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

Size: px
Start display at page:

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

Transcription

1 LOFAR Status Update Imaging Busy Week 5 Kickoff Meeting 25 January 2010 Michael Wise* *On behalf of the LOFAR collaboration 1

2 2

3 Current Rollout Status Station/Item Cabinet LBA HBA Fibre CEP connection Validated CS302 RS307 RS503 RS106 RS208 CS030 CS401 CS021 CS032 RS306 CS301 CS501 RS509 CS103 CS001 CS002 2 L nok CS003 2 H nok CS004 CS005 ~8 H nok CS006 CS007 CS024 CS201 CS101 CS026 RS205 CS017 RS104 RS210 RS310 RS404 RS406 RS407 RS409 RS410 RS508 Effelsberg Tautenburg Garching Potsdam G Juelich V Nancay? Onsala J Chilbolton E Totals r l R H H LBA HBA CEP OBS 3

4 Standard Imaging Pipeline Current Status All core components in place Basic data-taking working Running on new cluster Automated execution Next Steps Readiness for MSSS Robustness, performance, etc. Limited functionality upgrades Testing, testing, testing... 4

5 Progress in 2009 Integration of DPPP, BBS, Imager, Source Finding and GSM into a pipeline Distributed processing using VDS files DPPP Flagger algorithms, data compression BBS Global Solver, solution based flagging, spectral index, Gaussian sources, initial ionospheric model, initial station beam model Imager MWImager script for CImager and CASA Imager Initial facet based correction Initial performance measurements Documentation: wiki, cookbook Automated builds Testing, commissioning, improving, testing, commissioning, improving, testing, commissioning, improving, 5

6 Recent Imaging Results 3C196 field LOFAR (30 75 MHz) (courtesy J. McKean) 6

7 Recent Imaging Results Cygnus MHz 11 (out of 14) station residual image; 1 subband; 6 hours (courtesy R. van Weeren) 7

8 Recent Imaging Results (courtesy B. Scheers, N. Mohan, J. Swinbank) ASTRON 8 Imaging BW 5 Kickoff, 25 Jan 2010

9 Readiness Checklist Preparation Stations SAS / MAC OLAP SIP SIP - DPPP SIP - BBS SIP - Imager SIP - Source Finding SIP - Sky Models SIP - General CEP processing Archive Support tasks Developer Commissioner Status MSSS Observation proposal Nijboer, de Bruyn, Survey KSP draft MSSS scheduling Survey KSP, Observatory needed Flux scale Brentjens, Bout in progress Finalized station beam models Beam Team in progress 20 validated stations roll out team in progress HBA ring splitter implemented multi beam observations ready HBA station taper needed Station Calibration LBA Wijnholds working Station Calibration HBA Parisa Noorishad in progress single beam observations Overeem Brentjens implemented multi beam observations Overeem Brentjens implemented writing to new storage facilities Broekema / Mol ready multi beam observations Mol in progress queue scheduling de Jong in progress rapid switching Romein in progress parallel incoherent beam mode Pulsar group in progress Table based corrections? possibly needed Flagger Renting / Van Diepen / Offringa Rafferty in progress Clock phase correction De Gasperin / Van der Tol de Bruyn under investigation Bandpass correction Pandey Mohan under investigation A-team subtraction Mohan / Van Weeren? needed Data compression Renting ready Beam model Van Zwieten Brentjens / Yatawatta in progress Ionospheric model Van der Tol Birzan implemented Solution based flagging Van Zwieten Heald / McKean / Pandey implemented Spectral index Van Zwieten Heald / McKean / Pandey implemented Extended sources Van Zwieten Heald / McKean / Pandey implemented phase shifting and averaging Van Zwieten Birzan in progress Application of DD effects Van Diepen / Van Zwieten / Van der Tol Rol / Rafferty in progress Facetting ASKAP / CASA Rol implemented determination uv-plane taper needed implemented Implementation of LSM Swinbank / Scheers Mohan in progress Quality check before GSM update needed Data quality checks needed Pipeline control Swinbank in progress Mosaicing software? in progress data formats USG in progress Header meta data updates needed visualization various in progress profiling Swinbank in progress phase 2 cluster hardware Broekema? needed data ingest procedure Renting in progress observation database Renting in progress search functionality Astrowise in progress hardware procurement Holties needed storage and retrieval Holties needed reprocessing functionality Holties needed test suites Surveys / Rol needed documentation Surveys / Busy Weeks in progress Highlights Flagging comparisons Global bandpass Station beams in BBS Solution-based flagging in BBS DDE in imager being tested Source finding / GSM integrated MAC/SAS connection layer Flux scale Scheduling not started in progress ready for testing ready 9

