C. Ceccarelli

2.3k total citations
19 papers, 721 citations indexed

About

C. Ceccarelli is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, C. Ceccarelli has authored 19 papers receiving a total of 721 indexed citations (citations by other indexed papers that have themselves been cited), including 18 papers in Astronomy and Astrophysics, 16 papers in Spectroscopy and 13 papers in Atmospheric Science. Recurrent topics in C. Ceccarelli's work include Astrophysics and Star Formation Studies (18 papers), Molecular Spectroscopy and Structure (14 papers) and Atmospheric Ozone and Climate (13 papers). C. Ceccarelli is often cited by papers focused on Astrophysics and Star Formation Studies (18 papers), Molecular Spectroscopy and Structure (14 papers) and Atmospheric Ozone and Climate (13 papers). C. Ceccarelli collaborates with scholars based in France, United States and Netherlands. C. Ceccarelli's co-authors include B. Leflóch, S. Maret, A. G. G. M. Tielens, P. Caselli, F. F. S. van der Tak, E. Caux, A. Bacmann, Jonathan P. Williams, S. Bottinelli and A. Castets 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

C. Ceccarelli

19 papers receiving 706 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
C. Ceccarelli France 14 634 509 295 191 15 19 721
R. Peng United States 14 628 1.0× 372 0.7× 231 0.8× 171 0.9× 30 2.0× 32 714
D. N. Friedel United States 14 479 0.8× 411 0.8× 212 0.7× 198 1.0× 11 0.7× 21 572
Maxime Ruaud France 12 717 1.1× 527 1.0× 372 1.3× 291 1.5× 16 1.1× 23 845
G. Pineau des Forêts France 16 811 1.3× 388 0.8× 275 0.9× 256 1.3× 33 2.2× 20 901
Helen Roberts United States 7 466 0.7× 387 0.8× 197 0.7× 246 1.3× 14 0.9× 8 556
E. Bianchi France 16 614 1.0× 394 0.8× 247 0.8× 140 0.7× 10 0.7× 40 694
F. Helmich Netherlands 9 587 0.9× 418 0.8× 250 0.8× 165 0.9× 9 0.6× 18 634
Y. C. Minh United States 14 462 0.7× 348 0.7× 303 1.0× 266 1.4× 10 0.7× 34 664
Benoît Tabone France 19 1.0k 1.6× 504 1.0× 264 0.9× 142 0.7× 28 1.9× 53 1.1k
Hitomi Mikami Japan 9 423 0.7× 295 0.6× 163 0.6× 134 0.7× 11 0.7× 15 515

Countries citing papers authored by C. Ceccarelli

Since Specialization
Citations

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

Fields of papers citing papers by C. Ceccarelli

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. Ceccarelli

This figure shows the co-authorship network connecting the top 25 collaborators of C. Ceccarelli. A scholar is included among the top collaborators of C. Ceccarelli 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 C. Ceccarelli. C. Ceccarelli is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

