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Size: 715
Comment:
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Size: 1213
Comment:
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| Deletions are marked like this. | Additions are marked like this. |
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| The flux per kid is shown here using the calibration on Uranus Scan # | The flux per kid is shown here using the calibration on Mars Scan #55. This is an indication that the new camera with its dIdQ modulation scheme provides a big photometric improvement with respect to 2010 campaign. The average flux is compatible with the range of fluxes measured on this (variable) source. |
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=== SL, 07 Nov 2011 - Expected field distortion === [[attachment:NIKAv2_Grid_distortion.pdf | grid distortion ]] === FXD, 21 Nov 2011 - Technical note on kid frequencies === [[attachment:NIKA2011_TechNote1_v1.pdf | Kid frequencies and so on... ]] |
NIKA3 Offline Processing Results
2011 October run
=Private results for the collaboration only=
Public results
FXD, 24 Oct 2011 - Photometric quality
Here are the maps obtained on one OTF scan with IRC 10216. Sky noise decorrelation is used.
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The flux per kid is shown here using the calibration on Mars Scan #55. This is an indication that the new camera with its dIdQ modulation scheme provides a big photometric improvement with respect to 2010 campaign. The average flux is compatible with the range of fluxes measured on this (variable) source.
SL, 07 Nov 2011 - Expected field distortion