Prototype Correlator Testing

Slides:



Advertisements
Similar presentations
Thirteenth Synthesis Imaging Workshop 2012 May 29– June 5 Planning VLA Observations: Tutorial Michael P. Rupen NRAO/Socorro.
Advertisements

The EVLA and SKA pathfinder surveys Jim Condon NRAO, Charlottesville.
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Cross Correlators Walter Brisken.
C. ChandlerEVLA Advisory Committee Meeting September 6-7, Scientific Commissioning Plan Claire Chandler.
KAT-7/MeerKAT Commissioning SPT and Commissioning teams * * Bennett, T., Blose, S., Booth, R., de Villiers,
EVLA Early Science: Shared Risk Observing EVLA Advisory Committee Meeting, March 19-20, 2009 Claire Chandler Deputy AD for Science, NM Ops.
Spectral Line VLBI Chris Phillips JIVE The Netherlands Chris Phillips JIVE The Netherlands.
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The Expanded Very Large.
S.T. MyersEVLA Advisory Committee Meeting September 6-7, 2007 EVLA Algorithm Research & Development Steven T. Myers (NRAO) CASA Project Scientist with.
Which dipoles to use to optimize survey speed? –What tapering? –Trade-off between sensitivity, FOV and low side-lobe levels –Station beam stability, pointing.
Introducing the EVLA NRAO Postdoctoral Symposium, 29 April-1 May 2009 Michael P. Rupen Project Scientist for WIDAR.
1 SAGE Committee Meeting – December 19 & 20, 2008 National Radio Astronomy Observatory EVLA Goals, Progress, Status, and Projections Rick Perley Mark McKinnon.
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
JVLA capabilities to be offered for semester 2013A Claire Chandler.
1 EVLA System Commissioning Results EVLA Advisory Committee Meeting, March 19-20, 2009 Rick Perley EVLA Project Scientist.
EVLA Transition to Science Operations: An Overview EVLA Advisory Committee Meeting, March 19-20, 2009 Bob Dickman AD, NM Operations.
ASKAP Capabilities John Reynolds on behalf of the SEIC and ASKAP team.
Radio Interferometers’ Data Archives how to find, retrieve, and image radio data: a lay-person’s primer Michael P Rupen (NRAO)
Sanjay BhatnagarEVLA Advisory Committee Meeting May 8-9, EVLA Algorithm Research & Development Progress & Plans Sanjay Bhatnagar CASA/EVLA.
Murchison Widefield Array (MWA) : Design and Status Divya Oberoi, Lenoid Benkevitch MIT Haystack Observatory doberoi, On behalf.
Observing Strategies at cm wavelengths Making good decisions Jessica Chapman Synthesis Workshop May 2003.
ASKAP: Setting the scene Max Voronkov ASKAP Computing 23 rd August 2010.
Brent CarlsonEVLA System PDR (Correlator V2) December 4-5, Correlator.
1 SAGE Committee Meeting – December 19 & 20, 2008 National Radio Astronomy Observatory Correlator Status and Growth of Capabilities Michael P. Rupen Project.
Rick Perley 2 Nov 2001 EVLA Correlator Conceptual Design Review 1 Science Drivers for the EVLA Correlator Rick Perley EVLA Project Scientist 2 Nov 2001.
Recent progress in EVLA-specific algorithms EVLA Advisory Committee Meeting, March 19-20, 2009 S. Bhatnagar and U. Rau.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The Expanded Very Large.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array EVLA Early Science.
Rick PerleyEVLA Advisory Committee Meeting September 6-7, 2007 Some Illustrative Use Cases Rick Perley.
M.P. RupenEVLA Advisory Committee Meeting September 6-7, Correlator Test Plan Michael P. Rupen.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Correlator Specifications Michael P. Rupen.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Scientific Impact Michael P. Rupen.
Rick PerleyEVLA Front-End CDR – On the Sky Tests April 24, EVLA Front-End CDR On the Sky Tests.
Frazer OwenNSF EVLA Mid-Project Review May 11-12, Transition to EVLA
M.P. Rupen, Synthesis Imaging Summer School, 18 June Cross Correlators Michael P. Rupen NRAO/Socorro.
Michael RupenEVLA Phase II Definition Meeting Aug 23 – 25, EVLA Phase II Scientific Overview Michael P. Rupen.
SAGE meeting Socorro, May 22-23, 2007 WIDAR Correlator Overview Michael P. Rupen Project Scientist for WIDAR & Software.
WIDAR Correlator Options and Potential Craig Walker NRAO Socorro U.S. VLBI Technical Coordination Meeting May 14-15, 2007.
Imaging issues Full beam, full bandwidth, full Stokes noise limited imaging Algorithmic Requirements: –PB corrections: Rotation, Freq. & Poln. dependence,
Data Examination and Checking Programs--Requirements B. Carlson
Surveying Cosmic Time with the WIDAR Correlator
EVLA Spectral-Line Science Below 1200 MHz
EVLA Availability - or - When Can I Use It?
Observing Strategies for the Compact Array
S. Bhatnagar: ASTRON, Dwingeloo, June 29th 2010
Imaging and Calibration Challenges
Monitor and Control Software
EVLA Advisory Committee Meeting System Status
EVLA Prototype Correlator (PTC)
Oxford Algorithms Workshop
HERA Imaging and Closure
EVLA Status and Prospects
EVLA System PDR System Overview
Rick Perley National Radio Astronomy Observatory
Shared Risk Observing Claire Chandler EVLA SSS Review, June 5, 2009
VLA to EVLA Transition Plan
Some Illustrative Use Cases
Terry Cotter LO/IF Group Leader
EVLA Advisory Committee Meeting
Science Commissioning
Shared Risk Science with the EVLA
EVLA Advisory Committee Meeting, March 19-20, 2009
EVLA Algorithm Research & Development
Prototype Correlator Tests on the Critical Path
Correlator Growth Path
EVLA Construction Status
VLA EXPANSION PROJECT Correlator Issues.
EVLA Advisory Panel Mtg. System Overview
KFPA CDR R. Norrod Feb 27, 2008.
Presentation transcript:

