Photometry Diagnostics for m33_u90o11



Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u90o1101m F606W 1200.00 0.00 0.00 0.00 0.00 0.00 0.00
u90o1102m F606W 1200.00 0.05 0.18 0.00 0.00 0.05 0.18
u90o1103m F606W 1200.00 5.09 -2.63 5.21 -2.61 -0.12 -0.02
u90o1104m F606W 1200.00 5.15 -2.38 5.21 -2.61 -0.06 0.23
u90o1105m F606W 600.00 5.73 1.69 5.61 1.46 0.12 0.23
u90o1106m F606W 600.00 5.74 1.76 5.61 1.46 0.13 0.30
u90o1201m F814W 1200.00 -0.21 0.74 0.00 0.00 -0.21 0.74
u90o1202m F814W 1200.00 -0.19 0.94 0.00 0.00 -0.19 0.94
u90o1203m F814W 1200.00 4.80 -1.88 5.21 -2.61 -0.41 0.73
u90o1204m F814W 1200.00 4.83 -1.62 5.21 -2.61 -0.38 0.99
u90o1205m F814W 600.00 -0.03 4.84 0.42 4.09 -0.45 0.75
u90o1206m F814W 600.00 0.02 4.97 0.42 4.09 -0.40 0.88
u90o1207m F300W 700.00 -0.99 0.61 0.00 0.00 -0.99 0.61
u90o1208m F300W 700.00 2.91 0.80 3.73 0.00 -0.82 0.80
u90o1209m F300W 700.00 6.60 0.89 7.46 -0.03 -0.86 0.92


Mosaic images

F606W F814W F300W


HSTPHOT command log

Color magnitude diagrams

All chips
PC
WF2
WF3
WF4
PSF
Aperture


Error vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w


CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w


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
F606W F814W F300W

Aperture correction for each frame/chip, showing individual stars
All chips
PC
WF2
WF3
WF4
f606w
f606w
f606w
f814w
f814w
f814w
f300w
f300w
f300w


PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w


Artificial star diagrams


Completeness as a function of input magnitude
PSF photometry Aperture photometry

Recovered mag-input mag as a function of input mag (PSF photometry)
All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w

Average recovered magnitude as function of location in CMD (PSF photometry)
PC
WF2
WF3
WF4