10 Schedule Busy Weeks Engineering time MSSS Workshops 10

11 LOFAR Users Forum 11

12 The End

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

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

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: Lessons Learnt

LOFAR: Lessons Learnt LOFAR: Lessons Learnt Michiel van Haarlem van Weeren, Bonafede, Ferrari, Orrù, Pizzo, Shulevski, van der Tol, Macario Jason Hessels & Pulsar Team LOFAR 40 stations in NL and 8 stations throughout Europe

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

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 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

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

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

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

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

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 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

Data inspection and editing (Flagging, demixing & averaging)

Data inspection and editing (Flagging, demixing & averaging) Netherlands Institute for Radio Astronomy Data inspection and editing (Flagging, demixing & averaging) Tammo Jan Dijkema LOFAR Data Processing School, 18 September 2018 ASTRON is part of the Netherlands

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

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

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

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

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

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 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

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

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

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

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

Reionization with LOFAR

Reionization with LOFAR Reionization with LOFAR Léon V.E. Koopmans (Kapteyn Astronomical Institute) co-pi LOFAR-EoR-KSP Core team (currently active members) Ger de Bruyn (PI), Saleem Zaroubi, Leon Koopmans, Michiel Brentjens

More information

Wirtinger calibration and spectral deconvolution for the lowfrequency radio surveys

Wirtinger calibration and spectral deconvolution for the lowfrequency radio surveys Wirtinger calibration and spectral deconvolution for the lowfrequency radio surveys Cyril Tasse Observatoire de Paris Rhodes University Algorithms : Oleg Smirnov, Etienne Bonnassieux, Marcellin Atemkeng,

More information

Imaging and Calibration Algorithms for EVLA, e-merlin and ALMA. Robert Laing ESO

Imaging and Calibration Algorithms for EVLA, e-merlin and ALMA. Robert Laing ESO Imaging and Calibration Algorithms for EVLA, e-merlin and ALMA Socorro, April 3 2008 Workshop details Oxford, 2008 Dec 1-3 Sponsored by Radionet and the University of Oxford 56 participants http://astrowiki.physics.ox.ac.uk/cgi-bin/twiki/view/algorithms2008/webhome

More information

arxiv: v1 [astro-ph.im] 19 Nov 2018

arxiv: v1 [astro-ph.im] 19 Nov 2018 Astronomy & Astrophysics manuscript no. LOFARcal c ESO 2018 November 21, 2018 arxiv:1811.07954v1 [astro-ph.im] 19 Nov 2018 Systematic effects in LOFAR data: A unified calibration strategy F. de Gasperin

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

3 rd (and 4 th ) Generation Calibration. Jan Noordam ASTRON Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands. J.E.

3 rd (and 4 th ) Generation Calibration. Jan Noordam ASTRON Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands. J.E. 3 rd (and 4 th ) Generation Calibration Jan Noordam ASTRON Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands - 1 - The structure of this talk Posted title: The Minimum Ionospheric Model. This

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

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

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

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

Task Progress Milestone Summary. Page 1

Task Progress Milestone Summary. Page 1 1 ANTENNA RETROFITS 11/4/08 8/9/10 3 21 antennas retrofitted 4/13/09 4/13/09 4 24 antennas retrofitted 11/5/09 11/5/09 5 Last antenna retrofitted 8/9/10 8/9/10 6 WIDE-BAND RECEIVERS 2/4/08 10/15/12 7 L-Band

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

Recent imaging results with wide-band EVLA data, and lessons learnt so far

Recent imaging results with wide-band EVLA data, and lessons learnt so far Recent imaging results with wide-band EVLA data, and lessons learnt so far Urvashi Rau National Radio Astronomy Observatory (USA) 26 Jul 2011 (1) Introduction : Imaging wideband data (2) Wideband Imaging

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

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

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

VLBI techniques and LOFAR

VLBI techniques and LOFAR GLOW interferometry school VLBI techniques and LOFAR Olaf Wucknitz wucknitz@astro.uni-bonn.de Hamburg, 2 September 2010 VLBI techniques Need for long baselines What defines VLBI? Techniques VLBI science

More information

Introduction to SKA Regional Centres. Séverin Gaudet CADC

Introduction to SKA Regional Centres. Séverin Gaudet CADC Introduction to SKA Regional Centres Séverin Gaudet CADC Outline The need for SKA Regional Centres The SKA Regional Centre Model The SKA Regional Centre Coordination Group Thoughts on a Canadian SRC 2

More information

Observing Modes and Real Time Processing

Observing Modes and Real Time Processing 2010-11-30 Observing with ALMA 1, Observing Modes and Real Time Processing R. Lucas November 30, 2010 Outline 2010-11-30 Observing with ALMA 2, Observing Modes Interferometry Modes Interferometry Calibrations

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

Parameterized Deconvolution for Wide-Band Radio Synthesis Imaging

Parameterized Deconvolution for Wide-Band Radio Synthesis Imaging Parameterized Deconvolution for Wide-Band Radio Synthesis Imaging Urvashi Rao Venkata Ph.D. Thesis Defense Department of Physics, New Mexico Institute of Mining and Technology 17 May 2010 Advisors / Committee

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

Computing IPT. B.E. Glendenning (NRAO) J. Ibsen (JAO) G. Kosugi (NAOJ) G. Raffi (ESO) Computing IPT ALMA Annual External Review October

Computing IPT. B.E. Glendenning (NRAO) J. Ibsen (JAO) G. Kosugi (NAOJ) G. Raffi (ESO) Computing IPT ALMA Annual External Review October Computing IPT B.E. Glendenning (NRAO) J. Ibsen (JAO) G. Kosugi (NAOJ) G. Raffi (ESO) Computing IPT ALMA Annual External Review 25-28 October 2010 1 Outline Overall Status Software Development Organization

More information

What is CASA? Rachel Friesen. North American ALMA Science Center. Victoria BC, January 18, 2011 ALMA Software Tutorial 1

What is CASA? Rachel Friesen. North American ALMA Science Center. Victoria BC, January 18, 2011 ALMA Software Tutorial 1 What is CASA? Rachel Friesen North American ALMA Science Center Victoria BC, January 18, 2011 ALMA Software Tutorial 1 Outline Introduction and Current Status General tools and tasks CASA in use! CASA

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

Recent progress in EVLA-specific algorithms. EVLA Advisory Committee Meeting, March 19-20, S. Bhatnagar and U. Rau

Recent progress in EVLA-specific algorithms. EVLA Advisory Committee Meeting, March 19-20, S. Bhatnagar and U. Rau Recent progress in EVLA-specific algorithms EVLA Advisory Committee Meeting, March 19-20, 2009 S. Bhatnagar and U. Rau Imaging issues Full beam, full bandwidth, full Stokes noise limited imaging Algorithmic

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

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

Radio Frequency Monitoring for Radio Astronomy

Radio Frequency Monitoring for Radio Astronomy Radio Frequency Monitoring for Radio Astronomy Purpose, Methods and Formats Albert-Jan Boonstra IUCAF RFI-Mitigation Workshop Bonn, March 28-30, 2001 Contents Monitoring goals in radio astronomy Operational

More information

ASKAP commissioning. Presentation to ATUC. CSIRO Astronomy & Space Science Dave McConnell ASKAP Commissioning & Early Science 14 November 2016

ASKAP commissioning. Presentation to ATUC. CSIRO Astronomy & Space Science Dave McConnell ASKAP Commissioning & Early Science 14 November 2016 ASKAP commissioning Presentation to ATUC CSIRO Astronomy & Space Science Dave McConnell ASKAP Commissioning & Early Science 14 November 2016 PAF assembly line, Marsfield ASKAP is complicated 36 antennas

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

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

arxiv: v1 [astro-ph.im] 6 Nov 2013

arxiv: v1 [astro-ph.im] 6 Nov 2013 Astronomy & Astrophysics manuscript no. Detecting_cosmic_rays_with_the_LOFAR_radio_telescope c ESO 23 November 7, 23 arxiv:3.399v [astro-ph.im] 6 Nov 23 Detecting cosmic rays with the LOFAR radio telescope

