D. Paradis

4.6k total citations
26 papers, 702 citations indexed

About

D. Paradis is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, D. Paradis has authored 26 papers receiving a total of 702 indexed citations (citations by other indexed papers that have themselves been cited), including 25 papers in Astronomy and Astrophysics, 4 papers in Spectroscopy and 3 papers in Atmospheric Science. Recurrent topics in D. Paradis's work include Astrophysics and Star Formation Studies (25 papers), Stellar, planetary, and galactic studies (23 papers) and Galaxies: Formation, Evolution, Phenomena (15 papers). D. Paradis is often cited by papers focused on Astrophysics and Star Formation Studies (25 papers), Stellar, planetary, and galactic studies (23 papers) and Galaxies: Formation, Evolution, Phenomena (15 papers). D. Paradis collaborates with scholars based in France, United States and Finland. D. Paradis's co-authors include C. Mény, J.-P. Bernard, V. D. Gromov, J.-P. Bernard, N. Boudet, Akiko Kawamura, Kazuhito Dobashi, Y. Fukui, Toshikazu Onishi and W. T. Reach 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

D. Paradis

24 papers receiving 685 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. Paradis France 17 693 122 76 56 34 26 702
J. R. Dawson Australia 13 499 0.7× 64 0.5× 103 1.4× 75 1.3× 27 0.8× 45 525
J. C. Mottram United Kingdom 10 523 0.8× 74 0.6× 165 2.2× 36 0.6× 26 0.8× 12 529
F. Boulanger France 13 613 0.9× 106 0.9× 110 1.4× 37 0.7× 28 0.8× 33 636
G. A. P. Franco Brazil 15 598 0.9× 72 0.6× 115 1.5× 41 0.7× 32 0.9× 40 615
A. Traficante Italy 18 637 0.9× 101 0.8× 132 1.7× 19 0.3× 34 1.0× 46 675
Anna L. Rosen United States 14 605 0.9× 55 0.5× 47 0.6× 34 0.6× 81 2.4× 28 643
Yoshito Shimajiri Japan 17 655 0.9× 159 1.3× 227 3.0× 28 0.5× 30 0.9× 41 683
G. Garay Chile 15 652 0.9× 84 0.7× 154 2.0× 40 0.7× 18 0.5× 31 662
David Eden United Kingdom 13 762 1.1× 128 1.0× 222 2.9× 47 0.8× 47 1.4× 40 815
Xing Lu United States 17 633 0.9× 130 1.1× 162 2.1× 29 0.5× 38 1.1× 46 658

Countries citing papers authored by D. Paradis

Since Specialization
Citations

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

Fields of papers citing papers by D. Paradis

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Paradis

This figure shows the co-authorship network connecting the top 25 collaborators of D. Paradis. A scholar is included among the top collaborators of D. Paradis 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 D. Paradis. D. Paradis 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.
Paradis, D., et al.. (2024). Inferring the dust emission at submillimeter and millimeter wavelengths using neural networks. Astronomy and Astrophysics. 691. A241–A241.
2.
Paradis, D., et al.. (2023). Toward a better understanding of the mid-infrared emission in the Large Magellanic Cloud. Astronomy and Astrophysics. 674. A141–A141. 5 indexed citations
3.
Demyk, Karine, V. D. Gromov, C. Mény, et al.. (2022). Low-temperature optical constants of amorphous silicate dust analogues. Astronomy and Astrophysics. 666. A192–A192. 9 indexed citations
4.
Paradis, D., C. Mény, M. Juvela, A. Noriega‐Crespo, & I. Ristorcelli. (2019). Revisiting the dust properties in the molecular clouds of the Large Magellanic Cloud. Springer Link (Chiba Institute of Technology). 2 indexed citations
5.
Rivera-Ingraham, A., I. Ristorcelli, M. Juvela, et al.. (2017). Galactic Cold Cores. VIII. Filament formation and evolution: Filament properties in context with evolutionary models. CLOK (University of Central Lancashire). 5 indexed citations
6.
Figueira, M., A. Zavagno, L. Deharveng, et al.. (2017). Star formation towards the Galactic H II region RCW 120 Herschel observations of compact sources. Kölner Universitäts PublikationsServer (Universität zu Köln). 19 indexed citations
7.
Mény, C., George Papatheodorou, M. J. Toplis, et al.. (2017). Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues. Astronomy and Astrophysics. 600. A123–A123. 38 indexed citations
8.
Rivera-Ingraham, A., I. Ristorcelli, M. Juvela, et al.. (2017). Galactic cold cores. Astronomy and Astrophysics. 601. A94–A94. 10 indexed citations
9.
Rivera-Ingraham, A., I. Ristorcelli, M. Juvela, et al.. (2016). Galactic cold cores. Astronomy and Astrophysics. 591. A90–A90. 18 indexed citations
10.
Juvela, M., Yasuo Doi, D. J. Marshall, et al.. (2015). Galactic cold cores. Astronomy and Astrophysics. 584. A94–A94. 38 indexed citations
11.
Paradis, D., C. Mény, A. Noriega‐Crespo, et al.. (2014). Modeling and predicting the shape of the far-infrared to submillimeter emission in ultra-compact HII regions and cold clumps. Springer Link (Chiba Institute of Technology). 4 indexed citations
12.
Compiègne, M., L. Verstraete, A. P. Jones, et al.. (2013). DustEM: Dust extinction and emission modelling. ascl.
13.
Ysard, N., M. Juvela, Karine Demyk, et al.. (2012). Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties. Springer Link (Chiba Institute of Technology). 24 indexed citations
14.
Paradis, D., Kazuhito Dobashi, Tomomi Shimoikura, et al.. (2012). Dark gas in the solar neighborhood from extinction data. Astronomy and Astrophysics. 543. A103–A103. 58 indexed citations
15.
Paradis, D., J.-P. Bernard, C. Mény, & V. D. Gromov. (2011). Far-infrared to millimeter astrophysical dust emission. Astronomy and Astrophysics. 534. A118–A118. 27 indexed citations
16.
Paradis, D., M. Veneziani, A. Noriega‐Crespo, et al.. (2010). Variations of the spectral index of dust emissivity from Hi-GALobservations of the Galactic plane. Springer Link (Chiba Institute of Technology). 36 indexed citations
17.
Bot, Caroline, N. Ysard, D. Paradis, et al.. (2010). Submillimeter to centimeter excess emission from the Magellanic Clouds. Astronomy and Astrophysics. 523. A20–A20. 48 indexed citations
18.
Paradis, D., J.-P. Bernard, & C. Mény. (2009). Dust emissivity variations in the Milky Way. Springer Link (Chiba Institute of Technology). 32 indexed citations
19.
Dobashi, Kazuhito, J.-P. Bernard, Annie Hughes, et al.. (2008). Extinction and dust/gas ratio in LMC molecular clouds. Astronomy and Astrophysics. 484(1). 205–223. 45 indexed citations
20.
Mény, C., et al.. (2007). Far-infrared to millimeter astrophysical dust emission. Astronomy and Astrophysics. 468(1). 171–188. 68 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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