SETI Spectrometer Development for ALFA

Slides:



Advertisements
Similar presentations
Progress With iBOBs at Jodrell Bits & Bytes Meeting, JBO, th Dec 2007 Jonathan Hargreaves Electronic Engineer, Jodrell Bank Observatory.
Advertisements

West Coast Spectrometer Team Mark Wagner, Berkeley project manager, FPGA designer Terry Filiba, data transport: FPGA --> CPU --> GPU Suraj Gowda, boosting.
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.
NAIC Visiting Committee Meeting · March 4-6, 2008 FPGA SPECTROMETER COMMISSIONING Spectrometer description How it will be used Where we are at. What needs.
7th US VLBI Technical Meeting at Haystack Observatory, November 3-4, 2009 Arecibo VLBI Report Arecibo VLBI Team: V. Arun, R. Ganesan, T. Ghosh, C. Salter.
Jim Cordes and Dan Werthimer And Five Milliion Volunteers in 226 countries
SDSS7 - DSP and Backends Intro, 12 Jul 2013 Digital Signal Processing Basics and AO Back-Ends Luis A. Quintero Digital Section Head Electronics Department.
All things DBE… Francois Kapp Sub-system Manager: DBE On behalf of the DBE team present and past... S Rajan, E Bauermeister, A.
Shilpa Bollineni, Glen Langston, John Ford, Randy McCullough and Paul Demorest DATA ACQUISITION ON THE 43M TELESCOPE.
Digital FX correlator Samuel Tun. FASR Subsystem Testbed (FST) 1-9 GHz in 500 MHz band recorded at 1 GS/s from each antenna. Correlation carried out offline.
PELICAN Imaging Framework Imaging on short timescales leads to very large correlator output data rates. In order to cope with these rates and produce updated.
SciFi Tracker DAQ M. Yoshida (Osaka Univ.) MICE Tracker KEK Mar. 30, 2005.
NASA DSN Radio Astronomy Signal Processing Ambitions for DSN Radio Astronomy Tom Kuiper JPL - Caltech.
Rapid Development of Radio Astronomy Instrumentation Using Open Source FPGA Boards, Tools and Libraries Center for Astronomy Signal Processing and Electronics.
Andrew Siemion SSL Colloquium April 10, 2009 Andrew Siemion SSL Colloquium April 10, 2009 Searching for Radio Ephemera: The Fly’s Eye AstroPulse Searching.
Signal Processing for Aperture Arrays. AAVS1 256 antenna elements distributed over –4 stations –64 elements each.
Highly Scalable Packetised correlators Jason Manley CASPER workshop 2009.
Current Approaches to the Search for Life Dan Werthimer, UC Berkeley
A Low-Cost Phase Cal Monitor and RFI Spectrum Analyzer for VLBI2010 Mark-5 / Mark-6 using Cheap,COTS Software Defined Radio (SDR) Hardware & Software Gleaned.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array A New Multibeam Spectrometer.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The VLBA Sensitivity.
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Ron DuPlain, Scott Ransom, Paul Demorest, Patrick Brandt, John Ford, Amy Shelton CASPER information.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The VLBA Sensitivity.
Galfa Spectrometer Jeff Mock, Dan Werthimer Jeff Mock, Dan Werthimer Students: Henry Chen, Pavel Monat, Aaron Parsons, Wonsop Sim Science Advisors: Carl.
KuPol: A New Ku-Band Polarimeter for the OVRO 40-Meter Telescope Kirit Karkare Caltech Radio Astronomy Laboratory CASPER Workshop – August 17, 2010.
High Bandwidth Data Acquisition and Network Streaming in VLBI Jan Wagner, Guifré Molera et al. TKK / Metsähovi Radio Observatory.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Meeting Summary Richard.
The BEST-2 SKA pathfinder is composed by 32 receivers. The front ends are installed on the focal lines of 8 cylinders, offering a collecting area of about.
Next Generation Digital Back-ends at the GMRT Yashwant Gupta Yashwant Gupta National Centre for Radio Astrophysics Pune India CASPER meeting Cambridge.
Nov 3, 2009 RN - 1 Jet Propulsion Laboratory California Institute of Technology Current Developments for VLBI Data Acquisition Equipment at JPL Robert.
Hardware: Old, New, Future Hardware: Old, New, Future Dan Werthimer and Casper Collaborators.
CASPER Packetised correlators Jason Manley CASPER workshop 2009.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array CASPER Workshop 2009.
MeerKAT DBE Past Present Future Alan Langman 28 September 2009.
S.Montebugnoli BEST 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Stelio Montebugnoli IRA -INAF- Bologna –Italy- SKADS 4th -Lisbon- Oct 2-3, 2008.
Jason Manley, Aaron Parsons, Don Backer, Henry Chen, Terry Filiba, David MacMahon, Peter McMahon, Arash Parsa, Andrew Siemion, Dan Werthimer, Mel Wright.
Short introduction Pulsar Parkes. Outline PDFB – Single beam pulsar timing system CASPER – Single beam pulsar coherent dedispersion system.
VLBA Implementation of the ROACH Digital Backend Jonathan Romney on behalf of the VLBA Upgrade development team NRAO / Socorro First International VLBI.
A real-time software backend for the GMRT : towards hybrid backends CASPER meeting Capetown 30th September 2009 Collaborators : Jayanta Roy (NCRA) Yashwant.
Omnisys There are a few different activities at Omnisys that may be of your interests. –New correlation spectrometer IC’s. –New FFT spectrometers –Future.
ALFA Pulsar Surveys Jim Cordes, Cornell University Arecibo 16 March 2003 Pulsar Consortium meeting 1-2 Nov 2002 Preliminary survey plans Hardware needs.
Version 10.1 Xilinx Tools Update Terry Filiba CASPER Workshop II.
The Green Bank Telescope Frank Ghigo, National Radio Astronomy Observatory 7 th US VLBI Technical Meeting, Haystack, Nov 2009.
CASPER Open Source Hardware Current and Future ADC’s
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review John Ford September 28, 2009 Casper Instrumentation at Green Bank The NRAO is operated for.
1 MICE Tracker Readout Update Introduction/Overview TriP-t hardware tests AFE IIt firmware development VLSB firmware development Hardware progress Summary.
IR, Visible and Radio SETI Andrew Siemion, David Anderson, Bob Bankay, Henry Chen, Jeff Cobb, Griffin Foster, Andrew Howard, Eric Korpela,
Exploring the Unknown with CASPER Instrumentation Andrew Siemion CASPER Workshop 2011.
Possible Instrumentation Development Items for SKA at ASIAA Chau-Ching Chiong (ASIAA) and Yuh-Jing Hwang, Homin Jiang, Chao-Te Li.
FP7 Uniboard project Digital Receiver G. Comoretto, A. Russo, G. Tuccari, A Baudry, P. Camino, B. Quertier Dwingeloo, February 27, 2009.
ROACH II Review Introduction. ROACH II Review Agenda ● Agenda: – ROACH I, what was right, what was wrong? – Why ROACH II? – The place of ROACH II – Specifications.
JIVE UniBoard Correlator External Review
RF acceleration and transverse damper systems
GUPPI Software Overview
FRB Backend First Light
Mark 5 / VLBA Correlator Topics
Multifunctional Digital Backend (MDBE) for "Quasar" VLBI-network
Lessons from CASPER Correlators at GMRT
Status DETECTORS: We have a first baseline array (144 pixels) at 2mm. Average sensitivity: 6mK/Hz0.5 (1Hz) Without de-correlation. In 2009 it was roughly.
5 Gsps ADC Developement and Future Collaboration
The SERENDIP, SEVENDIP, Astropulse, and SPOCK SETI Programs
The High Time Resolution Universe Survey Backend
Progress Update Henry Chen December 17, 2010.
Eric oberla Herve grabas
iBOB Data Acquisition and Network Streaming
Arecibo and ALFA Telescope upgrade ALFA = Arecibo L-band Feed Array
ALFA/Arecibo pulsar surveys
SKAMP Square Kilometre Array Molonglo Prototype
Presentation transcript:

SETI Spectrometer Development for ALFA Laura Spitler CASPER Workshop II 3 August 2008

Collaboration UC Berkeley Cornell University / NAIC Dan Werthimer Andrew Siemion CASPER group SSL SETI group Cornell University / NAIC Laura Spitler Jim Cordes

Arecibo Observatory

ALFA receiver system 1.4 GHz 7 feeds 300 MHz BW Surveys PALFA ALFALPHA

SETI ALFA Survey Bandwidth: 200 MHz (300 MHz) Number of channels: 128 Mchannels  ~ 1.5 Hz Data rate: ~1 Mbyte/sec (more later?)

SETI spectrometer

SETI spectrometer hardware First generation iADC + iBOB + BEE2 Multiplex beams and polarization Second generation 7 ROACH boards

ADC + DDC + XAUI (iBOB)

4k PFB (BEE2)

Corner Turner & FFT (BEE2) 32k x 4k matrix transpose FFT 32k

Thresholder and Data Recorder Record events to Shared FIFO accessible via BORPH Read out as UDP packets via 10 Mb Ethernet Transfer data to Cornell / Berkeley via internet

SERENDIP pipeline Cleans raw data Prepares for database RFI extraction Candidate generation

Post processing