The Square Kilometre Array (SKA)

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A parsec scale X-ray extended structure from the X-ray binary Circinus X-1

(2008)

Authors:

P Soleri, S Heinz, R Fender, R Wijnands, V Tudose, D Altamirano, PG Jonker, M van der Klis, L Kuiper, C Kaiser, P Casella
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High energy astrophysics with the next generation of radio astronomy facilities

(2008)
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MAXI, LOFAR and Microquasars - All-sky monitoring of X-ray binaries in X-rays and radio

(2008)
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Spectral evidence for jets from Accreting Millisecond X-ray Pulsars

(2008)

Authors:

David M Russell, Rob P Fender, Peter Jonker, Dipankar Maitra
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The Cℓover experiment

Proceedings of SPIE - The International Society for Optical Engineering 7020 (2008)

Authors:

L Piccirillo, P Ade, MD Audley, C Baines, R Battye, M Brown, P Calisse, A Challinor, WD Duncan, P Ferreira, W Gear, DM Glowacka, D Goldie, PK Grimes, M Halpern, V Haynes, GC Hilton, KD Irwin, B Johnson, M Jones, A Lasenby, P Leahy, J Leech, S Lewis, B Maffei, L Martinis, PD Mauskopf, SJ Melhuish, CE North, D O'Dea, S Parsley, G Pisano, CD Reintsema, G Savini, RV Sudiwala, D Sutton, A Taylor, G Teleberg, D Titterington, VN Tsaneva, C Tucker, R Watson, S Withington, G Yassin, J Zhang

Abstract:

CℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. CℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of CℓOVER is to be sensitive to gravitational waves down to r ∼ 0.03 (at 3σ) in two years of operations.
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