Jeff Mangum (NRAO) Robert Lucas (IRAM) Baltasar Vila Vilaro (NAOJ)

Slides:



Advertisements
Similar presentations
National Radio Astronomy Observatory June 13/14, 2005 EVLA Phase II Proposal Review EVLA Phase II Computing Development Bryan Butler (EVLA System Engineer.
Advertisements

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Solar System Objects.
Twelfth Synthesis Imaging Workshop 2010 June 8-15 Observation Preparation Tool (OPT) Loránt Sjouwerman (NRAO/Socorro)
ALMA: The March to Early Science Al Wootten, ALMA/NA Project Scientist Cometary Radio Astronomy.
CSV Plan status Robert Laing ESO Science IPT. 2 Recent changes Complete rewrite to take account of rebaselining and revised delivery schedule Proposal.
Atmospheric phase correction for ALMA Alison Stirling John Richer Richard Hills University of Cambridge Mark Holdaway NRAO Tucson.
FIR Optics Meeting – January Calibration issues related to the optical performances David Teyssier.
Mopra 115GHz The MAGMA Perspective Annie Hughes & Tony Wong.
Prospects for High-Frequency Calibration with the SMA Dual-IF/Receiver System Todd R. Hunter, Jun-Hui Zhao (CfA) Sheng-Yuan Liu, Yu-Nung Su, Vivien Chen.
Antenna Gain and Source calibration Jim Gibson and Jack Welch.
Current mm interferometers Sébastien Muller Nordic ARC Onsala Space Observatory Sweden Turku Summer School – June 2009.
Prospects for High-Frequency Calibration with the SMA Dual-IF/Receiver System Todd R. Hunter, Jun-Hui Zhao (CfA) Sheng-Yuan Liu, Yu-Nung Su, Vivien Chen.
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Cross Correlators Walter Brisken.
Calibration with CASA Masaaki Hiramatsu 平松正顕 (ASIAA/NTHU) ALMA User Workshop, Feb 8-10, 2010.
ALMA Science Workshop, May 2004 Solar System Science with the ALMA Mark Gurwell Harvard-Smithsonian Center for Astrophysics ALMA Science Workshop, May.
C. ChandlerEVLA Advisory Committee Meeting September 6-7, Scientific Commissioning Plan Claire Chandler.
Hunt for Molecules, Paris, 2005-Sep-20 Software Development for ALMA Robert LUCAS IRAM Grenoble France.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing the Pluto.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Emmanuel Momjian (NRAO)
Mark Bowen Acting Theme Leader – Technologies for Radio Astronomy CSIRO Astronomy and Space Science 14 October 2010 Australia Telescope Users Committee.
Molecular Gas and Dust in SMGs in COSMOS Left panel is the COSMOS field with overlays of single-dish mm surveys. Right panel is a 0.3 sq degree map at.
TelCal Phasing Engine description Draft Robert Lucas
School of something FACULTY OF OTHER School of Physics & Astronomy FACULTY OF MATHEMATICS & PHYSICAL SCIENCES The Cornish Survey Workshop.
Polarization at IRAM Status and Plans S.Guilloteau Laboratoire d’Astrophysique de Bordeaux.
The ALMA TelCal subsystem Dominique Broguière, Institut de RadioAstronomie Millimétrique (IRAM) TelCal Phasing meeting – Grenoble -10/12/2012.
Designing Experiments T. Venturi Istituto di Radioastronomia, Bologna, INAF ERIS, Manchester, 9 September 2005.
N. RadziwillEVLA NSF Mid-Project Report May 11-12, 2006 NRAO End to End (e2e) Operations Division Nicole M. Radziwill.
K. Y. LoEVLA Advisory Committee Meeting September 6-7, 2007 Charge to the Committee K. Y. Lo.
Phase II: Issues Take home points: 1) Is it StandardInterferometry? (better to say No if you don’t know) 2) Note time increases for frequency issues (LO4/Hanning/IF.
Dual frequency interferometry and phase transfer at the Submillimeter Array Todd R. Hunter, Jun-Hui Zhao (CfA) Sheng-Yuan Liu, Yu-Nung Su, Vivien Chen.
Basic Concepts An interferometer measures coherence in the electric field between pairs of points (baselines). Direction to source Because of the geometric.
EVLA Software Bryan Butler. 2007May22EVLA SAGE Meeting2 Requirements and Goals of EVLA Software Maximize scientific throughput of the instrument At a.
Response to ASAC Report of May 2004 Response to ASAC The Atacama Large Millimeter Array Tom Wilson and Al Wootten Science IPT.
Observing Modes from a Software viewpoint Robert Lucas and Philippe Salomé (SSR)
J. Pfingstner Jitter studies February 12, 2014 Optics corrections in the ATF damping ring Jürgen Pfingstner, Yves Renier.
P. NapierEVLA Advisory Committee Meeting September 8-9, EVLA Advisory Committee Project Overview P. Napier, Project Manager Management, Schedule,
Observing Strategies at cm wavelengths Making good decisions Jessica Chapman Synthesis Workshop May 2003.
ALMA Week 2003 Victoria, B. C. Phase Calibration Al Wootten (based on work by many)
The ALMA Phasing Project (APP) APP is an ongoing ALMA Development Project (approved in 2012) to provide the hardware and software necessary to coherently.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing Scripts Basic.
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Overview of the High Frequency Observing System Richard Prestage.
Jan URSI1 Fast Switching Phase Compensation for ALMA Mark Holdaway NRAO/Tucson Other Fast Switching Contributors: Frazer Owen Michael Rupen Chris.
Atmospheric phase correction at the Plateau de Bure interferometer IRAM interferometry school 2006 Aris Karastergiou.
Astrochemistry with the Upgraded Combined Array for Research in Millimeter-wave Astronomy D. N. Friedel Department of Astronomy University of Illinois.
Jeff Kern NRAO/ALMA.  Scaling and Complexity ◦ SKA is not just a bigger version of existing systems  Higher Expectations  End to End Systems  Archive.
Beam Measurement Characterization and Optics Tolerance Analysis of a 900 GHz HEB receiver for the ASTE telescope Alvaro Gonzalez, K. Kaneko, Y. Uzawa.
Observing Strategies for the Compact Array
Computing Architecture
Data Taking Plans for 32T and 128T
EVLA Prototype Correlator (PTC)
Obs2script Bryan Butler.
Calibration of the ACA System
Polarization Calibration
What’s New in HIPE 10.0 (SPIRE FTS)
Max Voronkov Software Scientist – ASKAP 28th September 2010
Observational Astronomy
Observational Astronomy
EVLA Advisory Committee Meeting
Scheduling Toolkit Observation Scheduling Boyd Waters, NRAO
ALMA Calibration Introduction
Early indications of performance
Gustaaf van Moorsel September 9, 2003
Facilitators: Doug Johnstone & Debra Shepherd
Mark McKinnon EVLA Project Manager
EVLA Advisory Committee Meeting, March 19-20, 2009
Atmospheric phase correction for ALMA
EVLA Construction Status
Solar Systems - Near & Far
EVLA Technical Performance
Presentation transcript:

