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Marc Verheijen

Researcher at Kapteyn Astronomical Institute

Publications -  209
Citations -  11216

Marc Verheijen is an academic researcher from Kapteyn Astronomical Institute. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 53, co-authored 202 publications receiving 10327 citations. Previous affiliations of Marc Verheijen include University of Wisconsin-Madison & University of Groningen.

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Journal ArticleDOI

The link between light and mass in late-type spiral galaxy disks

TL;DR: In this paper, the correlation between the extrapolated central disk surface brightness (μ) and central surface mass density (Σ) for galaxies in the DiskMass sample was presented.
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Discovery of diffuse emission in the galaxy cluster A1689

TL;DR: In this article, the authors investigated the possible presence of extended diffuse synchrotron radio emission associated with the intracluster medium of the complex galaxy cluster A1689 and reported the detection of an extended, diffuse, low-surface brightness radio emission located in the central region of the galaxy cluster.
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THE DiskMass SURVEY. III. STELLAR KINEMATICS VIA CROSS-CORRELATION

TL;DR: In this paper, a new cross-correlation (CC) approach is proposed to derive stellar kinematics from galaxy-continuum spectroscopy, which is based on the formal error analysis derived by Statler, but properly handles spectral masks.
Proceedings ArticleDOI

Construction progress of WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope

TL;DR: An update on the overall construction progress of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), now that all the major fabrication contracts are in place.
Journal ArticleDOI

Dark and luminous matter in the NGC 3992 group of galaxies - I. The large barred spiral NGC 3992

TL;DR: In this article, a detailed neutral hydrogen observations have been obtained of the large barred spiral galaxy NGC 3992 and its three small companion galaxies, UGC 6923, uGC 6940, and uGC6969, showing some distinct features which can be explained by the non-exponential radial light distribution of NGC3992.