19 of 19 papers shown
1.
Quénard, D., C. Vastel, C. Ceccarelli, et al.. (2017). Detection of the HC3NH+ and HCNH+ ions in the L1544 pre-stellar core. Monthly Notices of the Royal Astronomical Society. 470(3). 3194–3205. 34 indexed citations
2.
Quénard, D., V. Taquet, C. Vastel, P. Caselli, & C. Ceccarelli. (2015). Detectability of deuterated water in prestellar cores. Springer Link (Chiba Institute of Technology). 4 indexed citations
3.
Walters, Adam, et al.. (2013). Extension of the millimeter- and submillimeter-wave spectral databases of deuterated methyl cyanides (CH2DCN and CHD2CN). Astronomy and Astrophysics. 553. A84–A84. 15 indexed citations
4.
Emprechtinger, M., D. C. Lis, R. Rolffs, et al.. (2013). THE ABUNDANCE, ORTHO/PARA RATIO, AND DEUTERATION OF WATER IN THE HIGH-MASS STAR-FORMING REGION NGC 6334 I. The Astrophysical Journal. 765(1). 61–61. 22 indexed citations
5.
Schilke, P., A. Schmiedeke, D. C. Lis, et al.. (2012). Molecular line survey of the high-mass star-forming region NGC 6334I withHerschel/HIFI and the Submillimeter Array. Astronomy and Astrophysics. 546. A87–A87. 38 indexed citations
6.
Emprechtinger, M., Raquel Rodriguez Monje, M. H. D. van der Wiel, et al.. (2012). HYDROGEN FLUORIDE IN HIGH-MASS STAR-FORMING REGIONS. The Astrophysical Journal. 756(2). 136–136. 23 indexed citations
7.
Faure, Alexandre, et al.. (2009). Constraining the ortho-to-para ratio of H2 with anomalous H2CO absorption. Astronomy and Astrophysics. 506(3). 1243–1247. 52 indexed citations
8.
Bottinelli, S., C. Ceccarelli, Jonathan P. Williams, & B. Leflóch. (2006). Hot corinos in NGC 1333-IRAS4B and IRAS2A. Astronomy and Astrophysics. 463(2). 601–610. 123 indexed citations
9.
Mamo, Carlo, et al.. (2005). Infortuni e mobilità lavorativa correlata a problemi di salute. Potenzialità e limiti della Rilevazione Trimestrale sulle Forze di Lavoro - Luglio 1999 dell'ISTAT.. ˜La œMedicina del lavoro. 85–92. 10 indexed citations
10.
Maret, S., C. Ceccarelli, A. G. G. M. Tielens, et al.. (2005). CH$_\mathsf{3}$OH abundance in low mass protostars. Astronomy and Astrophysics. 442(2). 527–538. 92 indexed citations
11.
Parise, B., C. Ceccarelli, & S. Maret. (2005). Theoretical HDO emission from low-mass protostellar envelopes. Astronomy and Astrophysics. 441(1). 171–179. 14 indexed citations
12.
Chiavassa, A., C. Ceccarelli, A. G. G. M. Tielens, E. Caux, & S. Maret. (2005). The 90–110μm dust feature in low to intermediate mass protostars: Calcite?. Astronomy and Astrophysics. 432(2). 547–557. 26 indexed citations
13.
Ceccarelli, C., S. Maret, A. G. G. M. Tielens, A. Castets, & E. Caux. (2003). Theoretical H$_\mathsf{2}$CO emission from protostellar envelopes. Astronomy and Astrophysics. 410(2). 587–595. 54 indexed citations
14.
Caselli, P., F. F. S. van der Tak, C. Ceccarelli, & A. Bacmann. (2003). Abundant H$\mathsf{_{2}}$D$\mathsf{^{+}}$ in the pre–stellar core L1544. Astronomy and Astrophysics. 403(3). L37–L41. 132 indexed citations
15.
Ceccarelli, C., A. C. A. Boogert, A. G. G. M. Tielens, et al.. (2002). Submm/FIR CO line emission from the disk of the Class I protostar EL 29. Astronomy and Astrophysics. 395(3). 863–871. 17 indexed citations
16.
Caux, E., C. Ceccarelli, L. Pagani, et al.. (2002). HD 112 $\mathsf{\mu}$m in absorption and extreme CO depletion in a cold molecular cloud. Astronomy and Astrophysics. 383(1). L9–L13. 10 indexed citations
17.
Boogert, A. C. A., M. R. Hogerheijde, C. Ceccarelli, et al.. (2002). The Environment and Nature of the Class I Protostar Elias 29: Molecular Gas Observations and the Location of Ices. The Astrophysical Journal. 570(2). 708–723. 48 indexed citations
18.
Ceccarelli, C., E. Caux, G. J. White, et al.. (1998). THE FAR INFRARED LINE SPECTRUM OF THE PROTOSTAR IRAS 16293-2422. Open Research Online (The Open University). 331(1). 372–382. 4 indexed citations
19.
Rudolph, Alexander, C. Ceccarelli, E. Caux, et al.. (1997). ISO Detection of CO(+) toward the Protostar IRAS 16293-2422. American Astronomical Society Meeting Abstracts. 191. 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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