COMICS camera filters

The 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.

Filter Wavelength (um) Sensitivity (1sig 1sec) Diffraction
limit(1)
Centre Width (mJy) (mJy/arcsec2)
N-band continuum filters
N8.8 8.8     0.8 67 420 0.27
N9.7 9.7     0.9 41 320 0.29
N10.5 10.5     1.0 58 550 0.32
N11.7 11.7     1.0 25 300 0.36
N12.4 12.4     1.2 55 680 0.38
N-band narrow filters
UIR8.6 8.59     0.42 29 520 0.26
ArIII 8.98     0.13 35 590 0.28
SIV 10.46     0.16 40 680 0.32
UIR11.2 11.24     0.60 32 530 0.35
NeII 12.81     0.21 75 1200 0.39
Q-band filters
Q17.7 17.7     0.9 320 TBD 0.54
Q18.8 18.8     0.9 360 TBD 0.58
Q20.5(2) 20.5     0.9 820(3) TBD 0.63
Q24.5 24.5     1.9 1100 TBD 0.75

(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



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