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| Session of pointing monitoring the 20-22 of July 2007 [[BR]] | Session of pointing monitoring the 20-25 of July 2007 [[BR]] |
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| * 81 pointing sources observed. * 72 sources have a new measured flux. * 4 sources are found to be too faint: J0750+827, J1056+702, J1909+486, J0121+044 |
* 100 pointing sources observed and usable for the analysis * 5 sources are found to be too faint (<100 mJy): J0121+044, J0750+827, J1056+702, J1628-143, J1909+486 J1628-143 * 16 observations of primary and secondary calibrators were done: Uranus, K3-50A, MWC349, LKHALF234, G34.3, CW-LEO, G10.62, NGC7538, G45.1 === Pointing status === The plot below shows the '''azimuth''' (blue) and '''elevation''' (red) corrections. attachment:pointingCorr20-25.06.07.png From that pointing session, a new pointing model was derived by JP and implemented. === Flux === === Conclusions === |
Session of pointing monitoring the 20-25 of July 2007 BR We check the evolution of the pointing sources used for the bolometer observations.
Summary
We observed the pointing sources doing a pointing and an Onf-Off measurements in most of the cases.
- 100 pointing sources observed and usable for the analysis
5 sources are found to be too faint (<100 mJy): J0121+044, J0750+827, J1056+702, J1628-143, J1909+486 J1628-143
- 16 observations of primary and secondary calibrators were done: Uranus, K3-50A, MWC349, LKHALF234, G34.3, CW-LEO, G10.62, NGC7538, G45.1
Pointing status
The plot below shows the azimuth (blue) and elevation (red) corrections.
attachment:pointingCorr20-25.06.07.png
From that pointing session, a new pointing model was derived by JP and implemented.
Flux