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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology 1 WSDC Quality Assurance (QA) October 20, 2009 Director’s Review – October 20, 2009

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Page 1: WSDC Quality Assurance (QA)...W2 W3 W1 W2 National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology 10 Current Implementation: ScanFrame

National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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WSDC Quality Assurance (QA)

October 20, 2009

Director’s Review – October 20, 2009

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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QA Overview

Philosophy: WISE data volume is large; timescale for public release is short. To be successful, QA must be quick and efficient. Automate it as much as possible, allowing the human to concentrate on the small percentage of data requiring detailed scrutiny.

Objectives –  Assess data through each stage of processing. –  Identify and flag data not meeting WISE science requirements. –  Characterize data so they can be correctly interpreted by the community.

Director’s Review – October 20, 2009

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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QA Overview

There are four flavors of WSDC QA needed to support launch activities

–  Ingest QA –  Quicklook QA –  ScanFrame QA –  Archive QA

Director’s Review – October 20, 2009

Current QA products have been tested using ORT/MST data and other simulated data from Ned.

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Current Implementation: QA summary page

Director’s Review – October 20, 2009

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: Ingest QA

Director’s Review – October 20, 2009

Daily summary for each ingested delivery:

• Files received and ingested • Error messages seen

Checks also performed against manifest from White Sands

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: Quicklook QA, “scan” level

Director’s Review – October 20, 2009

In Quicklook QA, we run 3% of the delivered data through processing and check diagnostics in the following areas:

• Image backgrounds and noise • Scan synchronization • Photometric calibration • Visual checks

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: Quicklook QA, “scan” level

Director’s Review – October 20, 2009

Visual checks

Two examples…

Scan synchronization monitor

W1 W2 W3 W4

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: ScanFrame QA, scan level

Operational Readiness Review – October 7-8, 2009

In ScanFrame QA, we run all data through processing and check diagnostics in the following areas:

• Frame statistics & overlaps • Image quality • Photometric calibration • Astrometric calibration • Completeness and reliability • Checks of solar system objects • Color-color/color-mag plots • Visual checks

Director’s Review – October 20, 2009

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: ScanFrame QA, scan level

Director’s Review – October 20, 2009

Two examples…

Photometric calibration

Mean counts in frames

W2 W3

W1 W2

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National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology

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Current Implementation: ScanFrame QA, frame level

Director’s Review – October 20, 2009

Two examples…

Row and column medians in this frame

Frame image quality via aperture/PSF photometry comparison

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Procedural Flow: Ingest QA

Director’s Review – October 20, 2009

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Procedural Flow: Quicklook QA

Director’s Review – October 20, 2009

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Procedural Flow: ScanFrame QA

Director’s Review – October 20, 2009

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Procedural Flow: Archive QA

Director’s Review – October 20, 2009

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Procedural Flow: Anomaly alerting & tracking

WSDC Anomaly Reports The WSDC uses Redmine software for

recording anomalies that impact the integrity of WISE science data. The software allows for the entering, assigning, and tracking of anomalies. Once an anomaly is analyzed and the issue closed, Redmine acts as a repository of the associated analysis reports.

For some anomalies assigned to them, MOS may track the same issues using their ISA system.

IRSA has their own issue tracking system, the IRSA Help Desk (via Test Track), which will be used to track problems with WISE online services

Director’s Review – October 20, 2009

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Key Tasks Remaining

•  Items needed to support launch –  Incorporate lessons learned from ORT2 and ORT3/MST7.

•  Better define the receivers and content for QA reports. •  Optimize workflow for QA reviewers.

–  Include color/flux checks for saturated sources. –  Exercise anomaly alerting system. –  Interface with SOC on quality scoring/reviewing/sign-off.

•  Items needed post-launch –  Refine thresholds for QA (e.g., what is the mean bkg noise on orbit and

what sized deviation should trigger review by QA scientist?). –  Some of these cannot be determined until IOC or after.

Director’s Review – October 20, 2009