Prototype Correlator Testing EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR

Prototype Correlator 4 antennas 1 GHz @ 8-bits, RCP only 4-bit re-quantization 8 x (8-128) MHz subbands 128 MHz: 1024 x 125 kHz per subband Dumptime 0.05-1 sec up to 7 MB/s 1.4 GB/hr with 1sec dumps Longest observations ~10 hours No on-line flagging No Tsys No referenced pointing CBE writes raw data scaled by data valid & FFT’d

4-station PTC W48 = ea17 10.5km N16 = ea18 1.4km E72 = ea23 21.0km

Critical On-the-sky Tests Primary purpose of Prototype Correlator (PTC) Designed to check for hardware problems, before going to full production Test plan originally outlined by Carlson (2006) Reviewed and revised by NRAO (December 2007) Final form: Rupen (2008) Carried out June-Dec 2008, culminating in successful WIDAR CDR

Overview of PTC CotS Tests Dynamic fringes at 1, 5, 8, 22, 45 GHz “Plug-&-play” D to A configuration Antenna changes New StB Phase & delay continuity when changing sources, frequencies, bands Closure phase and channel/time averaging Recirculation Deep integrations: high dynamic range (72,800:1), blank field Deep spectral line integration (3C84 HI) “Micro”SDM+BDF to move data into CASA & AIPS

1-2 GHz: continuum + RFI 1 GHz

3C84 @ 1.5 GHz 1244-1756 MHz 8192 x 62.5 kHz (13 km/s for local HI) 512 MHz

3C84 @ 1.5 GHz 512 MHz HI ABQ radars VLA polarizer satellites 8192 x 62.5 kHz (13 km/s for local HI) HI ABQ radars VLA polarizer satellites 512 MHz

3C84 @ 1.5 GHz 512 MHz HI ABQ radars VLA polarizer satellites 8192 x 62.5 kHz (13 km/s for local HI) HI ABQ radars VLA polarizer satellites Current VLA: 6.25 MHz @ 98 kHz 512 MHz

3C84 @ 1.5 GHz 512 MHz HI ABQ radars VLA polarizer satellites 8192 x 62.5 kHz (13 km/s for local HI) Final EVLA: 512 MHz (z=0-0.3) @ 7.8 kHz (1.7 km/s) HI ABQ radars VLA polarizer satellites Current VLA: 6.25 MHz @ 98 kHz 512 MHz

