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

Similar documents
LOFAR Long Baseline Calibration Commissioning

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

LOFAR: Lessons Learnt

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

LOFAR Calibration of the Ionosphere and Other Fun Things

LOFAR: Special Issues

Cosmic Rays with LOFAR

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

DiFX Correlator at Bonn

Smart Antennas in Radio Astronomy

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

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

LOFAR: From raw visibilities to calibrated data

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

Dense Aperture Array for SKA

LOFAR update: long baselines and other random topics

Overview of Survey KSP meeting Leiden March 2010

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

Assessment of RFI measurements for LOFAR

November SKA Low Frequency Aperture Array. Andrew Faulkner

Towards SKA Multi-beam concepts and technology

Detection of Radio Pulses from Air Showers with LOPES

How to SPAM the 150 MHz sky

March Phased Array Technology. Andrew Faulkner

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

LWA1 Technical and Observational Information

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

LOFAR DATA SCHOOL 2016

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

System Failure Operational Recovery

LWA Users Meeting Pulsars II: Software and Survey Kevin Stovall

Low-frequency radio observations at Lustbühel Observatory M. Panchenko(1), H.O. Rucker(2)

The AAMID consortium: Mid Frequency Aperture Array

Beam-formed Data with LOFAR. Richard Fallows, ASTRON

Practical Radio Interferometry VLBI. Olaf Wucknitz. Bonn, 21 November 2012

EMBRACE DS5 presentation

The LOFAR Telescope: System Architecture and Signal Processing

Casper Instrumentation at Green Bank

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

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

The SKA New Instrumentation: Aperture Arrays

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

Real-time Pulsar Timing signal processing on GPUs

The WVR at Effelsberg. Thomas Krichbaum

CALIBRATION AND IMAGING WITH LOFAR

May AA Communications. Portugal

Focal Plane Array Beamformer for the Expanded GMRT: Initial

Very Long Baseline Interferometry

Practical Radio Interferometry VLBI. Olaf Wucknitz.

Practical Radio Interferometry VLBI. Olaf Wucknitz.

N. Pingel, K. Rajwade, D.J. Pisano, D. Lorimer West Virginia University

Radio Astronomy Transformed

SKA1 low Baseline Design: Lowest Frequency Aspects & EoR Science

Green Bank Instrumentation circa 2030

Why Single Dish? Why Single Dish? Darrel Emerson NRAO Tucson

Why Single Dish? Darrel Emerson NRAO Tucson. NAIC-NRAO School on Single-Dish Radio Astronomy. Green Bank, August 2003.

Introduction to Radio Astronomy. Richard Porcas Max-Planck-Institut fuer Radioastronomie, Bonn

PDF hosted at the Radboud Repository of the Radboud University Nijmegen

Propagation effects (tropospheric and ionospheric phase calibration)

Radioastronomy in Space with Cubesats

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

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

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

Technologies for Radio Astronomy

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

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

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

VLBI DATA Acquisition Terminal modernization at the Deep Space Network

Why Single Dish? Darrel Emerson NRAO Tucson. NAIC-NRAO School on Single-Dish Radio Astronomy. Green Bank, August 2003.

Developments in Expanding the Event Horizon Telescope: Phased ALMA and South Pole Telescope

The CASPER Hardware Platform. Richard Armstrong

MISCELLANEOUS CORRECTIONS TO THE BASELINE DESIGN

NRC Herzberg Astronomy & Astrophysics

Radar astronomy and radioastronomy using the over-the-horizon radar NOSTRADAMUS. ONERA, Département Electromagnétisme et Radar

VLBI techniques and LOFAR

Cross Correlators. Jayce Dowell/Greg Taylor. University of New Mexico Spring Astronomy 423 at UNM Radio Astronomy

MWA Antenna Description as Supplied by Reeve

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

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

Recent progress and future development of Nobeyama 45-m Telescope

PROJECT CHARTER. (DRAFT Version 1.0, 16-AUG-07)

The GMRT: System Parameters and Current Status

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

Radio Frequency Monitoring for Radio Astronomy

Observing Modes and Real Time Processing

Allen Telescope Array & Radio Frequency Interference. Geoffrey C. Bower UC Berkeley

Data inspection and editing (Flagging, demixing & averaging)

A report on KAT7 and MeerKAT status and plans

Memo 149. Increased SKA-Low Science Capability through Extended Frequency Coverage. D. C. Price D. Sinclair J. Hickish M.E. Jones.