More information

Wide Bandwidth Imaging

Wide Bandwidth Imaging Wide Bandwidth Imaging 14th NRAO Synthesis Imaging Workshop 13 20 May, 2014, Socorro, NM Urvashi Rau National Radio Astronomy Observatory 1 Why do we need wide bandwidths? Broad-band receivers => Increased

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

DiFX Correlator at Bonn

DiFX Correlator at Bonn DiFX Correlator at Bonn 1 Alessandra Bertarini, IGG University of Bonn & MPIfR Bonn Walter Alef, MPIfR Bonn Arno Müskens, IGG University of Bonn Helge Rottmann, MPIfR Bonn Jan Wagner, MPIfR Bonn DiFX DiFX

More information

Components of Imaging at Low Frequencies: Status & Challenges

Components of Imaging at Low Frequencies: Status & Challenges Components of Imaging at Low Frequencies: Status & Challenges Dec. 12th 2013 S. Bhatnagar NRAO Collaborators: T.J. Cornwell, R. Nityananda, K. Golap, U. Rau J. Uson, R. Perley, F. Owen Telescope sensitivity

More information

Understanding and calibrating ionospheric effects. Dr Natasha Hurley-Walker Curtin University / ICRAR

Understanding and calibrating ionospheric effects. Dr Natasha Hurley-Walker Curtin University / ICRAR Understanding and calibrating ionospheric effects Dr Natasha HurleyWalker Curtin University / ICRAR Ionosphere Multiple layers during the day Transitions to fewer at night Smallscale turbulence Largescale

More information

Signal Processing on GPUs for Radio Telescopes

Signal Processing on GPUs for Radio Telescopes Signal Processing on GPUs for Radio Telescopes John W. Romein Netherlands Institute for Radio Astronomy (ASTRON) Dwingeloo, the Netherlands 1 Overview radio telescopes motivation processing pipelines signal-processing

More information

A model for the SKA. Melvyn Wright. Radio Astronomy laboratory, University of California, Berkeley, CA, ABSTRACT

A model for the SKA. Melvyn Wright. Radio Astronomy laboratory, University of California, Berkeley, CA, ABSTRACT SKA memo 16. 21 March 2002 A model for the SKA Melvyn Wright Radio Astronomy laboratory, University of California, Berkeley, CA, 94720 ABSTRACT This memo reviews the strawman design for the SKA telescope.

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

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

The processing system for the reduction of the INAF LBT imaging data. Authors: Diego Paris, Stefano Gallozzi and Vincenzo Testa

The processing system for the reduction of the INAF LBT imaging data. Authors: Diego Paris, Stefano Gallozzi and Vincenzo Testa The processing system for the reduction of the INAF LBT imaging data. Authors: Diego Paris, Stefano Gallozzi and Vincenzo Testa The LBT Italian Data Life Cycle Call Callfor for Proposals Proposals (t.a.c.)

More information

An FPGA-Based Back End for Real Time, Multi-Beam Transient Searches Over a Wide Dispersion Measure Range

An FPGA-Based Back End for Real Time, Multi-Beam Transient Searches Over a Wide Dispersion Measure Range An FPGA-Based Back End for Real Time, Multi-Beam Transient Searches Over a Wide Dispersion Measure Range Larry D'Addario 1, Nathan Clarke 2, Robert Navarro 1, and Joseph Trinh 1 1 Jet Propulsion Laboratory,

More information

Calibration. (in Radio Astronomy) Ishwara Chandra CH NCRA-TIFR. Acknowledgments:

Calibration. (in Radio Astronomy) Ishwara Chandra CH NCRA-TIFR. Acknowledgments: Calibration (in Radio Astronomy) Ishwara Chandra CH NCRA-TIFR Acknowledgments: Synthesis Imaging in Radio Astronomy II: Chapter 5 Low Frequency Radio Astronomy (blue book): Chapter 5 Calibration and Advanced

More information

Wide-Band Imaging. Outline : CASS Radio Astronomy School Sept 2012 Narrabri, NSW, Australia. - What is wideband imaging?

