G. W. Wilson

10.5k total citations
71 papers, 944 citations indexed

About

G. W. Wilson is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, G. W. Wilson has authored 71 papers receiving a total of 944 indexed citations (citations by other indexed papers that have themselves been cited), including 60 papers in Astronomy and Astrophysics, 16 papers in Instrumentation and 11 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in G. W. Wilson's work include Galaxies: Formation, Evolution, Phenomena (31 papers), Radio Astronomy Observations and Technology (23 papers) and Superconducting and THz Device Technology (21 papers). G. W. Wilson is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (31 papers), Radio Astronomy Observations and Technology (23 papers) and Superconducting and THz Device Technology (21 papers). G. W. Wilson collaborates with scholars based in United States, Mexico and Japan. G. W. Wilson's co-authors include Min S. Yun, I. Aretxaga, D. H. Hughes, Jason E. Austermann, K. S. Scott, P. Capak, Eva Schinnerer, M. Salvato, Ryohei Kawabe and N. Z. Scoville and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

G. W. Wilson

61 papers receiving 889 citations

Peers

G. W. Wilson

INSTR

NHEP

AMPO

SPECT

Rebecca A. Bernstein United States

M. Sauvage France

V. Casasola Italy

Torsten Böker United States

Nicolas Laporte United Kingdom

C. Kehrig Spain

Kimiaki Kawara Japan

M. Zemcov United States

Olivier Hernandez Canada

D. Alloin France

Rebecca A. Bernstein United States

G. W. Wilson

1.1k ×1.3

395 ×1.1

INSTR

192 ×1.1

NHEP

104 ×2.1

AMPO

23 ×0.6

SPECT

Citations per year, relative to G. W. Wilson G. W. Wilson (= 1×) peers Rebecca A. Bernstein

Countries citing papers authored by G. W. Wilson

Since Specialization

Citations

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

Fields of papers citing papers by G. W. Wilson

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of G. W. Wilson

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Wilson, G. W., Charlene E. Gamaldo, Doris G. Leung, et al.. (2025). Curriculum Innovation: The Osler Apprenticeship in Neurology. PubMed. 4(2). e200218–e200218.

Sayers, Jack, John ZuHone, Urmila Chadayammuri, et al.. (2024). ICM-SHOX. I. Methodology Overview and Discovery of a Gas–Dark Matter Velocity Decoupling in the MACS J0018.5+1626 Merger. The Astrophysical Journal. 968(2). 74–74.

Avila, M. L., H. Jayatissa, D. Santiago-Gonzalez, et al.. (2024). Direct cross-section measurement of the weak r-process Sr88(α,n)Zr91 reaction in ν-driven winds of core-collapse supernovae. Physical review. C. 109(6). 2 indexed citations

Pope, Alexandra, Jed McKinney, Patrick S. Kamieneski, et al.. (2023). ALMA Reveals a Stable Rotating Gas Disk in a Paradoxical Low-mass, Ultradusty Galaxy at z = 4.274. The Astrophysical Journal Letters. 951(2). L46–L46. 14 indexed citations

Wang, Q. Daniel, G. W. Wilson, M. H. Heyer, et al.. (2021). AzTEC survey of the central molecular zone: data reduction, analysis, and preliminary results. Monthly Notices of the Royal Astronomical Society. 505(2). 2392–2411. 8 indexed citations

Wilson, G. W., et al.. (2020). Developing a Large-Scale Cryogenic System for the Simultaneous Operation of Three Detector Focal Planes in TolTEC, A New Multichroic Imaging Polarimeter. Journal of Low Temperature Physics. 199(3-4). 789–797. 1 indexed citations

Sayers, Jack, Alfredo Montaña, Tony Mroczkowski, et al.. (2019). Imaging the Thermal and Kinematic Sunyaev–Zel’dovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities. The Astrophysical Journal. 880(1). 45–45. 27 indexed citations

Montaña, Alfredo, et al.. (2019). TolTEC: unveiling the hidden universe.. Memorie della Societa Astronomica Italiana. 90. 632.

Austermann, Jason E., James A. Beall, Sean Bryan, et al.. (2018). Large format arrays of kinetic inductance detectors for the TolTEC millimeter-wave imaging polarimeter (Conference Presentation). 28–28. 1 indexed citations

10.

Wall, W. F., I. Puerari, R. P. J. Tilanus, et al.. (2016). Continuum observations of M 51 and M 83 at 1.1 mm with AzTEC. Monthly Notices of the Royal Astronomical Society. 459(2). 1440–1467. 9 indexed citations

11.

Navarrete, Felipe, Manuel Aravena, O. Ilbert, et al.. (2012). Quest for COSMOS submillimeter galaxy counterparts using CARMA and VLA: Identifying three high-redshift starburst galaxies. ScholarWorks@UMassAmherst (University of Massachusetts Amherst). 12 indexed citations

12.

Capak, P., Dominik A. Riechers, N. Z. Scoville, et al.. (2011). A massive protocluster of galaxies at a redshift of z ≈ 5.3. Nature. 470(7333). 233–235. 129 indexed citations

13.

Yun, Min S., Daniela Calzetti, M. Dickinson, et al.. (2009). The formation and evolution of the cold gas component and the baryonic mass build-up history in galaxies. 2010. 330.

14.

Chapin, Edward L., Alexandra Pope, D. Scott, et al.. (2009). An AzTEC 1.1 mm survey of the GOODS-N field - II. Multiwavelength identifications and redshift distribution. Monthly Notices of the Royal Astronomical Society. 398(4). 1793–1808. 35 indexed citations

15.

Yun, Min S., I. Aretxaga, M. L. N. Ashby, et al.. (2008). <i>S</i>pitzer IRAC Infrared Colours of Submillimetre-Bright Galaxies. Smith ScholarWorks (Smith College). 22 indexed citations

16.

Kohno, Kotaro, Kazuyuki Muraoka, Bunyo Hatsukade, et al.. (2008). Tracing star formation in galaxies with molecular line and continuum observations. EAS Publications Series. 31. 65–71. 2 indexed citations

17.

Perera, T. A., T. P. Downes, S. S. Meyer, et al.. (2006). Optical performance of frequency-selective bolometers. Applied Optics. 45(29). 7643–7643. 8 indexed citations

18.

Wilson, G. W., E. S. Cheng, D. A. Cottingham, et al.. (2004). Frequency Selective Bolometers - Progress and Projections. Softwaretechnik-Trends. 106. 3 indexed citations

19.

Cottingham, D. A., et al.. (2003). Development of molybdenum–gold proximity bilayers as transition edge sensors for the SPEED camera. Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment. 520(1-3). 446–448. 5 indexed citations

20.

Wilson, G. W.. (1997). A Instrument and Technique for Measuring the Anisotropy in the Cosmic Microwave Background Radiation. PhDT. 1696.

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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