Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA Pipeline.

Slides:

Advertisements

Similar presentations

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

Advertisements

The Very Large Array Past and Future Dave Finley.

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

CSV Plan status Robert Laing ESO Science IPT. 2 Recent changes Complete rewrite to take account of rebaselining and revised delivery schedule Proposal.

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 Observing with ALMA.

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array A Crash Course in CASA.

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

Hunt for Molecules, Paris, 2005-Sep-20 Software Development for ALMA Robert LUCAS IRAM Grenoble France.

1 ANASAC Meeting – May 20, 2015 Al Wootten Science Overview & Publications.

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Emmanuel Momjian (NRAO)

ALMA Operations and the North American ALMA Science Center Al Wootten NRAO.

Workshop in ALMA Logs Prepared by Juan Pablo Gil – Arturo Hoffstadt

1 ANASAC Meeting – May 20, 2015 ALMA Pipeline Brian Glendenning (for Jeff Kern)

The Atacama Large Millimeter Array (ALMA) Test Facility in Retrospect Debra Shepherd National Radio Astronomy Observatory The ALMA Test Facility (ATF)

NAASC Status and NSF Proposal Review & Recommendations Carol Lonsdale Head, North American ALMA Science Center ANASAC Sept 2010.

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

EA ARC Ken Tatematsu East-Asian ARC Manager. ARC organization Difference between ARCS: NA: concentrated in Charlottesville Europe: distributed in different.

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Studies of Star.

The ALMA Software and Release Management Ruben Soto Software Operations Group & Release Manager Joint ALMA Observatory.

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array CASA Progress.

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

The ALMA TelCal subsystem Dominique Broguière, Institut de RadioAstronomie Millimétrique (IRAM) TelCal Phasing meeting – Grenoble -10/12/2012.

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

Scheduling Blocks: a generic description Andy Biggs (ESO, Garching)

ALMA Common Software Basic Track Logging and Error Systems.

NRAO Users Committee Meeting May 20-21, National Radio Astronomy Observatory NRAO Users Committee Meeting – May 20-21, 2008 ALMA Operations Chris.

1 ANASAC Meeting – May 20, 2015 P. Jewell, J. Hibbard, C. Lonsdale Cycle 1 & 2 Status & Cycle 3 results.

ALMA Integrated Computing Team Coordination & Planning Meeting #4 Santiago, November 2014 Telescope Calibration Planning Dominique Broguière.

1 ANASAC Meeting – May 20, 2015 P. Jewell, J. Hibbard, C. Lonsdale ALMA / NAASC Status – 2015 ANASAC Meeting.

EVLA Software Bryan Butler. 2007May22EVLA SAGE Meeting2 Requirements and Goals of EVLA Software Maximize scientific throughput of the instrument At a.

The North American ALMA Science Center Interim Director, Paul A. van den Bout.

The North American ALMA Science Center North America’s ALMA Regional Center The North American ALMA Science Center acts as the gateway to ALMA for North.

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

Observing Modes from a Software viewpoint Robert Lucas and Philippe Salomé (SSR)

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array GBT Control System.

1 KFPA Critical Design Review – Fri., Jan. 30, 2009 KFPA Data Pipeline Bob Garwood- NRAO-CV.

ALMA Polarization Commissioning and Verification Status Kouichiro Nakanishi (Joint ALMA Observatory/NAOJ) on behalf of ALMA Polarization Commissioning.

SAGE meeting Socorro, May 22-23, 2007 EVLA Science Operations: the Array Science Center Claire Chandler NRAO/Socorro.

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

1 ANASAC Meeting – May 20, 2015 Mark Lacy ALMA archive status and plans.

Radio Telescopes and Radiometers

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

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

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

ES Slowdown, Optimization, Testing. Plan for shutdown: Timeline April: Focus on resolution of major outstanding issues: – Bulk data deployment  stable.

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 Observing with NRAO.

