Current GBT Performance

Slides:



Advertisements
Similar presentations
The Green Bank Telescope Antenna Control (collimation and pointing) Richard Prestage Scientist / PTCS System Architect.
Advertisements

April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Richard Prestage GBT Future Instrumentation Workshop, September 2006 The Green Bank Telescope:
7. Radar Meteorology References Battan (1973) Atlas (1989)
First Flights of High-Altitude Imaging Wind and Rain Airborne Profiler (HIWRAP) During GRIP Lihua Li, Matt Mclinden, Martin Perrine, Lin Tian, Steve Guimond/
S-PASS, a new view of the polarized sky Gianni Bernardi SKA SA On behalf of the S-PASS team CMB2013, Okinawa, June th 2013.
W.O. Miller i T i VG 1 Bridge Analysis Objective Objective –Develop model suited to examining effect of low velocity air flow through the isolating air.
May 16, 2015 Sparse Surface Adjustment M. Ruhnke, R. Kümmerle, G. Grisetti, W. Burgard.
3mm amplitude test by Cheng-Jiun Ma. Observation Source : Orion SiO Frequency: GHz 256 channels within 64MHz bandwidth Ant 3 & Ant 4 no Tsys correction.
DVAC CONCEPT DESCRIPTION: OFFSET GREGORIAN DISH — DVAC-1 PRIME FOCUS DISH — DVAC-2 卢雨 (Yu Lu), Vice Joint Lab. for Radio.
Probing the field of Radio Astronomy with the SKA and the Hartebeesthoek Radio Observatory: An Engineer’s perspective Sunelle Otto Hartebeesthoek Radio.
WMAP. The Wilkinson Microwave Anisotropy Probe was designed to measure the CMB. –Launched in 2001 –Ended 2010 Microwave antenna includes five frequency.
Radar Many in a series of McGourty- Rideout Productions.
Günther Haase Tomas Landelius Daniel Michelson Generation of superobservations (WP2)
NAIC Visiting Committee Meeting · February 19-21, 2007 Telescope Performance 2007 Visiting Committee Meeting Phil Perillat.
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Mosaicing Tim Cornwell.
Polarization Surveys with the DRAO 26-m Telescope at 1.4 GHz Maik Wolleben, T. Landecker, O. Davison Dominion Radio Astrophysical Observatory W. Reich,
Tenth Summer Synthesis Imaging Workshop University of New Mexico, June 13-20, 2006 Antennas in Radio Astronomy Peter Napier.
P.Napier, Synthesis Summer School, 18 June Antennas in Radio Astronomy Peter Napier Interferometer block diagram Antenna fundamentals Types of antennas.
NAIC Visiting Committee Meeting February 15-16, 2005 Telescope Performance Pointing the telescope. Gain curves for all receivers Recent high frequency.
Large Binocular Telescope Interferometer LBTI/NOMIC data analysis B. Mennesson, D. Defrère, P. Hinz, B. Hoffmann, O. Absil, B. Danchi, R. Millan-Gabet,
5 Jan 2004, Boulder CO URSI The Current Status of the Green Bank Telescope.
ATCA synthesis workshop - May ATCA – Calibration at mm wavelengths Rick Forster University of California, Berkeley Hat Creek Radio Observatory Berkeley-Illinois-Maryland.
Making MOPRA go! Lucyna Kedziora-Chudczer Friend of the telescope (UNSW)
December 3-4, Green Bank GBT PTCS In Progress Review Laser Rangefinder Update 9/5/03 Experiment K. Constantikes.
The Robert C Byrd Green Bank Telescope Frank Ghigo, National Radio Astronomy Observatory US VLBI Meeting, Socorro, Nov 2011 VLBI usage: About 15% of GBT.
December 3-4, 2003 Green Bank GBT PTCS In Progress Review Future Development Program Kim Constantikes, Richard Prestage.
5 GHz observations of intraday variability in some AGNs  Huagang Song & Xiang Liu  Urumqi Observation, NAOCAS.
Phase Referencing Using More Than One Calibrator Ed Fomalont (NRAO)
RadioAstron space VLBI mission: early results. XXVIII GA IAU, Beijing, August RadioAstron space VLBI mission: early results. XXVIII GA IAU, Beijing,
IOTA/IONIC observations of Vega results and lessons learned Denis Defrère ANR kick-off meeting, IPAG.
Oct 13-15, 2003 ADASS 2003 The GBT Precision Telescope Control System Kim Constantikes.
Observing Strategies at cm wavelengths Making good decisions Jessica Chapman Synthesis Workshop May 2003.
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Overview of the High Frequency Observing System Richard Prestage.
AUSAC Meeting March 2-3, 2005 Telescope Performance Pointing the telescope. Gain curves for all receivers Reflector alignment Recent high frequency results.
SPIE – June 25, The Details….. SPIE – June 25, Previous Focus Tracking Curves.
December 3-4, Green Bank GBT PTCS In Progress Review Thermal Focus and Pointing Corrections K. Constantikes.
20 June 2006 Green Bank GBT Performance Dana S. Balser.
1 1 CORNISH WORKSHOP Leeds, 13 th April 2007 James Green The Methanol Multibeam Project Project MMB.
Update on B-analysis Introduction Towards a definition of a limited set of plots for TDR, using all available data. Based on few general.
January 6, 2005 URSI Nation Radio Science Meeting, Boulder, CO. Pointing and Focusing the GBT K. T. Constantikes NRAO Green Bank.
Fundamentals of the GBT and Single-Dish Radio Telescopes Dr. Ron Maddalena National Radio Astronomy Observatory Green Bank, WV March 2016 ©Associated Universities,
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Richard Prestage, Kim Constantikes, Dana Balser, Jim Condon The GBT Precision Telescope Control.
Information Warfare Technologies Inc. Calibration Techniques for Amplitude DF Systems AOC SYMPOSIUM OCTOBER 2005 Mr. Al Evans President Information Warfare.
DVAC PROGRESS OFFSET GREGORIAN DISH (DVAC-1) 郑元鹏 (Yuanpeng Zheng ) Joint Lab. for Radio Astronomy and Technology MAY 29, 2012.
A potted outline of the EVN data
Cassini Huygens EECS 823 DIVYA CHALLA.
Re-mapping the Residual B-Field in NA62
Antennas in Radio Astronomy
Visit for more Learning Resources
Circular Pointing Scans
Introduction to geodesy & accelerometry with Swarm
Example for a Satellite: Meteosat Second Generation
Monte Carlo Quality Assessment (MC-QA)
Remote Sensing Systems
Observing Strategies for the Compact Array
Introduction to Using Radio Telescopes
Imaging and Calibration Challenges
Institute of Low Temperature Science, Hokkaido University
ESA’s Deep Space Antennas
GBT and other Green Bank Capabilities
The pointing calibration of the WFCTA tracking system
Metrology Improves Pointing at 12m ALMA Telescopes
GBT Status: Current Observing Capabilities
Early indications of performance
Feed & Front End PDR—Sys. Reqts
Problems with the Run4 Preliminary Phi->KK Analysis
The Green Bank Telescope: Overview and Antenna Performance
EM COMPONENTS UPDATE & PERFORMANCE RESULTS
System Specifications Lab Tests
Molecular Imager: Focal Plane Array
Presentation transcript:

