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| == NIKA Run#3 Summary of Off line processing Results == | = NIKA Run#3 Summary of Off line processing Results = |
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| '''Index''' [[TableOfContents(2)]] |
Work in progress (Don't shoot) The main document is [[attachment:Run3_Analysis.pdf|here]] == Focal Plane Geometry and Beams == Both RZ (Mopsic) and NP (IDL, from [[OffProcNika3?action=AttachFile&do=view&target=FP_quicklook_120207.pdf|This pdf]]) have found a distortion of the focal plane geometry well beyond the expected one. {{attachment:OffProcNika3/avRPo1mmMeanEdge_1_9.png | average FoV 1mm RZ}} {{attachment:OffProcNika3/NIKA2mmPh6-20111019s52_indFFmxRef1mm22_1_rpp.png | 2mm beams in PF (RZ)}} {{attachment:FP_QLA_120207.png | FoV 1mm&2mm NP}} The focal plane distortion affects the beams in a correlated fashion with the Focal Plane Geometry distortion. This points towards a general optical distortion common to both detectors (an optical element is misplaced in the optical train). == Glitches and Mars plateau == {{attachment:OffProcNika3/NIKA1mm-20111019s52_3_Jy.png | plateau@1mm uPixs Jy}} |
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| = Focal Plane Geometry and Beams = | == Cosmetics == |
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| Both RZ (mopsic) and NP (IDL) have found a distortion of the focal plane geometry well beyond the expected one. | rms of maps per scan per kid per beam averaged over 5 scans |
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| [[OffProcNika3#FoVGeometry| here]] | {{attachment:Noise_PerKid_4C05.19_20111019_10_17.jpg | Noise per scan per kid per beam averaged over 5 scans}} == Photometry == Evolution of the sky opacity during Run#3 {{attachment:NIKA3OpacityCal/Study_atm2_4.jpg| Run#3 225GHz opacity at zenith | width=700}} |
NIKA Run#3 Summary of Off line processing Results
Work in progress (Don't shoot) The main document is here
Focal Plane Geometry and Beams
Both RZ (Mopsic) and NP (IDL, from This pdf) have found a distortion of the focal plane geometry well beyond the expected one.
The focal plane distortion affects the beams in a correlated fashion with the Focal Plane Geometry distortion. This points towards a general optical distortion common to both detectors (an optical element is misplaced in the optical train).
Glitches and Mars plateau
Cosmetics
rms of maps per scan per kid per beam averaged over 5 scans
Photometry
Evolution of the sky opacity during Run#3
