Photometry Diagnostics for m31_u8gpbe


Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u8gpbe01m F606W 700.00 0.00 0.00 0.00 0.00 0.00 0.00
u8gpbe02m F606W 40.00 0.04 0.00 0.00 0.00 0.04 0.00
u8gpbe05m F814W 200.00 -0.03 0.32 0.00 0.00 -0.03 0.32
u8gpbe06m F814W 100.00 -0.04 0.31 0.00 0.00 -0.04 0.31
u8gpbe07m F300W 300.00 8.14 11.65 0.00 0.00 8.14 11.65
u8gpbe08m F300W 40.00 -0.37 -0.05 0.00 0.00 -0.37 -0.05
u8gpbe09m F300W 300.00 -0.55 -0.07 0.00 0.00 -0.55 -0.07
u8gpbe03m F450W 600.00 -0.57 0.04 0.00 0.00 -0.57 0.04
u8gpbe04m F450W 40.00 -0.55 0.07 0.00 0.00 -0.55 0.07
u8gpbe0am F656N 200.00 -0.11 0.47 0.00 0.00 -0.11 0.47
u8gpbe0bm F656N 700.00 -0.13 0.40 0.00 0.00 -0.13 0.40

Mosaic images

F606W F814W F300W F450W 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
f606w
f814w
f300w
f450w
f656n

CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w
f450w
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
F606W F814W F300W F450W F656N

Aperture correction for each frame/chip, showing individual stars
All chips
PC
WF2
WF3
WF4
f606w
f606w
f814w
f814w
f300w
f300w
f300w
f450w
f450w
f656n

PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f606w
f814w
f300w
f450w
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
f606w
f814w
f300w
f450w
f656n

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