2k 2.0× 396 0.7× 213 0.6× 234 10.0k
R. F. Carswell United Kingdom 36 3.8k 0.4× 1.3k 0.5× 758 0.5× 396 0.7× 260 0.7× 134 4.2k
Stefano Casertano United States 41 10.2k 1.2× 4.4k 1.8× 2.0k 1.3× 409 0.8× 462 1.2× 143 10.5k
Maarten Schmidt United States 35 7.8k 0.9× 2.4k 1.0× 2.1k 1.3× 237 0.4× 247 0.7× 120 8.2k
Christopher W. Churchill United States 34 4.0k 0.5× 1.1k 0.5× 820 0.5× 482 0.9× 214 0.6× 95 4.4k
J. R. Mould United States 49 7.8k 0.9× 995 0.4× 2.7k 1.7× 311 0.6× 177 0.5× 298 8.1k
W. Forman United States 60 15.4k 1.8× 5.3k 2.1× 3.4k 2.1× 445 0.8× 405 1.1× 365 15.9k
E. Falco United States 36 6.5k 0.8× 1.3k 0.5× 1.9k 1.2× 875 1.6× 218 0.6× 119 6.7k
P. Petitjean France 41 4.2k 0.5× 928 0.4× 751 0.5× 375 0.7× 154 0.4× 148 4.5k
Scott Burles United States 44 6.9k 0.8× 2.5k 1.0× 2.3k 1.4× 713 1.3× 289 0.8× 73 7.6k

Countries citing papers authored by Arthur M. Wolfe

Since Specialization
Citations

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

Fields of papers citing papers by Arthur M. Wolfe

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Arthur M. Wolfe. 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 Arthur M. Wolfe. The network helps show where Arthur M. Wolfe may publish in the future.

Co-authorship network of co-authors of Arthur M. Wolfe

This figure shows the co-authorship network connecting the top 25 collaborators of Arthur M. Wolfe. A scholar is included among the top collaborators of Arthur M. Wolfe 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 Arthur M. Wolfe. Arthur M. Wolfe 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.
Chornock, R., J. S. Bloom, S. B. Cenko, et al.. (2010). クェーサーSDSS J1536+0441: 2重ピーク放射体. The Astrophysical Journal. 709. 39–43. 6 indexed citations
2.
Whitmore, J. B., et al.. (2009). Wavelength Accuracy of the Keck HIRES Spectrograph and Measuring Changes in the Fine Structure Constant. 213. 1 indexed citations
3.
Fox, Andrew J., J. X. Prochaska, C. Ledoux, et al.. (2009). Metal-enriched plasma in protogalactic halos. Astronomy and Astrophysics. 503(3). 731–746. 27 indexed citations
4.
Wolfe, Arthur M., Regina A. Jorgenson, Timothy Robishaw, Carl Heiles, & J. X. Prochaska. (2008). An 84-μG magnetic field in a galaxy at redshift z = 0.692. Nature. 455(7213). 638–640. 43 indexed citations
5.
Vladilo, G., J. X. Prochaska, & Arthur M. Wolfe. (2007). The color excess of quasars with intervening DLA systems. Astronomy and Astrophysics. 478(3). 701–715. 40 indexed citations
6.
Prochaska, J. X., J. Christopher Howk, & Arthur M. Wolfe. (2003). The elemental abundance pattern in a galaxy at z = 2.626. Nature. 423(6935). 57–59. 52 indexed citations
7.
Webb, John K., M. T. Murphy, V. V. Flambaum, et al.. (2001). Further Evidence for Cosmological Evolution of the Fine Structure Constant. Physical Review Letters. 87(9). 91301–91301. 534 indexed citations breakdown →
8.
Prochaska, J. X., Arthur M. Wolfe, & Eric Gawiser. (2000). New Metallicity Measurements of z > 3 Damped Lya Systems. American Astronomical Society Meeting Abstracts. 197. 1 indexed citations
9.
Prochaska, J. X. & Arthur M. Wolfe. (1996). A Keck HIRES Investigation of the Metal Abundances and Kinematics of the Z = 2.46 Damped LY alpha System toward Q0201+365. The Astrophysical Journal. 470. 403–403. 65 indexed citations
11.
Turnshek, David A., B. R. Espey, Michael Rauch, et al.. (1994). The HST quasar absorption line key project. 4: HST faint-object spectrograph and ground-based observations of the unusual low-redshift broad absorption-line quasi-stellar object PG 0043+039. The Astrophysical Journal. 428. 93–93. 21 indexed citations
12.
Wolfe, Arthur M.. (1993). THE PROGENITORS OF GALAXIES AND THE GAS CONTENT OF THE UNIVERSE AT LARGE REDSHIFTS. Annals of the New York Academy of Sciences. 688(1). 281–296. 7 indexed citations
13.
Lu, Limin, Arthur M. Wolfe, David A. Turnshek, & Kenneth M. Lanzetta. (1993). A spectroscopic study of damped Lyman-alpha systems in the Las Campanas/Palomar survey. The Astrophysical Journal Supplement Series. 84. 1–1. 24 indexed citations
14.
Briggs, F., et al.. (1989). The spatial extent of the Z = 2.04 absorber in the spectrum of PKS 0458-020. The Astrophysical Journal. 341. 650–650. 48 indexed citations
15.
Wolfe, Arthur M., et al.. (1987). The effect of a quasi-stellar object on its host galaxy - Dynamical and physical processes in the interstellar medium around a quasi-stellar object. The Astrophysical Journal. 322. 180–180. 13 indexed citations
16.
Junkkarinen, V. T., E. M. Burbidge, & Arthur M. Wolfe. (1978). A Spectroscopic Search for Absorption Lines in Radio Compact QSO's. Bulletin of the American Astronomical Society. 10. 688. 1 indexed citations
17.
Wolfe, Arthur M.. (1978). Pittsburgh Conference on BL Lac Objects, University of Pittsburgh, Pittsburgh, Pa., April 24-26, 1978, Proceedings. D-Scholarship@Pitt (University of Pittsburgh). 4 indexed citations
18.
Wolfe, Arthur M.. (1971). Hot Seyfert Winds.. Bulletin of the American Astronomical Society. 3. 474. 1 indexed citations
19.
Wolfe, Arthur M.. (1970). New Limits on the Shear and Rotation of the Universe from the X-Ray Background. Bulletin of the American Astronomical Society. 2. 225. 5 indexed citations
20.
Wolfe, Arthur M. & G. R. Burbidge. (1970). Can the Lumpy Distribution of Galaxies be reconciled with the Smooth X-ray Background?. Nature. 228(5277). 1170–1174. 11 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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