Inverse Compton X-ray halos around high-z radio galaxies: A feedback mechanism powered by far-infrared starbursts or the CMB?
(2012)
Observations of transients and pulsars with LOFAR international stations and the ARTEMIS backend
ArXiv 1210.4318 (2012)
Abstract:
The LOw Frequency ARray - LOFAR - is a new radio interferometer designed with emphasis on flexible digital hardware instead of mechanical solutions. The array elements, so-called stations, are located in the Netherlands and in neighbouring countries. The design of LOFAR allows independent use of its international stations, which, coupled with a dedicated backend, makes them very powerful telescopes in their own right. This backend is called the Advanced Radio Transient Event Monitor and Identification System (ARTEMIS). It is a combined software/hardware solution for both targeted observations and real-time searches for millisecond radio transients which uses Graphical Processing Unit (GPU) technology to remove interstellar dispersion and detect millisecond radio bursts from astronomical sources in real-time.The host galaxy of the super-luminous SN 2010gx and limits on explosive nickel-56 production
(2012)
Interacting Supernovae and Supernova Impostors. SN 2009ip, is this the end?
(2012)