M. G. Watson

3.8k total citations
60 papers, 1.3k citations indexed

About

M. G. Watson is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, M. G. Watson has authored 60 papers receiving a total of 1.3k indexed citations (citations by other indexed papers that have themselves been cited), including 57 papers in Astronomy and Astrophysics, 19 papers in Nuclear and High Energy Physics and 13 papers in Computational Mechanics. Recurrent topics in M. G. Watson's work include Astrophysical Phenomena and Observations (46 papers), Galaxies: Formation, Evolution, Phenomena (19 papers) and Gamma-ray bursts and supernovae (16 papers). M. G. Watson is often cited by papers focused on Astrophysical Phenomena and Observations (46 papers), Galaxies: Formation, Evolution, Phenomena (19 papers) and Gamma-ray bursts and supernovae (16 papers). M. G. Watson collaborates with scholars based in United Kingdom, Germany and United States. M. G. Watson's co-authors include R. Willingale, K. A. Pounds, A. Lawrence, M. Elvis, A. R. King, J. P. Osborne, Martin Turner, R. S. Warwick, F. J. Carrera and M. J. Ricketts and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

M. G. Watson

59 papers receiving 1.2k citations

Peers

M. G. Watson

NHEP

INSTR

GEOPH

K. P. Singh India

R. M. Wagner United States

K. A. Pounds United Kingdom

F. A. Primini United States

S. S. Holt United States

E. M. Schlegel United States

A. M. Read United Kingdom

Jr. Harnden F. R. United States

R. D. Saxton Spain

R. S. Warwick United Kingdom

K. P. Singh India

M. G. Watson

1.2k ×1.0

360 ×0.8

NHEP

79 ×0.8

91 ×1.0

INSTR

77 ×1.1

GEOPH

Citations per year, relative to M. G. Watson M. G. Watson (= 1×) peers K. P. Singh

Countries citing papers authored by M. G. Watson

Since Specialization

Citations

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

Fields of papers citing papers by M. G. Watson

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. G. Watson

This figure shows the co-authorship network connecting the top 25 collaborators of M. G. Watson. A scholar is included among the top collaborators of M. G. Watson 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 M. G. Watson. M. G. Watson 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

Traulsen, I., A. Schwope, G. Lamer, et al.. (2020). TheXMM-Newtonserendipitous survey. Astronomy and Astrophysics. 641. A137–A137. 38 indexed citations

Traulsen, I., A. Schwope, G. Lamer, et al.. (2019). The XMM-Newton serendipitous survey. Astronomy and Astrophysics. 624. A77–A77. 23 indexed citations

Pons, Estelle & M. G. Watson. (2016). A new sample of X-ray selected narrow emission-line galaxies. Astronomy and Astrophysics. 594. A72–A72. 11 indexed citations

Barcons, X., K. Nandra, D. Barret, et al.. (2015). Athena: the X-ray observatory to study the hot and energetic Universe. Journal of Physics Conference Series. 610. 12008–12008. 51 indexed citations

Pineau, F.‐X., C. Motch, F. J. Carrera, et al.. (2011). Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey. Springer Link (Chiba Institute of Technology). 38 indexed citations

Corral, A., K. L. Page, F. J. Carrera, et al.. (2008). Average Fe K$\mathsf{\alpha}$ emission from distant AGN. Astronomy and Astrophysics. 492(1). 71–80. 33 indexed citations

Carrera, F. J., J. Ebrero, S. Mateos, et al.. (2007). The XMM-Newton serendipitous survey - III. The AXIS X-ray source counts and angular clustering. Figshare. 35 indexed citations

Lane, K., O. Almaini, Sylvie Foucaud, et al.. (2007). The colour selection of distant galaxies in the UKIDSS Ultra Deep Survey Early Data Release. Leicester Research Archive (University of Leicester). 22 indexed citations

Caccianiga, A., P. Severgnini, R. Della Ceca, et al.. (2007). The XMM-Newton bright serendipitous survey. Astronomy and Astrophysics. 477(3). 735–746. 27 indexed citations

10.

Caccianiga, A., F. Cocchia, R. Della Ceca, et al.. (2007). Searching for absorbed AGN in the 2XMM-Newtonpre-release EPIC Serendipitous Source Catalogue. Astronomy and Astrophysics. 465(3). 759–764. 1 indexed citations

11.

Watson, M. G., T. P. Roberts, Masayuki Akiyama, & Yoshihiro Ueda. (2005). Discovery of multiple ultra-luminous X-ray sources in the galaxy\nKUG 0214-057. Springer Link (Chiba Institute of Technology). 2 indexed citations

12.

Barcons, X., F. J. Carrera, M. T. Ceballos, et al.. (2003). The XMM‐Newton Survey Science Centre Medium Sensitivity Survey. Astronomische Nachrichten. 324(1-2). 44–47. 4 indexed citations

13.

Severgnini, P., A. Caccianiga, V. Braito, et al.. (2003). XMM-Newtonobservations reveal AGN in apparently normal galaxies. Astronomy and Astrophysics. 406(2). 483–492. 59 indexed citations

14.

Lamer, G., A. Schwope, M. Elvis, D. J. Burke, & M. G. Watson. (2003). The XMM‐Newton SSC serendipitous cluster survey. Astronomische Nachrichten. 324(1-2). 156–156. 1 indexed citations

15.

Osborne, J. P., K. Borozdin, S. Trudolyubov, et al.. (2001). The central region of M 31 observed with $\vec{XMM}$-$\vec{Newton}$. Astronomy and Astrophysics. 378(3). 800–805. 41 indexed citations

16.

Shirey, R., Roberto Soria, K. Borozdin, et al.. (2001). The central region of M 31 observed withXMM-Newton. Astronomy and Astrophysics. 365(1). L195–L201. 47 indexed citations

17.

Wheatley, P. J., F. Verbunt, T. Belloni, et al.. (1996). The X-ray and EUV spectrum of the dwarf nova VW Hyi in outburst and quiescence. UvA-DARE (University of Amsterdam). 307(1). 137–148. 3 indexed citations

18.

Ishida, M., Taro Sakao, Kazuo Makishima, et al.. (1992). Ginga observations of the old nova GK Persei in quiescence and outburst. Monthly Notices of the Royal Astronomical Society. 254(4). 647–654. 13 indexed citations

19.

Fabian, A. C., K. A. Arnaud, P. E. J. Nulsen, et al.. (1985). An X-ray, optical and radio study of PKS 0745 – 191: a massive cooling flow. Monthly Notices of the Royal Astronomical Society. 216(4). 923–932. 16 indexed citations

20.

Watson, M. G.. (1979). Galactic X-ray sources. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 366(1726). 329–344. 2 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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