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Algorithms in SDSS DR8
This page contains detailed information about the algorithms used to process SDSS-III data.
General
Bitmasks
Survey coordinates
Images
Imaging quality flags
Astrometric calibration
Sky measurement
Creation of imaging masks
DR7 Photometry QA description
(at DR7 site)
Target selection
Legacy Target selection
Main Galaxy Sample
Luminous Red Galaxies (LRG)
Quasars
Stars
ROSAT All-Sky Survey sources
Serendipity
SEGUE Target Selection
Special Target selection
Legacy tiling
(assigning fibers & plate centers)
Spectroscopy
Wavelength Calibration
Spectrophotometry
Redshifts, classification, velocity dispersion
Stellar parameters (SSPP)
(in spectro pages)
Matching spectroscopy to photometry
Image catalogs
Photometric processing flags
IMPORTANT!
Recommendations
Summary of flags
Photometric flags detail
Full flag details
(link to Lupton's page)
Resolve
(removing repeat observations)
Magnitudes
Fiber
Model
cModel
Petrosian
PSF
Radial Profiles
Which magnitude should I use?
Classification & Morphology
Star/Galaxy Separation
Radial Profiles
Surface Brightnesses
Model Fits
Ellipticities
Isophotal Quantities
Adaptive Moments
Conversion between SDSS ugriz and UBVR
c
I
c
ugriz colors of Vega and the Sun
Flux calibration
Ubercal
.
Converting SDSS counts to SDSS (asinh) magnitudes
(and
vice versa
)
Converting SDSS to AB magnitudes
Converting SDSS asinh magnitudes to fluxes.
Deblending
Photometric redshifts
How to reconstruct the PSF at any position