|
Size: 477
Comment:
|
Size: 1284
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 8: | Line 8: |
| FXD, 24 Oct 2011 - Photometric quality\\ Here are the maps obtained on one OTF scan with IRC 10216 |
== [[List of offline processing tasks|NIKA3ListOfflineProcTask]] == |
| Line 11: | Line 10: |
| ||{{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}}|| | ==== 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}} === 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
[[List of offline processing tasks|NIKA3ListOfflineProcTask]]
FXD, 24 Oct 2011 - Photometric quality
Here are the maps obtained on one OTF scan with IRC 10216. Sky noise decorrelation is used.
|
|
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