Welcome to the home page of the fifth Kepler & K2 Science Conference! The conference will be take place from March 4-8, 2019 in Glendale, California. The meeting will be a celebration of Kepler's 10 years in space. Stay tuned for further information!
|August 31, 2018||registration and abstract submission open|
|November 15, 2018||regular deadline to submit abstracts for talks, breakout sessions, and poster; deadline to apply for travel support|
|December 20, 2018||conference schedule published|
|January 3, 2019||conference forecast deadline (NASA participants only)|
|January 15, 2019||late deadline to submit abstracts for posters|
|February 10, 2019||registration and hotel reservation deadline|
|March 4-8, 2019||Kepler & K2 Science Conference V|
There is no registration fee for this conference, however we ask that all attendees register to assist with planning. Register here by the Feb. 10, 2019 deadline.
Upon registering, participants can volunteer to judge a poster competition for students and post docs during the conference. Winners of the competition have the opportunity to give short talks about their results during the second half of the conference. Judges will rank posters of conference participants who agreed to enter the competition.
Abstracts for posters only can be submitted here until the late poster only deadline of Jan. 15, 2019. Abstracts for oral presentations and breakout sessions were due by the Nov. 15 deadline.
Note that Wednesday afternoon (March 6) is set aside for breakout sessions to enable the community to discuss and work on Kepler/K2 related projects. We envision these sessions will be more hands on, unconference sessions of broad interest to the community. Examples of breakout sessions include panel discussions, hack activities, work meetings of large collaborations, or tutorials to use data/software products related to Kepler/K2.
Monday, March 4, 2019
|Session 1: Kepler/K2 Mission History and Future|
|08:30-09:00||Bill Borucki (NASA Ames)||History of the Kepler Mission (invited)|
|09:00-09:30||Katelynn McCalmont (Ball Aerospace)||Flying the Kepler Spacecraft's Second Mission: K2 Operations (invited)|
|09:30-09:45||Douglas Caldwell (SETI Institute)||The Kepler Photometer|
|09:45-10:00||Geert Barentsen (NASA Ames)||Kepler's Discoveries Will Continue: 21 Scientific Opportunities with Kepler & K2 Archive Data|
|Session 2: Precise Stellar and Planetary Radii|
|10:30-11:00||Mia Lundkvist (Aarhus University)||Asteroseismology of Exoplanet Host Stars from the Kepler/K2 missions (invited)|
|11:00-11:15||Vincent Van Eylen (Princeton University)||Understanding Planet Formation through Asteroseismology|
|11:15-11:30||Hilke Schlichting (UCLA)||Observational Signatures of the Core-Powered Mass-Loss Mechanism: The Radius Valley as a Function of Stellar Mass|
|11:30-11:45||Travis Berger (University of Hawaii)||Precise Characterization of Kepler Stars and Planets Using Gaia DR2|
|11:45-12:00||Benjamin Fulton (Caltech/IPAC-NExScI)||Revisiting the Radius Gap in the Era of Gaia|
|Session 3: Stellar Magnetism and Activity|
|13:30-13:45||Matteo Cantiello (Flatiron Institute)||Internal Magnetic Fields Asteroseismology: Kepler's Legacy and TESS's Opportunities|
|13:45-14:00||Angela Santos (Space Science Institute)||Seismic Signatures of Magnetic Activity in Solar-type Stars Observed by Kepler|
|14:00-14:15||Ellianna Schwab Abrahams (UC Berkeley)||The Fundamental and Magnetic Characteristics of M Dwarfs in the Kepler Field|
|14:15-14:30||Michael Gully-Santiago (NASA Ames)||K2 Constraints on Stellar Surface Inhomogeneities and their Systematic Bias of Transit-derived Exoplanet Densities|
|14:30-14:45||Sharon Xuesong Wang (Carnegie DTM)||RVxK2: Using Simultaneous Kepler Photometry to Mitigate Stellar Jitter|
