G. Hill

460 total citations
25 papers, 272 citations indexed

About

G. Hill is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, G. Hill has authored 25 papers receiving a total of 272 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 12 papers in Instrumentation and 5 papers in Computational Mechanics. Recurrent topics in G. Hill's work include Stellar, planetary, and galactic studies (21 papers), Astronomy and Astrophysical Research (12 papers) and Astrophysics and Star Formation Studies (9 papers). G. Hill is often cited by papers focused on Stellar, planetary, and galactic studies (21 papers), Astronomy and Astrophysical Research (12 papers) and Astrophysics and Star Formation Studies (9 papers). G. Hill collaborates with scholars based in Canada, United States and United Kingdom. G. Hill's co-authors include R. W. Hilditch, Tim J. Harries, S. A. Bell, A. P. Reynolds, Saul J. Adelman, A. F. Gulliver, F. Royer, Richard Monier, M. Gebran and T. A. A. Sigut and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

G. Hill

23 papers receiving 267 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
G. Hill Canada 11 264 124 22 12 10 25 272
Michael S. Wiggs United States 8 183 0.7× 64 0.5× 21 1.0× 18 1.5× 10 1.0× 12 192
В. П. Архипова Russia 10 298 1.1× 124 1.0× 19 0.9× 18 1.5× 10 1.0× 64 308
S. Štefl Czechia 12 395 1.5× 113 0.9× 26 1.2× 9 0.8× 10 1.0× 30 400
A. W. Fullerton United States 12 412 1.6× 150 1.2× 24 1.1× 10 0.8× 9 0.9× 22 416
C. Morossi Italy 9 195 0.7× 79 0.6× 12 0.5× 8 0.7× 9 0.9× 38 201
W. A. Dziembowski Poland 6 269 1.0× 137 1.1× 22 1.0× 9 0.8× 8 0.8× 19 278
D. Schoênberner Germany 8 452 1.7× 205 1.7× 37 1.7× 12 1.0× 10 1.0× 27 467
W. Seggewiß Canada 12 361 1.4× 96 0.8× 53 2.4× 13 1.1× 8 0.8× 42 370
J. P. Caillault United States 7 315 1.2× 57 0.5× 18 0.8× 14 1.2× 11 1.1× 17 319
S. J. Smartt United Kingdom 7 360 1.4× 157 1.3× 25 1.1× 23 1.9× 10 1.0× 9 362

Countries citing papers authored by G. Hill

Since Specialization
Citations

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

Fields of papers citing papers by G. Hill

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of G. Hill

This figure shows the co-authorship network connecting the top 25 collaborators of G. Hill. A scholar is included among the top collaborators of G. Hill 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 G. Hill. G. Hill 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.
Royer, F., M. Gebran, Richard Monier, et al.. (2014). Normal A0--A1 stars with low rotational velocities. I. Abundance determination and classification. Americanae (AECID Library). 14 indexed citations
2.
Royer, F., M. Gebran, Richard Monier, et al.. (2013). Normal A0−A1 stars with low rotational velocities. Astronomy and Astrophysics. 562. A84–A84. 27 indexed citations
3.
Adelman, Saul J., et al.. (2011). Elemental abundance analyses with DAO spectrograms: XXXII. HR 6455 (A3 III), δ Aqr (A3 V), η Lep (F2 V), and 1 Boo (A1 V). Astronomische Nachrichten. 332(7). 681–689. 5 indexed citations
4.
Hilditch, R. W., D. Kilkenny, A. E. Lynas‐Gray, & G. Hill. (2003). New VIC photometry of the sdOB binary AA Dor and an improved photometric model. Monthly Notices of the Royal Astronomical Society. 344(2). 644–650. 17 indexed citations
5.
Harries, Tim J., R. W. Hilditch, & G. Hill. (1997). Interacting O-star binaries: V382 Cyg, V448 Cyg and XZ Cep. Monthly Notices of the Royal Astronomical Society. 285(2). 277–287. 27 indexed citations
6.
Hilditch, R. W., Tim J. Harries, & G. Hill. (1996). On the reflection effect in three sdOB binary stars. Monthly Notices of the Royal Astronomical Society. 279(4). 1380–1392. 44 indexed citations
7.
Ryabchikova, T., G. Hill, J. D. Landstreet, N. Piskunov, & T. A. A. Sigut. (1994). Astrophysical determination of optical oscillator strengths for Ti II. Monthly Notices of the Royal Astronomical Society. 267(3). 697–710. 23 indexed citations
8.
Reynolds, A. P., R. W. Hilditch, S. A. Bell, & G. Hill. (1993). Optical spectroscopy of the massive X-ray binary SMC X-1/Sk 160⋆. Monthly Notices of the Royal Astronomical Society. 261(2). 337–345. 19 indexed citations
9.
Hill, G., et al.. (1993). Studies of early-type variable stars. IX. The orbit and physical parameters of V1425 Cygni.. 276(1). 57–68. 1 indexed citations
10.
Henrichs, H. F., et al.. (1993). β Cep: a Magnetic Be Star?. International Astronomical Union Colloquium. 139. 186–187. 1 indexed citations
11.
Hilditch, R. W., G. Hill, & S. A. Bell. (1992). Radial velocities of the contact binary system RW Doradus. Monthly Notices of the Royal Astronomical Society. 255(2). 285–288. 10 indexed citations
12.
Hill, G., et al.. (1992). Studies of late-type binaries. V. The orbit and physical parameters of V 1073 Cygni.. 265(2). 597–604. 3 indexed citations
13.
Adelman, Saul J., et al.. (1991). Elemental abundance analyses with DAO spectrograms - VIII. The normal F main sequence stars Theta Cygni and Iota Piscium. Monthly Notices of the Royal Astronomical Society. 252(3). 329–333. 5 indexed citations
14.
Fletcher, J. M., et al.. (1991). The binary system Sigma 2173. Publications of the Astronomical Society of the Pacific. 103. 294–294. 3 indexed citations
15.
Bell, S. A., G. Hill, R. W. Hilditch, et al.. (1991). Eclipsing binaries in the Magellanic Clouds - I. Absolute dimensions and distance modulus for HV 2226 in the Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society. 250(1). 119–126. 15 indexed citations
16.
Adamson, A. J., et al.. (1988). Kinematics and properties of F stars near the North Galactic Pole - II. The isothermal disc. Monthly Notices of the Royal Astronomical Society. 230(2). 273–320. 2 indexed citations
17.
Stryker, L. L., et al.. (1985). The binary frequency of extreme subdwarfs revisited. Publications of the Astronomical Society of the Pacific. 97. 247–247. 16 indexed citations
18.
Batten, Alan H., et al.. (1983). A revised spectroscopic orbit for 93 Leonis (HD 102509). Publications of the Astronomical Society of the Pacific. 95. 768–768. 3 indexed citations
19.
Hill, G., et al.. (1976). Studies of A and F stars in the region of the North galactic pole—I. Radial velocities and MK classifications. 82. 69.
20.
Hill, G., et al.. (1971). Standard stars for the five-color photometric system of the Dominion Astrophysical Observatory. The Astronomical Journal. 76. 246–246.

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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