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The Archeops telescope is an off-axis Gregorian telescope with a 1.5
meter primary mirror that looks at 41 degrees of elevation. During the
flight, the gondola rotates at 2 rounds per minute around its vertical
axis and therefore performs scans on the sky at constant elevation.
While the Earth rotates, these scans end up forming a wide annulus on
the sky with scans crossing each other at various time scales allowing
an efficient monitoring of systematic signals. The gondola is shown in
Figure and the scanning strategy in
Figure . The gondola is hanged below a stratospheric
balloon that floats at an altitude of around 40 km. The data is taken
during 24 hours nighttime winter arctic flights.
Figure:
Schematic view of the Archeops gondola. The telescope observes at
41 degrees of elevation and rotates at 2 rounds per minute.
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Figure:
Scanning strategy on the sky (Molleweide projection): a circle
is plotted every hour. After 24 hours, the covered region has the
shape of an annulus.
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Next: Cryostat, bolometers and cold
Up: Archeops instrument
Previous: Archeops instrument
Jean-Christophe Hamilton ISN
2001-12-01