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- General Observer Investigations (GOs)

The Spitzer General Observer (GO) Program is the primary means by which scientists in the community at large conduct independent research programs using new Spitzer observations. Most of the observing time available during Spitzer's science mission will be devoted to peer-reviewed GO investigations. The GO Program is open to all investigators worldwide on a competitive basis.

     More information on the GO Program


- Legacy Science Program

The Legacy Science Program consists of large-scale competitively selected projects requesting substantial and coherent data sets without proprietary periods and promising to deliver products (often including ancillary data from other telescopes) to the community. The six original Legacy projects were selected in November 2000. Five additional projects selected as part of Cycle-2, eight additional projects selected as part of Cycle-3, and seven additional projects selected as part of Cycle-4 share many characteristics of Legacy programs, and so were included under the Legacy umbrella.

     More information on the Legacy Project


- Archival Research

Archival research investigators use Spitzer data that is publicly available through the Spitzer Archive. By the start of 2006, the entire original Legacy Science Program will be available. This also includes enhanced data products returned to the SSC by the Legacy teams for distribution to the community. Solicitations for funding support are a part of consolidated General Observer/Archival Research Calls for Proposals. For Cycle-5, archival research will be limited to data in the publicly available Archive by December 31, 2008.

     More information on the AR Program


- Theoretical Research

The Theoretical Research (TR) Program provides funding support for theoretical research of direct relevance to Spitzer science. The program should provide lasting benefit for current or future observational programs with Spitzer.

     More information on the TR Program


- Targets of Opportunity (ToOs)

Targets of opportunity are special cases of General Observer (GO) programs, designed for observations of transient or other time-limited phenomena. Up to 5 medium- and high-impact ToOs will be accepted for Cycle-5. Rapid response ToOs that require a ~6 K telescope when MIPS is not already on and the telescope is already cold are unlikely to be accommodated.

     More information on TOOs


- Director's Discretionary Time (DDT)

The SSC Director controls and allocates five percent of Spitzer observing time. This Director's Discretionary Time (DDT) is intended to cover emerging scientific topics or areas missed in the proposal review process.

     More information on the DDT Program


- First-Look Survey (FLS)

The First-Look Survey (FLS) is a special case of Director's Discretionary Time (DDT). It is intended to provide an early examination of the mid-infrared sky at sensitivities about 100 times deeper than any previous dataset.

     More information on the FLS


- Guaranteed Time Observations (GTOs)

The Guaranteed Time Observations (GTO) follow from a 1983 NASA Announcement of Opportunity and competitive selection of Instrument Teams and the Spitzer science team. For the first 2.5 years of the prime mission, 20 percent of Spitzer observing time will be allocated to the GTO program. The Principal Investigators (PIs) of the three science instrument teams will each be allocated 5 percent of the observing time. The balance will be shared equally among these members of the Spitzer Science Working Group (SWG). Beyond 2.5 years, the GTO allocation is reduced to 15 percent of the observing time, and is split equally among the three PIs of the instrument teams.

     More information on the GTO Program


- Spitzer Fellowship Program

The Spitzer Space Telescope Fellowship Program provides an opportunity for highly qualified recent postdoctoral scientists to conduct independent research with the goal of enhancing the overall scientific return from the Spitzer mission. This can be accomplished through a proposal to conduct new observations with Spitzer, through exploitation of Spitzer archival databases, or through research that aids in the interpretation of Spitzer results, including theoretical investigations and laboratory astrophysics. Research must be conducted at a U.S.-based Host Institution chosen by the Fellow.

     More information on the Spitzer Fellowship Program



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This file was last modified on Wed Aug 15 09:51:01 2007.

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