Mark G. Rawlings

19.6k total citations
18 papers, 251 citations indexed

About

Mark G. Rawlings is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Instrumentation. According to data from OpenAlex, Mark G. Rawlings has authored 18 papers receiving a total of 251 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 5 papers in Atmospheric Science and 3 papers in Instrumentation. Recurrent topics in Mark G. Rawlings's work include Astrophysics and Star Formation Studies (15 papers), Stellar, planetary, and galactic studies (13 papers) and Atmospheric Ozone and Climate (5 papers). Mark G. Rawlings is often cited by papers focused on Astrophysics and Star Formation Studies (15 papers), Stellar, planetary, and galactic studies (13 papers) and Atmospheric Ozone and Climate (5 papers). Mark G. Rawlings collaborates with scholars based in United States, Chile and Finland. Mark G. Rawlings's co-authors include A. J. Adamson, M. Juvela, D. C. B. Whittet, J. Malinen, Ph. André, D. Ward–Thompson, P. Palmeirim, E. Chapillon, Á. Juhász and I. de Gregorio‐Monsalvo and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

Mark G. Rawlings

16 papers receiving 245 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Mark G. Rawlings United States 9 239 85 52 29 12 18 251
M. Veneziani United States 9 289 1.2× 71 0.8× 35 0.7× 31 1.1× 13 1.1× 13 328
C. M. Wright Australia 9 331 1.4× 111 1.3× 60 1.2× 44 1.5× 16 1.3× 13 350
H. Arab France 6 175 0.7× 49 0.6× 42 0.8× 17 0.6× 16 1.3× 8 178
A. Cridland Netherlands 11 474 2.0× 117 1.4× 62 1.2× 16 0.6× 23 1.9× 20 484
A. Punanova Germany 9 189 0.8× 119 1.4× 88 1.7× 29 1.0× 11 0.9× 18 204
Arturo I. Gómez-Ruiz Mexico 11 256 1.1× 116 1.4× 77 1.5× 21 0.7× 5 0.4× 27 264
Norio Ikeda Japan 10 288 1.2× 95 1.1× 49 0.9× 11 0.4× 13 1.1× 20 292
A. Chacón-Tanarro Germany 8 149 0.6× 97 1.1× 67 1.3× 29 1.0× 6 0.5× 8 161
L. A. Montier France 8 293 1.2× 43 0.5× 51 1.0× 10 0.3× 21 1.8× 9 294
Charlène Lefèvre France 8 322 1.3× 144 1.7× 82 1.6× 37 1.3× 11 0.9× 15 330

Countries citing papers authored by Mark G. Rawlings

Since Specialization
Citations

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

Fields of papers citing papers by Mark G. Rawlings

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Mark G. Rawlings. 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 Mark G. Rawlings. The network helps show where Mark G. Rawlings may publish in the future.

Co-authorship network of co-authors of Mark G. Rawlings

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

All Works

18 of 18 papers shown
1.
Unnikrishnan, R., E. De Beck, L.-Å. Nyman, et al.. (2024). Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. Astronomy and Astrophysics. 684. A4–A4. 1 indexed citations
2.
Suh, Hyewon, J. Scharwächter, Emanuele Paolo Farina, et al.. (2024). A super-Eddington-accreting black hole ~1.5 Gyr after the Big Bang observed with JWST. Nature Astronomy. 9(2). 271–279. 5 indexed citations
3.
Rawlings, Mark G., et al.. (2019). Near-infrared diffuse interstellar bands towards Her 36. Monthly Notices of the Royal Astronomical Society. 485(3). 3398–3401. 6 indexed citations
4.
Parsons, Harriet, J. T. Dempsey, H. Thomas, et al.. (2018). The Dusty Galactic Center as Seen by SCUBA-2. The Astrophysical Journal Supplement Series. 234(2). 22–22. 19 indexed citations
5.
Rawlings, Mark G., A. J. Adamson, & T. H. Kerr. (2014). A HIGH-RESOLUTION STUDY OF NEAR-INFRARED DIFFUSE INTERSTELLAR BANDS. The Astrophysical Journal. 796(1). 58–58. 10 indexed citations
6.
Rawlings, Mark G., A. J. Adamson, & T. H. Kerr. (2014). A High-Resolution Study of Near-Infrared Diffuse Interstellar Bands. arXiv (Cornell University). 2011. 311.
7.
Klaassen, Pamela, Á. Juhász, G. S. Mathews, et al.. (2013). ALMA detection of the rotating molecular disk wind from the young star HD 163296. Springer Link (Chiba Institute of Technology). 25 indexed citations
8.
Malinen, J., M. Juvela, V.-M. Pelkonen, & Mark G. Rawlings. (2013). Mapping of interstellar clouds with infrared light scattered\n from dust: TMC-1N. Springer Link (Chiba Institute of Technology). 8 indexed citations
9.
Peng, T.-C., E. M. L. Humphreys, L. Testi, et al.. (2013). Silicon isotopic abundance toward evolved stars and its application for presolar grains. Springer Link (Chiba Institute of Technology). 2 indexed citations
10.
Mathews, G. S., Pamela Klaassen, Á. Juhász, et al.. (2013). ALMA imaging of the CO snowline of the HD 163296 disk with DCO+. Astronomy and Astrophysics. 557. A132–A132. 58 indexed citations
11.
Rawlings, Mark G., M. Juvela, K. Lehtinen, K. Mattila, & D. Lemke. (2012). Observations of 6–200 μm emission of the Ophiuchus cloud LDN 1688★. Monthly Notices of the Royal Astronomical Society. 428(3). 2617–2627. 8 indexed citations
12.
Malinen, J., M. Juvela, Mark G. Rawlings, et al.. (2012). Profiling filaments: comparing near-infrared extinction and submillimetre data in TMC-1. Astronomy and Astrophysics. 544. A50–A50. 43 indexed citations
13.
Lundgren, A., Lars-Åke Nyman, G. Mathys, et al.. (2012). ALMA: the first year of observations. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 8448. 844802–844802. 2 indexed citations
14.
Rawlings, Mark G., et al.. (2010). ALMA science operations and user support: software. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 7737. 77371A–77371A. 3 indexed citations
15.
Rawlings, Mark G., M. Juvela, K. Mattila, K. Lehtinen, & D. Lemke. (2005). ISOobservations of 3-200 μm emission by three dust populations in an isolated local translucent cloud. Monthly Notices of the Royal Astronomical Society. 356(3). 810–828. 14 indexed citations
16.
Bowey, J. E., Mark G. Rawlings, & A. J. Adamson. (2004). 10-μm absorption spectra of silicates for two new diffuse interstellar medium sightlines. Monthly Notices of the Royal Astronomical Society. 348(2). L13–L17. 10 indexed citations
17.
Rawlings, Mark G., A. J. Adamson, & D. C. B. Whittet. (2003). Infrared and visual interstellar absorption features towards heavily reddened field stars. Monthly Notices of the Royal Astronomical Society. 341(4). 1121–1140. 24 indexed citations
18.
Rawlings, Mark G., A. J. Adamson, & D. C. B. Whittet. (2000). A Search for Highly Reddened Early‐Type Stars: Optical Photometry and Spectroscopy of Stars in the Stephenson Objective Prism Survey. The Astrophysical Journal Supplement Series. 131(2). 531–559. 13 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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