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COMICS camera filtersThe following table lists the filters available in the camera section of COMICS, together with their sensitivities (noise equivalent flux densities). All sensitivities are for 1 sigma detections in 1 second of background-limited on-source integration. Extended source sensitivities are per arcsec2. Important: Sensitivities assume chopping only; limiting fluxes will be sqrt(2) times higher if chopping and nodding are required. You must read the information on Overheads and observing technique before planning your observations.
(1) The diffraction-limited image size (in arcseconds) for an 8.2-m telescope. (2) New filter installed in February 2004, replacig the old Q20.8-filter. Its sensitivity is yet to be measured, however, we are making it available for Open Use on a shared-risk basis. It is expected (based on its transmission curve and the theoretical atmospheric transparency in the relevant wavelength range) that its sensitivity will be similar to, or perhaps a little better than, that for the old Q20.8 with only a minor shift in the central wavelength (its width is more or less the same as that of the old Q20.8). (3) These values are for the old Q20.8-filter [see (2) above]. August 2004 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||