Differences between revisions 7 and 8
Revision 7 as of 2007-08-17 21:54:03
Size: 922
Editor: lt-sl
Comment:
Revision 8 as of 2007-08-18 08:40:22
Size: 971
Editor: lt-sl
Comment:
Deletions are marked like this. Additions are marked like this.
Line 25: Line 25:
From that pointing session, a new pointing model was derived by JP and implemented. From that pointing session, a new pointing model was derived by JP and implemented. The parameters P2 and P7 (offsets) were changed.

Session of pointing monitoring the 20-25 of July 2007 BR We check the evolution of the pointing sources used for the bolometer observations.

TableOfContents

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. The parameters P2 and P7 (offsets) were changed.

Flux

Conclusions

Pointing20-25.06.07 (last edited 2009-04-16 08:26:46 by localhost)