id |
Long |
unique ID |
coord |
Coord |
position in ra/dec |
parent |
Long |
unique ID of parent source |
calib.detected |
Flag |
Source was detected as an icSrc |
calib.psf.candidate |
Flag |
Flag set if the source was a candidate for PSF determination, as ... |
calib.psf.used |
Flag |
Flag set if the source was actually used for PSF determination, a ... |
flags.negative |
Flag |
set if source was detected as significantly negative |
deblend.nchild |
Int |
Number of children this object has (defaults to 0) |
deblend.deblended-as-psf |
Flag |
Deblender thought this source looked like a PSF |
deblend.psf-center |
PointD |
If deblended-as-psf, the PSF centroid |
deblend.psf-flux |
Double |
If deblended-as-psf, the PSF flux |
deblend.too-many-peaks |
Flag |
Source had too many peaks; only the brightest were included |
deblend.parent-too-big |
Flag |
Parent footprint covered too many pixels |
deblend.failed |
Flag |
Deblending failed on source |
deblend.skipped |
Flag |
Deblender skipped this source |
deblend.ramped.template |
Flag |
This source was near an image edge and the deblender used |
deblend.patched.template |
Flag |
This source was near an image edge and the deblender used |
deblend.has.stray.flux |
Flag |
This source was assigned some stray flux |
flags.badcentroid |
Flag |
the centroid algorithm used to feed centers to other algorithms f ... |
centroid.sdss |
PointD |
SDSS-algorithm centroid measurement |
centroid.sdss.err |
CovPointF |
covariance matrix for centroid.sdss |
centroid.sdss.flags |
Flag |
set if the centroid.sdss measurement did not fully succeed |
centroid.naive |
PointD |
unweighted 3x3 first moment centroid |
centroid.naive.err |
CovPointF |
covariance matrix for centroid.naive |
centroid.naive.flags |
Flag |
set if the centroid.naive measurement did not fully succeed |
flags.pixel.edge |
Flag |
source is in region labeled EDGE |
flags.pixel.interpolated.any |
Flag |
source’’s footprint includes interpolated pixels |
flags.pixel.interpolated.center |
Flag |
source’’s center is close to interpolated pixels |
flags.pixel.saturated.any |
Flag |
source’’s footprint includes saturated pixels |
flags.pixel.saturated.center |
Flag |
source’’s center is close to saturated pixels |
flags.pixel.cr.any |
Flag |
source’’s footprint includes suspected CR pixels |
flags.pixel.cr.center |
Flag |
source’’s center is close to suspected CR pixels |
flags.pixel.bad |
Flag |
source is in region labeled BAD |
flags.pixel.suspect.any |
Flag |
source’’s footprint includes suspect pixels |
flags.pixel.suspect.center |
Flag |
source’’s center is close to suspect pixels |
shape.sdss |
MomentsD |
shape measured with SDSS adaptive moment algorithm |
shape.sdss.err |
CovMomentsF |
covariance matrix for shape.sdss |
shape.sdss.flags |
Flag |
set if the shape.sdss measurement failed |
shape.sdss.centroid |
PointD |
centroid measured with SDSS adaptive moment shape algorithm |
shape.sdss.centroid.err |
CovPointF |
covariance matrix for shape.sdss.centroid |
shape.sdss.centroid.flags |
Flag |
set if the shape.sdss.centroid measurement did not fully succeed |
shape.sdss.flags.unweightedbad |
Flag |
even the unweighted moments were bad |
shape.sdss.flags.unweighted |
Flag |
adaptive moments failed; fall back to unweighted moments |
shape.sdss.flags.shift |
Flag |
centroid shifted while estimating adaptive moments |
shape.sdss.flags.maxiter |
Flag |
too many iterations for adaptive moments |
shape.sdss.psf |
MomentsD |
adaptive moments of the PSF model at the position of this object |
shape.sdss.flags.psf |
Flag |
failure in measuring PSF model shape |
flux.aperture |
ArrayD |
sum of pixels in apertures |
flux.aperture.err |
ArrayD |
uncertainty for flux.aperture |
flux.aperture.nProfile |
Int |
pixels |
flux.aperture.flags |
Flag |
success flag for flux.aperture |
flux.gaussian |
Double |
linear fit to an elliptical Gaussian with shape parameters set by ... |
flux.gaussian.err |
Double |
uncertainty for flux.gaussian |
flux.gaussian.flags |
Flag |
set if the flux.gaussian measurement failed |
flux.gaussian.psffactor |
Float |
‘’flux’’ from applying the algorithm to the PSF model |
flux.gaussian.flags.psffactor |
Flag |
set if the algorithm could not be applied to the PSF model |
flux.kron |
Double |
Kron photometry: photometry with aperture set to some multiple of ... |
flux.kron.err |
Double |
uncertainty for flux.kron |
flux.kron.flags |
Flag |
set if the flux.kron measurement failed |
flux.kron.psffactor |
Float |
‘’flux’’ from applying the algorithm to the PSF model |
flux.kron.flags.psffactor |
Flag |
set if the algorithm could not be applied to the PSF model |
flux.kron.radius |
Float |
Kron radius (sqrt(a*b)) |
flux.kron.radiusForRadius |
Float |
Radius used to estimate <radius> (sqrt(a*b)) |
flux.kron.flags.radius |
Flag |
Bad Kron radius |
flux.kron.flags.smallRadius |
Flag |
Measured Kron radius was smaller than that of the PSF |
flux.naive |
Double |
simple sum over pixels in a circular aperture |
flux.naive.err |
Double |
uncertainty for flux.naive |
flux.naive.flags |
Flag |
set if the flux.naive measurement failed |
flux.psf |
Double |
flux measured by a fit to the PSF model |
flux.psf.err |
Double |
uncertainty for flux.psf |
flux.psf.flags |
Flag |
set if the flux.psf measurement failed |
flux.psf.psffactor |
Float |
‘’flux’’ from applying the algorithm to the PSF model |
flux.psf.flags.psffactor |
Flag |
set if the algorithm could not be applied to the PSF model |
flux.sinc |
Double |
elliptical aperture photometry using sinc interpolation |
flux.sinc.err |
Double |
uncertainty for flux.sinc |
flux.sinc.flags |
Flag |
set if the flux.sinc measurement failed |
correctfluxes.apcorr |
Float |
correction applied to model fluxes to match to 7.000000-pixel ape ... |
correctfluxes.apcorr.flags |
Flag |
flag set if aperture correction failed |
focalplane |
PointF |
Focal plane position |
jacobian |
Double |
Jacobian correction |
classification.extendedness |
Double |
probability of being extended |
classification.exposure.photometric |
Flag |
set if source was used in photometric calibration |
classification.photometric |
Flag |
set if source was used in photometric calibration |