Quality Team Report
02/27/2007

Source: BHR14

AOR ID:	IRAC: 0005095168
	MIPS: 0009414912

Observation Dates: IRAC: 5/1/04	
		   MIPS: 4/13/04

Observing Strategy:

            IRAC: 1 epoch, 4 dithers each, 12 sec integration per exposure

            MIPS: 1 epoch, 24: 1 cycle of 3 sec exposures, large field size,
	    	           70: 1 cycle of 10 sec exposures, small field size,
			       1 map of 3 columns & 1 rows

Processing History (software version):

IRAC SSC: S13.2.0
MIPS SSC: S13.2.0
IRAC CC: v2
MIPS CC: v4
IRAC Map1: v11292006
MIPS Map1: v11292006
Map2: v6.6

Comments:

Extended emission in 70um may make the self-flatting dubious

Significant muxbleed and associated pinstriping, along with column pull-down,
from bright stars is present in IRAC bands 1 and 2.

Significant optical banding around bright stars is present in IRAC bands 3
and 4. 
### Catalog Statistics ###

# Total Number of sources: 1068 (1068 with epoch 3 detections)
2MASS:     237   22.2%
IRAC1:     599   56.1%
IRAC2:     584   54.7%
IRAC3:     221   20.7%
IRAC4:      93    8.7%
MIPS1:     166   15.5%

Number of sources detected in X 2MASS/IRAC/MIPS24 bands:
1 band:    477   44.7%
2 band:    313   29.3%
3 band:    146   13.7%
4 band:     34    3.2%
5 band:     20    1.9%
6 band:     25    2.3%
7 band:     45    4.2%
8 band:      8    0.7%

Sources detected in 3+ bands: 278
              Total            IRAC
2MASS:      83   29.9%        1    0.5%
Stars:     141   50.7%      133   70.7%
YSOc :       1    0.4%        1    0.5%
Galc :       2    0.7%        2    1.1%
Other:      51   18.3%       51   27.1%