| Version 6 (modified by , 14 years ago) ( diff ) |
|---|
SAS 9 FLAGS
There is a flag page here: http://web01.psps.ifa.hawaii.edu/psps-trac/wiki/PSPSFAQ which is out of date.
Some decent description of the flags (but warning these are out of date, just use for more explanations than given below)
Here is the short version (who has flags and where they come from)
| type | flags column name | definition |
| detectionfull | infoFlag | DVO dbflags << 32 | smf FLAGS |
| stackdetectionfull | infoFlag | cmf FLAGS2 << 32 | cmf FLAGS |
| objects | objInfoFlag | FLAGS from the DVO 'average' |
| objects | xFlag | FLAGS from the DVO 'secfilt' |
- dvo flags come from: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/browser/trunk/Ohana/src/libdvo/include/dvo.h
- smf/cmf flags come from: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/browser/trunk/psModules/src/objects/pmSourceMasks.h
Below is each of the current flags (for sa9)
DetectionFull.infoFlags (these are the dvo dbflags << 32)
ID_MEAS_NOCAL = 0x00000001, // detection ignored for this analysis (photcode, time range) -- internal only ID_MEAS_POOR_PHOTOM = 0x00000002, // detection is photometry outlier ID_MEAS_SKIP_PHOTOM = 0x00000004, // detection was ignored for photometry measurement ID_MEAS_AREA = 0x00000008, // detection near image edge ID_MEAS_POOR_ASTROM = 0x00000010, // detection is astrometry outlier ID_MEAS_SKIP_ASTROM = 0x00000020, // detection was ignored for astrometry measurement ID_MEAS_USED_OBJ = 0x00000040, // detection was used during update objects ID_MEAS_USED_CHIP = 0x00000080, // detection was used during update chips (XXX this probably does not make it into the db) ID_MEAS_BLEND_MEAS = 0x00000100, // detection is within radius of multiple objects ID_MEAS_BLEND_OBJ = 0x00000200, // multiple detections within radius of object ID_MEAS_UNDEF_3 = 0x00000400, // unused ID_MEAS_UNDEF_4 = 0x00000800, // unused ID_MEAS_BLEND_MEAS_X = 0x00001000, // detection is within radius of multiple objects across catalogs ID_MEAS_ARTIFACT = 0x00002000, // detection is thought to be non-astronomical ID_MEAS_UNDEF_5 = 0x00004000, // unused ID_MEAS_PHOTOM_UBERCAL = 0x00008000, // externally-supplied zero point from ubercal analysis ID_MEAS_STACK_PRIMARY = 0x00010000, // externally-supplied zero point from ubercal analysis
DetectionFull.infoFlags (these are FLAGs from smf)
FLAGS
PM_SOURCE_MODE_DEFAULT = 0x00000000, ///< Initial value: resets all bits PM_SOURCE_MODE_PSFMODEL = 0x00000001, ///< Source fitted with a psf model (linear or non-linear) PM_SOURCE_MODE_EXTMODEL = 0x00000002, ///< Source fitted with an extended-source model PM_SOURCE_MODE_FITTED = 0x00000004, ///< Source fitted with non-linear model (PSF or EXT; good or bad) PM_SOURCE_MODE_FAIL = 0x00000008, ///< Fit (non-linear) failed (non-converge, off-edge, run to zero) PM_SOURCE_MODE_POOR = 0x00000010, ///< Fit succeeds, but low-SN, high-Chisq, or large (for PSF -- drop?) PM_SOURCE_MODE_PAIR = 0x00000020, ///< Source