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An Eta-Earth Projection, Based on a New Analysis of Kepler Completeness
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Lessons Learned from the Kepler Mission and Space Telescope Management
This paper presents lessons learned over the course of several space telescope mission and instrument developments spanning two decades. These projects involved astronomical telescopes developed by the National Aeronautics and Space Administration (NASA) and were designed to further our understanding of the Universe. It is hoped that the lessons drawn from these experiences may be of use to future mission developers.
Optimization of Selected Remote Sensing Algorithms for Embedded NVIDIA Kepler GPU Architecture
This paper evaluates the potential of embedded Graphic Processing Units in the Nvidias Tegra K1 for onboard processing. The performance is compared to a general purpose multi-core CPU and full fledge GPU accelerator. This study uses two algorithms: Wavelet Spectral Dimension Reduction of Hyperspectral Imagery and Automated Cloud-Cover Assessment (ACCA) Algorithm. Tegra K1 achieved 51 for ACCA algorithm and 20 for the dimension reduction algorithm, as compared to the performance of the high-end 8-core server Intel Xeon CPU with 13.5 times higher power consumption.
Beyond Kepler: Direct Imaging of Exoplanets
The exoplanets field has been revolutionizing astronomy over the past 20+ years and shows no signs of stopping. The next big wave of exoplanet science may come from direct imaging of exoplanets. Several (non-habitable) exoplanets have already been imaged from the ground and NASA is planning an instrument for its 2020s flagship mission (WFIRST) to directly image large exoplanets. One of the key goals of the field is the detection and characterization of "Earth 2.0", i.e. a rocky planet with an atmosphere capable of supporting life. This appears possible with several potential instruments in the late 2020s such as WFIRST with a starshade, Extremely Large Telescopes (ELTs) from the ground, or one of NASA possible flagship missions in the 2030s (HabEx or LUVOIR). Also, if an Earth-like planet exists around Alpha Centauri (A or B), it may be possible to directly image it in the next approx. 5 years with a small space mission such as the Alpha Centauri Exoplanet Satellite (ACESat). I will describe the current challenges and opportunities in this exciting field, as well as the work we are doing at the Exoplanet Technologies group to enable this exciting science.
Chasing Shadows in the Night: How NASA's Kepler and TESS Missions are Revolutionizing Exoplanet Science
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Chasing Shadows in the Night: How NASA's Kepler and TESS Missions are Revolutionizing Exoplanet Science
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Improving Estimates of the Frequency of Earth-like Planets in the Habitable Zone of Sun-Like Stars by Reprocessing the Kepler Dataset
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Kepler K2 Campaign 9 – II. First space-based discovery of an exoplanet using microlensing
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Discovery and characterization of Kepler-36b
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Pulsation and rotation in NGC 6811: the Kepler short-cadence stars
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DA white dwarfs in the Kepler field
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Investigating the Atmospheric Mass Loss of the Kepler-105 Planets Straddling the Radius Gap
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Earths in Other Solar Systems’ N-body Simulations: The Role of Orbital Damping in Reproducing the Kepler Planetary Systems
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Stability of exomoons around the Kepler transiting circumbinary planets
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