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Aaron Chippendale, Ravi Subrahmanyan, Ron Ekers

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Title: PowerPoint Presentation Author: karlo_kempis Last modified by: Chippendale, Aaron (ATNF, Marsfield) Created Date: 8/5/2003 10:57:01 AM Document presentation format – PowerPoint PPT presentation

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Title: Aaron Chippendale, Ravi Subrahmanyan, Ron Ekers


1
The Cosmological Reionization ExperimentCoRE
  • Aaron Chippendale, Ravi Subrahmanyan, Ron Ekers
  • 20 January 2009

RRI
2
Overview
  • Science
  • Expected signal 30 mK / 5 MHz
  • Design implication
  • 1 mK / 1 MHz target
  • Instrument
  • Frequency independent antenna
  • Correlation spectrometer
  • Results
  • System stability 1(bandpass and constant)
  • 10 K / 2.5 MHz residuals in bandpass
    calibration
  • Constant not yet calibrated

3
Theoretical Limits on 21 cm Monopole
possible signal (qualitative)
4
Reionization Bubble Model
H
Ts TCBR
H
H
Ts Tm
H
H
H
H
H
H
H
e-
H
H
H
H
H
H
e-
H
H
H
e-
H
H
H
H
Tm gtgt TCBR
H
Tm lt TCBR
H
H
H
Sethi, 2005
5
Expected Signal (WMAP3 Parameters)
1 mK/MHz
multiply all numbers by 0.752 for He correction
6 mK/MHz
6
Correlation Receiver
r
7
Correlation Receiver Integrating Down
8
Frequency Independent Antenna
1 error at half power
9
Frequency Independent vs. Log Periodic
Frequency Independentdefined by angles
Log Periodicdefined by geometric ratio
10
Bandpass Calibration Residuals
11
Bandpass Calibrated Spectra 10 K Residuals
12
Bandpass Calibration ResidualsReference
Symmetric About Galactic Centre
13
Measurement Resembles Simulation of Squinted Beam
Rotating About Boresight
14
Normalized Drift-scans at all Frequencies
Measurement vs. Model
15
Band Average Drift-scanMeasurement vs. Model
16
System Stability 1 or better
17
Future
  • Future work
  • rotating antenna
  • split in free space

18
The End
  • End of main presentation
  • Design details follow for discussion

19
RFI Comparison
Culgoora, Narrabri (pop. 6000)
Murchison (pop. 110)
20
Wiener Model used for RF Amplifier
21
Nonlinear Response to Galaxy and RFI
RFI power equivalent to strongest narrowband
interferer at Narrabri
22
RFI power equivalent to strongest narrowband
interferer at MRO
RFI power equivalent to strongest narrowband
interferer at MRO
23
Aliased Bandpass
24
Quantization Distortion Simulation Design
25
Quantization Distortion Simulation Results
a25 dB
50th percentile at Narrabri
90th percentile at MRO
26
Ideal ADC Signal to Distortion and Quantization
Noise Ratio
Gaussian noise truncated atks
27
Ideal ADC Saturation Distortion as Fraction of
Total Power with Single Narrowband Interferer
Gaussian noise truncated atks
(10 dB)
28
RFI Comparison
Culgoora, Narrabri (pop. 6000)
Murchison (pop. 110)
29
Receivers and Correlator
Correlator
30
(No Transcript)
31
Correlation Receiver
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