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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 UBVRcIc
  • 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

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