|14:45-15:00||Lisa Bugnet (CEA Saclay)||FliPer: A Powerful Tool to Detect and Characterise Solar-like Pulsators|
|Session 4: Exoplanet Occurrence Rates|
|15:30-16:00||Courtney Dressing (UC Berkeley)||Probing the Frequency of Planetary Systems with Kepler and K2 (invited)|
|16:00-16:15||Gijs Mulders (University of Chicago)||Exoplanet Population Synthesis in the Era of Large Exoplanets Surveys|
|16:15-16:30||Timothy Morton (University of Florida)||The Probabilistic Validation Revolution: How Kepler Forced a Paradigm Shift in How We Treat Transiting Planet Candidates|
|16:30-16:45||Marko Sestovic (University of Bern)||The Occurence Rate of Planets Around Ultracool Dwarfs|
|16:45-17:00||Christina Hedges (NASA Ames)||Are There Any More Planets in the Kepler/K2 Data?|
Tuesday, March 5, 2019
|Session 1: Kepler Benchmark Systems|
|08:30-09:00||Sarah Ballard (MIT)||Lessons from the Multi-planet Systems (invited)|
|09:00-09:15||Christopher Shallue (Google Brain)||Can Deep Learning Help Find Earth Analogues?|
|09:15-09:30||Michelle Hill (UC Riverside)||Exploring Kepler Giant Planets in the Habitable Zone|
|09:30-09:45||Kai Rodenbeck (Institute for Astrophysics, Gottingen)||Revisiting the Exomoon Candidate Signal Around Kepler-1625 b|
|09:45-10:00||Ashley Chontos (University of Hawaii)||The Curious Case of KOI-4: Confirming Kepler’s First Exoplanet|
|Session 2: K2 Benchmark Systems|
|10:30-11:00||Andrew Vanderburg (Caltech/IPAC-NExScI||Benchmark Exoplanet Systems Discovered by the K2 Mission (invited)|
|11:00-11:15||Juliette Becker (University of Michigan)||Dynamically Determining Observationally Ill-Constrained Planet Parameters: Towards Precise Transit Ephemerides for the Benchmark System HIP 41378|
|11:15-11:30||Kevin Hardegree-Ullman (Caltech/IPAC-NExScI)||Space Telescope Synergy: Spitzer Follow-up of K2 Targets|
|11:30-11:45||Joey Rodriguez (Harvard-Smithsonian CfA)||K2-266: A Compact Multi-Planet System With A Planet That Is "Way Out of Line"|
|11:45-12:00||Fei Dai (MIT)||New Perspective on the Ultra-short-period Planets|
|Session 3: Microlensing and Accretion Physics|
|13:30-13:45||Domenico Nardiello (Universita degli Studi de Padova)||High-precision Photometry of Stars in K2 Crowded Fields - A PSF-based Approach to K2 Data|
|13:45-14:00||Sebastiano Calchi Novati (Caltech/IPAC)||An Isolated Microlens Observed from K2, Spitzer, and Earth|
|14:00-14:30||Krista Lynne Smith (Stanford University)||Kepler/K2 and Active Galactic Nuclei: New Insights into Accretion and High Energy Phenomena (invited)|
|14:30-14:45||Paula Szkody (University of Washington)||Insights into Accretion in Cataclysmic Variables Gleaned from Kepler|
|14:45-15:00||Ryan Ridden-Harper (Australian National University)||Hunting Transients in K2 with the K2: Background Survey|
|Session 4: Extragalactic Science|
|15:30-16:00||Peter Garnavich (University of Notre Dame)||Better Understanding Supernovae from Kepler/K2 Observations (invited)|
|16:00-16:15||Georgios Dimitriadis (UC Santa Cruz)||K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova|
|16:15-16:30||Thomas Holoien (Carnegie Observatories)||ASASSN-18bt: Evidence for Nickle on the Surface of a Type Ia Supernova Found by the Rising K2 Light Curve|
|16:30-16:45||Edward Shaya (University of Maryland)||A Tidal Disruption Event in a Seyfert 2 Observed with K2|
|16:45-17:00||Armin Rest (STScI)||A Fast-Evolving, Luminous Transient Discovered by K2/Kepler|
|17:00-18:30||Poster Session I|
Wednesday, March 6, 2019
|Session 1: Galactic Archaeology|
|08:30-09:00||Marc Pinsonneault (Ohio State University)||Galactic Archeology with Kepler and K2 (invited)|
|09:00-09:15||Dennis Stello (University of New South Wales)||The K2 Galactic Archaeology Program: revealing the jigsaw puzzle one campaign at a time|
