M
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.
Papers
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Proceedings ArticleDOI
HI Surveys with APERTIF
TL;DR: Apertif, the innovative new Focal Plane Array for the Westerbork Synthesis Radio Telescope (WSRT), will significantly increase the instantaneous field-of-view and bandwidth of the WSRT between 1.0 and 1.75 GHz, enabling efficient northern-sky HI surveys as well as searches for pulsars and transients.
Journal Article
Detection of a bright burst from FRB 121102 with Apertif at the Westerbork Synthesis Radio Telescope
L. C. Oostrum,J. van Leeuwen,Jisk Attema,W. A. van Cappellen,Liam Connor,B. Hut,Yogesh Maan,Tom Oosterloo,Emily Petroff,D. van der Schuur,Alessio Sclocco,Marc Verheijen +11 more
TL;DR: The authors observed the repeating FRB 121102 (Spitler et al. 2016) while commissioning the Apertif Radio Transient System (ARTS; van Leeuwen 2014) on the Westerbork Synthesis Radio Telescope.
Proceedings ArticleDOI
LADUMA: looking at the distant universe with the MeerKAT array
Sarah Blyth,Andrew J. Baker,Benne W. Holwerda,Benne W. Holwerda,Bruce A. Bassett,Bruce A. Bassett,Matthew A. Bershady,A. Bouchard,Frank H. Briggs,Barbara Catinella,Laurent Chemin,Steven M. Crawford,C. M. Cress,Daniel Cunnama,Jeremy Darling,Romeel Davé,Romeel Davé,Roger Deane,W. J. G. de Blok,W. J. G. de Blok,W. J. G. de Blok,Ed Elson,Andreas Faltenbacher,Sean February,Ximena Fernández,B. S. Frank,Eric Gawiser,Patricia A. Henning,Kelley M. Hess,Kelley M. Hess,I. Heywood,John P. Hughes,Matt J. Jarvis,Matt J. Jarvis,Sheila Kannappan,Neal S. Katz,Dušan Kereš,Hans Rainer Klöckner,Renee C. Kraan-Korteweg,Philip Lah,Matthew D. Lehnert,Adam K. Leroy,Michelle Lochner,Natasha Maddox,S. Makhathini,Gerhardt R. Meurer,Martin Meyer,Kavilan Moodley,Raffaella Morganti,Raffaella Morganti,Danail Obreschkow,Se Heon Oh,Tom Oosterloo,Tom Oosterloo,Daniel J. Pisano,Attila Popping,Gergö Popping,Swara Ravindranath,Eva Schinnerer,Anja C. Schröder,Kartik Sheth,Rosalind E. Skelton,Oleg Smirnov,Mathew Smith,Rachel S. Somerville,Raghunathan Srianand,Lister Staveley-Smith,Ian M. Stewart,Mattia Vaccari,Petri Väisänen,Kurt van der Heyden,Wim van Driel,Marc Verheijen,Fabian Walter,Eric M. Wilcots,Theodore B. Williams,Patrick Woudt,John F. Wu,Martin Zwaan,Jonathan T. L. Zwart,Jonathan T. L. Zwart,Steve Rawlings +81 more
TL;DR: The LADUMA project as mentioned in this paper is a large-scale L-band+UHF-band Looking At the Distant Universe with the MeerKAT Array (LADUma) survey, which will probe HI in emission within a single vuvuzela that extends to z = 1.4, when the universe was only a third of its present age.
Journal ArticleDOI
Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z=0.376
Ximena Fernández,Ximena Fernández,Hansung B. Gim,J. H. van Gorkom,Min S. Yun,Emmanuel Momjian,Attila Popping,Attila Popping,Laura Chomiuk,Kelley M. Hess,Lucas Hunt,Kathryn Kreckel,D. M. Lucero,Natasha Maddox,Tom Oosterloo,Daniel J. Pisano,Marc Verheijen,Christopher A. Hales,Aeree Chung,Richard Dodson,K. Golap,Julia Gross,Patricia A. Henning,John E. Hibbard,Yara L. Jaffé,Jennifer Donovan Meyer,Martin Meyer,Monica Sanchez-Barrantes,David Schiminovich,Andreas Wicenec,Eric M. Wilcots,Matthew A. Bershady,Nick Scoville,Jay Strader,Evangelia Tremou,R. Salinas,R. Chávez +36 more
TL;DR: In this article, the COSMOS HI Large Extragalactic Survey (CHILES) was conducted with the Karl G. Jansky Very Large Array, which is the first survey to simultaneously observe the neutral hydrogen (HI) in galaxies over large volumes at high redshifts.
Journal ArticleDOI
Galaxy evolution in dense environments: a concise HI perspective
TL;DR: In this article, the morphological and kinematic characteristics of the cold gas provided a sensitive tool to determine which mechanisms dominate in which environments, and the morphologies, star formation rates, and gas content may depend strongly on environment.