The Wide Field Camera (WFC) is an optical mosaic camera for use at the prime focus of the
2.5m
Isaac Newton Telescope (INT).
The WFC consists of 4 thinned EEV 2kx4k CCDs. The CCDs have a pixel
size of 13.5 microns corresponding to 0.33 arcsec/pixel. The edge to edge limit
of the mosaic, neglecting the ~1 arcmin inter-chip spacing, is 34.2 arcmins.
The cycle time for the whole mosaic is around 42 seconds.
Both broadband and Stromgren filtersets are available, as well as a
range of narrowband filters.
IMPORTANT: in case a long run is going to be covered by several observers, please let us know well in
advance so that student support can be scheduled each time a new team goes up.
News:
August 2010: On a shared-risk basis, binning is supported for all chips and windowing and/or binning are supported for chip 4 only
(more info here).
December 2006: New narrowband filters:
Filter name
|
Central
lambda
[Angstrom]
|
FWHM
[Angstrom]
|
Peak
Transmission
[%]
|
Hbeta narrow
|
4861
|
30
|
|
Hbeta broad
|
4861
|
170
|
|
He I
|
5869
|
43
|
87
|
Ha redshifted #227
|
6657
|
79
|
90
|
Ha redshifted #228
|
6805
|
93
|
95
|
Ha redshifted #226
|
6892
|
99
|
90
|