fitted with a double psf PM_SOURCE_MODE_PSFSTAR = 0x00000040, ///< Source used to define PSF model PM_SOURCE_MODE_SATSTAR = 0x00000080, ///< Source model peak is above saturation PM_SOURCE_MODE_BLEND = 0x00000100, ///< Source is a blend with other sources PM_SOURCE_MODE_EXTERNAL = 0x00000200, ///< Source based on supplied input position PM_SOURCE_MODE_BADPSF = 0x00000400, ///< Failed to get good estimate of object's PSF PM_SOURCE_MODE_DEFECT = 0x00000800, ///< Source is thought to be a defect PM_SOURCE_MODE_SATURATED = 0x00001000, ///< Source is thought to be saturated pixels (bleed trail) PM_SOURCE_MODE_CR_LIMIT = 0x00002000, ///< Source has crNsigma above limit PM_SOURCE_MODE_EXT_LIMIT = 0x00004000, ///< Source has extNsigma above limit PM_SOURCE_MODE_MOMENTS_FAILURE = 0x00008000, ///< could not measure the moments PM_SOURCE_MODE_SKY_FAILURE = 0x00010000, ///< could not measure the local sky PM_SOURCE_MODE_SKYVAR_FAILURE = 0x00020000, ///< could not measure the local sky variance PM_SOURCE_MODE_BELOW_MOMENTS_SN = 0x00040000, ///< moments not measured due to low S/N PM_SOURCE_MODE_BIG_RADIUS = 0x00100000, ///< poor moments for small radius, try large radius PM_SOURCE_MODE_AP_MAGS = 0x00200000, ///< source has an aperture magnitude PM_SOURCE_MODE_BLEND_FIT = 0x00400000, ///< source was fitted as a blend PM_SOURCE_MODE_EXTENDED_FIT = 0x00800000, ///< full extended fit was used PM_SOURCE_MODE_EXTENDED_STATS = 0x01000000, ///< extended aperture stats calculated PM_SOURCE_MODE_LINEAR_FIT = 0x02000000, ///< source fitted with the linear fit PM_SOURCE_MODE_NONLINEAR_FIT = 0x04000000, ///< source fitted with the non-linear fit PM_SOURCE_MODE_RADIAL_FLUX = 0x08000000, ///< radial flux measurements calculated PM_SOURCE_MODE_SIZE_SKIPPED = 0x10000000, ///< size could not be determined PM_SOURCE_MODE_ON_SPIKE = 0x20000000, ///< peak lands on diffraction spike PM_SOURCE_MODE_ON_GHOST = 0x40000000, ///< peak lands on ghost or glint PM_SOURCE_MODE_OFF_CHIP = 0x80000000, ///< peak lands off edge of chip
StackDetectionFull.infoFlags (FLAGS2 << 32 | FLAGS )
FLAGS
PM_SOURCE_MODE_DEFAULT = 0x00000000, ///< Initial value: resets all bits PM_SOURCE_MODE_PSFMODEL = 0x00000001, ///< Source fitted with a psf model (linear or non-linear) PM_SOURCE_MODE_EXTMODEL = 0x00000002, ///< Source fitted with an extended-source model PM_SOURCE_MODE_FITTED = 0x00000004, ///< Source fitted with non-linear model (PSF or EXT; good or bad) PM_SOURCE_MODE_FAIL = 0x00000008, ///< Fit (non-linear) failed (non-converge, off-edge, run to zero) PM_SOURCE_MODE_POOR = 0x00000010, ///< Fit succeeds, but low-SN, high-Chisq, or large (for PSF -- drop?) PM_SOURCE_MODE_PAIR = 0x00000020, ///< Source fitted with a double psf PM_SOURCE_MODE_PSFSTAR = 0x00000040, ///< Source used to define PSF model PM_SOURCE_MODE_SATSTAR = 0x00000080, ///< Source model peak is above saturation PM_SOURCE_MODE_BLEND = 0x00000100, ///< Source is a blend with other sources