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| === NIKA3 Offline Processing Results === | = NIKA3 Offline Processing Results = |
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| [[NIKA3ListOfflineProcTask| List of offline processing tasks]] ==== FXD, 24 Oct 2011 - Photometric quality ==== 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. The average flux is compatible with the range of fluxes measured on this (variable) source. {{attachment:Flux_PerKid_IRC10216_20111018_65_65.jpg|IRC 10216 Scan65 18th Flux per kid|width=400}} ==== RZ, 25 Nov 2011 - Pointing & focus effects ==== {{attachment:plGFeq.png}} Source positions in eq offsets. In red are shown positions of sources used for pointing model.Positions of planets are not shown. The pointing offsets are even 3 times larger than the normal values. {{attachment:plGFhor.png}} As above in hor system; positions of planets are also shown. === SL, 07 Nov 2011 - Expected field distortion === [[attachment:NIKAv2_Grid_distortion.pdf | grid distortion ]] === FXD, 21 Nov 2011 - Technical note on kid frequencies === ''FXD, 24 Nov 2011 updated v2 (Fits format exchange)'' [[attachment:NIKA2011_TechNote1_v2.pdf | Kid frequencies, fits format]] === AM,MC 24 Nov 2011 Spectral transmissions === {{attachment:Spectra-single pixel.jpg| (IN/LPSC) Martin-Pupplet Interferometer Spectral Bandpass transmission}} |
NIKA3 Offline Processing Results
2011 October run
=Private results for the collaboration only=
Public results
List of offline processing tasks
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.
RZ, 25 Nov 2011 - Pointing & focus effects
Source positions in eq offsets. In red are shown positions of sources used for pointing model.Positions of planets are not shown. The pointing offsets are even 3 times larger than the normal values.
As above in hor system; positions of planets are also shown.
SL, 07 Nov 2011 - Expected field distortion
FXD, 21 Nov 2011 - Technical note on kid frequencies
FXD, 24 Nov 2011 updated v2 (Fits format exchange)
AM,MC 24 Nov 2011 Spectral transmissions
