Photometry Diagnostics for lmc_u3y501

Frame list, with derived and commanded shifts

dataset	filter	exptime	derived dx	derived dy	header dx	header dy	delta dx	delta dy
u3y50101m	F555W	30.00	0.00	0.00	0.00	0.00	0.00	0.00
u3y50102m	F555W	500.00	-11.06	-5.69	-10.98	-5.49	-0.08	-0.20
u3y50103m	F555W	500.00	-16.60	-16.56	-16.47	-16.48	-0.13	-0.08
u3y50104m	F555W	500.00	-5.66	-10.97	-5.49	-10.99	-0.17	0.02
u3y5010hm	F555W	500.00	-0.02	0.04	0.00	0.00	-0.02	0.04
u3y5010im	F555W	30.00	-11.05	-5.58	-10.98	-5.49	-0.07	-0.09
u3y5010jm	F555W	30.00	-16.60	-16.58	-16.47	-16.48	-0.13	-0.10
u3y5010km	F555W	30.00	-5.65	-10.98	-5.49	-10.99	-0.16	0.01
u3y50109m	F814W	30.00	0.11	0.00	0.00	0.00	0.11	0.00
u3y5010am	F814W	500.00	-10.96	-5.56	-10.98	-5.49	0.02	-0.07
u3y5010bm	F814W	500.00	-16.65	-16.62	-16.47	-16.48	-0.18	-0.14
u3y5010cm	F814W	500.00	-5.44	-10.94	-5.49	-10.99	0.05	0.05
u3y5010dm	F814W	500.00	0.12	0.01	0.00	0.00	0.12	0.01
u3y5010em	F814W	30.00	-10.91	-5.57	-10.98	-5.49	0.07	-0.08
u3y5010fm	F814W	30.00	-16.51	-16.54	-16.47	-16.48	-0.04	-0.06
u3y5010gm	F814W	30.00	-5.40	-10.97	-5.49	-10.99	0.09	0.02
u3y50105m	F675W	30.00	-0.46	0.97	0.00	0.00	-0.46	0.97
u3y50106m	F675W	500.00	-11.45	-4.55	-10.98	-5.49	-0.47	0.94
u3y50107m	F675W	500.00	-17.20	-15.56	-16.47	-16.48	-0.73	0.92
u3y50108m	F675W	500.00	-6.09	-10.00	-5.49	-10.99	-0.60	0.99
u3y5010lm	F675W	500.00	-0.50	0.96	0.00	0.00	-0.50	0.96
u3y5010mm	F675W	30.00	-11.47	-4.54	-10.98	-5.49	-0.49	0.95
u3y5010nm	F675W	30.00	-17.18	-15.56	-16.47	-16.48	-0.71	0.92
u3y5010om	F675W	30.00	-6.11	-10.09	-5.49	-10.99	-0.62	0.90

Mosaic images

F555W	F814W	F675W

HSTPHOT command log

Color magnitude diagrams

	All chips	PC	WF2	WF3	WF4
PSF
Aperture

Error vs. magnitude diagrams

	All chips	PC	WF2	WF3	WF4
f555w
f814w
f675w

CHI vs. magnitude diagrams

	All chips	PC	WF2	WF3	WF4
f555w
f814w
f675w

Aperture corrections

Aperture corrections compared with those of entire database (green points are this field)
If aperture corrections appear to be significant outliers in the global trend, you should be cautious about their quality, and consider that the zeropoints of photometry and colors are more suspect