LOFAR: Lessons Learnt

Size: px
Start display at page:

Download "LOFAR: Lessons Learnt"

Transcription

1 LOFAR: Lessons Learnt Michiel van Haarlem van Weeren, Bonafede, Ferrari, Orrù, Pizzo, Shulevski, van der Tol, Macario Jason Hessels & Pulsar Team

2 LOFAR 40 stations in NL and 8 stations throughout Europe (DE(5), FR, SE, UK) Netherlands 24 core stations (2 HBA fields) and 16 remote stations (single HBA field) LBA: MHz (96 antennas) HBA: MHz (48 antennas) 48 (dual pol.) signal paths Bandwidth: 32 (48) MHz N beams > 8 Baselines up to 100 km in NL International International Stations 96 LBA, 96 (4x4) HBA tiles and 96 dual pol. signal paths International LOFAR Telescope (ILT) will provide access to LOFAR Operations by ASTRON in collaboration with local international stations Key Science Projects (6 in total) to play large role in first years Open time 10 & 20% in first two years, t.b.d. after that PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 2

3 Current Status (NL) Construction of stations started March 2009 Network + Phase 1 Central Processing Completed On-line CEP based on 3 IBM BlueGene/P racks 33 stations completed in 2009 and 2010 Phase 2 CEP complete by end of station to go in 2011 First LOFAR Station - CS 302 early May 2009 PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 3

4 Developing the Core Area, Building Stations early July August 2009 late July August 2009 September 2008 October March 2010 PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 4

5 23 May 2010 PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 5

6 Chilbolton (UK) Potsdam (D) Tautenburg (D) Effelsberg (D) Nançay (F) LOFAR Stations Across Europe PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 6 Unterweilenbach (D)

7 Software Pipelines Standard Imaging Pipeline Known Pulsar Pipeline Transient Detection Pipeline VHECR Pipeline PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 7

8 Timeline of LOFAR Project First Plans System Requirements Review Preliminary Design Review Complete Initial Test Station Critical Design Reviews (subsystems) Construction CS-01 First Results from CS-01 Final System Critical Design Review Start Procurement Start Roll-Out / early 2007 April 2007 December 2007 Summer 2008 PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 8

9 CS-01 (2006) 96 LBA antennas (30-80 MHz) 6 HBA tiles ( MHz) Distributed over 4 station locations (48/16/16/16) Max. baselines: 500 m Prototype hardware Tested Procurement Process Technical/System Tests: data transport, synchronization, correlation, stability, RFI, station calibration, Platform for Software Pipelines PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 9

10 Procurement Rounds European directives apply above threshold values (193k for public sector supply and service contracts, M for public sector and utility works contracts) Construction of CS-01 (early 2006): Rehearsal Main Roll-Out: three Invitations to Tender: 1. Printed Circuit Boards, Cabinets and Station Hardware (HBA, cables) December Network Equipment Januari Central Processing, Storage Cluster and Local Control Computers April 2008 (selected two preferred suppliers) Lessons learnt CS-01 procurements allowed overall cost estimate within 2% Demands from funding sources sometimes contradict directives Public tenders complicate collaboration with industry smaller companies will find it difficult to invest Get professionals to run procurements and manage contracts Freeze design if uncertainties exist incorporate escapes Be careful in running procurements, errors can cause serious delays PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 10

11 Supervising Mass Production Producibility before procurement otherwise costly initial production run Define test procedures early make them as short as possible. Watch out for changes in production large numbers, high cost Average 3% production loss PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 11

12 Producing High Band Antenna Contract awarded to local company Set up dedicated assembly line in Exloo Production of electronics, cables, connectors not part of this contract Uncertainties in roll-out (weather) affected start of production Delays, extra transport and storage all cost money PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 12

13 Station Construction Performed by contracted workforce under supervision of ASTRON roll-out team: Integration, testing and verification of electronics performed off-site Fully completed cabinet transported and installed Flattening and setting out antenna positions Cabling + placement of antennas Validation and initial testing Final testing, handover (including documentation) by ASTRON personnel PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 13

14 Requirements Formalize requirements early Lessons (1) Tough to get clear requirements from users (boring, repetitive) Users prefer to comment on/criticize a design Manage changing requirements Long project, many temptations, lots of good ideas Engineering Balance between simulations and prototyping End-to-End simulation approaches complexity of the full system Prototyping is costly, but worthwhile (don t forget software: integration & test cycles) When to stop developing does it need to be perfect? have clear requirements, and how they are assessed Operations Get operations involved early on (operators, maintenance) PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 14

15 Lessons (2) Software Software deserves a design process similar to all the hardware Get people working together in teams Write only the software you need (PVSS for monitoring and control) Use industry standards where possible Hire professional software developers (no PhDs and Postdocs) Roll Out Define standard transport sizes (truck, container, plane) for the equipment Release one software build for the roll out Planning, logistics and weather are unpredictable All parts should have unique barcode/version number configuration management, maintenance Commissioning Dedicated multi-disciplinary commissioning teams are a good idea (busy weeks PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 15

16 Summary Roll-Out complete in stations in NL + 8 in DE/FR/SE/UK Hard work needed to complete software pipelines Eagerly awaiting first scientific results! Lots of valuable experience for the SKA McKean (ASTRON) Griessmeier & LOFAR Planet WG PrepSKA WP2 Oxford - 28 March 2010 van Haarlem - LOFAR 16

Status of LOFAR. Ronald Nijboer (ASTRON) On behalf of the LOFAR team

Status of LOFAR. Ronald Nijboer (ASTRON) On behalf of the LOFAR team Status of LOFAR Ronald Nijboer (ASTRON) On behalf of the LOFAR team ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) -1- LOFAR: LOw Frequency ARray LBA: 10/30 80 MHz; HBA: 120

More information

LOFAR: Special Issues

LOFAR: Special Issues Netherlands Institute for Radio Astronomy LOFAR: Special Issues John McKean (ASTRON) ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) 1 Preamble http://www.astron.nl/~mckean/eris-2011-2.pdf

More information

LOFAR Status Update Imaging Busy Week 5 Kickoff Meeting 25 January 2010 Michael Wise*

LOFAR Status Update Imaging Busy Week 5 Kickoff Meeting 25 January 2010 Michael Wise* LOFAR Status Update Imaging Busy Week 5 Kickoff Meeting 25 January 2010 Michael Wise* *On behalf of the LOFAR collaboration 1 2 Current Rollout Status Station/Item Cabinet LBA HBA Fibre CEP connection

More information

LOFAR Calibration of the Ionosphere and Other Fun Things

LOFAR Calibration of the Ionosphere and Other Fun Things LOFAR Calibration of the Ionosphere and Other Fun Things anderson@mpifr-bonn.mpg.de LIONS (LOFAR IONospheric Simulations) http://www.strw.leidenuniv.nl/lofarwiki/doku.php?id=lions bemmel@strw.leidenuniv.nl

More information

Assessment of RFI measurements for LOFAR

Assessment of RFI measurements for LOFAR Assessment of RFI measurements for LOFAR Mark Bentum, Albert-Jan Boonstra, Rob Millenaar ASTRON, The Netherlands Telecommunication Engineering, University of Twente, The Netherlands Content LOFAR RFI situation

More information

Effelsberg Status. James M Anderson On behalf of MPIfR and the LOFAR collaboration

Effelsberg Status. James M Anderson On behalf of MPIfR and the LOFAR collaboration Effelsberg Status anderson@mpifr-bonn.mpg.de On behalf of MPIfR and the LOFAR collaboration 1/16 Overview of EF Anderson/MPIfR 2/16 Recent/Current Issues 3/16 HBA Field Repair 2012 Apr 03 A Horneffer 3

More information

Smart Antennas in Radio Astronomy

Smart Antennas in Radio Astronomy Smart Antennas in Radio Astronomy Wim van Cappellen cappellen@astron.nl Netherlands Institute for Radio Astronomy Our mission is to make radio-astronomical discoveries happen ASTRON is an institute for

More information

Overview of Survey KSP meeting Leiden March 2010

Overview of Survey KSP meeting Leiden March 2010 Netherlands Institute for Radio Astronomy Overview of Survey KSP meeting Leiden March 2010 George Heald LSM 20100317 ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) 1 Topics

More information

Dense Aperture Array for SKA

Dense Aperture Array for SKA Dense Aperture Array for SKA Steve Torchinsky EMBRACE Why a Square Kilometre? Detection of HI in emission at cosmological distances R. Ekers, SKA Memo #4, 2001 P. Wilkinson, 1991 J. Heidmann, 1966! SKA

More information

LOFAR Long Baseline Calibration Commissioning

LOFAR Long Baseline Calibration Commissioning LOFAR Long Baseline Calibration Commissioning anderson@mpifr-bonn.mpg.de On behalf of LOFAR and the LLBWG 1/31 No, No Fringes On Long Baseline Yet... I hate pretending to be an optimist when writing abstract

More information

LOFAR: From raw visibilities to calibrated data

LOFAR: From raw visibilities to calibrated data Netherlands Institute for Radio Astronomy LOFAR: From raw visibilities to calibrated data John McKean (ASTRON) [subbing in for Manu] ASTRON is part of the Netherlands Organisation for Scientific Research

More information

Processing Real-Time LOFAR Telescope Data on a Blue Gene/P

Processing Real-Time LOFAR Telescope Data on a Blue Gene/P Processing Real-Time LOFAR Telescope Data on a Blue Gene/P John W. Romein Stichting ASTRON (Netherlands Institute for Radio Astronomy) Dwingeloo, the Netherlands 1 LOw Frequency ARray radio telescope 10

More information

LOFAR update: long baselines and other random topics

LOFAR update: long baselines and other random topics LOFAR update: long baselines and other random topics AIfA/MPIfR lunch colloquium Olaf Wucknitz wucknitz@astro.uni-bonn.de Bonn, 6th April 20 LOFAR update: long baselines and other random topics LOFAR previous

More information

CALIBRATION AND IMAGING WITH LOFAR

CALIBRATION AND IMAGING WITH LOFAR CALIBRATION AND IMAGING WITH LOFAR Emanuela Orru on behalf of the Calibration and Imaging Tiger Team (CITT) BASIC COMPONENTS Calibration and imaging software HBA Goal: Facilitate the Radio Observatory

More information

LOFAR Data Products. First LOFAR Data Processing School 10 February Michael Wise

LOFAR Data Products. First LOFAR Data Processing School 10 February Michael Wise LOFAR Data Products First LOFAR Data Processing School 10 February 2009 Michael Wise MAC and Input section Aux. processing section system processing Input section Aux. processing section system processing

