MAXI, LOFAR and Microquasars - All-sky monitoring of X-ray binaries in X-rays and radio
(2008)
Spectral evidence for jets from Accreting Millisecond X-ray Pulsars
(2008)
The Cℓ over experiment
Proceedings of SPIE - The International Society for Optical Engineering 7020 (2008)
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.The CℓOVER experiment
Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 7020 (2008) 70201e-70201e-10
Blazing trails: Microquasars as head-tail sources and the seeding of magnetized plasma into the ISM
(2008)