Wide-Band Imaging. Outline : CASS Radio Astronomy School Sept 2012 Narrabri, NSW, Australia. - What is wideband imaging? Wide-Band Imaging 24-28 Sept 2012 Narrabri, NSW, Australia Outline : - What is wideband imaging? - Two Algorithms Urvashi Rau - Many Examples National Radio Astronomy Observatory Socorro, NM, USA 1/32

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 LOFAR Sensor Network. and New Scientific Use of Old Spectrum

The LOFAR Sensor Network. and New Scientific Use of Old Spectrum The LOFAR Sensor Network and New Scientific Use of Old Spectrum Willem A. Baan Netherlands Foundation for Research in Astronomy, ASTRON baan@astron.nl Drive towards higher sensitivity in RA Increase BW

More information

Astronomy. Astrophysics. Real-time calibration of the AARTFAAC array for transient detection

Astronomy. Astrophysics. Real-time calibration of the AARTFAAC array for transient detection A&A 568, A48 (04) DOI: 0.05/0004-636/043668 c ESO 04 Astronomy & Astrophysics Real-time calibration of the AARTFAAC array for transient detection P. Prasad,, S. J. Wijnholds, F. Huizinga, and R. A. M.

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

Archive data weblog and QA2 report. Obtaining information of the observation and calibration of ALMA Archive data

Archive data weblog and QA2 report. Obtaining information of the observation and calibration of ALMA Archive data Archive data weblog and QA2 report Obtaining information of the observation and calibration of ALMA Archive data Purpose of ALMA weblog/qa2 report Information about the observation: weather, antenna configuration,

More information

arxiv: v1 [astro-ph.im] 25 Mar 2013

arxiv: v1 [astro-ph.im] 25 Mar 2013 Astronomy & Astrophysics manuscript no. ionrm LOFAR ESO 2018 October 31, 2018 arxiv:1303.6230v1 [astro-ph.im] 25 Mar 2013 Calibrating High-Precision Faraday Rotation Measurements for LOFAR and the Next

More information

How small can you get? reducing data volume, retaining good imaging

How small can you get? reducing data volume, retaining good imaging How small can you get? reducing data volume, retaining good imaging Anita Richards UK ALMA Regional Centre Jodrell Bank Centre for Astrophysics University of Manchester thanks to Crystal Brogan and all

More information

Special Topics: AIPS. 24 February 2012 Socorro, NM USA. Eric Greisen. Robert C. Byrd Green Bank Telescope

Special Topics: AIPS. 24 February 2012 Socorro, NM USA. Eric Greisen. Robert C. Byrd Green Bank Telescope Special Topics: AIPS 4 February 01 Socorro, NM USA Eric Greisen Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Outline

More information

Focal Plane Arrays & SKA

Focal Plane Arrays & SKA Focal Plane Arrays & SKA Peter Hall SKA International Project Engineer www.skatelescope.org Dwingeloo, June 20 2005 Outline Today: SKA and antennas Phased arrays and SKA Hybrid SKA possibilities» A hybrid

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

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

Recent progress and future development of Nobeyama 45-m Telescope

Recent progress and future development of Nobeyama 45-m Telescope Recent progress and future development of Nobeyama 45-m Telescope Masao Saito: Director of Nobeyama Radio Observatory Tetsuhiro Minamidani: Nobeyama Radio Observatory Outline Nobeyama 45-m Telescope Recent

More information

SPES Control System. M. Bellato

SPES Control System. M. Bellato SPES Control System M. Bellato Topics Update on LLRF Update on CB controls Update on network infrastructure Update on Software infrastructure Update on Software developments Topics Update on LLRF Update

More information

Fourier Transforms in Radio Astronomy

Fourier Transforms in Radio Astronomy Fourier Transforms in Radio Astronomy Kavilan Moodley, UKZN Slides taken from N Gupta s lectures: SKA School 2013 van-cittert Zernike theorem Extended, quasi-monochromatic, incoherent source X (l,m) Y

More information

Update on SPIRE Photometer Pipeline

Update on SPIRE Photometer Pipeline Update on SPIRE Photometer Pipeline Kevin Xu NHSC/IPAC on behalf of the SPIRE ICC page 1 What s New in HIPE 9.1 Improved map-making, with destriper in standard processing Electrical crosstalk correction

