Radio interferometry and its application to arrays of element antennas enable sensitive
studies of celestial objects with angular resolutions comparable with, or surpassing, optical …

We describe the processing of the PHANGS–ALMA survey and present the PHANGS–ALMA
pipeline, a public software package that processes calibrated interferometric and total power …

An image from the Karl G. Jansky Very Large Array of the Galaxy Hercules A (also known as
3C348) showing powerful synchrotron jets emerging from its core, the site of a supermassive …

We combine new Parkes telescope observations of neutral hydrogen (Hi) in the Small
Magellanic Cloud (SMC) with an Australia Telescope Compact Array (ATCA) aperture …

Recent HI surveys of the Large Magellanic Cloud (LMC) with the Australia Telescope
Compact Array and the Parkes multibeam receiver have focused, respectively, on the small …

Page 1 Radio telescopes Second edition WN CHRISTIANSEN & JA HOGBOM Page 2 Page 3
Radiotelescopes Page 4 Page 5 Radiotelescopes SECOND EDITION WN CHRISTIANSEN …

New observations of CO (J= 1→ 0) line emission from M33, using the 25 element BEARS
focal plane array at the Nobeyama Radio Observatory 45 m telescope, in conjunction with …

L1498 is a classic example of a dense cold pre-protostellar core. To study the evolutionary
status, the structure, dynamics, and chemical properties of this core we have obtained high …

Context. High angular resolution (sub) millimetre observations of asymptotic giant branch
(AGB) stars, now possible with the Atacama Large Millimeter/submillimeter Array (ALMA) …

We report the results of high-resolution HI 21 cm line observations of the shocked interstellar
gas in the W51 complex. The shocked HI gas has been detected between v LSR ≃+ 85 …