Q Band results (with Zernikes enabled) (Todd)

Q Band results (with Zernikes enabled) from TPAR_18 (Todd)

Q Band results (Todd)

Q Band results (with Zernikes enabled) (Todd)

Because these scans were taken in AzEl? mode rather than Encoder mode, I had to compute azoff and eloff in

• scan 39 = 2008_01_08_07:03:19.fits
• scan 40 = 2008_01_08_07:08:56.fits
• scan 41 = 2008_01_08_07:14:33.fits (i.e. total time for 3 scans = 16.9 min)

Because these scans were taken in 'AzEl' mode rather than 'Encoder' mode, I had to compute azoff and eloff in

as it is <= 0.3 arcsec. The resulting scan pattern is very nearly centered at 0,0. The buildoof2008.py script will perform these corrections whenever it encounters data recorded in AzEl? mode.

as it is <= 0.3 arcsec. The resulting scan pattern is very nearly centered at (0,0). The buildoof2008.py script (attached below) will perform these corrections whenever it encounters data recorded in AzEl? mode.

• comparison of 7mm and 3mm phase maps:
  

• comparison of Q-band phase map (with Zernikes enabled) and Mustang phase map (with Zernikes disabled):
  

• comparison of 7mm and 3mm phase maps:
  

%META:FILEATTACHMENT{name="oof2.png" attr="" comment="comparison of 7mm and 3mm phase maps" date="1202160244" path="oof2.png" size="43645" user="ToddHunter" version="1.1"}%

%META:TOPICINFO{author="ToddHunter" date="1201899300" format="1.0" version="1.1"}% %META:TOPICPARENT{name="2008Jan08MustangOOFResults"}%

Q Band OOF results from Jan 8, 2008

Note: for contemporaneous Mustang results, goto this page

Q Band results (Todd)

Because these scans were taken in AzEl? mode rather than Encoder mode, I had to compute azoff and eloff in post-processing. This included calculating precession from J2000 to the current epoch, annual aberration, and applying the refraction correction from the Antenna file. The diurnal aberration term was ignored as it is <= 0.3 arcsec. The resulting scan pattern is very nearly centered at 0,0. The buildoof2008.py script will perform these corrections whenever it encounters data recorded in AzEl? mode. The fits on this page include up to 5th order Zernikes, to be consistent with the corresponding Mustang plots.

-- ToddHunter - 01 Feb 2008

• obsbeam-1.png:
  

• obsbeam-2.png:
  

• obsbeam-3.png:
  

• bestfitbeams-0.png:
  

• bestfitbeams-1.png:
  

• aperture-phase.png:
  

%META:FILEATTACHMENT{name="obsbeam-1.png" attr="" comment="" date="1201897627" path="obsbeam-1.png" size="9246" user="ToddHunter" version="1.2"}% %META:FILEATTACHMENT{name="obsbeam-2.png" attr="" comment="" date="1201897762" path="obsbeam-2.png" size="7681" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="obsbeam-3.png" attr="" comment="" date="1201897786" path="obsbeam-3.png" size="9687" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="bestfitbeams-0.png" attr="" comment="" date="1201897997" path="bestfitbeams-0.png" size="6035" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="bestfitbeams-1.png" attr="" comment="" date="1201898012" path="bestfitbeams-1.png" size="5481" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="bestfitbeams-2.png" attr="" comment="" date="1201898024" path="bestfitbeams-2.png" size="6075" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="aperture-phase.png" attr="" comment="" date="1201898035" path="aperture-phase.png" size="14708" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="buildoof2008.py" attr="" comment="invocation: buildoof2008.qbuild20080108()" date="1201898145" path="buildoof2008.py" size="17471" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="session.py" attr="" comment="precession, aberration calcs added for AzEl? mode" date="1201898195" path="session.py" size="11274" user="ToddHunter" version="1.1"}% %META:FILEATTACHMENT{name="s39-l-db.fits" attr="" comment="debaselined FITS file" date="1201898285" path="s39-l-db.fits" size="192960" user="ToddHunter" version="1.1"}%