Photometry Diagnostics for draco_u5er14



Frame list, with derived and commanded shifts
dataset filter exptime derived dx derived dy header dx header dy delta dx delta dy
u5er1401r F606W 500.00 0.00 0.00 0.00 0.00 0.00 0.00
u5er1402r F606W 400.00 41.88 13.67 41.89 13.47 -0.01 0.20
u5er1403r F606W 400.00 -10.99 -11.20 -10.74 -11.32 -0.25 0.12
u5er1404r F606W 500.00 -22.57 6.81 -22.51 6.61 -0.06 0.20
u5er1405r F814W 500.00 24.75 7.15 24.82 6.54 -0.07 0.61
u5er1406r F814W 400.00 -2.99 38.47 -2.83 37.72 -0.16 0.75
u5er1407r F814W 500.00 -1.40 4.88 -1.19 4.36 -0.21 0.52
u5er1408r F814W 500.00 26.70 -3.77 26.78 -4.21 -0.08 0.44


Mosaic images

F606W 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
f606w
f814w


CHI vs. magnitude diagrams

All chips
PC
WF2
WF3
WF4
f606w
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
F606W F814W

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


PSF vs. aperture photometry

All chips
PC
WF2
WF3
WF4
f606w
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
f606w
f814w

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