activity
19982026
most citedSquelched Galaxies and Dark Halos

159 citations · 449 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026★ 1 cited

The supersonic nature of jellyfish galaxies

Alessandro Ignesti, Francesca Loi, Antonino Marasco +20

All gas-rich galaxies in cluster environments are expected to experience ram-pressure stripping from the intra-cluster medium. However, only a fraction of these develop ongoing sta…

astro-ph.GA2026★ 1 cited

Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)

Benedetta Vulcani, Gabriella De Lucia, Daria Zakharova +28

[ABRIDGED] Galaxy evolution is shaped by internal and external mechanisms that regulate the baryon cycle and star formation activity. We present a theoretical framework based on th…

astro-ph.IM2025

Why the Northern Hemisphere Needs a 30-40m Telescope and the Science at Stake: Ultra-Low-Mass Dwarf Galaxies Across the Boreal Cosmic Web

J. Alfonso L. Aguerri, Jesús Falcón-Barroso, María Argudo-Fernández +22

Dwarf galaxies dominate the galaxy population in the nearby Universe and occupy the regime where feedback, reionization, and environment exert their strongest influence on galaxy f…

astro-ph.GA2023★ 11 cited

BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections

A. R. Gogate, M. A. W. Verheijen, J. M. van der Hulst +1

We present HI-based B- and R-band Tully-Fisher relations (TFRs) and the Baryonic TFR (BTFR) at z=0.2 using direct HI detections from the Blind Ultra-Deep HI Environmental Survey (B…

astro-ph.IM2022★ 4 cited

A comparative study of source-finding techniques in HI emission line cubes using SoFiA, MTObjects, and supervised deep learning

J. A. Barkai, M. A. W. Verheijen, E. T. Martínez +1

The 21 cm spectral line emission of atomic neutral hydrogen (HI) is one of the primary wavelengths observed in radio astronomy. However, the signal is intrinsically faint and the H…

astro-ph.GA2020★ 4 cited

A near-infrared study of the obscured 3C129 galaxy cluster

M. Ramatsoku, M. A. W Verheijen, R. C. Kraan-Korteweg +3

We present a catalogue of 261 new infrared selected members of the 3C129 galaxy cluster. The cluster, located at 0.02, forms part of the Perseus-Pisces filament and is…

astro-ph2005★ 1 cited

Local Galaxies as Damped Ly-Alpha Analogs

M. A. Zwaan, J. M. van der Hulst, F. H. Briggs +2

We calculate in detail the expected properties of low redshift DLA systems under the assumption that they arise in the gaseous disks of galaxies like those in the z=0 population. A…

astro-ph2003★ 51 cited

The Kinematics in the Core of the Low Surface Brightness Galaxy DDO 39

R. A. Swaters, M. A. W. Verheijen, M. A. Bershady +1

We present a high resolution, SparsePak two-dimensional velocity field for the center of the low surface brightness (LSB) galaxy DDO 39. These data are a significant improvement on…

astro-ph2001★ 59 cited

Hydrogen 21-Centimeter Emission from a Galaxy at Cosmological Distance

Martin Zwaan, Pieter van Dokkum, Marc Verheijen

We have detected the neutral atomic hydrogen (HI) emission line at a cosmologically significant distance (z=0.18) in the rich galaxy cluster Abell 2218 with the Westerbork Synthesi…

astro-ph2001★ 159 cited

Squelched Galaxies and Dark Halos

R. Brent Tully, Rachel S. Somerville, Neil Trentham +1

There is accumulating evidence that the faint end of the galaxy luminosity function might be very different in different locations. The luminosity function might be rising in rich…

astro-ph2000★ 12 cited

Star Formation and Tidal Encounters with the Low Surface Brightness Galaxy UGC 12695 and Companions

K. O'Neil, M. A. W. Verheijen, S. S. McGaugh

We present VLA H I observations of the low surface brightness galaxy UGC 12695 and its two companions, UGC 12687 and a newly discovered dwarf galaxy 2333+1234. UGC 12695 shows soli…

astro-ph1998★ 146 cited

Rotation curves of UMa galaxies in the context of modified Newtonian dynamics

R. H. Sanders, M. A. W. Verheijen

This is the third in a series of papers in which spiral galaxy rotation curves are considered in the context of Milgrom's modified dynamics (MOND). The present sample of 30 objects…