Jon M. Saken

515 total citations
12 papers, 274 citations indexed

About

Jon M. Saken is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Artificial Intelligence. According to data from OpenAlex, Jon M. Saken has authored 12 papers receiving a total of 274 indexed citations (citations by other indexed papers that have themselves been cited), including 10 papers in Astronomy and Astrophysics, 4 papers in Nuclear and High Energy Physics and 2 papers in Artificial Intelligence. Recurrent topics in Jon M. Saken's work include Stellar, planetary, and galactic studies (4 papers), Gamma-ray bursts and supernovae (4 papers) and Astrophysics and Cosmic Phenomena (4 papers). Jon M. Saken is often cited by papers focused on Stellar, planetary, and galactic studies (4 papers), Gamma-ray bursts and supernovae (4 papers) and Astrophysics and Cosmic Phenomena (4 papers). Jon M. Saken collaborates with scholars based in United States, Australia and Czechia. Jon M. Saken's co-authors include J. Michael Shull, Robert A. Fesen, S. R. Habbal, Adrian Daw, Martin Dietzel, A. Ding, Huw Morgan, M. B. Arndt, Miloslav Druckmüller and A. Hamilton and has published in prestigious journals such as Nature, The Astrophysical Journal and The Astrophysical Journal Supplement Series.

In The Last Decade

Jon M. Saken

11 papers receiving 269 citations

Peers

Jon M. Saken

AA

NHEP

INSTR

MB

EEE

Tess Jaffe United States

Matthew S. B. Coleman United States

Neng-Hui Liao China

K. Wiik Finland

Ronnie Jansson Germany

S. R. Dugad India

C. Melioli Brazil

Vishal Joshi India

M. Rupen United States

Theresa Wiegert United States

Tess Jaffe United States

Jon M. Saken

164 ×0.6

AA

135 ×1.0

NHEP

4 ×0.5

INSTR

5 ×0.7

MB

11 ×1.6

EEE

Citations per year, relative to Jon M. Saken Jon M. Saken (= 1×) peers Tess Jaffe

Countries citing papers authored by Jon M. Saken

Since Specialization

Citations

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

Fields of papers citing papers by Jon M. Saken

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Jon M. Saken

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

All Works

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12 of 12 papers shown

1.

Corbally, C. J., et al.. (2015). Short-term Activity in Young Solar Analogs. 18. 307–312.

2.

Habbal, S. R., Miloslav Druckmüller, Huw Morgan, et al.. (2011). THERMODYNAMICS OF THE SOLAR CORONA AND EVOLUTION OF THE SOLAR MAGNETIC FIELD AS INFERRED FROM THE TOTAL SOLAR ECLIPSE OBSERVATIONS OF 2010 JULY 11. The Astrophysical Journal. 734(2). 120–120. 56 indexed citations

3.

Saken, Jon M., Knox S. Long, William P. Blair, & P. F. Winkler. (1995). ROSAT observations of the supernova remnant 3C 400.2. The Astrophysical Journal. 443. 231–231. 14 indexed citations

4.

Shull, J. Michael & Jon M. Saken. (1995). Noncoeval star formation, starbursts, and the growth of supershells in OB associations. The Astrophysical Journal. 444. 663–663. 39 indexed citations

5.

Snow, Theodore P., et al.. (1994). Interstellar gas and dust in the young cluster IC 348. The Astrophysical Journal. 420. 632–632. 13 indexed citations

6.

Saken, Jon M., et al.. (1992). An infrared supershell surrounding the Cygnus OB1 association. The Astrophysical Journal. 397. 537–537. 19 indexed citations

7.

Edelson, Rick, G. Pike, Jon M. Saken, Anne L. Kinney, & J. Michael Shull. (1992). The Colorado IUE active galaxy survey. I - Blazars. The Astrophysical Journal Supplement Series. 83. 1–1. 7 indexed citations

8.

Saken, Jon M., Robert A. Fesen, & J. Michael Shull. (1992). An IRAS survey of Galactic supernova remnants. The Astrophysical Journal Supplement Series. 81. 715–715. 49 indexed citations

9.

Edelson, R., Jon M. Saken, G. Pike, et al.. (1991). Rapid ultraviolet variability in the BL Lacertae object PKS 2155 - 304. The Astrophysical Journal. 372. L9–L9. 8 indexed citations

10.

Fesen, Robert A., Jon M. Saken, & A. Hamilton. (1989). Discovery of the remnant of S Andromedae (SN 1885) in M31. The Astrophysical Journal. 341. L55–L55. 12 indexed citations

11.

Shull, J. Michael, Robert A. Fesen, & Jon M. Saken. (1989). Pulsar reenergization of old supernova remnant shells. The Astrophysical Journal. 346. 860–860. 42 indexed citations

12.

Fesen, Robert A., J. Michael Shull, & Jon M. Saken. (1988). Interaction between high-velocity pulsar in CTB80 and an infrared emission shell. Nature. 334(6179). 229–231. 15 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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