|09:15-09:30||Jie Yu (University of Sydney)||Ensemble Asteroseismology of 20,000 Oscillating Red Giants Observed by Kepler|
|09:30-09:45||Rafael Garcia (CEA Saclay)||A Comprehensive Full Kepler Red Giant Legacy Catalog|
|09:45-10:00||Daniel Huber (University of Hawaii)||An Asteroseismic Age for the Galactic Halo Measured with Distant Kepler Giants|
|Session 2: Binaries, Exoplanets, and Citizen Science|
|10:30-10:45||Adam Kraus (UT Austin)||The Perilous Lives of Planets in Binary Star Systems|
|10:45-11:00||Rachel Matson (NASA Ames)||Detecting Unresolved Binaries in Exoplanet Transit Surveys with Speckle Imaging|
|11:00-11:15||Nicole Hess (Southern Connecticut State University)||Identifying Bound Stellar Companions to Kepler Exoplanet Host Stars With Speckle Imaging|
|11:15-11:30||Wei Zhu (Canadian Institute of Theoretical Astrophysics)||Many Kepler Planets have Distant Companions|
|11:30-12:00||Chris Lintott (University of Oxford)||Citizen Science with Kepler and K2 (invited)|
|Simultaneous Breakout Sessions I|
|13:30-15:00||David Soderblom (STScI)||Opportunities and Limitations of the Cluster Data from Kepler/K2|
|13:30-15:00||Geert Barentsen (NASA Ames) and Christina Hedges (NASA Ames)||The Lightkurve package for Kepler & TESS data analysis: tutorials and consulting breakout|
|13:30-15:00||Eric Feigelson (Penn State University)||Finding Planets in Kepler Lightcurves with R|
|Simultaneous Breakout Sessions II|
|15:30-17:00||Ann Marie Cody (BAERI/NASA Ames)||A Crowded Field Photometry Challenge|
|15:30-17:00||Michael Gully-Santiago (NASA Ames)||Modeling Correlated Noise with Gaussian Processes|
|15:30-17:00||Lee Rosenthal (Caltech)||RadVel: The Radial Velocity Fitting Toolkit|
Thursday, March 7, 2019
|Session 1: Stellar Rotation and Gyrochronology|
|08:30-09:00||Ruth Angus (AMNH and The Flatiron Institute)||The Kepler Revolution: Stellar Rotation and Activity in Clusters and the Field (invited)|
|09:00-09:15||Jason Curtis (Columbia University)||Building Precision Stellar Clocks with Kepler and Gaia|
|09:15-09:30||Beate Stelzer (University of Tuebingen)||The Rotation-activity-age Relation of M Dwarfs in the Era of Kepler and K2|
|09:30-09:45||Lauren Doyle (Armagh Observatory and Planetarium)||The Rotational Phase Distribution of Stellar Flares on M dwarfs|
|09:45-10:00||Joshua Reding (UNC Chapel Hill)||The Confluence of Hardware Failures That Lead to the Discovery of the Most Rapidly Rotating Isolated White Dwarf|
|Session 2: Exoplanets Over Time|
|10:30-11:00||Andrew Mann (UNC Chapel Hill)||Tracing Planetary Evolution with K2 (invited)|
|11:00-11:15||Ann Marie Cody (BAERI/NASA Ames)||Young Stars in the Time Domain: The View with Kepler|
|11:15-11:30||Eric Gaidos (University of Hawaii)||What Orbits a Mysterious Young "Dipper" Star in Taurus?|
|11:30-11:45||Laura Venuti (NPP Fellow, NASA Ames Research Center)||A Dynamical View of Star-disk Interaction Processes in the Lagoon Nebula with Kepler/K2|
|11:45-12:00||Samuel Grunblatt (University of Hawaii)||Planetary Archaeology: Exploring the Planet Population of Evolved Stars|
|Session 3: Fundamental Stellar Parameters|
|13:30-14:00||Patrick Gaulme (Max Planck Institut fur Sonnensystemforschung)||Asteroseismology, Red Giants, and Eclipsing Binaries (invited)|
|14:00-14:15||Timothy White (Australian National University)||Testing Asteroseismic Ages of Red Giants with the Hyades|
|14:15-14:30||Benjamin Pope (New York University)||Naked-Eye Stars in Kepler and K2|
|14:30-14:45||Dominic Bowman (KU Leuven)||Blue Supergiants Reveal Diverse Pulsational Variability in K2 Photometry|
|14:45-15:00||Simon Murphy (University of Sydney)||Pulsating Stars in Binaries|