Current GBT Performance

Systematic Focus Errors Axial Focus Offset: air temperature versus elevation

Gravitational & Temperature Focus Effects Temperature Effect Gravitational Effect Measure focus over short time period NCP source 0117+8928

Systematic Pointing Errors

Plan of Attack Rationalize data acquisition Rationalize data analysis Implement temperature sensor system Concentrate efforts on pointing and focus Characterize performance with X-band (8 -10 GHz)

Data Quality Gaussian Fits (Az, El, Focus) Polarization (LCP – RCP) Direction (Forward – Backward) Jack Scan

Data Quality: Pointing (LCP – RCP)

Data Quality: Pointing (LCP – RCP) Flux (9 GHz) > 0.08 Jy RMS < 2.5 arcsec < 0.03 HPBW

Data Quality: Focus (LCP – RCP) Flux (9 GHz) > 0.08 Jy RMS < 3.8 mm << focus beamwidth

Data Quality: Pointing (F – B)

Data Quality: Wind

Observational Strategy NCP source to probe temperature effects Up-down sources at night to probe gravity effects All-sky for a combination

All-sky (Az, El) pointing Initial Results All-sky (Az, El) pointing Removed systematic pointing residuals Simultaneous fits to gravity and temperature Separate two effects Refine focus and pointing models

Current Performance Model: Datasets: Metrics Simultaneous solution to temperature and gravity effects Datasets: All-sky pointing run (2003 Nov 20) Half-power tracking (2003 Nov 20) Metrics Blind pointing Offset pointing Continuous Tracking

Blind Pointing: Azimuth

Blind Pointing: Elevation

Blind Focus

Offset Pointing: Azimuth and Elevation

Offset Focus

Tracking: Ku-band (14 GHz) El half-power track

Current Performance: (NO temperature corrections) Benign Conditions: (1) Exclude 10:00  18:00 (2) Wind < 2.5 m/s Blind Pointing: (1 point/focus) Offset Pointing: (90 min) Continuous Tracking: (30 min)

Supplemental Material

Blind Focus

Blind Pointing: residuals versus (A, Z)

Blind Pointing: residuals versus time

Blind Pointing: 2-D RMS Raw Residuals One PEAK at the start of the evening

Blind Pointing: Azimuth

Blind Pointing: Elevation

Blind Focus

Tracking: Ku-band (14 GHz) El half-power track

Tracking: Ku-band (14 GHz) El half-power track