A. M. Read

2.9k total citations · 1 hit paper
50 papers, 1.6k citations indexed

About

A. M. Read is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, A. M. Read has authored 50 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 50 papers in Astronomy and Astrophysics, 24 papers in Nuclear and High Energy Physics and 6 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in A. M. Read's work include Astrophysical Phenomena and Observations (43 papers), Astrophysics and Cosmic Phenomena (24 papers) and Galaxies: Formation, Evolution, Phenomena (24 papers). A. M. Read is often cited by papers focused on Astrophysical Phenomena and Observations (43 papers), Astrophysics and Cosmic Phenomena (24 papers) and Galaxies: Formation, Evolution, Phenomena (24 papers). A. M. Read collaborates with scholars based in United Kingdom, Spain and Germany. A. M. Read's co-authors include R. D. Saxton, P. Esquej, M. J. Freyberg, T. J. Ponman, Jennifer Carter, B. Altieri, G. Miniutti, W. Pietsch, K. D. Alexander and David Strickland and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and Geophysical Research Letters.

In The Last Decade

A. M. Read

48 papers receiving 1.5k citations

Hit Papers

Nine-hour X-ray quasi-periodic eruptions from a low-mass ... 2019 2026 2021 2023 2019 50 100 150

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. M. Read United Kingdom 24 1.6k 611 69 66 63 50 1.6k
R. D. Saxton Spain 25 1.8k 1.2× 646 1.1× 75 1.1× 74 1.1× 90 1.4× 88 1.9k
G. Leloudas Denmark 24 1.6k 1.0× 592 1.0× 51 0.7× 112 1.7× 55 0.9× 75 1.8k
A. R. Rao India 19 1.3k 0.8× 588 1.0× 106 1.5× 53 0.8× 116 1.8× 158 1.4k
A. A. Breeveld United Kingdom 18 1.3k 0.8× 413 0.7× 64 0.9× 115 1.7× 77 1.2× 64 1.3k
R. S. Warwick United Kingdom 15 1.1k 0.7× 640 1.0× 58 0.8× 35 0.5× 69 1.1× 43 1.2k
M. Ribó Spain 22 1.5k 0.9× 777 1.3× 72 1.0× 43 0.7× 78 1.2× 92 1.5k
M. G. Watson United Kingdom 22 1.2k 0.8× 468 0.8× 43 0.6× 88 1.3× 73 1.2× 60 1.3k
K. P. Singh India 17 1.2k 0.7× 360 0.6× 34 0.5× 91 1.4× 77 1.2× 144 1.2k
O. Godet France 20 1.4k 0.9× 443 0.7× 115 1.7× 87 1.3× 81 1.3× 75 1.5k
E. M. Schlegel United States 23 2.0k 1.3× 755 1.2× 60 0.9× 85 1.3× 142 2.3× 132 2.0k

Countries citing papers authored by A. M. Read

Since Specialization
Citations

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

Fields of papers citing papers by A. M. Read

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. M. Read

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

All Works

20 of 20 papers shown
1.
Miniutti, G., M. Giustini, R. Arcodia, et al.. (2023). Alive and kicking: A new QPE phase in GSN 069 revealing a quiescent luminosity threshold for QPEs. Astronomy and Astrophysics. 674. L1–L1. 40 indexed citations
2.
Miniutti, G., M. Giustini, R. Arcodia, et al.. (2022). Repeating tidal disruptions in GSN 069: Long-term evolution and constraints on quasi-periodic eruptions’ models. Astronomy and Astrophysics. 670. A93–A93. 60 indexed citations
3.
Saxton, R. D., A. M. Read, S. Komossa, et al.. (2019). XMMSL2 J144605.0+685735: a slow tidal disruption event. Astronomy and Astrophysics. 630. A98–A98. 21 indexed citations
4.
Saxton, R. D., A. M. Read, S. Komossa, et al.. (2016). XMMSL1 J074008.2-853927: a tidal disruption event with thermal and non-thermal components. Astronomy and Astrophysics. 598. A29–A29. 53 indexed citations
5.
Saxton, R. D., A. M. Read, S. Komossa, et al.. (2014). An X-ray and UV flare from the galaxy XMMSL1 J061927.1-655311. Astronomy and Astrophysics. 572. A1–A1. 24 indexed citations
6.
Warwick, R. S., R. D. Saxton, & A. M. Read. (2012). TheXMM-Newtonslew survey in the 2–10 keV band. Astronomy and Astrophysics. 548. A99–A99. 28 indexed citations
7.
Page, K. L., J. P. Osborne, A. M. Read, et al.. (2009). X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst. Springer Link (Chiba Institute of Technology). 3 indexed citations
8.
Read, A. M., R. D. Saxton, P. G. Jonker, et al.. (2009). XMMSL1 J060636.2-694933: an XMM-Newton slew discovery and Swift/Magellan follow up of a new classical nova in the LMC. Astronomy and Astrophysics. 506(3). 1309–1317. 3 indexed citations
9.
Bauer, Michael, W. Pietsch, G. Trinchieri, et al.. (2008). XMM-Newton observations of the diffuse X-ray emission in the starburst galaxy NGC 253\n. Springer Link (Chiba Institute of Technology). 19 indexed citations
10.
Esquej, P., R. D. Saxton, S. Komossa, et al.. (2008). Evolution of tidal disruption candidates discovered by XMM-Newton. Astronomy and Astrophysics. 489(2). 543–554. 98 indexed citations
11.
Carter, Jennifer & A. M. Read. (2007). The XMM-Newton EPIC background and the production of background blank sky event files. Springer Link (Chiba Institute of Technology). 62 indexed citations
12.
Read, A. M., R. D. Saxton, J. P. Osborne, et al.. (2007). XMM-Newton and Swift-XRT see declining X-ray flux from the nova XMMSL1 J070542.7-381442 (V598 Pup). The astronomer's telegram. 1301. 1. 1 indexed citations
13.
Warwick, R. S., et al.. (2007). An XMM–Newton view of M101 – III. Diffuse X-ray emission. Monthly Notices of the Royal Astronomical Society. 376(4). 1611–1620. 13 indexed citations
14.
Esquej, P., R. D. Saxton, M. J. Freyberg, et al.. (2006). Candidate tidal disruption events from the XMM-Newton slew survey. Astronomy and Astrophysics. 462(3). L49–L52. 79 indexed citations
15.
Read, A. M. & W. Pietsch. (2001). X-ray emission from the Sculptor galaxy NGC 300. Springer Link (Chiba Institute of Technology). 26 indexed citations
16.
Sciortino, S., G. Micela, F. Damiani, et al.. (2001). XMM-Newton survey of the low-metallicity open cluster NGC 2516. Springer Link (Chiba Institute of Technology). 18 indexed citations
17.
Warwick, R. S., J.-P. Bernard, F. Bocchino, et al.. (2001). The extended X-ray halo of the Crab-like SNR G21.5-0.9. Astronomy and Astrophysics. 365(1). L248–L253. 27 indexed citations
18.
Read, A. M., M. D. Filipović, W. Pietsch, & P. A. Jones. (2001). Radio jets and diffuse X-ray emission around the peculiar galaxy pair ESO 295-IG022. Astronomy and Astrophysics. 369(2). 467–472. 2 indexed citations
19.
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
20.
Hasinger, G., W. H. G. Lewin, E. A. Magnier, et al.. (2001). The second ROSAT PSPC survey of M 31 and the complete ROSAT PSPC source list. Astronomy and Astrophysics. 373(1). 63–99. 56 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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