V. Doublier

5.3k total citations
8 papers, 325 citations indexed

About

V. Doublier is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, V. Doublier has authored 8 papers receiving a total of 325 indexed citations (citations by other indexed papers that have themselves been cited), including 7 papers in Astronomy and Astrophysics, 3 papers in Instrumentation and 2 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in V. Doublier's work include Galaxies: Formation, Evolution, Phenomena (6 papers), Stellar, planetary, and galactic studies (6 papers) and Astronomy and Astrophysical Research (3 papers). V. Doublier is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (6 papers), Stellar, planetary, and galactic studies (6 papers) and Astronomy and Astrophysical Research (3 papers). V. Doublier collaborates with scholars based in Germany, France and United States. V. Doublier's co-authors include G. Comte, A. Caulet, D. Cormier, S. C. Madden, S. Hony, M. Galametz, F. Galliano, Frank Bigiel, N. P. Abel and A. Boselli and has published in prestigious journals such as Astronomy and Astrophysics, Astronomy and Astrophysics Supplement Series and CaltechAUTHORS (California Institute of Technology).

In The Last Decade

V. Doublier

8 papers receiving 318 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
V. Doublier Germany	6	322	95	28	14	7	8	325
O. Ł. Karczewski France	8	368 1.1×	60 0.6×	36 1.3×	14 1.0×	4 0.6×	12	372
N. Fiolet France	5	247 0.8×	76 0.8×	24 0.9×	14 1.0×	7 1.0×	5	250
G. Bosch Argentina	12	473 1.5×	118 1.2×	45 1.6×	10 0.7×	5 0.7×	33	480
A. Rémy-Ruyer France	8	432 1.3×	72 0.8×	35 1.3×	17 1.2×	5 0.7×	9	438
Alessandro Boselli Italy	5	223 0.7×	47 0.5×	25 0.9×	11 0.8×	7 1.0×	5	227
Н. П. Иконникова Russia	11	333 1.0×	128 1.3×	17 0.6×	11 0.8×	10 1.4×	72	340
Robert Cumming Sweden	12	452 1.4×	84 0.9×	71 2.5×	7 0.5×	9 1.3×	20	468
M. S. Westmoquette United States	14	560 1.7×	118 1.2×	57 2.0×	11 0.8×	11 1.6×	22	568
E. Recillas Mexico	8	184 0.6×	45 0.5×	43 1.5×	12 0.9×	8 1.1×	22	192
C. P. Pearson United Kingdom	4	205 0.6×	43 0.5×	25 0.9×	18 1.3×	5 0.7×	4	207

Countries citing papers authored by V. Doublier

Since Specialization

Citations

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

Fields of papers citing papers by V. Doublier

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of V. Doublier

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

8 of 8 papers shown

1.

Cormier, D., S. C. Madden, V. Lebouteiller, et al.. (2015). TheHerschelDwarf Galaxy Survey. Astronomy and Astrophysics. 578. A53–A53. 132 indexed citations

2.

Cormier, D., S. C. Madden, V. Lebouteiller, et al.. (2015). The Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy. CaltechAUTHORS (California Institute of Technology). 59 indexed citations

3.

Cormier, D., S. C. Madden, S. Hony, et al.. (2010). The effects of star formation on the low-metallicity ISM: NGC 4214 mapped withHerschel/PACS spectroscopy. Astronomy and Astrophysics. 518. L57–L57. 23 indexed citations

4.

Hummel, W., et al.. (2002). Quality control of VLT ISAAC data. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4844. 417–417. 2 indexed citations

5.

Doublier, V., A. Caulet, & G. Comte. (2001). The 1 to 2.5 $\mathsf{\mu}$ broad band emission of Blue Compact Dwarf Galaxies. Astronomy and Astrophysics. 367(1). 33–45. 16 indexed citations

6.

Doublier, V., J. M. Más-Hesse, A. Caulet, & D. Kunth. (2001). Red supergiant stars in blue compact dwarf galaxies: The case of Tol 0610-387. Astronomy and Astrophysics. 372(1). 22–28. 2 indexed citations

7.

Doublier, V., A. Caulet, & G. Comte. (1999). Multi-spectral study of a new sample of Blue Compact DwarfGalaxies. Astronomy and Astrophysics Supplement Series. 138(2). 213–245. 49 indexed citations

8.

Doublier, V., G. Comte, А. Р. Петросян, C. Surace, & M. Turatto. (1997). Multi-spectral study of a new sample of blue compact dwarf galaxies. Astronomy and Astrophysics Supplement Series. 124(3). 405–424. 42 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.

Explore authors with similar magnitude of impact