Observing

Available Filters

Available filters are shown in the table below. An ND filter with OD=1 is assumed to be used for observing in the 9.8-um band to avoid saturation.

NameCenter wavelength
(um)
Band width
(FWHM; um)
Note
7.7um7.670.21
9.8um+OD19.610.96OD1 means an ND filter with OD=1 required to avoid saturation.
11.5um11.51.02
13.1um13.10.6
16.7um16.710.43
17.8um17.870.83
20.9um20.861.73
24.5um24.971.94

Saturation limit

Saturation limits are calculated as shown in the Table below. The range of values shown for many bands indicates the variable range depending on PWV (assuming 0.3 to 1.5 mm). ND filters with other ODs may be available. By using ND filters or performing defocused observations, objects brighter than the flux densities below, although such observations require special care for calibration.

NameSaturation limit
7.7um900-1100 Jy
9.8um+OD12000 Jy
11.5um210 Jy
13.1um580 Jy
16.7um8300-9500 Jy
17.8um3000-3500 Jy
20.9um1300-1700 Jy
24.5um3700-5700 Jy

Sensitivity

Noise-equivalent flux density for one exposure is calculated as shown in the figures below. Corresponding 1-sigma 1-sec sensitivity is also plotted. This calculation assumes aperture photometry with an aperture diameter of 2.5 times the FWHM of the PSF in the medium seeing condition (see here). Since readout noise (assumed 4000e-/read) is the main noise source in short exposures, sensitivity improves with longer exposure times. In the bands at 7.7 um and in the Q band, significant PWV dependency is confirmed. The truncation in the right edge of each band shows the longest exposure time. For accurate subtraction of background emission, it may be better to limit the exposure time for one exposure to less than 0.20 sec.

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Noise equivalent flux density for one exposure in the N band. Corresponding 1-sigma 1-sec sensitivity is shown by dotted lines. Multiple lines for each filter set show different PWV conditions (from bottom to top, 0.3, 0.5, 0.7, 0.9, 1.2, and 1.5 mm).Same as the left figure, but for the Q band.

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