|Session 4: Planetary Architectures|
|15:30-16:00||Lauren Weiss (University of Hawaii)||Planetary System Architectures and Dynamics (invited)|
|16:00-16:15||Jack Lissauer (NASA Ames)||Architecture and Dynamics of Kepler’s Multi-Transiting Planet Systems: Comprehensive Investigation Using All Four Years of Kepler Mission Data|
|16:15-16:30||Darin Ragozzine (Brigham Young University)||Getting More Out of Information-rich Kepler Multis That Show TTVs|
|16:30-16:45||Sarah Millholland (Yale University)||Obliquity Tides and their Role in Understanding the Kepler Planet Period Ratio Distribution|
|16:45-17:00||Miranda Herman (University of Toronto)||Revisiting the Long-Period Transiting Planets from Kepler|
|17:00-18:30||Poster Session II|
Friday, March 8, 2019
|Session 1: Internal Rotation and Asteroseismology|
|08:30-09:00||Sebastian Deheuvels (IRAP Toulouse)||Monitoring the Internal Rotation of Stars Along Their Evolution with Kepler (invited)|
|09:00-09:15||Jim Fuller (Caltech)||A Solution to the Slow Spins of Stellar Cores|
|09:15-09:30||Barbara Endl (Baylor University)||Asteroseismology of White Dwarfs Observed by Kepler and K2|
|09:30-09:45||Roberto Szabo (MTA CSFK, Konkoly Observatory)||Classical Pulsating Variables in the Kepler/K2 Era|
|09:45-10:00||Katrien Kolenberg (KU Leuven, University of Antwerp)||RR Lyr: An Old Friend in a New Light, with Kepler|
|Session 2: Kepler/K2 Follow-Up Programs|
|10:30-10:45||David Ciardi (Caltech/IPAC-NExScI)||The Legacy of Kepler and K2: The Follow-up Observation Programs|
|10:45-11:00||David Latham (Harvard-Smithsonian CfA)||Contributions from HARPS-N to the Mass-Radius Diagram for Kepler/K2 Planets|
|11:00-11:15||Erik Petigura (Caltech)||Metal-rich Stars Host a Greater Diversity of Planets|
|11:15-11:30||Cintia Fernanda Martinez (Observatorio Nacional)||An Independent Spectroscopic Analysis of the California-Kepler Survey Sample: A Slope in the Small Planet Radius Gap|
|11:30-11:45||Eric Mamajek (NASA JPL/Caltech)||Small (In)temperate Planets: A Closer Look at Habitable Zone Terrestrial-sized Planet Candidates|
|11:30-11:45||Ian Crossfield (MIT)||Atmospheric Characterization of Kepler/K2 Planets|
|13:30-13:45||Poster Competition Winners (5+2 min each)|
|Session 3: Solar System Science, Other Missions, and Reflections|
|13:45-14:00||Andras Pal (Konkoly Observatory)||New Results with K2 in Solar System Exploration|
|14:00-14:15||Jessie Dotson (NASA Ames)||Observations of Solar System Objects with K2|
|14:15-14:30||Andrea Fortier (University of Bern)||The CHEOPS Mission|
|14:30-14:45||George Ricker (MIT)||The TESS Mission: Current Status and Future Plans|
|14:45-15:15||Jessie Christiansen (Caltech/IPAC-NExScI)||Reflections (invited)|
We encourage all presenters to use color-blind friendly figures in their talk and poster presentations. Resources to produce color-blind friendly presentations include this website.
The length for invited talks is 25 minutes + 5 minutes for questions, and contributed talks have 12 minutes + 3 minutes for questions.
Note that the projectors can handle both 16:9 and 4:3 format. Presenters should provide their presentations no later than during the break prior to the session in which the talk is being given.
All posters must be approved by the SOC – no late or extra posters are allowed due to space limitations.
Posters should be no larger than 42'' x 42'' (106 cm x 106 cm). Poster numbers will be placed in the upper corner of each poster board. Poster numbers will be assigned after January 15, 2019, the final deadline to submit poster abstracts.
All posters will be up for the entire duration of the meeting. Posters can be mounted starting at 8:00 AM PST on Monday, March 4 and should be taken down by 4:00 PM PST Friday, March 8.