ALMA and the Call for Early Science The Atacama Large (Sub)Millimeter Array (ALMA) is now under construction on the Chajnantor plain of the Chilean Andes.

Development Status and Priorities Jeff Kern NRAO.

ESO, 17 April 2007ESAC meeting1 ALMA offline User Test 5 Silvia Leurini, ESO.

Atacama Large Millimeter/ submillimeter Array - ALMA ASAC Charges For Oct 31 ASAC Report to ALMA Board Al Wootten JAO Interim Project Scientist.

An NSF Facility 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 Emmanuel Momjian (NRAO)

THE ALMA ORION BAND 6 SCIENCE VERIFICATION DATA SPECTRAL LINE SURVEY - CONTENT AND DISCOVERY AVAILABLE FOR ALL SCIENCE Anthony J. Remijan ALMA Program.

Charlottesville, November ALMA CSV Update Alison Peck Current status.

EVLA Data Processing PDR Pipeline design Tim Cornwell, NRAO.

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Short Spacing.

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

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ngVLA: Reconfigurability.

From delivery to acceptance

DMG internal tools currently in use and plans to ingest requirements to ICT deliverables E. Villard.

PRTS & KPI Nick Whyborn – Vasco Cortez

Obsprep Planning, 2017 Alan Bridger

Science Ready Data Products

ATACAMA LARGE MILLIMETER ARRAY

Welcome to ALMA Community Day!

An GHz integrated, multi-chip downconverter designed and built at the CDL by Matt Morgan and Tod Boyd. The white substrates are.

Presentation transcript:

Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA Pipeline Progress and Status ANASAC Face-to-Face Sept 16-17, 2013 Jeff Kern CASA Team Lead

ALMA Pipeline Status ALMA Interferometric Pipeline is ready to support Cycle 1 Data reduction – Calibration and Diagnostic Images of Phase and Bandpass Calibrators – Single Dish through imaging* – No support for combination – Some human intervention still required: Calibrator Fluxes Extraordinary Flagging Rapid progress made in past year: – Tiger Team led by Todd Hunter – Built on experience from cycle-0 reduction * Still developing global consensus on best single dish reduction. Pipeline is closely connected to this discussion. 2ANASAC Face-to-Face: Sept. 16,

ALMA Organization Pipeline Working Group now formed 3 Liz Humphries (Chair) Eric Villard (Deputy) Remy Indebetouw Hiroko Shinnaga Todd Hunter (ex officio: Tiger Team Lead) International test / user team – NAASC Data Analysts – JAO Data Content Managers

ALMA Cycle-1 Operations Early Cycle-1: Parallel Reduction – Each ARC organized slightly differently – Pipeline and manual scripts will be run in parallel results compared by reducer Common feedback forms to pipeline to describe meaningful differences from human reduction. Late Cycle-1: Pipeline Calibration – Pipeline does primary calibration for most projects Band 9, special cases still needs manual reduction. Data reducer starts with calibrated data from the archive and does reference imaging. Actually had hoped to already be at this state by now! 4

ALMA ALMA Pipeline Execution Summary 5

ALMA ALMA Pipeline Observation Summary 6

ALMA ALMA Pipeline Task Summary 7

ALMA ALMA Pipeline Task Summary 8

ALMA ALMA Pipeline Task Details 9

ALMA ALMA Pipeline Calibrator Image Production 10

ALMA ALMA Pipeline Target Imaging 11

ALMA Looking Forward Support for cycle-1 operations: – Dealing with bugs (ours and theirs) WebLog – Meeting existing requirements from first focus group meeting – Revisit WebLog requirements (Q1-2014) based on experience for Cycle 1 Cycle-2 Capabilities 12 More complicated SPW setups Initial Polarization Calibration Low SNR Cases (Band 9) [More] Flagging Heuristics Science Target Imaging: Are we meeting targets. Planning for user test prior to Cycle-2 Operations to gather responses from Cycle 1 Experience.

13 The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. science.nrao.edu