KEPLER Mission: development and overview
WJ Borucki - Reports on Progress in Physics, 2016 - iopscience.iop.org
Abstract The Kepler Mission is a space observatory launched in 2009 by NASA to monitor
170 000 stars over a period of four years to determine the frequency of Earth-size and larger …
170 000 stars over a period of four years to determine the frequency of Earth-size and larger …
[HTML][HTML] Exoplanetary atmospheres—chemistry, formation conditions, and habitability
Characterizing the atmospheres of extrasolar planets is the new frontier in exoplanetary
science. The last two decades of exoplanet discoveries have revealed that exoplanets are …
science. The last two decades of exoplanet discoveries have revealed that exoplanets are …
Identifying exoplanets with deep learning: A five-planet resonant chain around kepler-80 and an eighth planet around kepler-90
CJ Shallue, A Vanderburg - The Astronomical Journal, 2018 - iopscience.iop.org
Abstract NASA's Kepler Space Telescope was designed to determine the frequency of Earth-
sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission's …
sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission's …
batman: basic transit model calculation in Python
L Kreidberg - Publications of the Astronomical Society of the …, 2015 - iopscience.iop.org
I introduce batman, a Python package for modeling exoplanet transit and eclipse light
curves. The batman package supports calculation of light curves for any radially symmetric …
curves. The batman package supports calculation of light curves for any radially symmetric …
Kepler data validation I—architecture, diagnostic tests, and data products for vetting transiting planet candidates
JD Twicken, JH Catanzarite, BD Clarke… - Publications of the …, 2018 - iopscience.iop.org
Abstract The Kepler Mission was designed to identify and characterize transiting planets in
the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on …
the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on …
False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives
We present astrophysical false positive probability calculations for every Kepler Object of
Interest (KOI)—the first large-scale demonstration of a fully automated transiting planet …
Interest (KOI)—the first large-scale demonstration of a fully automated transiting planet …
The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets
Abstract The California-Kepler Survey (CKS) is an observational program developed to
improve our knowledge of the properties of stars found to host transiting planets by NASA's …
improve our knowledge of the properties of stars found to host transiting planets by NASA's …
Terrestrial planet occurrence rates for the Kepler GK dwarf sample
CJ Burke, JL Christiansen, F Mullally… - The Astrophysical …, 2015 - iopscience.iop.org
We measure planet occurrence rates using the planet candidates discovered by the Q1-Q16
Kepler pipeline search. This study examines planet occurrence rates for the Kepler GK dwarf …
Kepler pipeline search. This study examines planet occurrence rates for the Kepler GK dwarf …
Planetary candidates observed by Kepler. VII. The first fully uniform catalog based on the entire 48-month data set (Q1–Q17 DR24)
JL Coughlin, F Mullally, SE Thompson… - The Astrophysical …, 2016 - iopscience.iop.org
We present the seventh Kepler planet candidate (PC) catalog, which is the first catalog to be
based on the entire, uniformly processed 48-month Kepler data set. This is the first fully …
based on the entire, uniformly processed 48-month Kepler data set. This is the first fully …
Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities-No excess of cold Jupiters in small planet …
AS Bonomo, X Dumusque, A Massa, A Mortier… - Astronomy & …, 2023 - aanda.org
The exoplanet population characterized by relatively short orbital periods (P< 100 d) around
solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets …
solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets …