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Can I propose to search for exoplanets or work upon exoplanet-related science?
No. Exoplanet and exo-planet related science is reserved for the Kepler Science Team.
Furthermore, by proposing for Kepler GO targets, you are agreeing to the policy of non-disclosure of exoplanet information
obtained serendipitously or otherwise through your GO targets. This policy is described in the
NASA NRA and all GOs will sign non-disclosure agreements before receiving their data.
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What happens if I unexpectedly find an exoplanet around my source?
The Kepler Key Project will perform follow-up observations. If confirmed the
detection will be announced and published by the Kepler project. You will be invited to participate in the
exoplanet investigation and will be invited to co-author resulting papers. The non-disclosure agreement
applies in all cases.
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What is the difference between the GO program and the KASC program?
The KASC program belongs to the Kepler
Astroseismology Science Consortium. The KASC program has been initiated by the Kepler project to exploit the
asteroseismological potential of the Kepler data using guaranteed short- and long-cadence targets each quarter.
However the KASC program does not constrain the GO program. GOs can propose the same targets and science as the
KASC with no limitations. GOs have an advantage over KASC members - the GOs do not have to abide by the KASC
publication policies. Note that KASC is not a closed community; all interested researchers may join one or more
of the KASC working groups.
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What are the consequences of choosing a custom target?
A custom target is a source which requires the GO to propose a non-standard
pixel mask. Examples are extended sources, saturated stars and sources without KIC entries. Through Quarter 6
custom targets are processed so that the pixels are calibrated, but light curve products will not be generated
for the archive. As of January 2011, the target pixel files will begin to be archived, so that users can
construct their own light curves.
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I've missed the deadline for Guest Observer proposals - can I still propose for
observing time?
Yes. In between the annual call for proposals, one can request time under the
Discretionary Time program, for proposing targets of astrophysical interest.
- Annual Kepler Guest Observer Program Announcements of Opportunity are released as part of NASA's Research
Opportunities in Space and Earth Sciences (ROSES) Program. New announcements and updates can be found at the
NSPIRES website.
- Discretionary Targets (DDTs) are an unfunded competition held quarterly for individual or small
samples of targets that provide a faster turnaround between the proposal process and the archiving process.
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Can I propose a source which is *not* in the KIC?
Yes. Follow the instructions in the Announcement of Opportunity and
within the target table, and the
target checks GO web pages. The Guest Observer office
will work with proposers to optimally observe your propose source.
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Can I observe a source brighter than the saturation level?
Yes. Properly mapped pixel masks can capture the charge bleed from sources which
saturate the central pixel(s). Please see the details on the
target aperture, and target checks GO web pages.
You may contact the GO Office for further information on observing the brightest sources in the Kepler field.
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What do I need to include in my proposal? A budget ? A CV ?
For a checklist of required proposal components, please see the Proposal
Preparation Content page, and the NASA document
NRA 2010 Handbook.
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I'm breaking the page limit due to a long target table! What can I do?
Exceptions to the page limits will be made for long target tables, or proposals
with large numbers of Co-Is. Please note that the scientific justification section must adhere to the
standard page limits.
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Where do I obtain my Kepler data ?
All Kepler data is obtained from the MultiMission
Archive, at the Space Telescope Science Institute
using their Kepler Data Search
and Retrieval Tool.
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MAST tells me my GO data is proprietary and I cannot have access ?
The Guest Observer Office has supplied MAST with your email address and GO
program number. But these steps is not sufficient
for a GO to access their data. There are two further steps that a GO must perform themselves.
- Register as a user at MAST, creating a username
and password to link to your email address.
- Email MAST at archive@stsci.edu and request that your program number be registered with your MAST username.
Execution of this task will typically take <24h, but we recommend GOs complete the above steps before
their data becomes available.
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When I use the search engine at MAST, I only seem to get access to a portion of
my data. Where's the rest ?
To access your data using the MAST
Search and Retrieval Tool,
the GO enters their program number into the "Investigation ID" dialog box. You must use the wildcard
character before and after the program number for MAST to include ALL datasets marked with your program ID.
For example, to obtain all data for this program, one would enter: *GO10000*
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What is a .bz2 file?
A file ending in .bz2 has been encoded using the bzip2 data compression
algorithm. For more information on bzip2 files, see the bzip2 project pages.
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