R. J. Laureijs

19.1k total citations
39 papers, 412 citations indexed

About

R. J. Laureijs is a scholar working on Astronomy and Astrophysics, Instrumentation and Atmospheric Science. According to data from OpenAlex, R. J. Laureijs has authored 39 papers receiving a total of 412 indexed citations (citations by other indexed papers that have themselves been cited), including 34 papers in Astronomy and Astrophysics, 6 papers in Instrumentation and 6 papers in Atmospheric Science. Recurrent topics in R. J. Laureijs's work include Stellar, planetary, and galactic studies (26 papers), Astrophysics and Star Formation Studies (25 papers) and Astro and Planetary Science (9 papers). R. J. Laureijs is often cited by papers focused on Stellar, planetary, and galactic studies (26 papers), Astrophysics and Star Formation Studies (25 papers) and Astro and Planetary Science (9 papers). R. J. Laureijs collaborates with scholars based in Netherlands, Germany and United States. R. J. Laureijs's co-authors include F. O. Clark, T. Prusti, K. Leech, R. Siebenmorgen, C. del Burgo, P. Ábrahám, Csaba Kiss, C. Dominik, M. Jourdain de Muizon and Martin Kessler and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

R. J. Laureijs

38 papers receiving 400 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
R. J. Laureijs Netherlands 12 400 62 49 33 21 39 412
P. R. Roelfsema United States 8 310 0.8× 33 0.5× 51 1.0× 31 0.9× 18 0.9× 14 323
D. K. Aitken United Kingdom 9 408 1.0× 23 0.4× 38 0.8× 51 1.5× 19 0.9× 17 422
A. I. Sargent United States 9 354 0.9× 25 0.4× 73 1.5× 44 1.3× 14 0.7× 22 361
O. Miettinen Finland 11 250 0.6× 62 1.0× 90 1.8× 28 0.8× 24 1.1× 24 255
QING-ZENG YAN China 10 249 0.6× 38 0.6× 50 1.0× 28 0.8× 22 1.0× 38 271
K. Torstensson Germany 8 317 0.8× 42 0.7× 95 1.9× 30 0.9× 29 1.4× 13 324
Paul D. Hendry Canada 5 367 0.9× 34 0.5× 53 1.1× 31 0.9× 10 0.5× 6 373
M. W. Castelaz United States 11 306 0.8× 49 0.8× 62 1.3× 28 0.8× 9 0.4× 32 323
Jean‐Pierre Caillault United States 13 374 0.9× 21 0.3× 38 0.8× 38 1.2× 10 0.5× 20 384
Tomomi Shimoikura Japan 12 320 0.8× 72 1.2× 109 2.2× 13 0.4× 31 1.5× 28 329

Countries citing papers authored by R. J. Laureijs

Since Specialization
Citations

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

Fields of papers citing papers by R. J. Laureijs

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of R. J. Laureijs

This figure shows the co-authorship network connecting the top 25 collaborators of R. J. Laureijs. A scholar is included among the top collaborators of R. J. Laureijs 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 R. J. Laureijs. R. J. Laureijs 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.
Tibbs, C. T., F. P. Israel, R. J. Laureijs, et al.. (2018). Planck observations of M33. Monthly Notices of the Royal Astronomical Society. 477(4). 4968–4980. 6 indexed citations
2.
Tibbs, C. T., R. Paladini, Kieran Cleary, et al.. (2015). Using cm observations to constrain the abundance of very small dust grains in Galactic cold cores. Monthly Notices of the Royal Astronomical Society. 456(3). 2290–2300. 10 indexed citations
3.
Laureijs, R. J.. (2007). Polarization Maps at CMB Frequencies from Planck. EAS Publications Series. 23. 247–254. 2 indexed citations
4.
Kiss, Csaba, P. Ábrahám, R. J. Laureijs, A. Moór, & Stephan M. Birkmann. (2006). Constraints on the nature of dust particles by infrared observations. Monthly Notices of the Royal Astronomical Society. 373(3). 1213–1226. 16 indexed citations
5.
Burgo, C. del & R. J. Laureijs. (2005). New insights into the dust properties of the Taurus molecular cloud TMC-2 and its surroundings. Monthly Notices of the Royal Astronomical Society. 360(3). 901–914. 13 indexed citations
6.
Laureijs, R. J., et al.. (2003). The ISO Handbook, Volume IV - PHT - The Imaging Photo-Polarimeter. 11 indexed citations
7.
Dupac, X., C. del Burgo, J.-P. Bernard, et al.. (2003). The complete submillimetre spectrum of NGC 891. Monthly Notices of the Royal Astronomical Society. 344(1). 105–109. 18 indexed citations
8.
Klaas, U., P. Ábrahám, J. A. Acosta‐Pulido, et al.. (2003). ISOPHOT in-flight calibration strategies. Max Planck Institute for Plasma Physics. 481. 19–29. 1 indexed citations
9.
Schulz, B., R. J. Laureijs, J. A. Acosta‐Pulido, et al.. (2002). ISOPHOT – Photometric calibration of point sources. Astronomy and Astrophysics. 381(3). 1110–1130. 20 indexed citations
10.
Laureijs, R. J., M. Jourdain de Muizon, K. Leech, et al.. (2002). A 25 micron search for Vega-like disks around main-sequence stars withISO. Astronomy and Astrophysics. 387(1). 285–293. 43 indexed citations
11.
Siebenmorgen, R., E. Krügel, & R. J. Laureijs. (2001). The infrared continuum radiation of NGC 1808. Astronomy and Astrophysics. 377(3). 735–744. 21 indexed citations
12.
Laureijs, R. J. & R. Siebenmorgen. (1999). Workshop on ISO Polarisation Observations. CERN Document Server (European Organization for Nuclear Research). 435. 1 indexed citations
13.
Habing, H. J., C. Dominik, M. Jourdain de Muizon, et al.. (1999). Disappearance of stellar debris disks around main-sequence stars after 400 million years. Nature. 401(6752). 456–458. 44 indexed citations
14.
Laureijs, R. J., J. A. Acosta‐Pulido, P. Ábrahám, et al.. (1996). Very small grain emission in NGC 7023. 315(2).
15.
Laureijs, R. J., G. Hélou, & F. O. Clark. (1994). The 100 Micron Emission of Clouds. ASPC. 58. 133. 1 indexed citations
16.
Prusti, T., et al.. (1991). A study of the Chamaeleon I dark cloud and T-association - IV. Infrared objects near Cederblad 110. Monthly Notices of the Royal Astronomical Society. 251(2). 303–309. 27 indexed citations
17.
Laureijs, R. J., F. O. Clark, & T. Prusti. (1991). IRAS detection of very cold dust in the LYNDS 134 cloud complex. The Astrophysical Journal. 372. 185–185. 44 indexed citations
18.
Laureijs, R. J., G. Chlewicki, F. O. Clark, & P. R. Wesselius. (1989). DUST EMISSION FROM AN ISOLATED INTERSTELLAR CLOUD. University of Groningen research database (University of Groningen / Centre for Information Technology). 220. 226–234. 1 indexed citations
19.
Chlewicki, G., et al.. (1987). Infrared properties of dust grains derived from IRAS observations. 2466. 113–116. 1 indexed citations
20.
Laureijs, R. J., et al.. (1987). IRAS AND OPTICAL OBSERVATIONS OF THE HIGH-LATITUDE DUST CLOUD LYNDS 1642. Data Archiving and Networked Services (DANS). 184. 269–278. 1 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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