Il progetto SKA: misure di campo elettromagnetico mediante UAV

Very Long Baseline Interferometry. Richard Porcas Max-Planck-Institut fuer Radioastronomie, Bonn

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

New Guide to GNSS Base stations

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

Fast Fourier Transform Spectrometer (FFTS) Past, Present and Future

The SKA LOW correlator design challenges

Pulsar Timing Array Requirements for the ngvla Next Generation VLA Memo 42

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

BRAND EVN EVN) Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners

EHE Physics and ARIANNA

Transcription:

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 rubber tie-down straps broken 2 nylon anchor cords broken Significant amounts of styrofoam pellets between tiles (no sign of rodents) JM Anderson 4/16

RFI Problems RFI is preventing ASTRON software from producing RCU calibration tables for Effelsberg RFI source nearly certainly the 100 m Tests on Apr 03rd strange RFI stronger when 100 m drive motors turned off But as expected, RFI lower when 100 m pointed South (blockage by dish) Tests will continue Images by J Köhler 5/16

LBA Growth Hand in photos to get camera to focus properly, not intended for scale demonstration 6/16

Additional Hardware at EF 7/16

Antenna Wind Protection Cement blocks added to LBA filed in 2008 to help prevent wind damage Wooden posts installed at HBA field in 2010 to prevent tiles from moving Only edge tiles were observed to move significantly in strong wind 8/16

Electronics Container Changes Added an insulating roof Added automatic humidifier Reduce air conditioning bill in summer when Solar heating important Hopefully also reduce heating bill in winter when station not in use Extreme low humidity conditions encountered during winters, with many electronic component failures Dug a well for water, automatic filling of basin in container 9/16

Recording Equipment In EF Faraday room lofar1b 10 GE interface > 600 MB/s RAID write speed to record full station beamformed datastream lofar1a, lofar2a, lofar3a, lofar4a 4 separate machines with 1 GE interfaces Oxford type computer for pulsar observations Does not seem capable of raw data recording for full bandwidth lofar4 lofar3 lofar2 lofar1 Original EF recording computers (2007) 1 GE interface, 8x2 TB RAID each Used for raw beamformed/tbb data recording lofarsrv 40 TB storage server, 10 GE interface Transfer from ILT archive, raw data storage James M Anderson 10/16

VLBI Cluster (Bonn) 10 GE link from EF 60 node x 8 core Linux PC cluster Cluster primarily used for VLBI correlation and pulsar computing, but time available for LOFAR 200 TB spinning disk storage for LOFAR Expected to be upgraded in 2013 Old MkIV correlator at Bonn (2008, MPIfR) I could not find a photo of the current cluster 11/16

Ongoing Single Station Developments 12/16

Development Areas To be discussed at the Single Pulsar science (Transients KSP) Beamformed data processing (LuMP) Long baseline correlation All-sky imaging from TBB data with polarization calibration from pulsar beamformed data (Köhler) Spectrometer Mode (Solar KSP, EoR) Timing (LuMP, Kuniyoshi, dspsr software development) Polarization (LuMP, dspsr software, plus beam model software to correct polarization properties) Monitoring Polarization Imaging (Cosmic Magnetism KSP) Station Users Meeting in Nançay Recording and correlation of German stations Will include ability to coherently combine station data for pulsar experiments Transfer of ILT data from archive sites to Bonn Other projects... 13/16

Example: Pulsar Timing at EF First LOFAR timing over significant timerange Limited to bright pulsars by 5 ns problem Left: First verified LOFAR pulsar timing results (J Verbiest) Top Right: Pulsar timing covering 47 day range (J Verbiest) Bottom Right: Confirmation of timing model from higher frequency data (B Stappers) 14/16

Some of the Issues Important to EF 5 ns problem Agreement on scheduling station owner's 10% time and unused ILT time prior to start of ILT science operations Station beamformer calibration Requires new Foundry switch setups for EF and other German stations (Klaas?) New switch with more 10 GE ports to replace existing Foundry switch Should we be providing ASTRON with tables? LOFAR network configuration for sending German station data to EF EF less sensitive than one ear of a Core station Often cannot detect the brightest pulsar in the LOFAR sky because the station sensitivity is so bad Waiting for response from Klaas/Andre? Routine operations and emergency procedures manual... 15/16

The End 16/16