LAST_DP_PipeI_BitMask - EranOfek/AstroPack GitHub Wiki

LAST bit mask description

The images are accompanied by 32-bit mask images. Each pixel contains information about possible problems. In addition, the bitmask are propagated to the source catalogs and stored in the FLAGS column. For each source, the propagation is done using the OR operator for all the pixels found within a 3 pixel radius from the source position.

Bit mask description

Bit name Bit index Used Description
Saturated 0 T Pixel is saturated.
LowRN 1 T Pixel noise is low, Var < median(Var) * 0.03; probably a dead pixel.
HighRN 2 T Pixel noise is high, Var > 20 * median(Var); noisy pixel.
DarkHighVal 3 T Pixel bias/dark value is high, > 2 * Mean.
DarkLowVal 4 T Pixel bias/dark value is low, < 0.3 * Mean.
BiasFlaring 5 T Pixel is possibly flaring, > 20 sigma.
NaN 6 T Pixel is NaN due to illegal arithmetic operations.
FlatHighStd 7 T Flat standard error is high, Std / sqrt(N) > 0.01.
FlatLowVal 8 T Flat normalized value is low, < 0.3.
LowQE 9 T Pixel has low quantum efficiency, < 0.5 of the nominal value.
Negative 10 T Negative pixel after processing.
Interpolated 11 F Pixel value was interpolated.
Hole 12 T Hole, or anti-star.
Spike 13 F Diffraction spike.
CR_DeltaHT 14 T Cosmic ray identified using hypothesis testing against a delta function.
CR_Laplacian 15 F Cosmic ray identified using a Laplacian filter.
CR_Streak 16 F Cosmic-ray streak.
Ghost 17 F Ghost.
Persistent 18 F Persistent charge.
Xtalk 19 F Cross talk.
Streak 20 T Streak.
ColumnLow 21 F Bad column with low values.
ColumnHigh 22 F Bad column with high values.
NearEdge 23 T Pixel is near the image edge.
NonLinear 24 T Non-linear pixel response.
Bleeding 25 F Possible bleeding/blooming.
Overlap 26 T Pixel is in an overlap region.
SrcNoiseDominated 27 T (coadd) Source-noise-dominated pixel, (Val - Back) > Back.
GainHigh 28 F In dual-gain detectors: high-gain state.
CoaddLessImages 29 T Number of images contributing to the coadd is less than X percent.
SrcDetected 30 F Source detected; all pixels within a 1-FWHM radius from the detected source.
31 F Unused