Optical Spectra Overview

Single-fibre Optical Spectra

Data Release 14 includes the complete dataset of optical single-fibre spectroscopy of the Sloan Digital Sky Survey through July 2016 – more than four million spectra – comprising extra-galactic and galactic spectra.

Quick Look view of the host galaxy of supernova 2011V (<a href="http://adsabs.harvard.edu/abs/2012A%26A...544A..81H">Hakobyan et al. 2012</a>). Click on the image to go to the Quick Look tool for the latest Data Release.
Quick Look view of the host galaxy of supernova 2011V (Hakobyan et al. 2012). Click on the image to go to the Quick Look tool for the latest Data Release.

Galactic optical spectra includes all spectra and derived stellar parameters measured by the Sloan Extension for Galactic Understanding and Exploration (SEGUE) , during SDSS-I/II and SDSS-III. (Infrared spectra of galactic objects are also available from the APOGEE survey.)

Extra-galactic spectra includes all spectra from the following observing programs:

SDSS extra-galactic observing programs

A brief summary of these extra-galactic observing programs is given on the Extra-galactic Observing Programs page.

Get the Data: Spectroscopic Catalogs

SkyServer

The quickest way to view SDSS spectroscopic data is the SkyServer Quick Look tool. Quick Look shows an image and spectrum for all sky objects for which the SDSS has measured a “science primary” spectrum. The tool also shows the object’s spectroscopic classification (star/galaxy/quasar) and redshift, and gives links to further data, including the spectrum as a FITS file.

All spectroscopic catalog data is available through the search tools of SkyServer. The Spectroscopic Query Form lets you search for spectroscopic catalog objects by position, spectral classification, redshift, and other constraints in spectroscopy and imaging. SQL Search lets you create your own search; see the SkyServer SQL Tutorial to learn how to write SQL queries.

CasJobs

An even more flexible and powerful interface is CasJobs, which allows you to save and analyze all your search results.

Get the data: FITS spectra

Science Archive Server (SAS)

Summary FITS files containing the best-fit redshifts and parameters for optical spectroscopic objects, as well as all raw and processed SDSS/SEGUE/BOSS/SEQUELS/eBOSS data are available from the Science Archive Server (SAS), including all directories and files listed in the Data Model.
The Science Archive Webapp provides a searchable interface for optical spectra, and includes an interactive spectrum viewer, and a data download facility (supports both rsync and wget):

More information about SDSS spectra

These pages describe how to use SDSS spectroscopic data. Use the links below (echoed on the left sidebar menu on each page) to learn more.

Understanding SDSS spectra:
describes how SDSS spectroscopic data are organized, and the various spectroscopic observing programs that compose the full SDSS.
Pipeline:
describes the steps in
the spectroscopic data processing, and the files created at each step.
Available data:
describes in detail what spectroscopic data products are available through the Science Archive Server and SkyServer.
Target flags:
describes how to track the way in which a spectrum was chosen (targeted) for spectroscopic follow-up.
Spectroscopic catalogs:
describes the parameters available in SDSS spectroscopic catalogs, such as redshifts and classifications.
Galaxies:
describes additional galaxy parameters calculated from SDSS spectra.
Stars (SSPP):
describes the SEGUE Stellar Parameter Pipeline, which estimates stellar atmospheric parameters, and how to use SSPP data.
SEGUE SQL cookbook:
describes getting stellar parameters out of the SQL database, with examples.
Caveats:
describes some important caveats in using SDSS spectroscopic data, including how to check data quality.

To learn how the SDSS chose objects for spectroscopic observation, see the SDSS Target Selection pages.