More information

How to SPAM the 150 MHz sky

How to SPAM the 150 MHz sky How to SPAM the 150 MHz sky Huib Intema Leiden Observatory 26/04/2016 Main collaborators: Preshanth Jagannathan (UCT/NRAO) Kunal Mooley (Oxford) Dale Frail (NRAO) Talk outline The need for a low-frequency

More information

Radio Interferometers Around the World. Amy J. Mioduszewski (NRAO)

Radio Interferometers Around the World. Amy J. Mioduszewski (NRAO) Radio Interferometers Around the World Amy J. Mioduszewski (NRAO) A somewhat biased view of current interferometers Limited to telescopes that exist or are in the process of being built (i.e., I am not

More information

Il progetto SKA: misure di campo elettromagnetico mediante UAV

Il progetto SKA: misure di campo elettromagnetico mediante UAV Applied Electromagnetics and Electronic Devices group Il progetto SKA: misure di campo elettromagnetico mediante UAV in collaboration with POLITECNICO DI TORINO Environment, Land and Infrastructures Department

More information

Towards SKA Multi-beam concepts and technology

Towards SKA Multi-beam concepts and technology Towards SKA Multi-beam concepts and technology SKA meeting Meudon Observatory, 16 June 2009 Philippe Picard Station de Radioastronomie de Nançay philippe.picard@obs-nancay.fr 1 Square Kilometre Array:

More information

Phased Array Feeds for the SKA. WP2.2.3 PAFSKA Consortium CSIRO ASTRON DRAO NRAO BYU OdP Nancay Cornell U Manchester

Phased Array Feeds for the SKA. WP2.2.3 PAFSKA Consortium CSIRO ASTRON DRAO NRAO BYU OdP Nancay Cornell U Manchester Phased Array Feeds for the SKA WP2.2.3 PAFSKA Consortium CSIRO ASTRON DRAO NRAO BYU OdP Nancay Cornell U Manchester Dish Array Hierarchy Dish Array L5 Elements PAF Dish Single Pixel Feeds L4 Sub systems

More information

The LOFAR Telescope: System Architecture and Signal Processing

The LOFAR Telescope: System Architecture and Signal Processing The LOFAR Telescope: System Architecture and Signal Processing M. de Vos, A.W. Gunst, R. Nijboer ASTRON, P.O Box 2, 7990 AA Dwingeloo, The Netherlands Abstract The Low Frequency Array (LOFAR) is a large

More information

2-PAD: An Introduction. The 2-PAD Team

2-PAD: An Introduction. The 2-PAD Team 2-PAD: An Introduction The 2-PAD Team Workshop, Jodrell Bank, 10 Presented th November 2009 by 2-PAD: Dr An Georgina Introduction Harris Georgina Harris for the 2-PAD Team 1 2-PAD Objectives Demonstrate

More information

TROPOSPHERIC CHARACTERISATION OF SKA SITES

TROPOSPHERIC CHARACTERISATION OF SKA SITES TROPOSPHERIC CHARACTERISATION OF SKA SITES Document number... WP3 040.020.000 R 001 Revision... 2 Author... R.P. Millenaar Date... 2011 02 09 Status... Approved for release Name Designation Affiliation

More information

Pulsar Observation with the Effelsberg LOFAR station (Stand alone mode)

Pulsar Observation with the Effelsberg LOFAR station (Stand alone mode) Pulsar Observation with the Effelsberg LOFAR station (Stand alone mode) + some results with Superterp Masaya Kuniyoshi (MPIfR) (MKSP and Pulsar working Group) On behalf of LOFAR collaboration Outline Difference

More information

The Australian SKA Pathfinder Project. ASKAP Digital Signal Processing Systems System Description & Overview of Industry Opportunities

The Australian SKA Pathfinder Project. ASKAP Digital Signal Processing Systems System Description & Overview of Industry Opportunities The Australian SKA Pathfinder Project ASKAP Digital Signal Processing Systems System Description & Overview of Industry Opportunities This paper describes the delivery of the digital signal processing

More information

Overview of the SKA. P. Dewdney International SKA Project Engineer Nov 9, 2009

Overview of the SKA. P. Dewdney International SKA Project Engineer Nov 9, 2009 Overview of the SKA P. Dewdney International SKA Project Engineer Nov 9, 2009 Outline* 1. SKA Science Drivers. 2. The SKA System. 3. SKA technologies. 4. Trade-off space. 5. Scaling. 6. Data Rates & Data

More information

NRC Herzberg Astronomy & Astrophysics

NRC Herzberg Astronomy & Astrophysics NRC Herzberg Astronomy & Astrophysics SKA Pre-Construction Update Séverin Gaudet, Canadian Astronomy Data Centre David Loop, Director Astronomy Technology June 2016 update SKA Pre-Construction NRC Involvement

More information

Cosmic Rays with LOFAR

Cosmic Rays with LOFAR Cosmic Rays with LOFAR Andreas Horneffer for the LOFAR-CR Team Cosmic Rays High energy particles Dominated by hadrons (atomic nuclei) Similar in composition to solar system Broad range in flux and energy

More information

CoDR_SKA-AAVP_AvA SKA_AAVP. Arnold van Ardenne

CoDR_SKA-AAVP_AvA SKA_AAVP. Arnold van Ardenne Agenda Courtesy: Lofar & SKADS/AAVP teams SKA AA System Design (Early R&D 1995-2004) 2005-20122012 SKADS - EC funded SKA design Study 2005-2009 EC FP6 funding 2005-20092009 ( 10.0M) 0M) plus additional

