![]() |
|||||
---|---|---|---|---|---|
FORS1 SKY BRIGHTNESS |
|||||
|
QC1 ASCII DATA |
QC1 database (expert mode) |
General |
Since Period 65 (April-September 2000), the value of the sky
brightness of Paranal is constantly monitored using FORS1. Preliminar
results from measurements obtained during sunspot maximum are reported
and discussed in A&A
400, 1183 (2003).
The sky brightness is measured from the reduced SCIENCE images by
running a code created by F. Patat (ESO) and described in in A&A
401, 797 (2003). The code has been integrated in the DFO system to
obtain automatically, for each reduced science image, the sky
brightness measurements as part of the QC process. Images are scan to
select those best suited for a reliable sky brightness measurement. In
this phase, the image sky background is evaluated automatically and
those images affected by a very noisy backgrounds, by enhanced objects
crowding, by saturation problems and by reflections or ghost images
are filtered out. The measured sky brightness values (in instrumental
magnitudes/arcsec sq.) were then calibrated on-the-fly using the
photometric zeropoints of the day, and corrected for the atmospheric
extinction and for the instrument color-terms using the closest in
time values logged in the QC1 database. Corrections for the
contributions of the zodiacal light and of the moon are also
applied.
Since 2005-11-15 we use instead the zeropoints obtained for
photometric nights within the last 3 months. Also the corrections for
zodiacal light and moon light are provided, but not applied.
The final values are then automatically ingested in the sky
brightness QC1 database. Here, only calibrated sky
brightness values in the UBVRI passbands are trended. Both raw
and calibrated sky brightness values are available in the QC1
database.
Related Publications |
|
![]() ![]() ![]() |
|