PM_SOURCE_MODE_EXTERNAL = 0x00000200, ///< Source based on supplied input position PM_SOURCE_MODE_BADPSF = 0x00000400, ///< Failed to get good estimate of object's PSF PM_SOURCE_MODE_DEFECT = 0x00000800, ///< Source is thought to be a defect PM_SOURCE_MODE_SATURATED = 0x00001000, ///< Source is thought to be saturated pixels (bleed trail) PM_SOURCE_MODE_CR_LIMIT = 0x00002000, ///< Source has crNsigma above limit PM_SOURCE_MODE_EXT_LIMIT = 0x00004000, ///< Source has extNsigma above limit PM_SOURCE_MODE_MOMENTS_FAILURE = 0x00008000, ///< could not measure the moments PM_SOURCE_MODE_SKY_FAILURE = 0x00010000, ///< could not measure the local sky PM_SOURCE_MODE_SKYVAR_FAILURE = 0x00020000, ///< could not measure the local sky variance PM_SOURCE_MODE_BELOW_MOMENTS_SN = 0x00040000, ///< moments not measured due to low S/N PM_SOURCE_MODE_BIG_RADIUS = 0x00100000, ///< poor moments for small radius, try large radius PM_SOURCE_MODE_AP_MAGS = 0x00200000, ///< source has an aperture magnitude PM_SOURCE_MODE_BLEND_FIT = 0x00400000, ///< source was fitted as a blend PM_SOURCE_MODE_EXTENDED_FIT = 0x00800000, ///< full extended fit was used PM_SOURCE_MODE_EXTENDED_STATS = 0x01000000, ///< extended aperture stats calculated PM_SOURCE_MODE_LINEAR_FIT = 0x02000000, ///< source fitted with the linear fit PM_SOURCE_MODE_NONLINEAR_FIT = 0x04000000, ///< source fitted with the non-linear fit PM_SOURCE_MODE_RADIAL_FLUX = 0x08000000, ///< radial flux measurements calculated PM_SOURCE_MODE_SIZE_SKIPPED = 0x10000000, ///< size could not be determined PM_SOURCE_MODE_ON_SPIKE = 0x20000000, ///< peak lands on diffraction spike PM_SOURCE_MODE_ON_GHOST = 0x40000000, ///< peak lands on ghost or glint PM_SOURCE_MODE_OFF_CHIP = 0x80000000, ///< peak lands off edge of chip
FLAGS2
PM_SOURCE_MODE2_DEFAULT = 0x00000000, ///< Initial value: resets all bits
PM_SOURCE_MODE2_DIFF_WITH_SINGLE = 0x00000001, ///< diff source matched to a single positive detection
PM_SOURCE_MODE2_DIFF_WITH_DOUBLE = 0x00000002, ///< diff source matched to positive detections in both images
PM_SOURCE_MODE2_MATCHED = 0x00000004, ///< diff source matched to positive detections in both images
PM_SOURCE_MODE2_ON_SPIKE = 0x00000008, ///< > 25% of (PSF-weighted) pixels land on diffraction spike
PM_SOURCE_MODE2_ON_STARCORE = 0x00000010, ///< > 25% of (PSF-weighted) pixels land on starcore
PM_SOURCE_MODE2_ON_BURNTOOL = 0x00000020, ///< > 25% of (PSF-weighted) pixels land on burntool
PM_SOURCE_MODE2_ON_CONVPOOR = 0x00000040, ///< > 25% of (PSF-weighted) pixels land on convpoor
PM_SOURCE_MODE2_PASS1_SRC = 0x00000080, ///< source detected in first pass analysis
PM_SOURCE_MODE2_HAS_BRIGHTER_NEIGHBOR = 0x00000100, ///< peak is not the brightest in its footprint
PM_SOURCE_MODE2_BRIGHT_NEIGHBOR_1 = 0x00000200, ///< flux_n / (r^2 flux_p) > 1
PM_SOURCE_MODE2_BRIGHT_NEIGHBOR_10 = 0x00000400, ///< flux_n / (r^2 flux_p) > 10
PM_SOURCE_MODE2_DIFF_SELF_MATCH = 0x00000800, ///< positive detection match is probably this source
