M. Eracleous

2.2k total citations
9 papers, 48 citations indexed

About

M. Eracleous is a scholar working on Astronomy and Astrophysics, Instrumentation and Global and Planetary Change. According to data from OpenAlex, M. Eracleous has authored 9 papers receiving a total of 48 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 2 papers in Instrumentation and 1 paper in Global and Planetary Change. Recurrent topics in M. Eracleous's work include Astrophysical Phenomena and Observations (7 papers), Galaxies: Formation, Evolution, Phenomena (6 papers) and Gamma-ray bursts and supernovae (3 papers). M. Eracleous is often cited by papers focused on Astrophysical Phenomena and Observations (7 papers), Galaxies: Formation, Evolution, Phenomena (6 papers) and Gamma-ray bursts and supernovae (3 papers). M. Eracleous collaborates with scholars based in United States, United Kingdom and France. M. Eracleous's co-authors include J. C. Charlton, J. P. Halpern, K. Horne, T. R. Marsh, A. Bruch, Fuhua Cheng, Sowgat Muzahid, R. Srianand, D. O’Donoghue and Finn E. Christensen and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Proceedings of the International Astronomical Union.

In The Last Decade

M. Eracleous

8 papers receiving 47 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
M. Eracleous United States	5	47	11	7	3	3	9	48
A.-S. Bak Nielsen Netherlands	4	45 1.0×	15 1.4×	7 1.0×		2 0.7×	5	47
Teagan A. Clarke Australia	4	48 1.0×	7 0.6×	4 0.6×	3 1.0×		6	49
D. W. Kim Italy	2	52 1.1×	17 1.5×	2 0.3×	5 1.7×	2 0.7×	2	53
E. T. Lin Taiwan	4	53 1.1×	17 1.5×	2 0.3×	3 1.0×	3 1.0×	6	56
V. Fafone Italy	2	28 0.6×	5 0.5×	6 0.9×		2 0.7×	2	28
Shu Koyama Japan	4	35 0.7×	19 1.7×	6 0.9×	2 0.7×		9	42
Antonella Fruscione United States	3	36 0.8×	13 1.2×	3 0.4×	3 1.0×	1 0.3×	4	38
J. Fischera Germany	4	51 1.1×	10 0.9×	2 0.3×	2 0.7×		4	54
C. Delvaux Germany	6	96 2.0×	30 2.7×	10 1.4×	3 1.0×	4 1.3×	10	96
N. Khetan Australia	3	60 1.3×	22 2.0×	4 0.6×	3 1.0×		6	60

Countries citing papers authored by M. Eracleous

Since Specialization

Citations

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

Fields of papers citing papers by M. Eracleous

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Eracleous

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

9 of 9 papers shown

1.

Charlton, J. C., et al.. (2019). Probing quasar winds using intrinsic narrow absorption lines. Monthly Notices of the Royal Astronomical Society. 488(4). 4690–4731. 4 indexed citations

2.

Maccarone, Thomas J., Mihoko Yukita, A. E. Hornschemeier, et al.. (2016). Demonstrating the likely neutron star nature of five M31 globular cluster sources withSwift-NuSTAR spectroscopy. Monthly Notices of the Royal Astronomical Society. 458(4). 3633–3643. 10 indexed citations

3.

Muzahid, Sowgat, R. Srianand, J. C. Charlton, & M. Eracleous. (2016). On the covering fraction variability in an EUV mini-BAL outflow from PG 1206+459. Monthly Notices of the Royal Astronomical Society. 457(3). 2665–2674. 8 indexed citations

4.

Binder, Breanna A., Benjamin F. Williams, M. Eracleous, et al.. (2013). THECHANDRALOCAL VOLUME SURVEY: THE X-RAY POINT-SOURCE POPULATION OF NGC 404. The Astrophysical Journal. 763(2). 128–128. 2 indexed citations

5.

Eracleous, M., M. Sipior, & Steinn Sigurðsson. (2005). Models for the Evolution of X-Ray Binaries in a Young Stellar Population. Proceedings of the International Astronomical Union. 1(S230). 417–422.

6.

Eracleous, M., et al.. (2004). Simulations of the evolution of the X-Ray properties of a young stellar population. Proceedings of the International Astronomical Union. 2004(IAUS222). 165–166. 2 indexed citations

7.

Eracleous, M., Bradley E. Schaefer, J. Mader, & Coral Wheeler. (2002). GRB021004: optical spectroscopy.. GRB Coordinates Network. 1579. 1. 2 indexed citations

8.

Halpern, J. P. & M. Eracleous. (2000). The End of the Lines for OX 169: No Binary Broad‐Line Region. The Astrophysical Journal. 531(2). 647–653. 5 indexed citations

9.

Marsh, T. R., K. Horne, Fuhua Cheng, et al.. (1996). Superhumps and ultraviolet superdips: HST observations of OY Car. Monthly Notices of the Royal Astronomical Society. 279(4). 1274–1288. 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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