Observations of transients and pulsars with LOFAR international stations and the ARTEMIS backend
Proceedings of the International Astronomical Union Cambridge University Press (CUP): STM Journals - No Cambridge Open 8:S291 (2012) 492-494
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.Cosmological measurements with forthcoming radio continuum surveys
\mnras 424 (2012) 801-819-801-819
Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z \lt 0.5
ArXiv e-prints (2012)
Long timescale radio emission variability and spin-down changes in PSR J0738-4042
Proceedings of the International Astronomical Union Cambridge University Press (CUP) 8:S291 (2012) 161-161
Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
\apj 755 (2012) 146-146