KeplerThe NASA Kepler mission recently announced over 1200 exoplanet candidates. While some are common Hot Jupiters, a large number are Neptune size and smaller, transit depths suggest sizes down to the radius of Earth. The Kepler project has a fairly high confidence that most of these candidates are real exoplanets. Many analysis steps and lessons learned from Kepler light curves are used during the vetting process. This talk will cover some new results in the areas of stellar variability, solar systems with multiple planets, and how transit-like signatures are vetted for false positives, especially those indicative of small planets.
Document ID
20110012490
Acquisition Source
Ames Research Center
Document Type
Presentation
Authors
Howell, Steve B. (NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
September 8, 2013
Publication Date
March 31, 2011
Subject Category
Astronomy
Report/Patent Number
ARC-E-DAA-TN3353Report Number: ARC-E-DAA-TN3353
Meeting Information
Meeting: Steward Observatory -- NOAO Joint Colloquium Series
Location: Tucson, AZ
Country: United States
Start Date: March 31, 2011
Sponsors: National Optical Astronomy Observatories