activity
20112023
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 3k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2023★ 5 cited

Shear, writhe and filaments: turbulence in the high latitude molecular cloud MBM 40

Marco Monaci, Loris Magnani, Steven N. Shore +2

Context. It is almost banal to say that the interstellar medium (ISM) is structurally and thermodynamically complex. But the variety of the governing processes, including stellar f…

astro-ph.SR2019★ 20 cited

HD101584: Circumstellar characteristics and evolutionary status

H. Olofsson, T. Khouri, M. Maercker +8

We have performed a study of the characteristics of the circumstellar environment of the binary object HD101584, that provides information on a likely evolutionary scenario. We hav…

astro-ph.SR2018★ 33 cited

Circumstellar environment of the M-type AGB star R Dor. APEX spectral scan at GHz

E. De Beck, H. Olofsson

Our current insights into the circumstellar chemistry of asymptotic giant branch (AGB) stars are largely based on studies of carbon-rich stars and stars with high mass-loss rates.…

astro-ph.SR2017★ 38 cited

Sulphur-bearing molecules in AGB stars I: The occurrence of hydrogen sulfide

T. Danilovich, M. Van de Sande, E. De Beck +4

Through a survey of (sub-)millimetre emission lines of various sulphur-bearing molecules, we aim to determine which molecules are the primary carriers of sulphur in different types…

astro-ph.SR2014★ 30 cited

The wind of W Hya as seen by Herschel. II. The molecular envelope of W Hya

T. Khouri, A. de Koter, L. Decin +18

The evolution of low- and intermediate-mass stars on the asymptotic giant branch (AGB) is mainly controlled by the rate at which these stars lose mass in a stellar wind. Understand…

astro-ph.IM2014★ 9 cited

Future mmVLBI Research with ALMA: A European vision

R. P. J. Tilanus, T. P. Krichbaum, J. A. Zensus +165

Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated…

astro-ph.IM2013★ 2.7k cited

LOFAR: The LOw-Frequency ARray

M. P. van Haarlem, M. W. Wise, A. W. Gunst +197

LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR…

astro-ph.IM2011★ 218 cited

Observing pulsars and fast transients with LOFAR

B. W. Stappers, J. W. T. Hessels, A. Alexov +91

Low frequency radio waves, while challenging to observe, are a rich source of information about pulsars. The LOw Frequency ARray (LOFAR) is a new radio interferometer operating in…