z-logo
open-access-imgOpen Access
The Kepler end-to-end model: creating high-fidelity simulations to test Kepler ground processing
Author(s) -
Steve Bryson,
Jon M. Jenkins,
Dan J. Peters,
Peter P. Tenenbaum,
Todd C. Klaus,
Jay P. Gunter,
Miles T. Cote,
Douglas A. Caldwell
Publication year - 2010
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.857560
Subject(s) - transit (satellite) , kepler , spacecraft , stars , planet , pipeline (software) , physics , astronomy , computer science , aerospace engineering , engineering , public transport , programming language , transport engineering
The Kepler mission is designed to detect the transit of Earth-like planets around Sun-like stars by observing 100,000 stellar targets. Developing and testing the Kepler ground-segment processing system, in particular the data analysis pipeline, requires high-fidelity simulated data. This simulated data is provided by the Kepler Endto- End Model (ETEM). ETEM simulates the astrophysics of planetary transits and other phenomena, properties of the Kepler spacecraft and the format of the downlinked data. Major challenges addressed by ETEM include the rapid production of large amounts of simulated data, extensibility and maintainability.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom