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| FXD, 24 Oct 2011 - Photometric quality\\ Here are the maps obtained on one OTF scan with IRC 10216 |
==== FXD, 24 Oct 2011 - Photometric quality ==== |
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| ||{{attachment:Map2Radec2_A_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th 2mm map}}||{{attachment:Map2Radec2_B_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th 1mm map}}|| | Here are the maps obtained on one OTF scan with IRC 10216. Sky noise decorrelation is used. ||{{attachment:Map2Radec2_A_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th 2mm map|width=400}}||{{attachment:Map2Radec2_B_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th 1mm map|width=400}}|| 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: {{attachment:Flux_PerKid_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th Flux per kid|width=400}} |
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:
