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systematicswg:telecons:2018-01-31:start [2018/01/31 10:49] – created joydidiersystematicswg:telecons:2018-01-31:start [2018/01/31 12:29] (current) joydidier
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-   +=== Polarization Angle === 
-  * Notes on Polarization Angle:+ 
 +Uncertainty in polarization calibration creates EB leakage. Sacrifice cosmic birefringence limits to zero TB,TE,EB. Improvement of calibration sources: difficult across broad bands and large. Onboard calibrator? Compact polarized source measurements should be revisited? Hardware solution potentially?   
 + 
 +  * Analysis:
     * Planck:     * Planck:
       * [[https://www.aanda.org/articles/aa/full_html/2010/12/aa13054-09/aa13054-09.html | Planck HFI ground calibration]] measured detector polarization angles to ~ 1  degree relative uncertainty and claimed 0.3 degrees absolute uncertainty.       * [[https://www.aanda.org/articles/aa/full_html/2010/12/aa13054-09/aa13054-09.html | Planck HFI ground calibration]] measured detector polarization angles to ~ 1  degree relative uncertainty and claimed 0.3 degrees absolute uncertainty.
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       * Re-do analysis with PICO sensitivity estimate?       * Re-do analysis with PICO sensitivity estimate?
       * Investigate how much we really lose any birefringence science?       * Investigate how much we really lose any birefringence science?
 +
 +
 +Some more references:
 +  * [[http://iopscience.iop.org/article/10.1088/2041-8205/762/2/L23/meta | SELF-CALIBRATION OF COSMIC MICROWAVE BACKGROUND POLARIZATION EXPERIMENTS by Keating, Shimon and Yadav]]
 +  * See more references in the systematics table
systematicswg/telecons/2018-01-31/start.1517417353.txt.gz · Last modified: 2018/01/31 10:49 by joydidier