More information

November SKA Low Frequency Aperture Array. Andrew Faulkner

November SKA Low Frequency Aperture Array. Andrew Faulkner SKA Phase 1 Implementation Southern Africa Australia SKA 1 -mid 250 15m dia. Dishes 0.4-3GHz SKA 1 -low 256,000 antennas Aperture Array Stations 50 350/650MHz SKA 1 -survey 90 15m dia. Dishes 0.7-1.7GHz

More information

MANUAL flagging by the data reducing astronomer used to be sufficient for dealing with. The LOFAR RFI pipeline. Chapter 3

MANUAL flagging by the data reducing astronomer used to be sufficient for dealing with. The LOFAR RFI pipeline. Chapter 3 Chapter 3 The LOFAR RFI pipeline Based on: A LOFAR RFI detection pipeline and its first results (Offringa et al., 2010, Proc. of RFI2010) Interference detection results with LOFAR (Offringa and de Bruyn,

More information

PDF hosted at the Radboud Repository of the Radboud University Nijmegen

PDF hosted at the Radboud Repository of the Radboud University Nijmegen PDF hosted at the Radboud Repository of the Radboud University Nijmegen The following full text is a publisher's version. For additional information about this publication click this link. http://hdl.handle.net/2066/173576

More information

ASTRON/LOFAR Reproduction in whole or in part is prohibited without written consent of the 1au

ASTRON/LOFAR Reproduction in whole or in part is prohibited without written consent of the 1au The Data Explosion in Radio-Astronomy Virtual Instruments and E-LOFAR Marco de Vos ASTRON Director of R&D (devos@astron.nl) Drenthe-light Early history and near future Start of radio-astronomy: Grote Reber,

More information

Radio Astronomy Transformed

Radio Astronomy Transformed Radio Astronomy Transformed - Aperture Arrays: Past, Present & Future Prof. Michael Garrett ASTRON, the Netherlands Institute for Radio Astronomy Leiden University. Mike Garrett / NAC 1 Early Antenna Arrays

More information

Recent Results with the UAV-based Array Verification and Calibration System

Recent Results with the UAV-based Array Verification and Calibration System Recent Results with the UAV-based Array Verification and Calibration System Giuseppe Virone POLITECNICO DI TORINO DIATI Framework Research contract between INAF and CNR-IEIIT Title: Power Pattern Measurements

More information

Technologies for Radio Astronomy

Technologies for Radio Astronomy Technologies for Radio Astronomy CSIRO Astronomy and Space Science Alex Dunning in lieu of Tasso Tzioumis Facilities Program Director Technologies June 2017 Directions for ATNF Engineering (Update since

More information

Focal Plane Array Beamformer for the Expanded GMRT: Initial

Focal Plane Array Beamformer for the Expanded GMRT: Initial Focal Plane Array Beamformer for the Expanded GMRT: Initial Implementation on ROACH Kaushal D. Buch Digital Backend Group, Giant Metrewave Radio Telescope, NCRA-TIFR, Pune, India kdbuch@gmrt.ncra.tifr.res.in

More information

March Phased Array Technology. Andrew Faulkner

March Phased Array Technology. Andrew Faulkner Aperture Arrays Michael Kramer Sparse Type of AA selection 1000 Sparse AA-low Sky Brightness Temperature (K) 100 10 T sky A eff Fully sampled AA-mid Becoming sparse Aeff / T sys (m 2 / K) Dense A eff /T

More information

EMBRACE DS5 presentation

EMBRACE DS5 presentation EMBRACE presentation Paris 4 th September 2006 ASTRON, The Netherlands Acknowledgement The authors wish to acknowledge the enormous contribution of the whole EMBRACE team presently located at: ASTRON,

More information

The AAMID consortium: Mid Frequency Aperture Array

The AAMID consortium: Mid Frequency Aperture Array The consortium: Mid Frequency Aperture Array Wim van Cappellen, Consortium Lead Livingstone curves Brought to our attention by Ron Ekers Technological capability leads to discovery in astronomy A single

More information

arxiv: v1 [astro-ph.im] 7 Dec 2010

arxiv: v1 [astro-ph.im] 7 Dec 2010 arxiv:1012.1583v1 [astro-ph.im] 7 Dec 2010 University of Amsterdam (UvA), Amsterdam, The Netherlands E-mail: a.alexov@uva.nl Jason W. T. Hessels Netherlands Institute for Radio Astronomy (ASTRON), Dwingeloo,

More information

THE LOW-FREQUENCY ARRAY (LOFAR) is a new antenna array that observes the sky. The LOFAR radio environment. Chapter 5

THE LOW-FREQUENCY ARRAY (LOFAR) is a new antenna array that observes the sky. The LOFAR radio environment. Chapter 5 Chapter 5 The LOFAR radio environment Based on: The LOFAR radio environment (Offringa et al., in preparation) THE LOW-FREQUENCY ARRAY (LOFAR) is a new antenna array that observes the sky from 1 9 and 11

More information

Published in: 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities

Published in: 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities University of Groningen Towards real-time identification of cosmic rays with LOw-Frequency ARray radio antennas Bonardi, Antonio; Buitink, Stijn; Corstanje, Arthur; Enriquez, J. Emilio; Falcke, Heino;

More information

The LOFAR Known Pulsar Data Pipeline Alexov, A.; Hessels, J.W.T.; Mol, J.D.; Stappers, B.W.; van Leeuwen, A.G.J.

