-
41
Planet Hunters X. KIC 8462852 - Where's the Flux?
Published 2016“…Over the duration of the Kepler mission, KIC8462852 was observed to undergo irregularly shaped, aperiodic dips in flux of up to $\sim 20$\%. …”
Journal article -
42
K2SC: Flexible systematics correction and detrending of K2 light curves using Gaussian Process regression
Published 2016“…We apply k2sc to publicly available K2 data from Campaigns 3-5 showing that we obtain photometric precision approaching that of the original Kepler mission. We compare our results to other publicly available K2 pipelines, showing that we obtain similar or better results, on average. …”
Journal article -
43
THE KEPLER DICHOTOMY IN PLANETARY DISKS: LINKING KEPLER OBSERVABLES TO SIMULATIONS OF LATE-STAGE PLANET FORMATION
Published 2017“…NASA's Kepler Mission uncovered a wealth of planetary systems, many with planets on short-period orbits. …”
Get full text
Article -
44
The Detectability Of Transit Depth Variations Due To Exoplanetary Oblateness And Spin Precession
Published 2011“…The detectability of the TδV signal would be enhanced by moons (which would decrease the precession period) or planetary rings (which would increase the amplitude). The Kepler mission should find several planets for which precession-induced T[delta]V signals will be detectable. …”
Get full text
Get full text
Article -
45
-
46
The High Albedo of the Hot Jupiter Kepler-7 B
Published 2012“…However, only a handful of hot Jupiters have been observed with high enough photometric precision at visible wavelengths to investigate these expectations. The NASA Kepler mission provides a means to widen the sample and to assess the extent to which hot Jupiter albedos are low. …”
Get full text
Get full text
Article -
47
A Novel Approach to Classify Telescopic Sensors Data Using Bidirectional-Gated Recurrent Neural Networks
Published 2022-10-01“…According to a recent state by NASA Kepler mission, 7000 HeB and RGB were observed. A study based on an advanced system needs to be implemented to classify RGB and HeB, which helps astronomers. …”
Get full text
Article -
48
Exo-C: a probe-scale space observatory for direct imaging and spectroscopy of extrasolar planetary systems
Published 2018“…Exo-C has a similar telescope aperture, orbit, lifetime, and spacecraft bus requirements to the highly successful Kepler mission (which is our cost reference). Much of the needed technology development is being pursued under the WFIRST coronagraph study and would support a mission start in 2017, should NASA decide to proceed. …”
Get full text
Get full text
Article -
49
Water Vapor and Clouds on the Habitable-zone Sub-Neptune Exoplanet K2-18b
Published 2020“…Results from the Kepler mission indicate that the occurrence rate of small planets (<3 R ⊕) in the habitable zone of nearby low-mass stars may be as high as 80%. …”
Get full text
Article -
50
Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data
Published 2012“…On 2011 February 1 the Kepler mission released data for 156,453 stars observed from the beginning of the science observations on 2009 May 2 through September 16. …”
Get full text
Get full text
Article -
51
ASTEROSEISMIC DETERMINATION OF OBLIQUITIES OF THE EXOPLANET SYSTEMS KEPLER-50 AND KEPLER-65
Published 2014“…We consider two systems observed by the NASA Kepler mission which have multiple transiting small (super-Earth sized) planets: the previously reported Kepler-50 and a new system, Kepler-65, whose planets we validate in this paper. …”
Get full text
Get full text
Article -
52
Mergers and Tidal Breakups of Binary Systems of Primordial DM Planets with Baryon Admixture and Emission of Gravitational Waves
Published 2023-02-01“…So far, thousands of exoplanets have been discovered by the Kepler mission and more will be found by NASA’s Transiting Exoplanet Survey Satellite (TESS) mission, which is observing the entire sky to locate planets orbiting the nearest and brightest stars. …”
Get full text
Article -
53
The Asteroseismic Poltential of TESS: Exoplanet-Host Stars
Published 2017“…Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. …”
Get full text
Get full text
Get full text
Article -
54
Kepler's First Rocky Planet: Kepler-10b
Published 2012“…NASA's Kepler Mission uses transit photometry to determine the frequency of Earth-size planets in or near the habitable zone of Sun-like stars. …”
Get full text
Get full text
Article -
55
-
56
REVISED STELLAR PROPERTIES OF KEPLER TARGETS FOR THE QUARTER 1-16 TRANSIT DETECTION RUN
Published 2015“…We present revised properties for 196,468 stars observed by the NASA Kepler mission and used in the analysis of Quarter 1-16 (Q1-Q16) data to detect and characterize transiting planets. …”
Get full text
Article -
57
-
58
Gaussian Processes and Nested Sampling Applied to Kepler's Small Long-period Exoplanet Candidates
Published 2024-01-01“…There are more than 5000 confirmed and validated planets beyond the solar system to date, more than half of which were discovered by NASA’s Kepler mission. The catalog of Kepler’s exoplanet candidates has only been extensively analyzed under the assumption of white noise (i.i.d. …”
Get full text
Article -
59
HAT-P-30b: A TRANSITING HOT JUPITER ON A HIGHLY OBLIQUE ORBIT
Published 2012Get full text
Get full text
Article -
60
KOI-2700b—A PLANET CANDIDATE WITH DUSTY EFFLUENTS ON A 22 hr ORBIT
Published 2015“…The transit is not sufficiently deep to allow for a study of the transit-to-transit variations, as is the case for KIC 1255b; however, it is clear that the transit depth is slowly monotonically decreasing by a factor of ~2 over the duration of the Kepler mission. We infer a mass-loss rate in dust from the planet of ~2 lunar masses per Gyr. …”
Get full text
Get full text
Article