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MegaPrime is the wide-field optical imaging facility at CFHT. It represented
a major upgrade of the telescope upper-end as well as the largest astronomical
CCD mosaic ever built at the time of the official first light in January 2003
and for many years that followed.
The wide-field imager, MegaCam (built by CEA, France),
consists of 36 2048 x 4612 pixel CCDs (a total of 340 megapixels),
covering a full 1 degree x 1 degree field-of-view with a resolution of
0.187 arcsecond per pixel to properly sample the 0.7 arcsecond median seeing
offered by the CFHT at Mauna Kea. The new prime focus upper end includes
an image stabilization unit and a guide/autofocus unit with two independent
guide CCD detectors.
MegaPrime is an optical & near infrared instrument mounted on the telescope
for 15 to 18 days periods centered on the New Moon. It uses
most of the telescope dark and grey time to conduct the typical Principal
Investigators scientific programs and the CFHT Legacy Survey
which represents by itself a total of 450 nights committed over five years,
starting in 2003.
MegaPrime/MegaCam is operated exclusively through the CFHT New Observing
Process (NOP). Observations are carried out through Queued Service
Observing (QSO), the data are preprocessed (removal of the instrumental
signature) and calibrated (photometry and astrometry) by Elixir, and
eventually sent to the Principal Investigators on tapes by the
Data Archiving & Distribution System (DADS). The raw data are archived
at the Canadian Astronomy Data Centre (CADC) in Victoria, and become
public after a one year proprietary period (except for the CFHTLS data).
The Terapix data processing center based in Paris, primarily focused on
handling the CFHTLS data, also proposes its services to the whole CFHT community
with the data stacking, fine astrometric calibration and catalogs generation.
MegaPrime is a CFHT project, funded through the instrumentation fund
by the Canadian and French Agencies (NRC and CNRS/INSU). The
Observatoire de Paris and HIA (Victoria) have been contracted for
the design and fabrication of some of the MegaPrime components.
MegaCam was built in France by CEA. The section
"Instrument Description"
covers in detail the various parts of the instrument and the entities
responsible for building them.
Note to the Principal Investigators preparing a time proposal:
All the information relevant to the preparation of a time proposal
and/or preparing the time distribution for the QSO's PH2 phase can be
found in the "Specifications & Performance" and " New Observing Process"
sections of the left menu (instrument specifications, exposure time
calculator, etc...).
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