The LOFAR Known Pulsar Data Pipeline Alexov, A.; Hessels, J.W.T.; Mol, J.D.; Stappers, B.W.; van Leeuwen, A.G.J. UvA-DARE (Digital Academic Repository) The LOFAR Known Pulsar Data Pipeline Alexov, A.; Hessels, J.W.T.; Mol, J.D.; Stappers, B.W.; van Leeuwen, A.G.J. Published in: Proceedings of science Link to publication

More information

LOFAR DATA SCHOOL 2016

LOFAR DATA SCHOOL 2016 LOFAR DATA SCHOOL 2016 Tied Array Imaging (II), with contributions from: RRL group Scintillation (R. Fallows) Pulsar Working Group Radio Observatory Outline Tools Calibration (Cyg A imaging) Beams Scientific

More information

PDF hosted at the Radboud Repository of the Radboud University Nijmegen

PDF hosted at the Radboud Repository of the Radboud University Nijmegen PDF hosted at the Radboud Repository of the Radboud University Nijmegen The following full text is a preprint version which may differ from the publisher's version. For additional information about this

More information

Detection of Radio Pulses from Air Showers with LOPES

Detection of Radio Pulses from Air Showers with LOPES Detection of Radio Pulses from Air Showers with LOPES Andreas Horneffer for the LOPES Collaboration Radboud University Nijmegen Radio Emission from Air Showers air showers are known since 1965 to emit

More information

THE KAROO ARRAY TELESCOPE (KAT) & FPA EFFORT IN SOUTH AFRICA

THE KAROO ARRAY TELESCOPE (KAT) & FPA EFFORT IN SOUTH AFRICA THE KAROO ARRAY TELESCOPE (KAT) & FPA EFFORT IN SOUTH AFRICA Dr. Dirk Baker (KAT FPA Sub-system Manager) Prof. Justin Jonas (SKA SA Project Scientist) Ms. Anita Loots (KAT Project Manager) Mr. David de

More information

Investigating diffuse radio emission with LOFAR: The complex merging galaxy cluster Abell 2069

Investigating diffuse radio emission with LOFAR: The complex merging galaxy cluster Abell 2069 Investigating diffuse radio emission with LOFAR: The complex merging galaxy cluster Abell 2069 Alexander Drabent (Thüringer Landessternwarte Tautenburg) Matthias Hoeft, Annalisa Bonafede, Roberto F. Pizzo,

More information

Green Bank Instrumentation circa 2030

Green Bank Instrumentation circa 2030 Green Bank Instrumentation circa 2030 Dan Werthimer and 800 CASPER Collaborators http://casper.berkeley.edu Upcoming Nobel Prizes with Radio Instrumentation Gravitational Wave Detection (pulsar timing)

More information

The EISCAT_3D Preparatory Phase Project

The EISCAT_3D Preparatory Phase Project The EISCAT_3D Preparatory Phase Project Ian McCrea STFC Rutherford Appleton Laboratory Chilton, Oxfordshire, UK ian.mccrea@stfc.ac.uk On behalf of the EISCAT_3D Project Consortium EISCAT: 5-10 years from

More information

Pulsar polarimetry. with. Charlotte Sobey. Dr. Aris Noutsos & Prof. Michael Kramer

Pulsar polarimetry. with. Charlotte Sobey. Dr. Aris Noutsos & Prof. Michael Kramer Pulsar polarimetry with Dr. Aris Noutsos & Prof. Michael Kramer Outline Introduction Observations Ionosphere Outline Pulsars as objects Pulsars as probes of the ISM Faraday rotation using RM synthesis

More information

SKA1 low Baseline Design: Lowest Frequency Aspects & EoR Science

SKA1 low Baseline Design: Lowest Frequency Aspects & EoR Science SKA1 low Baseline Design: Lowest Frequency Aspects & EoR Science 1 st science Assessment WS, Jodrell Bank P. Dewdney Mar 27, 2013 Intent of the Baseline Design Basic architecture: 3-telescope, 2-system

More information

SOFTWARE AND COMPUTING CONCEPT DESIGN REVIEW PLAN

SOFTWARE AND COMPUTING CONCEPT DESIGN REVIEW PLAN SOFTWARE AND COMPUTING CONCEPT DESIGN REVIEW PLAN Document number... WP2-050.020.010-PLA-001 Revision... I Author... D. Hall Date... 2012-01-27 Status... Approved for Release Name Designation Affiliation

More information

ASKAP Industry technical briefing. Tim Cornwell, ASKAP Computing Project Lead Australian Square Kilometre Array Pathfinder

ASKAP Industry technical briefing. Tim Cornwell, ASKAP Computing Project Lead Australian Square Kilometre Array Pathfinder ! ASKAP Industry technical briefing Tim Cornwell, ASKAP Computing Project Lead Australian Square Kilometre Array Pathfinder The Square Kilometre Array 2020 era radio telescope Very large collecting area

More information

The North America Array

The North America Array The North America Array Technology Development and the Realization of the SKA-High Steven T. Myers & Jim Ulvestad NRAO 15 Oct 2009 USSKA Consortium Meeting Pasadena, CA The North America Array is... Technology

More information

Practical Aspects of Focal Plane Array Testing

Practical Aspects of Focal Plane Array Testing Practical Aspects of Focal Plane Array Testing Lessons from an FPA Test-bed at CSIRO, Marsfield Douglas B. Hayman1-3, Trevor S. Bird2,3, Karu P. Esselle3 and Peter J. Hall4 1 2 3 CSIRO Astronomy and Space

