Armed with the characterization of the background level (see § 4.4), we can proceed to estimate the required exposure time. The first stop is the IRAC webpage for the instrument sensitivity. See:
For IRAC, the current estimate of the
confusion limit is
(this does not represent a hard
sensitivity limit, but rather indicates where source confusion affects the
reliability of source extractions; see the IRAC chapter of the SOM for
more information). At 3.6 microns, we reach the limit quickly: with a
single cycle of the 100 sec frame time for low background. The longest
IRAC waveband, 8 microns, reaches the confusion limit last, requiring
total integration (for low background) to be
confusion limited. See the SOM for more information.
We determine the exposure time required for this proposal to reach
at 8 microns. For medium background, with a
100 sec frame time4.3, the
IRAC point-source
sensitivity is
for the
3.6, 4.5, 5.8 and 8.0 micron bands respectively. For long frame times,
the noise essentially scales with
. Hence, to reach
in the 8.0 micron band, we require
One word of caution however: while our science goal is to probe deeply
at 8 microns, the 3.6 and 4.5 micron arrays will be well below the
confusion limit with
Since the 3.6 and 5.8 arrays are paired (data are obtained in both arrays
simultaneously), and similarly for the 4.5 and 8 micron arrays. So, if
we also want (for whatever scientific reasons) the deep 5.8 micron data
from 49 repeats of the 100 sec frame time, we must be aware that we will
not be increasing the S/N as
in the 3.6 micron data
once the confusion limit is reached in that waveband. A similar argument
applies for 4.5 micron data, while we collect the deep 8 micron data.
Gillian Wilson 2006-11-09