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Automatic Omniscope Calibration Using Redundant Baselines

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si = signal measured by antenna i ; gi = gain of antenna i. y = true corr; cij = measured corr ... measured by antenna i ; gi = gain of antenna i. y = true ... – PowerPoint PPT presentation

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Title: Automatic Omniscope Calibration Using Redundant Baselines


1
Automatic Omniscope Calibration Using Redundant
Baselines
  • SwFRT, Fermilab, 2009
  • Adrian Liu
  • (with Max Tegmark, Andy Lutomirski, Scott
    Morrison, Matias Zaldarriaga)

2
Unlike Traditional Interferometers, Omniscopes
Have Many Redundant Baselines
3
In Reality, Identical Baselines Will Give
Different Results
4
Main Idea Demand that redundant baselines give
the same results and fit for everything
5
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6
Mathematically, an over-determined system
Inputs Parameters being fit for
nxny(nxny1)/2 complex correlations nxny complex gains 2 nxny - nx - ny 1 unique baselines
7
True sky signal
Instrumental noise
Measured signal
Complex gain
where
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
8
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
9
Real Part Gains
Have this (data)
Know this
Want this
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
10
Real Part Gains
d
A
b
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
11
A Problem With Degeneracies
  • Real part (gains)
  • No knowledge of absolute gain.
  • Imaginary part (phases)
  • No knowledge of absolute phase.
  • No knowledge of x-tilt.
  • No knowledge of y-tilt.

si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
12
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
13
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
14
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
15
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19
A Weighty Issue
20
Weighted Fit
21
si signal measured by antenna i gi gain of
antenna i ?? y true corr cij measured corr
22
Some Bias
23
Differences Between This and Traditional
Calibration
Traditional Scheme Redundant Baselines
Use closure phases Amplitude (gain) calibration requires point source Modeling may be required Any sky signal can be used for calibration Redundancy provided by identical baselines
24
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25
Summary
  • Redundant baselines provided by omniscopes can be
    exploited for calibration
  • Proposed automatic calibration scheme works on
    simulated data
  • Using redundant baselines allows one to sidestep
    certain problems with traditional techniques
    (like the necessity of having isolated point
    sources).
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