APSR: digital signal processing at Parkes Willem van Straten, Andrew Jameson and Matthew Bailes Centre for Astrophysics & Supercomputing Third ATNF Gravitational.

Slides:



Advertisements
Similar presentations
E-VLBI down-under Tasso Tzioumis ATNF, CSIRO July 2005 Towards e-VLBI.
Advertisements

Ben Barsdell Matthew Bailes Christopher Fluke David Barnes.
E-VLBI progress in the South Tasso Tzioumis ATNF, CSIRO September 2006 “Towards e-VLBI”  “e-VLBI”
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review John Ford August 5, 2008 CICADA Project The NRAO is operated for the National Science Foundation.
Implementation of a streaming database management system on a Blue Gene architecture for measurement data processing. Erik Zeitler Uppsala data base lab.
Low-Frequency Pulsar Surveys and Supercomputing Matthew Bailes.
Baseband Processing and SKA Simulations using Supercomputers: Enhancing Australia‘s radio astronomy facilities and its bid for the SKA Steven Tingay Swinburne.
Measuring Dispersion in Signals from the Crab Pulsar Jared Crossley National Radio Astronomy Observatory Tim Hankins & Jean Eilek New Mexico Tech Jared.
DFT Filter Banks Steven Liddell Prof. Justin Jonas.
The Transient Radio Sky to be Revealed by the SKA Jim Cordes Cornell University AAS Meeting Washington, DC 8 January 2002.
The New GHz Pulsar Digital Filter Bank System Grant Hampson ATNF Research Engineer 23 November 2005.
Prototype SKA Technologies at Molonglo: 3. Beamformer and Correlator J.D. Bunton Telecommunications and Industrial Physics, CSIRO. Australia. Correlator.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Digital Signal Processing.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Spectrometer PDR John.
VLBI Report LBA Operations & eVLBI Tasso Tzioumis ATNF May 2008.
Backend electronics for radioastronomy G. Comoretto.
P ulsa R E xploration and S earch TO Jintao Luo NRAO-CV CREDIT: Bill Saxton, NRAO/AUI/NSF.
FPGA-based Dedispersion for Fast Transient Search John Dickey 23 Nov 2005 Orange, NSW.
RN /08/05 National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Implementation of an Antenna.
1 of 22 Glaciers and Ice Sheets Interferometric Radar (GISIR) Center for Remote Sensing of Ice Sheets, University of Kansas, Lawrence, KS
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The VLBA Sensitivity.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The VLBA Sensitivity.
Design and performance of fast transient detectors Cathryn Trott, Nathan Clarke, J-P Macquart ICRAR Curtin University.
200/MAPLD 2004 Craven1 Super-Sized Multiplies: How Do FPGAs Fare in Extended Digit Multipliers? Stephen Craven Cameron Patterson Peter Athanas Configurable.
Results of automatic, high time resolution GRB follow-up with the Parkes 12 m Keith Bannister Sydney Institute for Astronomy.
The Control System for the Caltech Millimeter Array Steve Scott OVRO.
NTD/xNTD Signal Processing Presented by: John Bunton Signal Processing team: Joseph Pathikulangara, Jayasri Joseph, Ludi de Souza and John Bunton Plus.
Accelerating a Software Radio Astronomy Correlator By Andrew Woods Supervisor: Prof. Inggs & Dr Langman.
XNTD/SKAMP/LFD Correlator 4th RadioNet Engineering Forum Workshop Next Generation Correlators for Radio Astronomy and Geodesy June 2006, Groningen,
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
Next Generation Digital Back-ends at the GMRT Yashwant Gupta Yashwant Gupta National Centre for Radio Astrophysics Pune India CASPER meeting Cambridge.
GPU DAS CSIRO ASTRONOMY AND SPACE SCIENCE Chris Phillips 23 th October 2012.
1 Advanced ATNF Correlators Dick Ferris AT Electronics Development Group May 2003.
Field Trials of an RFI Adaptive Filter for Pulsar Observations M. Kesteven, R.N. Manchester, G. Hampson & A. Brown Australia Telescope National Facility.
Australian Astronomy MNRF Development of Monolithic Microwave Integrated Circuits (MMIC) ATCA Broadband Backend (CABB)
Astrophysical Applications on Superclusters Matthew Bailes Swinburne Centre for Astrophysics and Supercomputing.
DiFX Performance Testing Chris Phillips eVLBI Project Scientist 25 June 2009.
Real-time Acquisition and Processing of Data from the GMRT Pulsar Back- ends Ramchandra M. Dabade (VNIT, Nagpur) Guided By, Yashwant Gupta.
An FX software correlator for VLBI Adam Deller Swinburne University Australia Telescope National Facility (ATNF)
LIGO-G D Global Diagnostics and Detector Characterization 9 th Marcel Grossmann Meeting Daniel Sigg, LIGO Hanford Observatory.
GSB : A real-time Software back-end for the GMRT Jayanta Roy National Centre for Radio Astrophysics Pune, India 12 th December 2008 Collaborators.
Adaptive Filters for RFI Mitigation in Radioastronomy
The Correlators ( Spectrometers ) Mopra Induction - May 2005.
The ATNF Pulsar Data Archive Matthew Whiting (ATNF) Albert Teoh, David Smith, Lucyna Kedziora-Chudczer, Dick Manchester, Vince McIntyre 2nd Gravitational.
Ramesh Bhat Centre for Astrophysics & Supercomputing Swinburne University of Technology Time Domain Astronomy Meeting, Marsfield, 24 October 2011 Searching.
Large Area Surveys - I Large area surveys can answer fundamental questions about the distribution of gas in galaxy clusters, how gas cycles in and out.
by Arjun Radhakrishnan supervised by Prof. Michael Inggs
Short introduction Pulsar Parkes. Outline PDFB – Single beam pulsar timing system CASPER – Single beam pulsar coherent dedispersion system.
Review of developments in Australasia and mainland Asia Steven Tingay Swinburne University of Technology Next Generation correlator meeting, JIVE 27 -
A real-time software backend for the GMRT : towards hybrid backends CASPER meeting Capetown 30th September 2009 Collaborators : Jayanta Roy (NCRA) Yashwant.
APSR Matthew Bailes Swinburne University Of Technology.
Coherent Dedispersion Pulsar Timing Machines Matthew Bailes + Swinburne, Caltech, ATNF, CASPER.
Philippe Picard 2 nd SKADS Workshop October 2007 Station Processing Philippe Picard Observatoire de Paris Meudon, 11th October 2007.
ATCA GPU Correlator Strawman Design ASTRONOMY AND SPACE SCIENCE Chris Phillips | LBA Lead Scientist 17 November 2015.
Parkes ATUC Report Nov Stats Scheduled observing time (2007) –85% Downtime (last 12 months): –1% system faults –3.1% high wind.
Low Frequency Observations of the ISM and Pulsar Timing Joris Verbiest Xiaopeng You (Southwest University, China) William Coles (UCSD) George Hobbs (ATNF)
VLBI Developments in Australia ASTRONOMY AND SPACE SCIENCE Chris Phillips| LBA Lead Scientist 11 November 2014.
FP7 Uniboard project Digital Receiver G. Comoretto, A. Russo, G. Tuccari, A Baudry, P. Camino, B. Quertier Dwingeloo, February 27, 2009.
Searching FRB with Jiamusi-66m Radio Telescope
“Lunar UHE Neutrino Astrophysics with the Square Kilometre Array”
Telescopes and Images.
Pulsar Timing with ASKAP Simon Johnston ATNF, CSIRO
LOFAR Beam Formed (BF) Data & Pipeline Overview September 9, 2010
Synopsis “The Matrix”: polarisation and pulsar timing
Efficient mitigation of RFI at radio astronomy observatories
The High Time Resolution Universe Survey Backend
Improving Pulsar Timing
The Uniboard  FPGA Processing for Astronomy
SKAMP Square Kilometre Array Molonglo Prototype
Presentation transcript:

