R. M. Blake

420 total citations
10 papers, 285 citations indexed

About

R. M. Blake is a scholar working on Astronomy and Astrophysics, Instrumentation and Ophthalmology. According to data from OpenAlex, R. M. Blake has authored 10 papers receiving a total of 285 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 3 papers in Instrumentation and 1 paper in Ophthalmology. Recurrent topics in R. M. Blake's work include Stellar, planetary, and galactic studies (7 papers), Astro and Planetary Science (6 papers) and Astrophysics and Star Formation Studies (5 papers). R. M. Blake is often cited by papers focused on Stellar, planetary, and galactic studies (7 papers), Astro and Planetary Science (6 papers) and Astrophysics and Star Formation Studies (5 papers). R. M. Blake collaborates with scholars based in Canada, Poland and United States. R. M. Blake's co-authors include James R. Thomson, G. Stachowski, S. M. Ruciński, Christopher C. Capobianco, Wenxian Lu, S. W. Mochnacki, W. Ogłoza, W. Pych, K. Gazeas and T. Pribulla and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and The Astronomical Journal.

In The Last Decade

R. M. Blake

9 papers receiving 270 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
R. M. Blake Canada 6 281 65 36 35 17 10 285
R. Lopes de Oliveira Brazil 10 279 1.0× 38 0.6× 39 1.1× 32 0.9× 10 0.6× 25 293
D. Chochol Slovakia 9 275 1.0× 73 1.1× 13 0.4× 27 0.8× 17 1.0× 76 280
J. E. Solheim Norway 9 275 1.0× 106 1.6× 21 0.6× 20 0.6× 12 0.7× 29 287
M. Vaňko Slovakia 11 360 1.3× 125 1.9× 14 0.4× 40 1.1× 16 0.9× 73 367
E. Zietsman South Africa 8 248 0.9× 73 1.1× 24 0.7× 27 0.8× 12 0.7× 12 256
J. Lorenzo Spain 10 267 1.0× 75 1.2× 28 0.8× 16 0.5× 7 0.4× 14 271
S. R. Duck United Kingdom 8 337 1.2× 84 1.3× 18 0.5× 27 0.8× 6 0.4× 10 346
H. J. Hagen Germany 8 339 1.2× 73 1.1× 34 0.9× 34 1.0× 5 0.3× 17 344
Matthew W. Hosek United States 11 249 0.9× 84 1.3× 16 0.4× 20 0.6× 23 1.4× 27 260
В. П. Архипова Russia 10 298 1.1× 124 1.9× 18 0.5× 19 0.5× 10 0.6× 64 308

Countries citing papers authored by R. M. Blake

Since Specialization
Citations

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

Fields of papers citing papers by R. M. Blake

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of R. M. Blake

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

All Works

10 of 10 papers shown
1.
Pribulla, T., S. M. Ruciński, R. M. Blake, et al.. (2009). RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. XV. The Astronomical Journal. 137(3). 3655–3667. 48 indexed citations
2.
Gies, Douglas R., R. M. Blake, S. M. Caballero‐Nieves, et al.. (2008). Stellar Wind Variations during the X‐Ray High and Low States of Cygnus X‐11,2. The Astrophysical Journal. 678(2). 1237–1247. 41 indexed citations
3.
Tomov, T., M. Hajduk, A. Zajczyk, et al.. (2005). Spectroscopic Observations of the Ee Cep Eclipse in 2003. Astrophysics and Space Science. 296(1-4). 451–455.
4.
Blake, R. M. & S. M. Ruciński. (2004). Photometry and Spectroscopy of Short-Period Binary Stars in Four Old Open Clusters. American Astronomical Society Meeting Abstracts. 205. 1 indexed citations
5.
Vinkó, J., R. M. Blake, K. Sárneczky, et al.. (2004). Distance of the hypernova SN 2002ap via the expanding photosphere method. Astronomy and Astrophysics. 427(2). 453–464. 24 indexed citations
6.
Pych, W., S. M. Ruciński, James R. Thomson, et al.. (2004). Radial Velocity Studies of Close Binary Stars. IX.. The Astronomical Journal. 127(3). 1712–1719. 51 indexed citations
7.
Ruciński, S. M., Christopher C. Capobianco, Wenxian Lu, et al.. (2003). Radial Velocity Studies of Close Binary Stars. VIII.. The Astronomical Journal. 125(6). 3258–3264. 59 indexed citations
8.
Ruciński, S. M., Wenxian Lu, Christopher C. Capobianco, et al.. (2002). Radial Velocity Studies of Close Binary Stars. VI.. The Astronomical Journal. 124(3). 1738–1745. 56 indexed citations
9.
Blake, R. M., Houman Khosravani, & Paul Delaney. (2000). Period Changes in the SX Phoenicis Stars. part I. BL Camelopardalis and DY Pegasi. JRASC. 94. 124. 4 indexed citations
10.
Blake, R. M.. (1997). Differential Photometry of 700 Auravictrix. 24. 30. 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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