'Lofar' diaporamas de présentation

Skyalert: Rapid Transients for you and your Robot

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LOFAR Cosmic Ray KSP

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Choose your own adventure! fast radio bursts

Choose your own adventure! fast radio bursts . Vikram Ravi University of Melbourne and CASS With Ryan Shannon and Paul Lasky. And with particular thanks to the Swinburne CAS staff and students.

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Galactic Magnetic Field Research with LOFAR

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Olaf Scholten KVI, Groningen For the NuMoon collaboration

Radio detection of UHE Neutrinos off the Moon. Olaf Scholten KVI, Groningen For the NuMoon collaboration. Principle of the measurement. Cosmic ray. Detection: Westerbork antennas. 10 7 km 2. 100MHz Radio waves. Radio emission Mechanisms. In air: Geo-synchotron radiation

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Large-scale Data Processing Challenges

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SKA/LOFAR Ray Norris ATNF Outreach workshop 2 Dec 2003

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Calibration with StEFCal : progress, advances and successes

Calibration with StEFCal : progress, advances and successes. Stef Salvini , Stefan Wijnholds. The Problem. Given D the observed visibility matrix , M the model sky visibility matrix, n the number of antennas Minimise where the Frobenius norm is

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Radio source surveys and populations

Radio source surveys and populations. Ken Kellermann. National Radio Astronomy Observatory. R adio S urvey Discoveries. R adio galaxies (1949) Cosmic evolution (1955 ) Quasars (1963) IPS (1964 ) Pulsars (1967) Gravitational lenses (1979). Radio source surveys and populations.

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4th Solar KSP Meeting Potsdam 2010 November 08

4th Solar KSP Meeting Potsdam 2010 November 08. Solar Imaging with the Standard Imaging Pipeling Frank Breitling Astrophysikalisches Institut Potsdam. Overview. Introduction to the pipeline Status of solar imaging New results Conclusions. The LOFAR Standard Imaging Pipeline.

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The EISCAT_3D Science Case: Current Status

The EISCAT_3D Science Case: Current Status. Ian McCrea STFC RAL. Preparatory Phase WP3: Science Case Work Package. Engaging with potential new users Holding targeted workshops Gathering requirements for new science Revising/developing the science case

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LOFAR project

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LOFAR Status

LOFAR Status. Internal review of the project (April-July 2007): Main conclusions: R&D developments in good shape (CS1 results) Development costs in line with original estimates Original 77-station LOFAR relied on significant matching from original international partners (e.g. ATNF, MIT, NRL)

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Pulsar Wind Nebulae with LOFAR

Pulsar Wind Nebulae with LOFAR. Jason Hessels (ASTRON/UvA). Astrophysics with E-LOFAR - Hamburg - Sept. 16 th -19 th , 2008. Outline Observing Pulsar Wind Nebulae (PWNe) with LOFAR. General theoretical model of PWNe Observational properties of PWNe Observing PWNe with LOFAR.

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Searching for Transients with LOFAR/CS1

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The Grid Beyond Physics

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Science with the SKA in East Asia

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LOFAR UK

LOFAR UK. Rob Fender. LOFAR-UK [est. 2004] www.lofar-uk.org Management committee formed based on internal MoU P.I. Fender (Southampton) Co-P.I. Rawlings (Oxford) Current membership (22 institutions):

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PELICAN Imaging Framework

Design of a 96 Element FX Correlator for the LOFAR-UK Station. ring. AP0. serdes. Inter board interface (IBI). AP1. BP. LCU. CEP. AP2. Inter board interface (IBI). serdes. AP3. ring. G. Foster 1,2 and K. Zarb Adami 1. 1 University of Oxford 2 griffin.foster@astro.ox.ac.uk.

166 views • 1 slides