Injecting W-band power (from Gunn oscillator) into QUIET receiver module
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Transcript of Injecting W-band power (from Gunn oscillator) into QUIET receiver module
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1Injecting W-band power (from Gunn oscillator)
into QUIET receiver module
KEK and Fermilab Collaborating at Lab 3
Status of QUIET-II at Fermilab
Fritz DeJongh, Scott Dodelson, Donna Kubik, Hogan Nguyen, Albert Stebbins
FCPA Retreat May 13th, 2011
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QUIET-I HighlightsAnnouncement of Q-band(40 GHz) Result
Fermilab Wine & CheeseA. KusakaMarch 4th 2011
6 sigma detection of EE peak at 1.2 degreeangular scale (confirms BICEP with less data, at different freq)
See 3σ evidence of Synchroton Foregroundin a supposedly clean patch of sky
Limit on B mode (r < 2.2)
Lowest published systematics(rsys ~ 0.1)
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QUIET-I Highlights (with Emphasis on Fermilab)
Large Sparse Wire Grid Concept for channel-to-channelcalibration and gain tracking worked very well.
Important tool for monitoring W-band detectorperformance.
W-band Data Analysis
Detector Noise Monitoring(Kubik)
Detector Calibration using Moon Signal(Nguyen)
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Main QUIET-II Detector R&D Program Goal: Maximize Raw Sensitivity
Figure of Merit (to good approximation):
Receiver Noise Sensitivity [K-sec1/2] = Temperature [K]
(Bandwidth [Hz])1/2
or equivalently
White Noise Sensitivity [K-sec1/2] = [mV - sec1/2]
Gain [mV/K]
W-band Noise Per Module
Quiet I 500 μK-sec1/2
Quiet-II (goal) 200 μK-sec1/2
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QUIET 1 Module in Cryostat at Lab 3
* This module didn’t pass quality cuts. Was not installed in QUIET-I array.
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6Black Body Temperature (Kelvins)
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First Receiver Noise Temperature Measurement at Fermilab (a.k.a. Y-factor Measurement)
DetectorOutput(arbitraryunits)
DifferentAmplifierGain Settings
Good Agreementwith Caltech-JPLMeasurements
Receiver Noise Temperatureappears to be ingood controlfor this chip design.
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First Sensitivity Measurements at Fermilab (KEK + Fermilab)
Sensitivity ~ 1.75 mK-sec1/2
* This module failedother quality cuts... was not installedinto QUIET-1 array
Noise Power Spectrum (1/f noise has been cancelled)
Frequency [Hz] Frequency Noise Power
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Maximizing the Module Sensitivity
Replace Lossy Passive Planar RF Structures with Pure Waveguide
Reduce 1st Amplifier’s Noiseto ~ 50K, and increase BW
0.75mm
0.25 mm
Improve DC Amplifiers down stream of Detector Diodes(RF DC converter)
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QUIET-II Module New Design Component Design and Fabrication
Caltech/JPLManchesterSLAC/StanfordFermilab
ElectronicsKEK and Chicago
TestingCIT, KEK, Chicago/Fermilab
Detector Diode Housingprovided by Fermilab(RF DC converter)
Prototype for QUIET-II
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Towards QUIET-II
• The death of Bruce Winstein was a huge loss.
• QUIET-II proposal was turned down by NSF. Cost of ~$20M is main issue.
• Funding for QUIET-II R&D to improve modules and reduce cost.
- KECK Space Science Institute grant to fund Caltech Cahill Lab - Stanford (2nd year of NSF ATI Grant) - Foreign Contributions ( KEK and Manchester) - Caltech-led NSF-ATI Grant was turned down in April 2011. - Chicago PFC Proposal (contains funding for HEMT R&D) is awaiting final decision. - Fermilab KA13 (0.2 FTE) and KA15 (0.5 FTE and M&S)
• PI’s are meeting in late May at JPL. Topics for discussion:
- When to resubmit for Phase II - New Spokesperson - Possible low-cost intermediate experiment before Phase II.