Differences between revisions 20 and 21
Revision 20 as of 2011-11-25 14:41:55
Size: 2544
Comment:
Revision 21 as of 2011-11-25 14:43:15
Size: 2550
Comment:
Deletions are marked like this. Additions are marked like this.
Line 26: Line 26:
The pointing offsets after the installation of the pointing model are very large, even 3-5 times larger than the normal values. The pointing offsets after the installation of the pointing model are still very large, even 3-5 times larger than the normal values.

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.

IRC 10216 Scan65 18th 2mm map

IRC 10216 Scan65 18th 1mm map

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.

IRC 10216 Scan65 18th Flux per kid

RZ, 25 Nov 2011 - Pointing & focus effects

plGFeq.png

Source positions in eq offsets. Positions of planets are not shown. In red are shown positions of sources used for pointing model, in black after the installation of the pointing model. The pointing run was apparently performed with Nasmyth offsets of EMIR ! The pointing offsets after the installation of the pointing model are still very large, even 3-5 times larger than the normal values.

plGFhor.png

As above in hor system; positions of planets are also shown.

MarsUranus_azOff_extCorr.png MarsUranus_elOff_extCorr.png

Effekt of defocusing: the source moves by a couple of arcsec in azim & elev. Note the larger scatter of the elev-positions.

Both, pointings and foci were done by mapping. However, to correctly process maps the correct beam parameters, i.e. the pixel positions and their flat field are mandatory. The effective FoV geometry, the flat field and their errors will come next.

SL, 07 Nov 2011 - Expected field distortion

grid distortion

FXD, 21 Nov 2011 - Technical note on kid frequencies

  • FXD, 24 Nov 2011 updated v2 (Fits format exchange)

Kid frequencies, fits format

AM,MC 24 Nov 2011 Spectral transmissions

(IN/LPSC) Martin-Pupplet Interferometer Spectral Bandpass transmission

OffProcNika3 (last edited 2012-05-25 09:50:44 by NikaBolometer)