J. W. Isbell

513 total citations
11 papers, 139 citations indexed

About

J. W. Isbell is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Nuclear and High Energy Physics. According to data from OpenAlex, J. W. Isbell has authored 11 papers receiving a total of 139 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 4 papers in Atomic and Molecular Physics, and Optics and 3 papers in Nuclear and High Energy Physics. Recurrent topics in J. W. Isbell's work include Galaxies: Formation, Evolution, Phenomena (7 papers), Astrophysics and Star Formation Studies (4 papers) and Adaptive optics and wavefront sensing (3 papers). J. W. Isbell is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (7 papers), Astrophysics and Star Formation Studies (4 papers) and Adaptive optics and wavefront sensing (3 papers). J. W. Isbell collaborates with scholars based in United States, Germany and United Kingdom. J. W. Isbell's co-authors include A. J. Dessler, J. H. Waite, Rui Xue, Hai Fu, David A. Wake, Dmitry Bizyaev, Lihwai Lin, Kaike Pan, Y. Sophia Dai and D. Asmus and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

J. W. Isbell

11 papers receiving 127 citations

Peers

J. W. Isbell

AA

MB

INSTR

AMPO

NHEP

Shigeru Eto Japan

A. López Ariste France

Antonino Petralia Italy

A. Fossum Norway

M. Steller Austria

Klaus Fricke Germany

Jeffrey W. Reep United States

Damien Przybylski Germany

A. Morgenthaler France

B. Hancock United Kingdom

Shigeru Eto Japan

J. W. Isbell

232 ×1.8

AA

35 ×0.7

MB

22 ×1.3

INSTR

9 ×0.8

AMPO

14 ×1.3

NHEP

Citations per year, relative to J. W. Isbell J. W. Isbell (= 1×) peers Shigeru Eto

Countries citing papers authored by J. W. Isbell

Since Specialization

Citations

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

Fields of papers citing papers by J. W. Isbell

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by J. W. Isbell. 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 J. W. Isbell. The network helps show where J. W. Isbell may publish in the future.

Co-authorship network of co-authors of J. W. Isbell

This figure shows the co-authorship network connecting the top 25 collaborators of J. W. Isbell. A scholar is included among the top collaborators of J. W. Isbell 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 J. W. Isbell. J. W. Isbell is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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11 of 11 papers shown

1.

Isbell, J. W., Steve Ertel, Jörg‐Uwe Pott, et al.. (2025). Direct imaging of active galactic nucleus outflows and their origin with the 23 m Large Binocular Telescope. Nature Astronomy. 9(3). 417–427. 2 indexed citations

2.

Isbell, J. W., Steve Ertel, Kevin Wagner, et al.. (2024). The LBTI: pioneering the ELT era. 5–5. 1 indexed citations

3.

Isbell, J. W., Jörg‐Uwe Pott, K. Meisenheimer, et al.. (2023). The dusty heart of Circinus. Astronomy and Astrophysics. 678. A136–A136. 6 indexed citations

4.

Isbell, J. W., L. Burtscher, D. Asmus, et al.. (2021). Subarcsecond Mid-infrared View of Local Active Galactic Nuclei. IV. The L- and M-band Imaging Atlas*. The Astrophysical Journal. 910(2). 104–104. 9 indexed citations

5.

Fu, Hai, Y. Sophia Dai, J. W. Isbell, et al.. (2018). SDSS-IV MaNGA: Galaxy Pair Fraction and Correlated Active Galactic Nuclei. The Astrophysical Journal. 856(2). 93–93. 31 indexed citations

6.

Brown, Shea, B. M. Gaensler, J. W. Isbell, et al.. (2018). Classifying Complex Faraday Spectra with Convolutional Neural Networks. Monthly Notices of the Royal Astronomical Society. 7 indexed citations

7.

Sánchez-Bermúdez, J., F. Millour, Fabien Baron, et al.. (2018). Why chromatic imaging matters. Experimental Astronomy. 46(3). 457–473. 4 indexed citations

8.

Isbell, J. W., Rui Xue, & Hai Fu. (2018). The Evolution of Molecular Gas Fraction Traced by the CO Tully–Fisher Relation. The Astrophysical Journal Letters. 869(2). L37–L37. 7 indexed citations

9.

Xue, Rui, Hai Fu, J. W. Isbell, et al.. (2018). Flat Rotation Curves Found in Merging Dusty Starbursts at z = 2.3 through Tilted-ring Modeling. The Astrophysical Journal Letters. 864(1). L11–L11. 4 indexed citations

10.

Fu, Hai, Joseph F. Hennawi, J. X. Prochaska, et al.. (2016). THE CIRCUMGALACTIC MEDIUM OF SUBMILLIMETER GALAXIES. I. FIRST RESULTS FROM A RADIO-IDENTIFIED SAMPLE. The Astrophysical Journal. 832(1). 52–52. 3 indexed citations

11.

Isbell, J. W., A. J. Dessler, & J. H. Waite. (1984). Magnetospheric energization by interaction between planetary spin and the solar wind. Journal of Geophysical Research Atmospheres. 89(A12). 10716–10722. 65 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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