APSR: digital signal processing at Parkes Willem van Straten, Andrew Jameson and Matthew Bailes Centre for Astrophysics & Supercomputing Third ATNF Gravitational Wave Workshop 2009

ATNF Parkes Swinburne Recorder Combination of FPGAs and CPUs  PDFB3 implements polyphase filterbank  16 processing nodes receive sub-band as UDP stream Real-time and/or offline data reduction  record data to disk at 1.6 GB/s for 2.5 hours Remote control and monitoring  web-based interface

Parkes Digital Filterbank Designed/developed at ATNF  2 x Compact Array Broad-band (CABB) board  up to 2048 channel polyphase filterbank  real-time RFI mitigation CABB = 2GHz correlator  modularity of FPGA design  hardware re-use

APSR Features Phase-coherent dispersion removal (up to 1024 MHz) Automatic impulsive interference excision  RFI, lightning, etc. Single-pulse capability  with real-time calibration and/or giant pulse selection Fold multiple pulsars simultaneously  globular clusters, binary pulsar Computation of auxiliary statistics  e.g. fourth-order moments

Phase-coherent dispersion removal Observed voltage signal is deconvolved  impulse response function of ISM plasma dispersion Convolution performed in frequency domain  more efficient, requires FFT N fft proportional to DM  2 / 3

Phase-coherent dispersion removal flops = 5NlogN / t FFT on each APSR node: (assuming DM=10) centre frequency bandwidth per node optimal N fft required Gflops 3.1 GHz64 MHz128k GHz16 MHz128k MHz4 MHz64k0.7

FFT benchmarks 700 MHz 1.4 GHz 3.1 GHz

Multi-threaded dspsr thread-safe revisions to underlying library thread-shared buffering of overlap regions  overlap-save method of discrete convolution thread-coordinated output of results  threads combine results every 10 seconds near linear scaling of performance!

Coherent Dedispersion - History Arecibo  XDS Sigma 5 magnetic tape  20% duty cycle for 3 minutes MHz  Reticon R5601 chip  real-time! Parkes  S2, VHS tape Parkes  CPSR, DLT tape MHz  CPSR2, high-speed disk MHz  APSR, real-time

XDS Sigma 5: picture

XDS Sigma 5 vs iPod

APSR web-based interface

: DFB3

: APSR

CAL lightning: DFB3

CAL lightning: APSR

Single pulse

Average pulse

Testing & Commissioning Polarimetric Calibration High-precision timing Frequency response tests User and TCS interface improvements GOAL: National Facility Instrument