More information

Plan for Imaging Algorithm Research and Development

Plan for Imaging Algorithm Research and Development Plan for Imaging Algorithm Research and Development S. Bhatnagar July 05, 2009 Abstract Many scientific deliverables of the next generation radio telescopes require wide-field imaging or high dynamic range

More information

EVLA Science Operations: the Array Science Center. Claire Chandler NRAO/Socorro

EVLA Science Operations: the Array Science Center. Claire Chandler NRAO/Socorro EVLA Science Operations: the Array Science Center Claire Chandler NRAO/Socorro SAGE meeting Socorro, May 22-23, 2007 The need for an Array Science Center 2 The VLA/VLBA currently supply users with raw

More information

SKA-low and the Aperture Array Verification System

SKA-low and the Aperture Array Verification System SKA-low and the Aperture Array Verification System Randall Wayth AADCC Project Scientist On behalf of the Aperture Array Design & Construction Consortium (AADCC) AADCC partners ASTRON (Netherlands) ICRAR/Curtin

More information

Portfolio of Staff Exchange Training at ASTRON 4 (Part 1)

Portfolio of Staff Exchange Training at ASTRON 4 (Part 1) Project Building on Advanced Lofar Technology for Innovation, Collaboration, and Sustainability (Nr. 692257 BALTICS) Portfolio of Staff Exchange Training at ASTRON 4 (Part 1) May, 2018 BALTICS 1 CONTENTS

More information

escience: Pulsar searching on GPUs

escience: Pulsar searching on GPUs escience: Pulsar searching on GPUs Alessio Sclocco Ana Lucia Varbanescu Karel van der Veldt John Romein Joeri van Leeuwen Jason Hessels Rob van Nieuwpoort And many others! Netherlands escience center Science

More information

RF Shielded rooms. Controlled Electromagnetic Environments

RF Shielded rooms. Controlled Electromagnetic Environments RF Shielded rooms Controlled Electromagnetic Environments RF shielded rooms 03 Inner finishing 05 Tempest qualified rooms 05 Radio astronomy applications 06 MRI rooms 07 Controlled Electromagnetic Environments

More information

Correlator Development at Haystack. Roger Cappallo Haystack-NRAO Technical Mtg

Correlator Development at Haystack. Roger Cappallo Haystack-NRAO Technical Mtg Correlator Development at Haystack Roger Cappallo Haystack-NRAO Technical Mtg. 2006.10.26 History of Correlator Development at Haystack ~1973 Mk I 360 Kb/s x 2 stns. 1981 Mk III 112 Mb/s x 4 stns. 1986

More information

SKA Site Characterisation and Array Configuration; Overview and Status WP Rob Millenaar, SPDO

SKA Site Characterisation and Array Configuration; Overview and Status WP Rob Millenaar, SPDO SKA Site Characterisation and Array Configuration; Overview and Status WP2 2011 Rob Millenaar, SPDO Site Characterisation 1. Intro SKA Site Characterisation/Selection 2. Request for Information 1. In situ

More information

Status of Design Planning for Construction

Status of Design Planning for Construction Status of Design Planning for Construction Alistair McPherson 18 May 2016 International Design Teams Project Management and System Engineering based at Jodrell Bank, Manchester, UK ~500 scientists & engineers

More information

SURFACE MOVEMENT RADAR

SURFACE MOVEMENT RADAR SMR_AF.fh11 24/2/09 15:45 P gina 1 C M Y CM MY CY CMY K Supplying ATM systems around the world for more than 30 years Friendly user interface to manage all configuration parameters indracompany.com Able

More information

Evolution of the Capabilities of the ALMA Array

Evolution of the Capabilities of the ALMA Array Evolution of the Capabilities of the ALMA Array This note provides an outline of how we plan to build up the scientific capabilities of the array from the start of Early Science through to Full Operations.

More information

CERN-EC SUPPORT FOR SESAME MAGNETS

CERN-EC SUPPORT FOR SESAME MAGNETS 1. PUBLISHABLE SUMMARY CERN-EC SUPPORT FOR SESAME MAGNETS WP1 Project Management and Technical Coordination A complex preparation involving several CERN offices (Director-General, Legal service, Procurement

More information

Active Impedance Matched Dual-Polarization Phased Array Feed for the GBT

Active Impedance Matched Dual-Polarization Phased Array Feed for the GBT Active Impedance Matched Dual-Polarization Phased Array Feed for the GBT Karl F. Warnick, David Carter, Taylor Webb, Brian D. Jeffs Department of Electrical and Computer Engineering Brigham Young University,

More information

Software Correlators for Dish and Sparse Aperture Arrays of the SKA Phase I

Software Correlators for Dish and Sparse Aperture Arrays of the SKA Phase I Software Correlators for Dsh and Sparse Aperture Arrays of the SKA Phase I Jongsoo Km Korea Astronomy and Space Scence Insttute Collaborators: Paul Alexander (Unv. of Cambrdge) Andrew Faulkner (Unv. of

More information

LWA Station Design. S. Ellingson, Virginia Tech N. Kassim, U.S. Naval Research Laboratory. URSI General Assembly Chicago Aug 11, 2008 JPL

LWA Station Design. S. Ellingson, Virginia Tech N. Kassim, U.S. Naval Research Laboratory. URSI General Assembly Chicago Aug 11, 2008 JPL LWA Station Design S. Ellingson, Virginia Tech N. Kassim, U.S. Naval Research Laboratory URSI General Assembly Chicago Aug 11, 2008 JPL Long Wavelength Array (LWA) An LWA Station State of New Mexico, USA

