SDSS data products
DR6 and other data releases
About DR6 explains the
contents of this data release and its relation to other data releases
(also see the SDSS data release
schedule).
Data products overview
SDSS provides FITS image files of the corrected frames in five
bands, a mask that records how each pixel was used in the imaging
pipelines, 4 x 4 binned images of the corrected frames after detected
objects have been removed, and "atlas" images, which include all
significant pixels around each object. This page describes imaging
frames, how to get them and related files from the survey archive, and
how to work with them.
The calibrated object lists are FITS tables containing positions,
fluxes, and shapes of all objects detected at >5 sigma on the
images. This page describes the lists, how to get them and related
files from the archive, and how to work with them.
- "2d" spectra: FITS files of the flux- and
wavelength-calibrated, sky-subtracted spectra, with error and mask
arrays and resolution at each pixel. 640 spectra per file.
- "1d" spectra: FITS files with the calibrated spectra and error and
mask arrays, redshift, spectral classification, and detected lines of
each spectrum.
The page describes calibrated spectra, how to get them and related
files from the archive, and how to work with them.
"Tiling" means optimising the placement of spectroscopic tiles on
the sky and assignment of spectroscopic fibers to targets in the
spectroscopic survey. This section describes the tiling files, how to
get them and related files from the archive, and how to characterise
the survey's non-uniformity using them.
Other data products
These include astrometric calibrations, photometric calibrations,
gif and postscript plots of spectra, and finding
charts in postscript/jpeg/fits formats.
The SDSS collaboration has created catalogs and
other data products based on public survey data that are of general use.
IAU designations for SDSS objects
Use IAU designations in publications.
Data access
All data products are available from the data access page as fits images and
tables from the Data Archive
Server (DAS). All catalogs are also available through the Catalog Archive Server (CAS)
which provides fast search capabilities.
Data model
The flat-file data model
contains detailed descriptions of all data generated by the data
processing. The Archive
Intro page and the SQL
Schema Browser describe how data are stored in the Catalog Archive Server (CAS).
Data quality overviews
Imaging
There are various quality assurance algorithms for photometry, some
of which consider each run in isolation, and some of which consider
overlapping parts of different runs. Since DR4, we make available the
summary and single-run QA data and plots, which analyze the PSF, the
difference between aperture and PSF magnitudes of stars, and the
location of the stellar locus in color-color space. Details are
available on the QA pages.
The following overviews cover the quality of other aspects
of imaging.
Spectroscopy
SDSS Webmaster
Last modified: Thu Jun 14 18:08:10 CEST 2007
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