The active operational phase of the project is the SDSS-IV, which began on July 1, 2014. SDSS-III observing is complete, but activities will continue through the final SDSS-III data release in January 2015 and the scientific analyses of the completed surveys.
The SDSS-IV collaboration is still growing and continues to actively recruit new institutional partners. For more information about joining SDSS-IV, see the Joining Document and the Principles of Operation below.
The SDSS-IV Advisory Council is the collaboration’s governing body, formulating recommendations on project scope and budget to the Board of Governors of the Astrophysical Research Consortium (ARC), which has responsibility for all activities at Apache Point Observatory. Collaboration policies are developed and implemented by the SDSS Collaboration Council (CoCo), which has a representative from all of the full and associate institutional partners. The CoCo is chaired by the SDSS Spokesperson, who is elected by the collaboration for a 3-year term.
For more detailed information about the SDSS collaboration, and how it operates, please see the important policy documents below.
More detailed implementation policies, most importantly the Publication Policy and the External Collaborator Policy, are developed by the CoCo and approved by the Advisory Council.
These are the four main collaboration policies used within the SDSS projects are:
The publication policy outlines how SDSS publications are created and organized. The SDSS-III Publication Policy, an update to the policies of SDSS-I/II, is available on the SDSS-III website. The SDSS-IV Publication Policy is under review and will be available shortly.
The procedure for requesting external collaborator status as well as discussing other external participant rules is viewable on the SDSS-III website. These policies are essentially identical to the original SDSS-I/II policies, but the language updated for the SDSS-III collaboration.
Survey Science Teams & Working Groups
As described in the PoO and the Publication Policy, all science projects using non-public SDSS data must be announced to the Collaboration via the project-list web page when they are initiated. At a level above these individual projects, which will typically encompass one or several papers led by a few active team members, scientists may wish to collaborate and coordinate in larger groupings and thus create a “working group” (WG) for the sharing of common knowledge, facilities and information.
Image Use Policy
Any SDSS image on the SDSS Web site may be downloaded, linked to, or otherwise used for non-commercial purposes, provided that you agree to the following conditions:
- You must maintain the image credits. Unless otherwise stated, images should be credited to the Sloan Digital Sky Survey
- Your use of the image cannot be construed as an endorsement of any product or service
- If the image is to be used on a Web page, we also ask as a courtesy that you provide a link back to our site at http://www.sdss3.org/
SDSS Images may be used in commercial publications, or for other commercial purposes, only with the explicit approval of the Astrophysical Research Consortium (ARC). Requests for such use should be directed to the ARC Corporate Office via ARC’s Business Manager as follows:Michael Evans
ARC Business Manager
c/o Department of Astronomy, Box 351580
University of Washington
Seattle, WA 98195
Please provide the exact URL of the image you are requesting.
If you have further questions about the appropriate usage of SDSS-III images, please contact the helpdesk.
Each of the individual surveys has its own Survey Science Team (SST), which acts as the highest level of working group for science associated with that survey.
Additional information on SSTs and WGs can be seen on the SDSS-III website.
There are full member institutions, associate member institutions, and participation groups.
Full member institutions:
- Carnegie Institution for Science
- Carnegie Mellon University
- Instituto de Astrofisica de Canarias
- The Johns Hopkins University
- Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo
- Lawrence Berkeley National Laboratory
- Max-Planck-Intitut für Astrophysik (MPA Garching)
- Max-Planck-Intitut für Extraterrestrische Physik (MPE)
- Max-Planck-Intitut für Astronomie (MPIA Heidelberg)
- National Astronomical Observatory of China
- New Mexico State University
- New York University
- The Ohio State University
- Pennsylvania State University
- Shanghai Astronomical Observatory
- Universidad Nacional Autónoma de México
- University of Colorado Boulder
- University of Portsmouth
- University of Utah
- University of Wisconsin
- Yale University
Associate member institutions:
- Academia Sinica Institute of Astronomy and Astrophysics (ASIAA)
- École Polytechnique Fédérale de Lausanne
- Leibniz Institut für Astrophysik Potsdam (AIP)
- Nanjing University
- Princeton University
- Texas Christian University
- Tsinghua Center for Astrophysics
- Universidad Autónoma de Madrid
- University of Alabama, Tuscaloosa
- University of Arizona
- University of California, Irvine
- University of Edinburgh
- University of Iowa
- University of Kentucky
- University of Pennsylvania
- University of Pittsburgh
- University of Toronto
- University of Washington
- University of Wyoming
- Vanderbilt University
- Harvard-Smithsonian Center for Astrophysics
- Israel Center of Research Excellence (I-CORE)
- Tel Aviv University
- Korean Participation Group
- Korea Institute for Advanced Study
- Korea Astronomy and Space Science Institute
- United Kingdom Participation Group
- Liverpool John Moores University
- University of Cambridge
- University of Nottingham
- University of Oxford
For further information about the SDSS Collaboration, please contact the Spokesperson at email@example.com.
Official SDSS Acknowledgment
We request that the following be added to the acknowledgment section of any paper using data from the SDSS.
Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.
SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), Max-Planck-Institut für Astronomie (MPIA Heidelberg), National Astronomical Observatory of China, New Mexico State University, New York University, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Portsmouth, University of Utah, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.