J. Bernard‐Salas

7.1k total citations · 1 hit paper
86 papers, 2.9k citations indexed

About

J. Bernard‐Salas is a scholar working on Astronomy and Astrophysics, Instrumentation and Organic Chemistry. According to data from OpenAlex, J. Bernard‐Salas has authored 86 papers receiving a total of 2.9k indexed citations (citations by other indexed papers that have themselves been cited), including 84 papers in Astronomy and Astrophysics, 24 papers in Instrumentation and 7 papers in Organic Chemistry. Recurrent topics in J. Bernard‐Salas's work include Stellar, planetary, and galactic studies (73 papers), Astrophysics and Star Formation Studies (70 papers) and Astro and Planetary Science (28 papers). J. Bernard‐Salas is often cited by papers focused on Stellar, planetary, and galactic studies (73 papers), Astrophysics and Star Formation Studies (70 papers) and Astro and Planetary Science (28 papers). J. Bernard‐Salas collaborates with scholars based in United States, France and United Kingdom. J. Bernard‐Salas's co-authors include E. Peeters, J. Cami, H. W. W. Spoon, J. R. Houck, V. Charmandaris, Bernhard R. Brandl, S. R. Pottasch, D. Devost, L. Armus and V. Lebouteiller and has published in prestigious journals such as Science, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

J. Bernard‐Salas

80 papers receiving 2.8k citations

Hit Papers

Detection of C 60 and C 70 in a Young Planetary Nebula 2010 2026 2015 2020 2010 100 200 300 400 500

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
J. Bernard‐Salas United States 30 2.7k 531 448 401 319 86 2.9k
D. A. García–Hernández Spain 31 3.2k 1.2× 1.2k 2.2× 242 0.5× 326 0.8× 158 0.5× 184 3.6k
M. Jura United States 40 4.2k 1.6× 605 1.1× 339 0.8× 141 0.4× 344 1.1× 140 4.6k
S. Hony France 28 2.8k 1.0× 355 0.7× 383 0.9× 95 0.2× 580 1.8× 65 3.0k
E. Peeters United States 31 3.4k 1.3× 241 0.5× 1.2k 2.6× 704 1.8× 1.0k 3.2× 96 4.0k
Г. А. Галазутдинов Russia 23 1.6k 0.6× 160 0.3× 631 1.4× 112 0.3× 607 1.9× 146 1.9k
L. M. Hobbs United States 32 2.7k 1.0× 360 0.7× 455 1.0× 76 0.2× 364 1.1× 134 3.1k
A. Kovács United States 20 1.5k 0.6× 269 0.5× 335 0.7× 40 0.1× 382 1.2× 55 1.8k
L. Verstraete France 20 1.3k 0.5× 80 0.2× 327 0.7× 72 0.2× 287 0.9× 41 1.4k
J. Krełowski Poland 26 1.8k 0.7× 86 0.2× 876 2.0× 160 0.4× 881 2.8× 136 2.2k
Isabelle Cherchneff Switzerland 20 1.2k 0.5× 70 0.1× 424 0.9× 72 0.2× 367 1.2× 45 1.5k

Countries citing papers authored by J. Bernard‐Salas

Since Specialization
Citations

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

Fields of papers citing papers by J. Bernard‐Salas

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by J. Bernard‐Salas. 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 J. Bernard‐Salas. The network helps show where J. Bernard‐Salas may publish in the future.

