PDF-What is ASKAP?

Author : conchita-marotz | Published Date : 2015-08-21

ASKAP is a nextgeneration radio telescope incorporating novel receiver technologies and leadingedge ICT systems It will be made up of antennas each metres in diameter

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What is ASKAP?: Transcript

ASKAP is a nextgeneration radio telescope incorporating novel receiver technologies and leadingedge ICT systems It will be made up of antennas each metres in diameter working together a. Lisa Harvey-. Smith & Aidan . Hotan. . | ASKAP Project . Scientists. August 5. th. 2013. ASTRONONY & SPACE SCIENCE. ASKAP funding, fabrication, integration, commissioning is phased.. Science can also be phased.. CSIRO Astronomy and Space Science. David Brodrick. EPICS [Spring] Collaboration Meeting. 22nd October 2014. Australia Telescope Compact Array (Narrabri, NSW). We measure the spatial coherence function. DIFX . Users and Developers Meeting. CSIRO Astronomy and Space Science. Dr. Grant Hampson . | . ADE Team Leader. 4 September . 2012. ASKAP Overview. 36x12-metre antennas. 630 baselines. 188-port PAF receiver. S. urveys . of . Local Galaxies. Michael . Brown. ARC Future Fellow. Monash. University. Where are we now?. NVSS / FIRST / SUMMS. 0.5 . mJy. RMS per beam. 15”-1’ beam. ~30 . uJy. RMS per beam in 12 hours . Lawrence Rudnick, University of Minnesota. Deep+wideband+polarization. ~30. m. Jy,800sq . deg. 700-1800. More science using subsamples. This is single project from large survey. Feasible with JVLA only: NVSS level investment. Bryan Gaensler. , Tom Landecker, Russ Taylor. and the POSSUM team. askap.org. /possum. New Discovery Space with ASKAP-12. Radio polarimetry: a highly sensitive probe of density, magnetic field and turbulence at all redshifts. Project Update. CSIRO Astronomy and Space Science. Antony Schinckel, ASKAP Director. 30 October 2012. ATUC Meeting . | Antony Schinckel | Page . 1. SKA Office visits Australia, October 2012. Members of the international SKA Office recently visited Australia on a . CSIRO Astronomy & Space Science, . Detecting the . Unexpected: Discovery . in the Era . of Astronomically . Big . Data. . Detecting the Unexpected . (. Discovery in the Era of Astronomically Big Data). AIV consortium. Manchester. June 2013. AIV consortium responsibility. Identify constraints (interfaces) between:. SKA1 elements and existing infrastructure. SKA1 elements and pre-cursors. For the purpose of this meeting:. of . Local Galaxies. Michael . Brown. ARC Future Fellow. Monash. University. Where are we now?. NVSS / FIRST / SUMMS. 0.5 . mJy. RMS per beam. 15”-1’ beam. ~30 . uJy. RMS per beam in 12 hours .

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