Photometry Diagnostics for m33_u2ab02



Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u2ab0201t F555W 600.00 0.00 0.00 0.00 0.00 0.00 0.00
u2ab0202t F555W 200.00 -0.01 -0.01 0.00 0.00 -0.01 -0.01
u2ab0203t F814W 200.00 0.04 0.11 0.00 0.00 0.04 0.11
u2ab0204t F814W 200.00 0.01 0.10 0.00 0.00 0.01 0.10
u2ab0207t F336W 200.00 -0.52 -1.07 0.00 0.00 -0.52 -1.07
u2ab0208t F336W 600.00 -0.46 -1.13 0.00 0.00 -0.46 -1.13
u2ab0205t F656N 600.00 -0.02 0.23 0.00 0.00 -0.02 0.23
u2ab0206t F656N 1000.00 -0.04 0.20 0.00 0.00 -0.04 0.20


Mosaic images

F555W F814W F336W F656N


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
f336w
f656n


CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f555w
f814w
f336w
f656n


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
F555W F814W F336W F656N

Aperture correction for each frame/chip, showing individual stars
All chips
PC
WF2
WF3
WF4
f555w
f814w
f336w
f656n


PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f555w
f814w
f336w
f656n


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
f555w
f814w
f336w
f656n

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