More information

Integration of ETCS in the Danish fleet

Integration of ETCS in the Danish fleet Integration of ETCS in the Danish fleet Agenda: o Signalling Programme overview o Scope of the onboard project o Survey process o Fitment process o Main challenges o Lessons learned 2015 Signalling programme

More information

Calibratability and its impact on configuration design for the LOFAR and SKA phased array radio telescopes

Calibratability and its impact on configuration design for the LOFAR and SKA phased array radio telescopes RADIO SCIENCE, VOL. 46,, doi:10.1029/2011rs004733, 2011 Calibratability and its impact on configuration design for the LOFAR and SKA phased array radio telescopes S. J. Wijnholds, 1 J. D. Bregman, 1 and

More information

Time-Frequency System Builds and Timing Strategy Research of VHF Band Antenna Array

Time-Frequency System Builds and Timing Strategy Research of VHF Band Antenna Array Journal of Computer and Communications, 2016, 4, 116-125 Published Online March 2016 in SciRes. http://www.scirp.org/journal/jcc http://dx.doi.org/10.4236/jcc.2016.43018 Time-Frequency System Builds and

More information

A report on KAT7 and MeerKAT status and plans

A report on KAT7 and MeerKAT status and plans A report on KAT7 and MeerKAT status and plans SKA SA, Cape Town Office 3rd Floor, The Park, Park Road, Pinelands, Cape Town, South Africa E mail: tony@hartrao.ac.za This is a short memo on the current

More information

Applying full polarization A-Projection to very-wide fields of view instruments: An imager for LOFAR Cyril Tasse

Applying full polarization A-Projection to very-wide fields of view instruments: An imager for LOFAR Cyril Tasse Applying full polarization A-Projection to very-wide fields of view instruments: An imager for LOFAR Cyril Tasse ASTRON/Leiden: Joris van Zwieten, Bas van der Tol, Ger van Diepen NRAO: Sanjay Bhatnagar

More information

A Multi-Fielding SKA Covering the Range 100 MHz 22 GHz. Peter Hall and Aaron Chippendale, CSIRO ATNF 24 November 2003

A Multi-Fielding SKA Covering the Range 100 MHz 22 GHz. Peter Hall and Aaron Chippendale, CSIRO ATNF 24 November 2003 A Multi-Fielding SKA Covering the Range 100 MHz 22 GHz Peter Hall and Aaron Chippendale, CSIRO ATNF 24 November 2003 1. Background Various analyses, including the recent IEMT report [1], have noted that

More information

European Wind Energy Technology Roadmap

European Wind Energy Technology Roadmap European Wind Energy Technology Roadmap Making Wind the most competitive energy source 1 TPWind The European Wind Energy Technology Platform Key data: Official Technology Platform Launched in 2007 150

More information

Software Spectrometer for an ASTE Multi-beam Receiver. Jongsoo Kim Korea Astronomy and Space Science Institute

Software Spectrometer for an ASTE Multi-beam Receiver. Jongsoo Kim Korea Astronomy and Space Science Institute Software Spectrometer for an ASTE Multi-beam Receiver Jongsoo Kim Korea Astronomy and Space Science Institute Design Consideration software spectrometer for a near future ASTE multi-beam receiver spectrometer

More information

Beamforming for IPS and Pulsar Observations

Beamforming for IPS and Pulsar Observations Beamforming for IPS and Pulsar Observations Divya Oberoi MIT Haystack Observatory Sunrise at Mileura P. Walsh Function, Inputs and Outputs Function - combine the voltage signal from each of the 512 tiles

More information

Cathodic Protection & Monitoring

Cathodic Protection & Monitoring Cathodic Protection & Monitoring THE COMPLETE SOLUTION MEASUREMENT COMMUNICATION INSIGHT Contents Cathodic Protection Services 2 Consultancy 3 Systems 5 Monitoring 8 Insight 10 1 Aquatec was founded by

More information

Workshop Summary: RFI and its impact on the new generation of HI spectral-line surveys

Workshop Summary: RFI and its impact on the new generation of HI spectral-line surveys Workshop Summary: RFI and its impact on the new generation of HI spectral-line surveys Lisa Harvey-Smith 19 th June 2013 ASTRONONY & SPACE SCIENCE Workshop Rationale How will RFI impact HI spectral line

More information

The SKA New Instrumentation: Aperture Arrays

The SKA New Instrumentation: Aperture Arrays The SKA New Instrumentation: Aperture Arrays A. van Ardenne, A.J. Faulkner, and J.G. bij de Vaate Abstract The radio frequency window of the Square Kilometre Array is planned to cover the wavelength regime

More information

May AA Communications. Portugal

May AA Communications. Portugal SKA Top-level description A large radio telescope for transformational science Up to 1 million m 2 collecting area Operating from 70 MHz to 10 GHz (4m-3cm) Two or more detector technologies Connected to

More information

Hans van der Marel Radio Observatory Division, ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands

Hans van der Marel Radio Observatory Division, ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands Radio Observatory Division, ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands E-mail: marel@astron.nl Pieter Donker Radio Observatory Division, ASTRON, Oude Hoogeveensedijk 4, 7991 PD

More information

arxiv: v1 [astro-ph.im] 1 Oct 2012

arxiv: v1 [astro-ph.im] 1 Oct 2012 Astronomy & Astrophysics manuscript no. aa2293-12 c ESO 214 May 3, 214 arxiv:121.393v1 [astro-ph.im] 1 Oct 212 The LOFAR radio environment A. R. Offringa 1,2, A. G. de Bruyn 1,3, S. Zaroubi 1, G. van Diepen

More information

OLFAR Orbiting Low-Frequency Antennas for Radio Astronomy. Mark Bentum

OLFAR Orbiting Low-Frequency Antennas for Radio Astronomy. Mark Bentum Orbiting Low-Frequency Antennas for Radio Astronomy Mark Bentum JENAM, April 22, 2009 Outline Presentation of a new concept for low frequency radio astronomy in space Why low frequencies? Why in space?

