At intervals, NASA selects funded proposals for
the Kepler Participating Scientists Program (PSP). The Kepler PSP
is designed to augment the skill set of the Kepler Science Team,
thereby enabling it to more effectively execute the science
program of the mission. Participating Scientists serve as members
of the Kepler Science Team and participate in Science Team
activities, such as data processing and analysis, transit
candidate follow-up and characterization, and publication.
The deadline for Cycle 2 Participating Scientist proposals was
11 Feb 2011. Proposal instructions and element details are provided in
NASA Research Announcement NNH10ZDA001N-KPS. Proposals will be evaluated in Spring
2011, with a nominal start date of 1 October 2011, contingent on funding.
1. Scope of Participating Science
The proposed investigations can be analytical or observational in nature.
Investigations may include any research activity that:
- Directly relates to the detection, characterization, or understanding of
extrasolar planets.
- Helps to achieve the Kepler prime mission goals listed in Section 2.
Examples of possible analytic programs include:
- Detection of nontransiting planets by timing of the variations of the transit
epochs
- Improvement of stellar atmosphere models through the use of Kepler observations
- Estimates of the sizes of stars, and, therefore, the sizes of transiting planets,
through the application of stellar atmosphere models
- Development of open-source tools for performing alternate photometric and
detrending analyses
- Efforts to understand systematic biases, target selection effects, background
contamination, and pipeline detection efficiency
Examples of possible observational programs include:
- Determination of the multiplicity of stars with planets, especially those with
stellar orbital periods exceeding one year and with mass ratios of five or more
- Elimination of false positive planet detections caused by very close background
eclipsing binaries using ground-based color photometry of the transits
The abstracts for successful Cycle 1 PSP proposals are available
here, and abstracts for successful Cycle 2 PSP proposals are available
here.
In addition to conducting science investigations addressing the broad science goals
of the mission based on the nature of their proposals, Kepler Participating Scientists
will also join one or more of the Kepler discipline groups described in Section
2. The selected Participating Scientists will be expected to coordinate their activities.
The Kepler PSP is complementary to, but distinct from, the Kepler Guest Observer
(GO) program. The Kepler GO program offers the opportunity for members of the scientific
community to select targets of general astrophysical interest in the Kepler field-of-view
(both stellar and nonstellar), in pursuit of investigations that fall outside of the scope
of the Kepler Science Team.
2. Kepler Science Objectives
The primary scientific objectives of the Kepler mission are:
- Provide a statistically significant value for the frequency of Earth-size and
larger planets in and near the habitable zone of their host stars
- Characterize the size and orbital distributions of planets around other stars
- Estimate the frequency of planets and orbital distribution of planets in
multiple-stellar systems;
- Determine the distributions of semimajor axis, albedo, size, mass and density of
short-period giant planets
- Identify additional members of each photometrically discovered planetary system
using complementary techniques
- Identify correlations between the presence and characteristics of planetary
systems with stellar properties of the host star
3. Period of Performace
Proposers should provide budgets and justification for participation in the Kepler
mission with a period of performance beginning on October 1, 2011. This start date is
contingent on funding availability. It is expected that investigators will propose for
two years of PSP support running through October 1, 2013, which effectively corresponds
to the end of the Kepler prime mission. It is anticipated that the annual budget for the
PSP will be approximately $1.0M, sufficient to support the selection of 7-10 Participating
Scientist investigations.
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