J. P. Baluteau

3.2k total citations
24 papers, 613 citations indexed

About

J. P. Baluteau is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Spectroscopy. According to data from OpenAlex, J. P. Baluteau has authored 24 papers receiving a total of 613 indexed citations (citations by other indexed papers that have themselves been cited), including 15 papers in Astronomy and Astrophysics, 10 papers in Atmospheric Science and 7 papers in Spectroscopy. Recurrent topics in J. P. Baluteau's work include Astrophysics and Star Formation Studies (11 papers), Stellar, planetary, and galactic studies (11 papers) and Atmospheric Ozone and Climate (10 papers). J. P. Baluteau is often cited by papers focused on Astrophysics and Star Formation Studies (11 papers), Stellar, planetary, and galactic studies (11 papers) and Atmospheric Ozone and Climate (10 papers). J. P. Baluteau collaborates with scholars based in France, Netherlands and United Kingdom. J. P. Baluteau's co-authors include P. Cox, E. Bussoletti, D. Schaerer, E. Peeters, N. L. Martín-Hernández, C. Morisset, F. Damour, A. G. G. M. Tielens, J. S. Mathis and P. R. Roelfsema and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

J. P. Baluteau

22 papers receiving 585 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
J. P. Baluteau France 12 529 129 112 70 59 24 613
A. Phillips Australia 9 285 0.5× 148 1.1× 90 0.8× 119 1.7× 34 0.6× 18 380
F. J. Vrba United States 18 678 1.3× 163 1.3× 76 0.7× 28 0.4× 50 0.8× 40 692
M. Pérault France 12 478 0.9× 82 0.6× 93 0.8× 24 0.3× 30 0.5× 34 513
P. Deroo United States 13 597 1.1× 182 1.4× 188 1.7× 65 0.9× 163 2.8× 19 708
A. Winnberg Sweden 14 545 1.0× 153 1.2× 150 1.3× 58 0.8× 48 0.8× 94 619
Lynne K. Deutsch United States 16 642 1.2× 87 0.7× 48 0.4× 36 0.5× 94 1.6× 29 661
Loris Magnani United States 16 825 1.6× 213 1.7× 273 2.4× 72 1.0× 29 0.5× 64 914
M. F. Kessler Netherlands 9 476 0.9× 104 0.8× 78 0.7× 65 0.9× 68 1.2× 29 518
D. A. Beintema Netherlands 11 625 1.2× 66 0.5× 101 0.9× 57 0.8× 95 1.6× 26 669
D. A. Naylor Canada 10 713 1.3× 113 0.9× 130 1.2× 41 0.6× 88 1.5× 21 752

Countries citing papers authored by J. P. Baluteau

Since Specialization
Citations

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

Fields of papers citing papers by J. P. Baluteau

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by J. P. Baluteau. 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. P. Baluteau. The network helps show where J. P. Baluteau may publish in the future.

