'Askap' presentation slideshows

The Australian SKA Pathfinder

990 views • 83 slides

The status and science of ASKAP

The status and science of ASKAP. Philip Diamond Chief, CSIRO Astronomy & Space Science RTS 2012 19 April 2012. Australian SKA Pathfinder (ASKAP). ASKAP, currently being developed by CSIRO, at the Murchison Radio-astronomy Observatory (MRO) in Western Australia

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ASKAP Correlator

We acknowledge the Wajarri Yamatji people as the traditional owners of the Murchison Radio Observatory site. ASKAP Correlator. The 7th International VLBI Technology Workshop Thailand. CASS.

430 views • 28 slides

The Galactic Australia SKA Pathfinder Spectral Line Survey (GASKAP)

The Galactic Australia SKA Pathfinder Spectral Line Survey (GASKAP). Milky Way Galaxy Workshop in Kagoshima University on 2012 September 6. Hiroshi Imai Graduate School of Science and Engineering, Kagoshima University

366 views • 23 slides

ASKAP Update

ASKAP Update. David DeBoer ASKAP Project Director 26 May 2010. ASKAP Design Goals. High-dynamic range, wide field-of-view imaging Number of dishes 36 (3-axis) Dish diameter 12 m Max baseline 6km Resolution 30 ? Sensitivity 65 m 2 /K Speed 1.3x10 5 m 4 /K 2. deg 2

329 views • 19 slides

Science status of the Australian Square Kilometre Array Pathfinder (ASKAP)

Science status of the Australian Square Kilometre Array Pathfinder (ASKAP). Simon Johnston ASKAP Project Scientist 14 May 2009 ATUC Open Session. ASKAP Design Goals. High-dynamic range, wide field-of-view imaging Number of dishes 36 Dish diameter 12 m

284 views • 17 slides

Science status of the Australian Square Kilometre Array Pathfinder (ASKAP)

Science status of the Australian Square Kilometre Array Pathfinder (ASKAP). Simon Johnston ASKAP Project Scientist 14 May 2009 ATUC Open Session. ASKAP Design Goals. High-dynamic range, wide field-of-view imaging Number of dishes 36 Dish diameter 12 m

174 views • 17 slides

ASKAP and DVP

ASKAP and DVP. David DeBoer ASKAP Project Director 15 April 2010 Arlington, VA. ASKAP Design Goals. High-dynamic range, wide field-of-view imaging Number of dishes 36 (3-axis) Dish diameter 12 m Max baseline 6km Resolution 30 ? Sensitivity 65 m 2 /K

291 views • 14 slides

GASKAP The Galactic ASKAP Survey

242 views • 14 slides

ASKAP and DVP

ASKAP and DVP. David DeBoer ASKAP Project Director 15 April 2010 Arlington, VA. ASKAP Design Goals. High-dynamic range, wide field-of-view imaging Number of dishes 36 (3-axis) Dish diameter 12 m Max baseline 6km Resolution 30 ? Sensitivity 65 m 2 /K

208 views • 14 slides

Spectrum Management: Parkes & ATCA

Spectrum Management: Parkes & ATCA. Briefing for ATUC members. Erik Lensson | Head, ATNF Engineering Operations . 30 October 2012. CSIRO ASTRONOMY AND SPACE SCIENCE. Background.

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ASKAP: Setting the scene

ASKAP: Setting the scene. Max Voronkov ASKAP Computing 23 rd August 2010. ASKAP overview. http://www.atnf.csiro.au/projects/askap/. Located at radio-quiet site approx. 300 km inland from Geraldton Array of 36 12m antennas with phased array feeds (PAF)

226 views • 9 slides