QA for run 3606 (rerun 40, strip 28N), fields: 11-166

The Estimates of Photometric Zeropoint Errors:

Zeropoint corrections to flatten background

	Zeropoint Corrections to Flatten Background
band:	u	g	r	i	z
Col. 1	0.023*	0.009	0.017	0.004	0.016
Col. 2	-0.005	-0.006	-0.009	0.001	-0.011
Col. 3	0.006	0.005	0.013	0.006	-0.013
Col. 4	0.023*	0.009	0.003	0.002	0.005
Col. 5	-0.034*	-0.028*	-0.005	-0.020	-0.030
Col. 6	-0.032*	-0.016	-0.002	0.004	0.002

*Red entries are triggered by abs(entry) > (0.02 0.02 0.02 0.02 0.03) in (u g r i z)
The table above lists the photometric zeropoint corrections
required for a flat background across all camera columns.

Zeropoint corrections from principal colors

	Zeropoint Corrections to Fix Principal Colors
band:	u	g	r	i	z
Col. 1	0.037*	0.012	-0.005	-0.007	-0.009
Col. 2	0.070*	0.011	0.004	-0.015	-0.028
Col. 3	0.059*	0.018	-0.005	-0.012	0.012
Col. 4	0.042*	0.005	0.000	-0.005	-0.009
Col. 5	0.052*	0.012	-0.013	0.001	0.001
Col. 6	0.033*	0.008	-0.003	-0.006	-0.009

*Red entries are triggered by abs(entry) > (0.02 0.02 0.02 0.02 0.03) in (u g r i z)
The table above lists the photometric zeropoint corrections
required to make the median principal colors (for all fields in
a camera column) to be 0 (assuming that errors in gri add up to 0)

	Mean Values for All Columns
QUANTITY	u	g	r	i	z
Sky: RMS	0.002	0.002	0.001	0.001	0.002
Sky: Max Dev	0.006	0.008	0.005	0.004	0.006
m(apert7)-m(psf): Max Dev	0.161*	0.059*	0.145*	0.070*	0.067
m(apert7)-m(psf): Med Off	0.012*	0.005	0.004	0.003	0.008
m(apert7)-m(psf): RMS	0.016	0.009	0.008	0.007	0.010
m(mod)-m(psf): Max Dev	0.080	0.057*	0.163*	0.132*	0.208*
m(mod)-m(psf): Med Off	0.004	0.006	0.003	0.003	0.003
m(mod)-m(psf): RMS	0.009	0.008	0.007	0.006	0.007

Click here for expanded tables with links to plots.

Relative Astrometry, mean values for 6 columns: