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Theme 7 Group 1
Goal of Workshop
To develop a joint Sino-Australian proposal to ERIDANUS (波江座) for RFI mitigation in Radio Astronomy data using Big Data approaches.
Workplan
• Motivation
• Target
• Tentative solutions
Motivation
• RFI : a generic problem for radio astronomical data analysis...
• Challenges• Very high sensitivity for SKA, MWA, ASKAP, FAST, …• Appearing in many steps of the SKA processing system • For the SKA it would be nice to have (near) real-time requirement
• Useful for • Imaging pipeline • Non-imaging pipeline • Identifying local plant equipment generating RFI
RFI in IMAGINELocal RFI
RFI in IMAGINE
RFI in pulsar data
narrow and wideband RFI in pulsar data
RFI sources Specific mitigation
techniques
Common
techniques
Man made
interference
Local plant equipment Knowledge base Pattern recognition,
machine learning, esp.
deep learning
(parameter/feature
models)
Pseudo-random
sources (e.g., military,
local planes, cameras
etc.)
Anomaly detection,
data mining
Regular sources (e.g.,
planes/satellites, etc.)
Knowledge base
Pattern recognition
Natural
interference
Environmental / space
noise (e.g., lightning,
the sun, mice, etc.)
Data mining
Knowledge base
RFI categorization
ADC FIR+FFT BeamformingBands
FIR+FFTBeams Channels
Corrections
Correlate
Baselines
VisibilitiesRFI mitigation
Initial calibration & A-team removal
VisibilitiesRFI mitigationGriddingDirty image
ImagingSources
Sky modelSky image
De-gridding
Data Collection
Central Signal Processing
Imaging pipeline
Finer frequency channels Time-frequency Source fusion
SDP subsystem
Station subsystem
Calibration
De-dispersionSingle PulseFFT
Single pulse RFI mitigation
Periodic RFI mitigation
detectionSift/ general RFIPulsars / FRBs
RFI mitigationNon-imaging pipeline
Data and Methodology
• Data Methods• Unified architecture —— Big data technique, machine learning, data mining,
Spark, Keras, Tensorflow… for SKA Low and Mid
• Data available from telescopes• Interferometer——LOFAR, MWA, MeerKat , ASKAP, jVLA, ATCA
• Single Dish —— FAST (sensitivity same as SKA), Parkes, Arecibo,
Lessons from different telescopes for SKA
Research topics
• Building knowledge base based on different RFI sources
• Feature models by Deep Neural Networks (DNNs) (GPU, (Keras)Tensorflow/Theano/MXNET/Torch/Caffe(CNN))
• Machine learning, data mining, pattern recognition techniques for RFI detection
• Parallel computing in Spark platform
• Science use cases (imaging and non-imaging)
• …
Unified architecture
Longer Term Goals
Write two papers:1. The development of a database to be hosted at Fudan University (复旦大学) to characterise RFI
2. Overview paper of the existing approaches to RFI and why our approach will deliver better results for the community
Develop a joint proposal to ERIDANUS to use Big Astronomy Data techniques to mitigate RFI in radio astronomy data. This includes:• Pulsar data• Spectral line and Continuum dataThis will work on single dish and interferometers
Deliverables
• Data Files with Spark/Keras/…. Format (meta data)
• RFI knowledge base
• Feature models learnt by deep neural networks
• Machine learning/data mining/pattern recognition techniques suitable for RFI detection
• Computing platform on Spark (CPU-based) and DL (GPU-based) platform
A unified architecture for RFI mitigation especially for SKA Low and Mid
Conclusion
• We feel this is a problem that Big Data approaches including Machine Learning, Deep Learning and Adaptive Learning can help mitigate.
• Over the last three days of this workshop our group cannot be accused, in any way, of floccinaucinihilipilification about the workshop.
Thank you -谢谢
Kevin's important lessons learnt
1. When using Google translate remember to switch from English to 普通话, to 普通话 to English when translating menus
2. For a Vegetarian being able to say 我是一個素食者 is really handy at Restaurants
3. Chinese food somehow tastes better in China
4. Tones are important Wěi wěi is 炜玮's name, but said with a different tone wèi wèi (喂喂) it means "hello, hello" and is someone testing a microphone not someone calling him from the other side of the room