Co-authorship network of co-authors of J. Bernard‐Salas

This figure shows the co-authorship network connecting the top 25 collaborators of J. Bernard‐Salas. A scholar is included among the top collaborators of J. Bernard‐Salas 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 J. Bernard‐Salas. J. Bernard‐Salas 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.
Sahai, R., G. C. Van de Steene, P. A. M. van Hoof, et al.. (2025). JWST Observations of the Ring Nebula (NGC 6720). III. A Dusty Disk around Its Central Star. The Astrophysical Journal. 985(1). 101–101. 2 indexed citations
2.
Corre, Daniel Le, et al.. (2025). New candidate cave entrances on the Moon found using deep learning. Icarus. 441. 116675–116675.
4.
Aleman, Isabel, J. Bernard‐Salas, Joel H. Kastner, Toshiya Ueta, & E. Villaver. (2020). WORKPLANS: Workshop on Planetary Nebula Observations. Galaxies. 8(1). 23–23. 1 indexed citations
5.
Bernard‐Salas, J., et al.. (2018). Neon, sulphur, and argon abundances of planetary nebulae in the sub-solar metallicity Galactic anti-centre. Astronomy and Astrophysics. 615. A29–A29. 3 indexed citations
6.
Pearson, Chris, D. Rigopoulou, Peter D. Hurley, et al.. (2016). HERUS: A CO ATLAS FROM SPIRE SPECTROSCOPY OF LOCAL ULIRGs. The Astrophysical Journal Supplement Series. 227(1). 9–9. 24 indexed citations
7.
Habart, E., J. Bernard‐Salas, J. R. Goicoechea, et al.. (2016). Spatial distribution of far-infrared rotationally excited CH+and OH emission lines in the Orion Bar photodissociation region. Astronomy and Astrophysics. 599. A20–A20. 16 indexed citations
8.
Guillard, P., F. Boulanger, M. D. Lehnert, et al.. (2015). Exceptional AGN-driven turbulence inhibits star formation in the 3C 326N radio galaxy. Springer Link (Chiba Institute of Technology). 32 indexed citations
9.
Pottasch, S. R. & J. Bernard‐Salas. (2015). Abundances of planetary nebulae in the Galactic bulge. Astronomy and Astrophysics. 583. A71–A71. 4 indexed citations
10.
Köhler, M., E. Habart, H. Arab, et al.. (2014). Physical structure of the photodissociation regions in NGC 7023. Astronomy and Astrophysics. 569. A109–A109. 13 indexed citations
11.
Pottasch, S. R. & J. Bernard‐Salas. (2013). Dust properties in the Galactic bulge. Springer Link (Chiba Institute of Technology). 5 indexed citations
12.
Sloan, G. C., et al.. (2011). Standard stars observed with the Infrared Spectrograph on the Spitzer Space Telescope. AAS. 217. 1 indexed citations
13.
Pottasch, S. R., et al.. (2011). Abundances in planetary nebulae: NGC 1535, NGC 6629, He2-108, and Tc1. Astronomy and Astrophysics. 531. A23–A23. 20 indexed citations
14.
Pottasch, S. R., J. Bernard‐Salas, & Thomas L. Roellig. (2009). Abundances in the planetary nebula NGC 6210. Astronomy and Astrophysics. 499(1). 249–256. 17 indexed citations
15.
Pottasch, S. R. & J. Bernard‐Salas. (2008). Abundances of planetary nebulae NGC 3242 and NGC 6369. Astronomy and Astrophysics. 490(2). 715–724. 10 indexed citations
16.
Bernard‐Salas, J., et al.. (2007). Abundances of planetary nebula M 1-42. Astronomy and Astrophysics. 471(3). 865–872. 6 indexed citations
17.
Bernard‐Salas, J. & A. G. G. M. Tielens. (2005). Physical conditions in Photo-Dissociation Regions around Planetary Nebulae. Astronomy and Astrophysics. 431(2). 523–538. 27 indexed citations
18.
Pottasch, S. R., Siek Hyung, L. H. Aller, et al.. (2003). Abundances of the planetary nebula Hu 1-2. University of Groningen research database (University of Groningen / Centre for Information Technology). 7 indexed citations
19.
Bernard‐Salas, J., S. R. Pottasch, P. R. Wesselius, & W. A. Feibelman. (2003). Abundances of Planetary Nebulae BD+30 3639 and NGC 6543. Astronomy and Astrophysics. 406(1). 165–174. 24 indexed citations
20.
Bernard‐Salas, J., S. R. Pottasch, D. A. Beintema, & P. R. Wesselius. (2003). The ISO–SWS spectrum of planetary nebula NGC 7027. Astronomy and Astrophysics. 406(1). 175–175. 2 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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