Photometry Diagnostics for lmc_u5ay02



Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u5ay0201r F555W 350.00 0.00 0.00 0.00 0.00 0.00 0.00
u5ay0202r F555W 350.00 0.04 0.02 0.00 0.00 0.04 0.02
u5ay0203r F555W 350.00 0.06 0.07 0.00 0.00 0.06 0.07
u5ay0207r F555W 10.00 5.43 5.70 5.49 5.49 -0.06 0.21
u5ay0208r F555W 350.00 5.51 5.61 5.49 5.49 0.02 0.12
u5ay0204r F814W 350.00 0.10 0.06 0.00 0.00 0.10 0.06
u5ay0205r F814W 350.00 0.07 0.10 0.00 0.00 0.07 0.10
u5ay0206r F814W 350.00 0.06 0.13 0.00 0.00 0.06 0.13
u5ay0209r F814W 10.00 5.60 5.70 5.49 5.49 0.11 0.21
u5ay020ar F814W 350.00 5.60 5.62 5.49 5.49 0.11 0.13


Mosaic images

F555W F814W


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


CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f555w
f814w


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

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


PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f555w
f814w


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

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