G. Meylan

500 total citations
9 papers, 211 citations indexed

About

G. Meylan is a scholar working on Astronomy and Astrophysics, Instrumentation and Infectious Diseases. According to data from OpenAlex, G. Meylan has authored 9 papers receiving a total of 211 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 4 papers in Instrumentation and 0 papers in Infectious Diseases. Recurrent topics in G. Meylan's work include Galaxies: Formation, Evolution, Phenomena (9 papers), Astronomy and Astrophysical Research (4 papers) and Astrophysical Phenomena and Observations (4 papers). G. Meylan is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (9 papers), Astronomy and Astrophysical Research (4 papers) and Astrophysical Phenomena and Observations (4 papers). G. Meylan collaborates with scholars based in Switzerland, Belgium and United States. G. Meylan's co-authors include F. Courbin, Pierre Magain, E. Eulaers, Dominique Sluse, C. Vuissoz, I. M. Asfandiyarov, Sushil Kumar, H. Van Winckel, T. P. Prabhu and Sh. A. Ehgamberdiev and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Proceedings of the International Astronomical Union.

In The Last Decade

G. Meylan

9 papers receiving 202 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
G. Meylan Switzerland	8	204	67	35	17	9	9	211
Brice Ménard United States	5	156 0.8×	60 0.9×	23 0.7×	14 0.8×	10 1.1×	5	158
J. M. Miralles Germany	8	202 1.0×	111 1.7×	45 1.3×	23 1.4×	7 0.8×	13	211
I. M. Asfandiyarov Uzbekistan	6	236 1.2×	60 0.9×	56 1.6×	23 1.4×	15 1.7×	12	244
M. Lerchster Germany	6	185 0.9×	104 1.6×	27 0.8×	26 1.5×	14 1.6×	9	189
K. Holhjem Germany	3	128 0.6×	62 0.9×	19 0.5×	13 0.8×	12 1.3×	5	134
Stefania Giodini United Kingdom	3	199 1.0×	130 1.9×	22 0.6×	18 1.1×	12 1.3×	3	201
F. Kenn Netherlands	4	300 1.5×	136 2.0×	19 0.5×	36 2.1×	7 0.8×	9	307
R. T. Corrigan Canada	4	253 1.2×	47 0.7×	70 2.0×	35 2.1×	6 0.7×	4	260
R. Kayser Germany	8	221 1.1×	52 0.8×	29 0.8×	37 2.2×	4 0.4×	23	228
Massimo Pascale United States	7	189 0.9×	106 1.6×	21 0.6×	6 0.4×	4 0.4×	12	207

Countries citing papers authored by G. Meylan

Since Specialization

Citations

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

Fields of papers citing papers by G. Meylan

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

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

Eulaers, E., M. Tewes, Pierre Magain, et al.. (2013). COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses. Astronomy and Astrophysics. 553. A121–A121. 41 indexed citations

2.

Kumar, Sushil, M. Tewes, C. S. Stalin, et al.. (2013). COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses XIV. Time delay of the doubly lensed quasar SDSS J1001+5027. arXiv (Cornell University). 28 indexed citations

3.

Vuissoz, C., F. Courbin, Dominique Sluse, et al.. (2008). COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses VII. Time delays and the Hubble constant from WFI J2033-4723. Zurich Open Repository and Archive (University of Zurich). 33 indexed citations

4.

Djorgovski, S. G., F. Courbin, G. Meylan, et al.. (2007). Discovery of a Probable Physical Triple Quasar. The Astrophysical Journal. 662(1). L1–L5. 33 indexed citations

5.

Bergond, G., E. Athanassoula, S. Léon, et al.. (2007). Globular clusters and dwarf galaxies in Fornax. Astronomy and Astrophysics. 464(2). L21–L24. 28 indexed citations

6.

Rejkuba, M., P. Dubath, D. Minniti, & G. Meylan. (2007). Masses and M/L Ratios of Bright Globular Clusters in NGC 5128. Proceedings of the International Astronomical Union. 3(S246). 418–422. 1 indexed citations

7.

Saha, Prasenjit, F. Courbin, Dominique Sluse, S. Dye, & G. Meylan. (2006). COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses IV. Models of prospective time-delay lenses. ArXiv.org. 11 indexed citations

8.

Courbin, F., J. Poels, Pierre Magain, et al.. (2005). Photometric monitoring of the doubly imaged quasar UM 673: possible evidence for chromatic microlensing. Astronomy and Astrophysics. 441(2). 443–450. 7 indexed citations

9.

Eigenbrod, A., et al.. (2005). COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses III. Redshift of the lensing galaxy in eight gravitationally lensed quasars. ArXiv.org. 29 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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