More information

Planning (VLA) observations

Planning (VLA) observations Planning () observations 14 th Synthesis Imaging Workshop (May 2014) Loránt Sjouwerman National Radio Astronomy Observatory (Socorro, NM) Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very

More information

EUPHEME. Prof Len Shaffrey, National Centre for Atmospheric Science Department of Meteorology University of Reading, UK

EUPHEME. Prof Len Shaffrey, National Centre for Atmospheric Science Department of Meteorology University of Reading, UK EUPHEME Prof Len Shaffrey, National Centre for Atmospheric Science Department of Meteorology University of Reading, UK EUPHEME EUPHEME is a 3-year 2.5M project funded through the ERA4CS ERA-NET (Coordinator:

More information

Joeri van Leeuwen The dynamic radio sky: Pulsars

Joeri van Leeuwen The dynamic radio sky: Pulsars Joeri van Leeuwen The dynamic radio sky: Pulsars Joeri van Leeuwen The dynamic radio sky: Pulsars Coenen, van Leeuwen et al. 2015 Joeri van Leeuwen The dynamic radio sky: Pulsars Joeri van Leeuwen The

More information

The discrete charms of Redundant Spacing Calibration (RSC) J.E.Noordam. Madroon Community Consultants (MCC)

The discrete charms of Redundant Spacing Calibration (RSC) J.E.Noordam. Madroon Community Consultants (MCC) The discrete charms of Redundant Spacing Calibration (RSC) J.E.Noordam Madroon Community Consultants (MCC) Outline What is RSC? Advantages Limitations The place of RSC in the GST Diagnostic tool Fast first

More information

arxiv: v1 [astro-ph.im] 16 Aug 2016

arxiv: v1 [astro-ph.im] 16 Aug 2016 Separating Nightside Interplanetary and Ionospheric Scintillation with LOFAR arxiv:1608.04504v1 [astro-ph.im] 16 Aug 2016 R.A. Fallows ASTRON - the Netherlands Institute for Radio Astronomy, Postbus 2,

More information

LBA Operations. Cormac Reynolds, Chris Phillips, Phil Edwards + LBA Team 19 November 2015 CSIRO ASTRONOMY & SPACE SCIENCE

LBA Operations. Cormac Reynolds, Chris Phillips, Phil Edwards + LBA Team 19 November 2015 CSIRO ASTRONOMY & SPACE SCIENCE LBA Operations Cormac Reynolds, Chris Phillips, Phil Edwards + LBA Team 19 November 2015 CSIRO ASTRONOMY & SPACE SCIENCE Hartebeesthoek 8000 km Real-time e-vlbi LBA 6 ant 1700km 40 ujy/beam (Ceduna) +Auscope

More information

Etudes d antennes et distribution pour une Super Station LOFAR à Nançay Antenna design and distribution for a LOFAR Super Station in Nançay

Etudes d antennes et distribution pour une Super Station LOFAR à Nançay Antenna design and distribution for a LOFAR Super Station in Nançay LES RADIOTELESCOPES DU FUTUR : TECHNOLOGIES ET AVANCEES SCIENTIFIQUES Etudes d antennes et distribution pour une Super Station LOFAR à Nançay Antenna design and distribution for a LOFAR Super Station in

More information

Update on Optics Design for SKA Reflector Antennas with Wide Band Single Pixel Feeds

Update on Optics Design for SKA Reflector Antennas with Wide Band Single Pixel Feeds Update on Optics Design for SKA Reflector Antennas with Wide Band Single Pixel Feeds William Imbriale (2), Germán Cortés (1), and Lynn Baker (1) (1) NAIC, Cornell University, Ithaca, NY, 14853, USA (2)

More information

5790A/AF AC Measurement Standard

5790A/AF AC Measurement Standard AC Measurement Standard General Description The 5790A/AF is similar to the standard 5790A AC Measurement Standard except for different performance specifications and added accessories as noted below. The

More information

Square Kilometre Array where Science meets Industry

Square Kilometre Array where Science meets Industry Square Kilometre Array where Science meets Industry Nigel Rix, Director of Electronics; ESP KTN Technology Strategy Board The vision of the Technology Strategy Board: UK to be a global leader in innovation

More information

Specifications for the GBT spectrometer

Specifications for the GBT spectrometer GBT memo No. 292 Specifications for the GBT spectrometer Authors: D. Anish Roshi 1, Green Bank Scientific Staff, J. Richard Fisher 2, John Ford 1 Affiliation: 1 NRAO, Green Bank, WV 24944. 2 NRAO, Charlottesville,

More information

Wind Energy Technology Roadmap

Wind Energy Technology Roadmap Wind Energy Technology Roadmap Making Wind the most competitive energy source Nicolas Fichaux, TPWind Secretariat 1 TPWind involvement in SET-Plan process SRA / MDS Programme Report / Communication Hearings

More information