Table 8.11: Accuracy Expected in WFPC2 Observations
Procedure |
Estimated Accuracy |
Notes |
Calibration (flatfielding, bias subtraction, dark correction) |
Bias subtraction |
0.1 DN rms |
Unless bias jump is present |
Dark subtraction |
0.1 DN/hr rms |
Error larger for warm pixels; absolute error uncertain because of dark glow |
Flatfielding |
<1% rms large scale |
Visible, near UV |
0.3% rms small scale |
3-5% rms |
F218W, F255W, F300W |
5-10% rms |
F122M, F160BW, F170W, F185W; uncertain |
|
Residuals in CTE correction |
< 1% rms (above 1000 DN) |
|
3% rms (at 100 DN, <1997) |
|
3% rms (100 to 500 DN, background <1 DN/pixel, >1997) |
|
5% rms (<100 DN, background <1 DN/pixel, >1997) |
|
Long vs. short anomaly (uncorrected) |
< 1% rms (above 10000 DN) |
|
5% (at 1000 DN) |
|
15% (at 100 DN) |
|
Aperture correction |
4% rms focus dependence (1 pixel aperture) |
Can (should) be determined from data |
1-2% field dependence (1 pixel aperture) |
<1% focus dependence (> 5 pixel) |
|
Contamination correction |
3% rms max (28 days after decon) (F160BW) |
|
1% rms max (28 days after decon) (filters bluer than F555W) |
|
Background determination |
0.1 DN/pixel (background > 10 DN/pixel) |
May be difficult to exceed, regardless of image S/N |
Pixel centering |
~ 2% |
|
|
Sensitivity |
< 2% rms for standard photometric filters |
Red leaks are uncertain by ~10% |
2% rms for broad and intermediate filters in visible |
< 5% rms for narrow-band filters in visible |
2-8% rms for UV filters |
5-10% rms for linear ramp filters |
|
Relative astrometry |
0.005" rms (after geometric correction) |
Same chip |
0.15" (measured) |
Across chips |
Absolute astrometry |
1" rms (estimated) |
|
|
Fractional polarization |
1.5% rms |
Larger errors occasionally seen |