Spectroscopic follow-up of a cluster candidate at z=1.45

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 382:3 (2007) 971-984

Authors:

Caroline van Breukelen, Garret Cotter, Steve Rawlings, Tony Readhead, David Bonfield, Lee Clewley, Rob Ivison, Matt Jarvis, Chris Simpson, Mike Watson

Discovery of Twin kHz QPOs in the Peculiar X-Ray Binary Circinus X-1

The Astrophysical Journal American Astronomical Society 653:2 (2006) 1435-1444

Authors:

S Boutloukos, M van der Klis, D Altamirano, M Klein-Wolt, R Wijnands, PG Jonker, RP Fender

Active Galactic Nuclei as scaled-up Galactic black holes

(2006)

Authors:

IM McHardy, E Koerding, C Knigge, P Uttley, RP Fender

Evidence for deceleration in the radio jets of GRS1915+105?

(2006)

Authors:

JCA Miller-Jones, MP Rupen, RP Fender, A Rushton, GG Pooley, RE Spencer

Adapting and expanding the Plateau de Bure interferometer

AIP Conference Proceedings 848 (2006) 857-863

Authors:

A Karastergiou, R Neri

Abstract:

We were recently faced with the following problem: The T-shaped Plateau de Bure Interferometer is expanding its tracks to achieve higher spatial resolution in astronomical images at mm wavelengths. Two more stations for positioning the antennas during observations are being built at the ends of the extended tracks. Which of the given stations should the remaining four antennas occupy to accommodate the new stations? What is the optimal set of antenna configurations, given the new extended one, to achieve necessary coverage of the uv-plane at a variety of spatial resolutions? We present in this paper the solutions to the above questions, resulting from a novel method we have recently developed. The method is based on identifying which placement of elements provides the most appropriate uv-plane sampling. © 2006 American Institute of Physics.