Co-authorship network of co-authors of J. P. Baluteau

This figure shows the co-authorship network connecting the top 25 collaborators of J. P. Baluteau. A scholar is included among the top collaborators of J. P. Baluteau 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. P. Baluteau. J. P. Baluteau 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.
Zavagno, A., D. Russeil, F. Motte, et al.. (2010). Star formation triggered by the Galactic H II region RCW 120. Astronomy and Astrophysics. 518. L81–L81. 53 indexed citations
2.
Zavagno, A., D. Russeil, F. Motte, et al.. (2010). Star formation triggered by the Galactic HII region RCW 120: First results from the Herschel Space Observatory. arXiv (Cornell University). 44 indexed citations
3.
Barlow, M. J., B. M. Swinyard, J. R. Goicoechea, et al.. (2006). A far-infrared molecular and atomic line survey of the Orion KL region. UCL Discovery (University College London). 19 indexed citations
4.
Peeters, E., N. L. Martín-Hernández, F. Damour, et al.. (2002). ISO spectroscopy of compact HII regions in the Galaxy. Astronomy and Astrophysics. 381(2). 571–605. 97 indexed citations
5.
Morisset, C., D. Schaerer, N. L. Martín-Hernández, et al.. (2002). A photoionization model of the compact HII region G29.96-0.02. Astronomy and Astrophysics. 386(2). 558–570. 25 indexed citations
6.
Martín-Hernández, N. L., E. Peeters, C. Morisset, et al.. (2002). ISO spectroscopy of compact HII regions in the Galaxy. Astronomy and Astrophysics. 381(2). 606–627. 85 indexed citations
7.
Martín-Hernández, N. L., E. Peeters, C. Morisset, et al.. (2001). ISO spectroscopy of compact HII regions in the Galaxy. II Ionization and elemental abundances. University of Groningen research database (University of Groningen / Centre for Information Technology). 72 indexed citations
8.
Liu, X.-W., M. J. Barlow, M. Cohen, et al.. (2001). ISO LWS observations of planetary nebula fine-structure lines. Monthly Notices of the Royal Astronomical Society. 323(2). 343–361. 76 indexed citations
9.
Roelfsema, P. R., J. P. Baluteau, E. Peeters, et al.. (1999). ISO spectroscopy of dense regions. UCL Discovery (University College London). 427. 631. 1 indexed citations
10.
Barlow, M. J., A. Dalgarno, Jonathan Tennyson, et al.. (1997). An ISO Long Wavelength Spectrometer detection of CH in NGC 7027 and an HeH + upper limit. Monthly Notices of the Royal Astronomical Society. 290(4). L71–L75. 46 indexed citations
11.
Coron, N., Jean‐Pierre Moalic, G. Dambier, & J. P. Baluteau. (1980). Composite vacuum-tight window for simultaneous far-infrared and optical observations. Infrared Physics. 20(1). 53–57. 2 indexed citations
12.
13.
Moorwood, A. F. M., M. Anderegg, J. P. Baluteau, Y. Biraud, & N. Coron. (1978). Infrared line emission from H II regions. II - Airborne observations of the Orion Nebula, W3, and NGC 7538. The Astrophysical Journal. 224. 101–101. 5 indexed citations
14.
Baluteau, J. P., A. Marten, E. Bussoletti, et al.. (1977). High resolution infrared spectra of the earth's atmosphere III—airborne observations in the 100–140 cm−1 range. Infrared Physics. 17(4). 283–291. 7 indexed citations
15.
Baluteau, J. P., M. Anderegg, A. F. M. Moorwood, et al.. (1977). High resolution Michelson interferometer for airborne infrared astronomical observations 1: Concept and performance. Applied Optics. 16(7). 1834–1834. 8 indexed citations
16.
Baluteau, J. P., E. Bussoletti, M. Anderegg, A. F. M. Moorwood, & N. Coron. (1976). Infrared line emission from the Orion Nebula - Detection of forbidden S III /18.71 microns/ and forbidden O III /88.35 microns/. The Astrophysical Journal. 210. L45–L45. 13 indexed citations
17.
Bussoletti, E., N. Epchtein, & J. P. Baluteau. (1974). Calculation of infrared spectra from dust in planetary nebulae.. 34. 141–146.
18.
Bussoletti, E. & J. P. Baluteau. (1974). Determination of H2O/O2 stratospheric mixing ratio from high resolution spectra in the far infrared. Infrared Physics. 14(4). 293–302. 17 indexed citations
19.
Baluteau, J. P., E. Bussoletti, & N. Epchtein. (1973). Evidence of Features in Atmospheric Spectra at around 8 cm−1 of Probable Solar Origin. Nature. 244(5418). 562–563. 7 indexed citations
20.
Baluteau, J. P.. (1971). SOLAR BRIGHTNESS MEASUREMENT BETWEEN 12 AND 24 MICRONS.. 14. 428. 3 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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