C. M. Gaskell

8.2k total citations
100 papers, 3.1k citations indexed

About

C. M. Gaskell is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, C. M. Gaskell has authored 100 papers receiving a total of 3.1k indexed citations (citations by other indexed papers that have themselves been cited), including 90 papers in Astronomy and Astrophysics, 35 papers in Instrumentation and 13 papers in Nuclear and High Energy Physics. Recurrent topics in C. M. Gaskell's work include Galaxies: Formation, Evolution, Phenomena (59 papers), Astrophysical Phenomena and Observations (42 papers) and Astronomy and Astrophysical Research (35 papers). C. M. Gaskell is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (59 papers), Astrophysical Phenomena and Observations (42 papers) and Astronomy and Astrophysical Research (35 papers). C. M. Gaskell collaborates with scholars based in United States, Chile and France. C. M. Gaskell's co-authors include R. W. Goosmann, B. M. Peterson, D. Burstein, L. S. Sparke, Anuradha Koratkar, S. M. Faber, N. Krumm, E. D. Friel, S. M. Faber and E. J. Wampler and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

C. M. Gaskell

94 papers receiving 2.9k citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
C. M. Gaskell United States	30	3.0k	729	640	139	71	100	3.1k
Craig B. Foltz United States	32	3.6k 1.2×	868 1.2×	780 1.2×	116 0.8×	47 0.7×	68	3.7k
David A. Turnshek United States	36	3.8k 1.3×	786 1.1×	851 1.3×	139 1.0×	45 0.6×	105	3.8k
Jill Bechtold United States	33	3.5k 1.2×	1.1k 1.5×	711 1.1×	102 0.7×	36 0.5×	101	3.5k
Joseph C. Shields United States	33	3.5k 1.2×	649 0.9×	882 1.4×	146 1.1×	69 1.0×	93	3.6k
William G. Mathews United States	32	3.0k 1.0×	769 1.1×	597 0.9×	160 1.2×	47 0.7×	112	3.2k
Beverley J. Wills United States	32	2.9k 1.0×	1.0k 1.4×	398 0.6×	95 0.7×	50 0.7×	78	2.9k
F. La Franca Italy	34	3.3k 1.1×	1.1k 1.5×	748 1.2×	76 0.5×	43 0.6×	103	3.4k
I. Hook United Kingdom	27	3.0k 1.0×	755 1.0×	975 1.5×	120 0.9×	33 0.5×	88	3.1k
T. Miyaji United States	26	3.4k 1.1×	1.2k 1.6×	993 1.6×	68 0.5×	45 0.6×	92	3.5k
C. S. Crawford Russia	26	3.6k 1.2×	1.3k 1.7×	629 1.0×	87 0.6×	43 0.6×	81	3.7k

Countries citing papers authored by C. M. Gaskell

Since Specialization

Citations

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

Fields of papers citing papers by C. M. Gaskell

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. M. Gaskell

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Gaskell, C. M., et al.. (2023). Estimating reddening of the continuum and broad-line region of active galactic nuclei: the mean reddening of NGC 5548 and the size of the accretion disc. Monthly Notices of the Royal Astronomical Society. 519(3). 4082–4093. 15 indexed citations

Gaskell, C. M., et al.. (2023). Interpretation of IR variability of AGNs in the hollow bi-conical dust outflow model. Proceedings of the International Astronomical Union. 19(S378). 3–7.

Kraemer, S. B., Travis C. Fischer, D. M. Crenshaw, et al.. (2020). Hubble Space Telescope observations of [O iii] emission in nearby QSO2s: physical properties of the ionized outflows. Monthly Notices of the Royal Astronomical Society. 500(1). 1491–1504. 20 indexed citations

Gaskell, C. M., V. Lipunov, N. I. Shatsky, et al.. (2017). Multi-Wavelength Monitoring of the Changing-Look AGN NGC 2617 during State Changes. Conicet. 3 indexed citations

Taranova, O. G., et al.. (2014). REVERBERATION MEASUREMENT OF THE INNER RADIUS OF THE DUST TORUS IN NGC 4151 DURING 2008-2013. SHILAP Revista de lepidopterología.

Marin, Frédéric, R. W. Goosmann, C. M. Gaskell, D. Porquet, & Michal Dovčiak. (2012). Modeling optical and UV polarization of AGNs. Astronomy and Astrophysics. 548. A121–A121. 56 indexed citations

Gaskell, C. M., R. W. Goosmann, & E. S. Klimek. (2008). Structure and kinematics of the broad-line region and torus of Active Galactic Nuclei. Memorie della Societa Astronomica Italiana. 79. 1090. 1 indexed citations

Goosmann, R. W. & C. M. Gaskell. (2007). Modeling optical and UV polarization of AGNs. Astronomy and Astrophysics. 465(1). 129–145. 83 indexed citations

Goosmann, R. W. & C. M. Gaskell. (2005). Modeling optical and UV polarization of AGNs I. Imprints of individual scattering regions. arXiv (Cornell University). 56 indexed citations

10.

Snedden, Stephanie A. & C. M. Gaskell. (1999). The Effect of Abundance Variations on Estimates of the Densities of Broad-Line Region Clouds in Quasars. The Astrophysical Journal. 521(2). L91–L94. 13 indexed citations

11.

Cheng, F. H., C. M. Gaskell, & Anuradha Koratkar. (1991). The shape of the ultraviolet continuum of quasars and intergalactic dust. The Astrophysical Journal. 370. 487–487. 18 indexed citations

12.

Baldwin, J. A., E. J. Wampler, & C. M. Gaskell. (1989). Emission-line properties of optically and radio-selected complete quasar samples. The Astrophysical Journal. 338. 630–630. 55 indexed citations

13.

Gaskell, C. M.. (1988). Direct evidence for gravitational domination of the motion of gas within one light-week of the central object in NGC 4151 and the determination of the mass of the probable black hole. The Astrophysical Journal. 325. 114–114. 57 indexed citations

14.

Gaskell, C. M., et al.. (1986). Pre-discovery Imaging &High-Resolution Spectroscopy at Maximum Light of the Unique Supernova 1984 in NGC 3169. Bulletin of the American Astronomical Society. 18. 953. 1 indexed citations

15.

Gaskell, C. M.. (1984). Reddening of the narrow-line regions of active galactic nuclei and the intrinsic Balmer decrement II. 24(1). 43–48. 3 indexed citations

16.

Gaskell, C. M.. (1984). Astrophysics: The origin of gas in quasars — reverse stellar evolution?. Nature. 307(5948). 210–210. 2 indexed citations

17.

Gaskell, C. M. & G. J. Ferland. (1984). Theoretical hydrogen-line ratios for the narrow-line regions of active galactic nuclei. Publications of the Astronomical Society of the Pacific. 96. 393–393. 54 indexed citations

18.

Gaskell, C. M.. (1983). Quasars as supermassive binaries. 24. 473–477. 4 indexed citations

19.

Gaskell, C. M.. (1982). The Origin of Displaced Broad Emission Lines in QSOs - Supermassive Binaries?. Bulletin of the American Astronomical Society. 14. 909. 1 indexed citations

20.

Gaskell, C. M.. (1980). Two-photon continuum emission in quasar spectra. Observatory. 100. 148–151. 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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