Photometry Diagnostics for mw_bulge_u2c901



Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u2c90101t F555W 300.00 0.00 0.00 0.00 0.00 0.00 0.00
u2c90102t F555W 1000.00 0.01 0.04 0.00 0.00 0.01 0.04
u2c90103t F555W 1000.00 -0.07 0.05 0.00 0.00 -0.07 0.05
u2c90104t F555W 1000.00 -0.10 0.07 0.00 0.00 -0.10 0.07
u2c90105t F555W 10.00 -0.08 0.10 0.00 0.00 -0.08 0.10
u2c90106t F814W 100.00 0.05 0.15 0.00 0.00 0.05 0.15
u2c90107t F814W 1000.00 0.04 0.02 0.00 0.00 0.04 0.02
u2c90108t F814W 1000.00 0.03 0.08 0.00 0.00 0.03 0.08
u2c90109t F814W 1000.00 0.06 0.08 0.00 0.00 0.06 0.08
u2c9010at F814W 10.00 0.05 0.09 0.00 0.00 0.05 0.09
u2c9010bt F439W 100.00 -0.27 -0.19 0.00 0.00 -0.27 -0.19
u2c9010ct F439W 100.00 -0.32 -0.15 0.00 0.00 -0.32 -0.15
u2c9010dt F439W 1000.00 -0.28 -0.09 0.00 0.00 -0.28 -0.09


Mosaic images

F555W F814W F439W


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
f439w


CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f555w
f814w
f439w


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 F439W

Aperture correction for each frame/chip, showing individual stars
All chips
PC
WF2
WF3
WF4
f555w
f555w
f555w
f814w
f814w
f814w
f439w
f439w


PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f555w
f814w
f439w


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
f439w

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