Each author is responsible for mounting his/her material prior to the opening of the poster session and for removing it at the end of the meeting. Pins will be available in the poster room.
If you are not planning on taking your poster with you at the end of the conference, please put it in a blue recycling bin in the corner of the room prior to your departure. The Kepler/K2 mission will not assume responsibility for materials left behind.
Registration for the poster competition for graduate students and postdocs will open at the registration desk on Monday morning. Each participant should mark their poster with a sticker which will be provided at the registration desk. Competition winners will be notified on Wednesday evening and will present a 5+2 min talk immediately after lunch on Friday.
Lodging, Parking, and Venue Information
NOTE: Some conference registrants have reported receiving phone calls from the hotel asking for dates and other information. This is a scam and you should not respond! All registrants wishing to stay at the Glendale Hilton must make their reservations themselves; you will not receive a phone call asking for this information!
The conference location and hotel is the Hilton Los Angeles North/Glendale & Executive Meeting Ctr located at 100 West Glenoaks Blvd, Glendale, California, 91202. A block of rooms has been reserved for March 2, 2019 - March 9, 2019. The special sleeping room rate includes free wifi and will be available until February 10, 2019 or until the group block is sold-out, whichever comes first. Rooms in the block can be reserved by following this link.
If you are interested in shared housing, please contact us so we can connect you with others interested as well. You can also indicate interest upon registering for the meeting.
For Attendees Staying at the Hotel: Self parking is free for this conference and includes in/out privileges.
For Attendees Not Staying at the Hotel (Day Guests): Self parking is still free. Just inform the attendant that you are attending the Kepler meeting.
Everyone: If you wish to use valet parking, the rate is $19/day.
We have limited funding to support local costs (hotel and per diem) for a limited number of participants who would otherwise be unable to attend the meeting. Applications for travel support were due on Nov. 15 and are no longer being accepted. Applicants will receive a decision by Dec. 20.
Code of Conduct
We expect all attendees to agree with and abide by our code of conduct. Upon registration, attendees will be asked to click a box to confirm that they agree with this code. If you have concerns, suggestions, or would like to report a violation, please contact Jessie Dotson at 650-701-7040.
- Ruth Angus, American Museum of Natural History / Flatiron Institute / Columbia University
- Sarah Ballard, Massachusetts Institute of Technology
- Bill Borucki, NASA Ames Research Center
- Jessie Christiansen, NASA Exoplanet Science Institute
- Sébastien Deheuvels, Research Institute in Astrophysics and Planetology (IRAP Toulouse)
- Courtney Dressing, University of California, Berkeley
- Peter Garnavich, University of Notre Dame
- Patrick Gaulme, Max Planck Institute for Solar System Research
- Chris Lintott, Oxford University
- Mia Lundkvist, Aarhus University
- Andrew Mann, University of North Carolina at Chapel Hill
- Katelynn McCalmont, Ball Aerospace
- Marc Pinsonneault, The Ohio State University
- Krista Lynne Smith, Stanford University
- Andrew Vanderburg, University of Texas at Austin
- Lauren Weiss, University of Hawaii, Manoa
Scientific Organizing Committee
- Knicole Colón, NASA Goddard Space Flight Center (co-Chair)
- JJ Hermes, University of North Carolina at Chapel Hill (co-Chair)
- Suzanne Aigrain, University of Oxford
- Geert Barentsen, NASA Ames Research Center
- David Ciardi, Caltech/IPAC-NASA Exoplanet Science Institute
- Jessie Dotson, NASA Ames Research Center
- Dawn Gelino, Caltech/IPAC-NASA Exoplanet Science Institute
- Matt Holman, Harvard University
- Andrew Howard, Caltech
- Steve Howell, NASA Ames Research Center
- Katrien Kolenberg, KU Leuven
- Savita Mathur, Instituto de Astrofísica de Canarias
- Armin Rest, Space Telescope Science Institute
Local Organizing Committee
- Geert Barentsen, NASA Ames Research Center
- Knicole Colón, NASA Goddard Space Flight Center
- Jessie Dotson, NASA Ames Research Center
- Dawn Gelino, Caltech/IPAC-NASA Exoplanet Science Institute
- Ellen O'Leary, Caltech/IPAC-NASA Exoplanet Science Institute
If you have questions regarding the conference, please send an email to email@example.com.