hundreds of planet candidates from k2 - blue waters...intro to kepler & k2 methods & why...
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Hundreds of Planet Candidates from K2
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Ethan Kruse@ethan_kruse
4 June 2018
Collaborators:Eric Agol
Rodrigo LugerDan Foreman-Mackey
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Outline
✦Intro to Kepler & K2
✦Methods & Why Blue Waters
✦Results & Future Plans
Ethan Kruse4 June 2018
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Finding Transiting Planets
Ethan Kruse4 June 2018
✦Depths
✦Earth: 0.01%
✦Jupiter: 1%
✦Odds of transit at 1AU: 1 in 200
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Finding Transiting Planets
Ethan Kruse4 June 2018
✦Depths
✦Earth: 0.01%
✦Jupiter: 1%
✦Odds of transit at 1AU: 1 in 200
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Kepler Telescope
Ethan Kruse4 June 2018
✦Launched 2009
✦1.4 m mirror
✦96 Megapixel camera
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Kepler Field of View
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Kepler Planets (2009-2011)
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Kepler Planets (2009-2011)
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Kepler Planets (2009-2013)
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2013 Disaster
Ethan Kruse4 June 2018
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2013 Disaster
Ethan Kruse4 June 2018
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2013 Disaster
Ethan Kruse4 June 2018
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2013 Disaster
Ethan Kruse4 June 2018
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2013 Disaster
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K2 Overview
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K2 Overview
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K2 Overview
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K2 Degraded Quality
Kepler star (4x5 pixels)
K2: TRAPPIST-1 (11x11 pixels)
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K2 Degraded Quality
Kepler star (4x5 pixels)
K2: TRAPPIST-1 (11x11 pixels)
Ethan Kruse4 June 2018
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Outline
✦Intro to Kepler & K2
✦Methods & Why Blue Waters
✦Results & Future Plans
Ethan Kruse4 June 2018
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EVEREST: Fix K2’s Data Quality
Ethan Kruse4 June 2018
Luger et al. (2016)
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Finding Planets
Ethan Kruse4 June 2018
✦Unknown parameters:
✦Depth (~10)
✦Duration (16)
✦Period + Phase (7000)
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Blue Waters Assist
Ethan Kruse4 June 2018
✦4D grid of parameters to search
✦~1 million grid points per star
✦Searching 1 star takes ~30 minutes
✦500,000 stars to search
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Outline
✦Intro to Kepler & K2
✦Methods & Why Blue Waters
✦Results & Future Plans
Ethan Kruse4 June 2018
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My K2 Planet Candidates
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Period Ratios
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What’s Next: TESS
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TESS Data Challenge
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TESS Data Challenge
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Conclusions
✦EVEREST returns K2 data to Kepler’s quality
✦I’ve found lots of multi-planet & dynamically active systems in K2
✦Only half of K2 data analyzed so far: hundreds more planets to come!
✦TESS is about to change everything
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TTVs
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Ultra Short Periods
P=0.47d P=0.71d
P=0.77d P=0.57d
P=0.67dEthan Kruse4 June 2018
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Single Transits
Ethan Kruse4 June 2018