F. R. Harnden

1.4k total citations
39 papers, 563 citations indexed

About

F. R. Harnden is a scholar working on Astronomy and Astrophysics, Instrumentation and Radiation. According to data from OpenAlex, F. R. Harnden has authored 39 papers receiving a total of 563 indexed citations (citations by other indexed papers that have themselves been cited), including 32 papers in Astronomy and Astrophysics, 9 papers in Instrumentation and 6 papers in Radiation. Recurrent topics in F. R. Harnden's work include Stellar, planetary, and galactic studies (17 papers), Astrophysical Phenomena and Observations (13 papers) and Astrophysics and Star Formation Studies (12 papers). F. R. Harnden is often cited by papers focused on Stellar, planetary, and galactic studies (17 papers), Astrophysical Phenomena and Observations (13 papers) and Astrophysics and Star Formation Studies (12 papers). F. R. Harnden collaborates with scholars based in United States, Italy and Netherlands. F. R. Harnden's co-authors include G. Micela, S. Sciortino, H. E. Payne, E. Flaccomio, F. Favata, S. J. Wolk, Hsien Shang, Eric D. Feigelson, F. Damiani and P. Gorenstein and has published in prestigious journals such as Nature, The Astrophysical Journal and The Astrophysical Journal Supplement Series.

In The Last Decade

F. R. Harnden

35 papers receiving 543 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
F. R. Harnden United States	11	534	79	73	29	24	39	563
Kwang‐Il Seon South Korea	12	381 0.7×	81 1.0×	55 0.8×	35 1.2×	14 0.6×	77	434
R. Bertram United States	11	488 0.9×	134 1.7×	80 1.1×	46 1.6×	6 0.3×	15	515
B. S. Carter South Africa	12	546 1.0×	80 1.0×	118 1.6×	24 0.8×	10 0.4×	20	563
R. Wade United Kingdom	13	389 0.7×	66 0.8×	52 0.7×	36 1.2×	7 0.3×	26	428
Ch. Theis Germany	12	557 1.0×	119 1.5×	201 2.8×	17 0.6×	40 1.7×	29	627
N. Mouawad Germany	8	571 1.1×	60 0.8×	36 0.5×	25 0.9×	9 0.4×	20	578
J. Jugaku Japan	11	345 0.6×	73 0.9×	51 0.7×	35 1.2×	15 0.6×	52	398
Doron Chelouche Israel	16	791 1.5×	176 2.2×	119 1.6×	74 2.6×	19 0.8×	47	819
Jr. Chaffee Frederic H. United States	11	408 0.8×	56 0.7×	51 0.7×	49 1.7×	5 0.2×	20	449
B. J. McNamara United States	14	578 1.1×	90 1.1×	153 2.1×	46 1.6×	5 0.2×	67	627

Countries citing papers authored by F. R. Harnden

Since Specialization

Citations

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

Fields of papers citing papers by F. R. Harnden

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by F. R. Harnden. 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 F. R. Harnden. The network helps show where F. R. Harnden may publish in the future.

Co-authorship network of co-authors of F. R. Harnden

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

All Works

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20 of 20 papers shown

Albacete-Colombo, J. F., F. Damiani, G. Micela, S. Sciortino, & F. R. Harnden. (2008). An X-ray survey of low-mass stars in Trumpler 16 with Chandra. Astronomy and Astrophysics. 490(3). 1055–1070. 10 indexed citations

Pillitteri, I., G. Micela, S. Sciortino, F. Damiani, & F. R. Harnden. (2004). XMM-Newton observations of the young open cluster Blanco 1. I. X-ray spectroscopy and photometry.. Nova Science Publishers (Nova Science Publishers, Inc.). 10 indexed citations

Maggio, A., J. J. Drake, V. Kashyap, et al.. (2004). X‐Ray Spectroscopy of the Unsteady Quiescent Corona of AD Leonis withChandra. The Astrophysical Journal. 613(1). 548–566. 16 indexed citations

Pillitteri, I., G. Micela, S. Sciortino, F. Damiani, & F. R. Harnden. (2004). XMM-Newton observations of the young open clusterBlanco 1. Astronomy and Astrophysics. 421(1). 175–186. 12 indexed citations

Favata, F., G. Micela, S. L. Baliunas, et al.. (2004). High-amplitude, long-term X-ray variability in the solar-type star HD 81809: The beginning of an X-ray activity cycle?. Astronomy and Astrophysics. 418(1). L13–L16. 34 indexed citations

Flaccomio, E., F. Damiani, G. Micela, et al.. (2002). Chandra X-ray Observation of the Orion Nebula Cluster. ASPC. 277. 155. 2 indexed citations

Barbera, Marco, F. Bocchino, F. Damiani, et al.. (2002). ROSAT PSPC/HRI observations of the open cluster NGC 2422. Astronomy and Astrophysics. 387(2). 463–478. 6 indexed citations

Harnden, F. R., et al.. (2001). Astronomical Data Analysis Software and Systems X. ASPC. 238. 84 indexed citations

Micela, G., S. Sciortino, F. R. Harnden, & R. Rosner. (1998). X-ray Variability and Rotation in the Pleiades Cluster. Astrophysics and Space Science. 261(1-4). 105–106. 2 indexed citations

10.

Flaccomio, E., S. Sciortino, G. Micela, et al.. (1997). X-ray and optical observations of the star forming region NGC 2264.. MmSAI. 68. 1073–1076. 1 indexed citations

11.

Micela, G., F. R. Harnden, R. Rosner, S. Sciortino, & G. S. Vaiana. (1989). Spatial and spectral features of soft diffuse X ray background seen by the Einstein observatory. 296. 1005–1010. 1 indexed citations

12.

Fink, H. H., J. H. M. M. Schmitt, & F. R. Harnden. (1988). The scattered solar X-ray background in low earth orbit. NASA Technical Reports Server (NASA). 193. 345–356. 9 indexed citations

13.

Murray, S. S., M. Elvis, W. Forman, et al.. (1987). The AXAF High Resolution Camera (HRC) and its Use for Observations of Distant Clusters of Galaxies. 26. 113. 7 indexed citations

14.

Harnden, F. R.. (1987). Einstein Observatory Limits on Neutron Star Surface Temperatures. Symposium - International Astronomical Union. 125. 457–457. 1 indexed citations

15.

Schmitt, J. H. M. M., et al.. (1984). X-ray Spectra of RS CVn Binaries. Bulletin of the American Astronomical Society. 16. 514.

16.

Harnden, F. R., Daniel G. Fabricant, D. E. Harris, & J. Schwarz. (1984). Scientific Specification of the Data Analysis System for the EINSTEIN Observatory (HEAO-2) Imaging Proportional Counter. 393. 3 indexed citations

17.

Weisskopf, Martin C., Ronald F. Elsner, D. A. Leahy, et al.. (1983). The period history of the X-ray pulsar in MSH 15-52. The Astrophysical Journal. 267. 711–711. 6 indexed citations

18.

Fabricant, Daniel G., et al.. (1979). Lexan coating to eliminate the UV sensitivity of soft x-ray proportional counters with a polypropylene window. Review of Scientific Instruments. 50(6). 727–729. 6 indexed citations

19.

Topka, K., et al.. (1977). Soft X-Ray Structure of the Coma Cluster of Galaxies. Bulletin of the American Astronomical Society. 9. 560. 1 indexed citations

20.

Gorenstein, P., K. Topka, Daniel G. Fabricant, & F. R. Harnden. (1976). The Relation Between Temperature and X-ray Luminosity for Clusters of Galaxies.. Bulletin of the American Astronomical Society. 8. 553. 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.

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