3C84 @ 1.5 GHz 1376-1384 MHz (one 8 MHz subband) 4096 x 1.95 kHz (0.4 km/s)

3C84 @ 1.5 GHz 1382.95 MHz 1420.35 MHz 1395.5 MHz 8 x 8 MHz subbands 8 x 4096 channels Avg’d x2 (3.9 kHz) or x64 (470 kHz) Zoomed in here! Tau~0.15 Tau~0.21 32 km/s 17 km/s 1382.95 MHz 1420.35 MHz Tau~0.003 430 km/s 1395.5 MHz

3C84 @ 1.5 GHz 1382.95 MHz 1420.35 MHz 1395.5 MHz 8 x 8 MHz subbands 8 x 4096 channels Avg’d x2 (3.9 kHz) or x64 (470 kHz) Zoomed in here! Full EVLA: 64 independently tunable subband pairs Different bandwidth & resolution for each subband pair Tau~0.15 Tau~0.21 32 km/s 17 km/s 1382.95 MHz 1420.35 MHz Tau~0.003 430 km/s 1395.5 MHz

3C84 @ 22 GHz 21988-23012 MHz 8192 x 125 kHz (1.7 km/s) 1 GHz

3C84 @ 22 GHz 1 GHz 21988-23012 MHz 8192 x 125 kHz (1.7 km/s) Full EVLA: 8 GHz (BWR 1.5:1) Full pol’n 8192 x 1 MHz (14 km/s) 1 GHz

Recirculation: Orion water masers 128 MHz, no recirc. 125 kHz/channel

Recirculation: Orion water masers 128 MHz, no recirc. 125 kHz/channel 64 MHz, x2 recirc. 31.25 kHz/channel 1.4% shown here

Recirculation: Orion water masers 128 MHz, no recirc. 125 kHz/channel 64 MHz, x2 recirc. 31.25 kHz/channel Smoothed to match

Image not limited by closure errors 0217+738 4 Jy “dot” 2hr10min on-source 4588-5612 MHz Self-cal’d image Peak:rms= 72,800:1

Deep images of strong calibrators 4844-4972 MHz 4972-5100 MHz 4844-5100 MHz 3C84: 5.2 hours 0217+738: 2.2 hours 0157+747: 0.8 hours N.B. noise matches SEFD to 10% !

Deep image of a blank field J1900+2815 9012-7988 MHz 2.3 hours on-source Rms in 125 kHz: 2.84 mJy/beam Rms in 103 MHz (825 channels): 0.11 mJy/bm Rms in 825 MHz (825x8 channels): 0.052 mJy/bm

Backup slides

PTC CotS Tests: The List 2.1 Fringe check with delay tracking Phase, delay vs. time Autocorr’ns, state counts, etc. 2.2 Phase continuity Phase, delay consistent when changing sources, frequencies, bands 2.3 Closure Stability for hours Integrates down with time and frequency averaging Clean images 2.4 Deep continuum observation 10 hours

PTC CotS Tests: The List 2.5 Spectral line consistency Different subband bandwidths 2.6 Subband aliasing Leakage between subbands 2.7 Recirculation 2.8 Deep spectral integration

Filter response 0217+738 4 Jy “dot” 40min on-source 7656-7784 MHz Subband 4 128 MHz: Stage 1 only

Closure phase: averaging down 0217+738 4 Jy “dot” 2hr10min on-source 4588-5612 MHz Averages down to 0.03-0.11 degs. Avg x2 in freq, then time DR~ 31,000:1 Corresponds to pol’n leakage of a few %

Averaging down in frequency 0217+738 4 Jy “dot” 40min on-source 7784-7912 MHz Subband 3 128 MHz, 1024 channels Boxcar averaging by 4, 16, 64, 128, 256,… Within 1% of theoretical through box=64

Averaging down in frequency J0012+3053 16 mJy “dot” 2 hours on-source 8288-8416 MHz subband 3 128 MHz, 1024 channels Boxcar averaging: 2, 4, 8, 16, … channels Noise goes down by sqrt(2) within 1% through box=64