Campaign 9 of the K2 Mission: Observational Parameters, Scientific Drivers, and Community Involvement for a Simultaneous Space- and Ground-based Microlensing Survey
Abstract
K2's Campaign 9 (K2C9) will conduct a ~3.7 deg^2 survey toward the Galactic bulge from 2016 April 22 through July 2 that will leverage the spatial separation between K2 and the Earth to facilitate measurement of the microlens parallax πE for ≳170 microlensing events. These will include several that are planetary in nature as well as many short-timescale microlensing events, which are potentially indicative of free-floating planets (FFPs). These satellite parallax measurements will in turn allow for the direct measurement of the masses of and distances to the lensing systems. In this article we provide an overview of the K2C9 space- and ground-based microlensing survey. Specifically, we detail the demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of K2C9, and the array of resources dedicated to concurrent observations. Finally, we outline the avenues through which the larger community can become involved, and generally encourage participation in K2C9, which constitutes an important pathfinding mission and community exercise in anticipation of WFIRST.
Additional Information
© 2016 The Astronomical Society of the Pacific. Received 2016 March 7; Accepted 2016 July 15; Published 2016 October 26. C.B.H., R.P., M.P., R.A.S., D.P.B., D.W.H., and B.S.G. were supported through the NASA K2 Guest Observer Program. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Work by C.B.H. and Y.S. was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Universities Space Research Association through a contract with NASA. The OGLE project has received funding from the National Science Centre, Poland, grant MAESTRO 2014/14/A/ST9/00121 to A.U. G.D. acknowledges Regione Campania for support from POR-FSE Campania 2014-2020. TCH is funded through KASI grant #2016-1-832-01. SM was supported by the Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences grant No. XDB09000000, and by the National Natural Science Foundation of China (NSFC) under grant number 11333003 and 11390372 (SM). C.B.H. thanks graphic designer Kathryn Chamberlain for her generous assistance with Figure 4. © California Institute of Technology. Government sponsorship acknowledged.Attached Files
Published - pasp_128_970_124401.pdf
Submitted - 1512.09142v2.pdf
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Additional details
- Eprint ID
- 70332
- Resolver ID
- CaltechAUTHORS:20160914-083754165
- NASA/JPL/Caltech
- NASA Postdoctoral Program
- Narodowe Centrum Nauki (NCN)
- MAESTRO 2014/14/A/ST9/00121
- Regione Campania
- Korea Astronomy and Space Science Institute (KASI)
- 2016-1-832-01
- Chinese Academy of Sciences
- XDB09000000
- National Natural Science Foundation of China
- 11333003
- National Natural Science Foundation of China
- 11390372
- Created
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2016-09-29Created from EPrint's datestamp field
- Updated
-
2021-11-11Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)