Jeff Mangum (NRAO) Robert Lucas (IRAM) Baltasar Vila Vilaro (NAOJ) ALMA Calibration Plan Jeff Mangum (NRAO) Robert Lucas (IRAM) Baltasar Vila Vilaro (NAOJ) February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA Calibration Development Roadmap February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA ASAC Meeting Florence September 2006 Calibration Examples Atomic-level descriptions of each type of calibration. Derive from science and system requirements and characteristics coupled with experience. Evolve into hardware and software observation sequences which implement each type of calibration. February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA ASAC Meeting Florence September 2006 Calibration Examples Document Author(s) Amplitude and Flux Lucas & Mangum Phase Holdaway Bandpass Lucas Polarization Fomalont, Myers, & Holdaway Pointing Mangum & Lucas Antenna Location Mangum, Fomalont, & Holdaway Antenna and Electronic Delay Optics Vila-Vilaro Primary Beam Mangum & Holdaway ACA Calibration Issues Fomalont & Holdaway Green = Complete; Blue = Reviewed / In Revision; Red = Draft February 24, 2019 ALMA ASAC Meeting Florence September 2006

HW/SW Observation Sequences Method-level descriptions of each type of calibration. Detailed descriptions of how hardware is commanded by software to effect each calibration measurement. February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA ASAC Meeting Florence September 2006 Observing Modes Integration of HW/SW Observation Sequences into scheduling blocks February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA ASAC Meeting Florence September 2006 Calibration Matrix February 24, 2019 ALMA ASAC Meeting Florence September 2006

ALMA ASAC Meeting Florence September 2006 Phase Calibration Target Sequence: Over a period of 15 to 30 seconds the following measurement sequence is observed involving the target and phase calibration source located typically less than or equal to 2 degrees away from the target source: Tune to the calibration frequency if cross-band calibration required. Phase calibrator measurement (tint ≤ 1 second). Tune to the source frequency if cross-band calibration required. Target source measurement (tint ≤ 25 seconds). Instrumental Sequence: This cycle of measurements is required for cross-band calibration of dual-frequency fast switching measurements. Over a period of 10 to 25 seconds a strong phase calibrator source which can be detected at both the target and calibration frequency is used to provide the phase scaling from the target (usually higher) frequency to the calibration (usually 90 GHz) frequency: Tune to calibration frequency. Tune to target frequency. Repeat this sequence. February 24, 2019 ALMA ASAC Meeting Florence September 2006

Phase Calibration Sequence February 24, 2019 ALMA ASAC Meeting Florence September 2006

Absolute Amplitude Calibration Research topic Absolute Amplitude Calibration Focus Group recently formed Bryan Butler (NRAO) Mark Gurwell (SAO) Jack Welch (Berkeley) Charter: Develop list of potential primary and secondary flux calibration sources Planets (Mars, Uranus, etc.) Asteriods Stars (Main Sequence, Giant, Supergiant) Large Ice Bodies (Titan, Galilean Satellites, Triton, etc.) For each candidate define measurements or calculations required to define status as a primary or secondary flux calibrator Initiate measurement program where appropriate (CARMA, SMA, ALMA, etc.) February 24, 2019 ALMA ASAC Meeting Florence September 2006

Calibration and ALMA Operations Operations/Maintenance Calibration Pointing Polarization Antenna Location Antenna and Electronic Delay Optics Primary Beam User Calibration Reference Pointing Amplitude Phase Bandpass Polarization February 24, 2019 ALMA ASAC Meeting Florence September 2006

Calibration and ALMA Operations How does calibration planning get incorporated into ALMA Operations? Example: Pointing Pointing calibrator list development and maintenance Required interval Monitoring requirements for antenna/array vital signs Weather monitoring analysis and requirements Antenna-based behavior and trends February 24, 2019 ALMA ASAC Meeting Florence September 2006