More information

ARRAY DESIGN AND SIMULATIONS

ARRAY DESIGN AND SIMULATIONS ARRAY DESIGN AND SIMULATIONS Craig Walker NRAO Based in part on 2008 lecture by Aaron Cohen TALK OUTLINE STEPS TO DESIGN AN ARRAY Clarify the science case Determine the technical requirements for the key

More information

System design and wide-field imaging aspects of synthesis arrays with phased array stations Bregman, Jacob Dirk

System design and wide-field imaging aspects of synthesis arrays with phased array stations Bregman, Jacob Dirk University of Groningen System design and wide-field imaging aspects of synthesis arrays with phased array stations Bregman, Jacob Dirk IMPORTANT NOTE: You are advised to consult the publisher's version

More information

CALIM and SP(D)O. the role of the domain experts. Jan Noordam CALIM 2011, Manchester (UK)

CALIM and SP(D)O. the role of the domain experts. Jan Noordam CALIM 2011, Manchester (UK) CALIM and SP(D)O the role of the domain experts Jan Noordam noordam@astron.nl A slight change of plan I was going to repeat a talk I recently gave at Zadar About lowering some threshold That talk is attached,

More information

Beam-formed Data with LOFAR. Richard Fallows, ASTRON

Beam-formed Data with LOFAR. Richard Fallows, ASTRON Beam-formed Data with LOFAR Richard Fallows, ASTRON Beam-formed Data Main Uses Pulsars already covered Single-station science Dynamic spectra: Solar radio bursts Planetary emission Scintillation Imaging

More information

EVLA and LWA Imaging Challenges

EVLA and LWA Imaging Challenges EVLA and LWA Imaging Challenges Steven T. Myers IGPP, Los Alamos National Laboratory and National Radio Astronomy Observatory, Socorro, NM 1 EVLA key issues 2 Key algorithmic issues ambitious goals / hard

More information

THE VLA LOW-FREQUENCY SKY SURVEY

THE VLA LOW-FREQUENCY SKY SURVEY The Astronomical Journal, 134:1245 Y 1262, 2007 September # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE VLA LOW-FREQUENCY SKY SURVEY A. S. Cohen, 1 W. M. Lane, 1

More information

RFI Mitigation Project at Italian Radio Telescopes

RFI Mitigation Project at Italian Radio Telescopes Workshop Detection and measurement of RFI in radio astronomy Yebes Observatory (IGN, Spain), June 8-9, 2017 RFI Mitigation Project at Italian Radio Telescopes G. Serra and many other people from Italian

More information

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Basics of Interferometry Data Reduction Scott Schnee (NRAO) ALMA Data

More information

Introduction to Imaging in CASA

Introduction to Imaging in CASA Introduction to Imaging in CASA Mark Rawlings, Juergen Ott (NRAO) Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Overview

More information

REDUCTION OF ALMA DATA USING CASA SOFTWARE

REDUCTION OF ALMA DATA USING CASA SOFTWARE REDUCTION OF ALMA DATA USING CASA SOFTWARE Student: Nguyen Tran Hoang Supervisor: Pham Tuan Anh Hanoi, September - 2016 1 CONTENS Introduction Interferometry Scientific Target M100 Calibration Imaging

More information

Error Recognition Emil Lenc (and Arin)

Error Recognition Emil Lenc (and Arin) Error Recognition Emil Lenc (and Arin) University of Sydney / CAASTRO www.caastro.org CASS Radio Astronomy School 2017 Based on lectures given previously by Ron Ekers and Steven Tingay CSIRO; Swinburne

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

Data Quality Monitoring of the CMS Pixel Detector

Data Quality Monitoring of the CMS Pixel Detector Data Quality Monitoring of the CMS Pixel Detector 1 * Purdue University Department of Physics, 525 Northwestern Ave, West Lafayette, IN 47906 USA E-mail: petra.merkel@cern.ch We present the CMS Pixel Data

More information

EDGES. Judd D. Bowman, Arizona State University Alan E. E. Rogers, Haystack Observatory

EDGES. Judd D. Bowman, Arizona State University Alan E. E. Rogers, Haystack Observatory EDGES Judd D. Bowman, Arizona State University Alan E. E. Rogers, Haystack Observatory Kristina Davis, ASU Sarah Easterbrook, ASU Hamdi Mani, ASU Raul Monsalve, ASU Thomas Mozdzen, ASU Outline Instrument

More information