Parkes “The Dish”. 19’ M83 Parkes “The Dish” VLA, Very Large Array New Mexico.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank...
-
Upload
james-sanders -
Category
Documents
-
view
221 -
download
0
Transcript of Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank...
Atacama Large Millimeter/submillimeter ArrayExpanded Very Large Array
Robert C. Byrd Green Bank TelescopeVery Long Baseline Array
Data ProcessingProgress and PlanningJune 2014
Jeff KernData Processing Group
Lead
CASASummary Status• CASA-4.2.2 brings capabilities desired for cycle 2 data
reduction– Currently under test issues with plotMS, otherwise
looking good– Key deliverables:
• Weight handling (per SPW)• Flag Data Improvement (Tbuff parameter to avoid
quacking)• Strict Flagging in Applycal• Single Dish Interface Update
• Pipeline – Provisional Acceptance in March– Long punch list, mostly cosmetic. Largely addressed at
this point– Doing integration testing against CASA-4.2.2
CASAPlanning: Near Future• June 27: Prerelease of CASA-4.2.2 and Pipeline to PLWG for
testing• July 1: Release of CASA-4.2.2 (Public)
– Both OSX and Linux• ~July 1: Release of ALMA Pipeline to project
– Based on testing from PLWG• ~July 15: CASA-4.2.2-Pipeline release available to public
These dates are all very tight, and are based on not finding issues in the testing. Small slips can have large impact as we
are in vacation season
CASACASA Planning• September 2014 CASA-4.3
– Weight Spectrum– Imaging Refactor V1– Parallelization
(Calibration)
– SetJy Improvements– VO Viewer
• March 2015 CASA-4.4– Imaging Refactor V2
• Support for Pipeline– OTF Cal Application
– Pipeline Parallelization– Enhanced Phase
Connection
CASAPipeline Planning• From ObsMode Meeting
– Support for Cycle 2 Operations• This could stop all other progress!
– Data Flagging Heuristics– Bandwidth Switching Heuristics
• First of low SNR Heuristics– Science Target Imaging
• 1 Cube per Science SPW per Science Target
• In parallel:– Automated trigger and cluster exectuion– This is NOT a magic bullet.
5
CASAWeblog Example
Pipeline Regression Server
6
CASAPLWG: User Test
• Pipeline Working Group will perform a user test to receive feedback on Weblog– Format TBD either special run and request comments or
just survey of Cycle 2 Pis
• Will need to prioritize feedback from this vs. functional testing
7
CASAPipeline Single Dish
• Well developed and tested– Not much knowledge outside of NAOJ so far
• Hoped to be doing parallel testing at this point– Need lots of data (Project wide issue)
• Concerned about connection between manual reduction, script generator, and pipeline
ICT CPM-3 June 17-19 Socorro New Mexico 8
CASA
Prelim
inar
y
Pipeline Releases• November Update
– Bandwidth Switching– Data Flagging– Other Cycle 2 Experience (TBD)
• March 2015– Imaging capabilities V1– Long Baseline capabilities– Low SNR (?)
• Q3 2015– Continuum Subtraction– Self Cal– Other Calibration
9
Infrastructure
&Automation
CASASteps to Pipeline Use in Operations
First Pipeline-assisted deliveries
Jun
e/J
uly
2014
Cycle 2 Phase C testing
Test commissioned observing modes for Cycle 2 data
Test commissioned observing modes for Cycle 2 data
Pipeline documentation review
Send final drafts broad review within Observatory
Submit final drafts to SciOpsIPT and DRM WG for review
PWG full acceptance recommendation Submit report to SciOpsIPT
Submit full acceptance report to Observatory
PWG full acceptance testing
Test full acceptance criteria
Test full acceptance criteria implementation
DRM WG end-to-end testing
Test e-2-e QA2 process, packaging & documentation
Test e-2-e QA2 process, packaging & QA2 documentation
Pipeline-assisted QA2 in operations
For commissioned observing modes, data calibrated by Pipeline and imaged manually
Pipeline released to users
CASA 4.2.2 tarball including Pipeline
CASAPipeline Issues• Staffing:
– Pipeline has exactly 1 full time developer– Currently stepdown another 0.5 FTE at end of year
• Formally 3.0 -> 2.5 but realistically 1.8 -> 1.3 on interferometric
– “Borrowing” expertise from CASA but not the same as dedicated staff
• Maintenance / Support– Tracking down errors for failed SBs could halt progress on new
targets– Need robust QA0 process at observatory
• Balance between Cosmetic and Functional requirements– Weblog has grown very large, suspect it may be overspecified at
this point
11
CASA
www.nrao.eduscience.nrao.edu
The National Radio Astronomy Observatory is a facility of the National Science Foundation
operated under cooperative agreement by Associated Universities, Inc.
CASACASA and CASA Based Pipelines
Pipeline Weblog: Home Page
CASACASA and CASA Based Pipelines
Pipeline Weblog: Observation Summary
CASACASA and CASA Based Pipelines
Pipeline Weblog: Topics Page
CASACASA and CASA Based Pipelines
Pipeline Weblog: Task Summary
CASACASA and CASA Based Pipelines
Pipeline Weblog: Task Detail
CASACASA and CASA Based Pipelines
Pipeline Weblog: Plot Details
CASACASA and CASA Based Pipelines
Pipeline Weblog: Detail Zoom
CASACASA and CASA Based Pipelines
Pipeline Weblog: Imaging Summary
CASACASA and CASA Based Pipelines
Pipeline Weblog: Imaging Details