PM_SOURCE_MODE2_SATSTAR_PROFILE = 0x00001000, ///< saturated source is modeled with a radial profile
Object.objInfoFlags
ID_STAR_FEW = 0x00000001, // used within relphot: skip star ID_STAR_POOR = 0x00000002, // used within relphot: skip star * ID_PROPER = 0x00000400, // star with large proper motion * ID_TRANSIENT = 0x00001000, // is this mutually exclusive with USNO? * ID_VARIABLE = 0x00002000, // not currently set? * ID_ASTEROID = 0x00002000, // identified with an asteroid * ID_BAD_OBJECT = 0x00004000, // if all measurements are bad, set this bit * ID_MOVING = 0x00008000, // is a moving object * ID_ROCK = 0x0000a000, // 0x8000 + 0x2000 * ID_GHOST = 0x0000c001, // 0x8000 + 0x4000 + 0x0001 * ID_TRAIL = 0x0000c002, // 0x8000 + 0x4000 + 0x0002 * ID_BLEED = 0x0000c003, // 0x8000 + 0x4000 + 0x0003 * ID_COSMIC = 0x0000c004, // 0x8000 + 0x4000 + 0x0004 ID_STAR_FIT_AVE = 0x00010000, // average position fitted ID_STAR_FIT_PM = 0x00020000, // proper motion fitted ID_STAR_FIT_PAR = 0x00040000, // parallax fitted ID_STAR_USE_AVE = 0x00080000, // average position used (not PM or PAR) ID_STAR_USE_PM = 0x00100000, // proper motion used (not AVE or PAR) ID_STAR_USE_PAR = 0x00200000, // parallax used (not AVE or PM) ID_STAR_NO_ASTROM = 0x00400000, // mean astrometry could not be measured ID_OBJ_EXT = 0x01000000, // extended in our data (eg, PS) ID_OBJ_EXT_ALT = 0x02000000, // extended in external data (eg, 2MASS) ID_OBJ_GOOD = 0x04000000, // good-quality measurement in our data (eg,PS) ID_OBJ_GOOD_ALT = 0x08000000, // good-quality measurement in external data (eg, 2MASS)
the items marked * are deprecated and not set in sa9. They are here for historical purposes.
Object.xFlags
ID_SECF_STAR_FEW = 0x00000001, // used within relphot: skip star ID_SECF_STAR_POOR = 0x00000002, // used within relphot: skip star ID_SECF_USE_SYNTH = 0x00000004, // synthetic photometry used in average measurement ID_SECF_USE_UBERCAL = 0x00000008, // synthetic photometry used in average measurement ID_SECF_HAS_PS1 = 0x00000010, // PS1 photometry used in average measurement ID_SECF_HAS_STACK = 0x00000020, // PS1 stack photometry exists ID_PHOTOM_PASS_0 = 0x00000100, // average magnitude calculated in 0th pass ID_PHOTOM_PASS_1 = 0x00000200, // average magnitude calculated in 1th pass ID_PHOTOM_PASS_2 = 0x00000400, // average magnitude calculated in 2th pass ID_PHOTOM_PASS_3 = 0x00000800, // average magnitude calculated in 3th pass ID_PHOTOM_PASS_4 = 0x00001000, // average magnitude calculated in 4th pass ID_PSPS_OBJ_EXT = 0x00002000, // extended in this band (PSPS only) ID_SECF_OBJ_EXT = 0x01000000, // DVO location of "extended in this band" For PSPS this bit is moved
The gap between ID_SECF_HAS_STACK and ID_PHOTOM_PASS_0 is intentional (the bits between are not used)
Note: ID_PSPS_OBJ_EXT contains the value of the bit ID_SECF_OBJ_EXT in DVO. For PSPS it is moved to fit into the 16 bit Object.xFlags
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