'Planet detection' presentation slideshows

The Small Star Opportunity to Find and Characterize Habitable Planets

The Small Star Opportunity to Find and Characterize Habitable Planets. Jacob Bean. Harvard-Smithsonian Center for Astrophysics. Collaborators:. Texas Fritz Benedict Chris Sneden Barbara McArthur Amber Armstrong (ugrad, now STScI) Germany Andreas Seifahrt (now UC Davis) Ansgar Reiners

717 views • 61 slides

The Small Star Opportunity to Find and Characterize Habitable Planets

The Small Star Opportunity to Find and Characterize Habitable Planets. Jacob Bean. Harvard-Smithsonian Center for Astrophysics. Collaborators:. Texas Fritz Benedict Chris Sneden Barbara McArthur Amber Armstrong (ugrad, now STScI) Germany Andreas Seifahrt (now UC Davis) Ansgar Reiners

614 views • 61 slides

Diversity of Data in the Search for Exoplanets Rachel Akeson NASA Exoplanet Science Institute

417 views • 33 slides

407 views • 28 slides

Jian Ge, University of Florida

A Global Network for Planet Detection and Asteroseismology Study using Extremely high Precision Extrasolar Planet Tracker Instruments. Jian Ge, University of Florida. UF team members:

371 views • 27 slides

Before and Beyond

262 views • 21 slides

UKIRT: Current Status and Future Plans

UKIRT: Current Status and Future Plans. Natonal Astronomy Meeting 20 th April 2009 Professor Gary Davis, Director. Vital Statistics: primary diameter 3.8m first light 1979 operates exclusively in the infrared Mauna Kea, Hawaii funded 100% by the UK member of OPTICON

292 views • 14 slides

UKIRT: Current Status and Future Plans

UKIRT: Current Status and Future Plans. Natonal Astronomy Meeting 20 th April 2009 Professor Gary Davis, Director. Vital Statistics: primary diameter 3.8m first light 1979 operates exclusively in the infrared Mauna Kea, Hawaii funded 100% by the UK member of OPTICON

149 views • 14 slides

Observing Very Young Stars with GPI

Observing Very Young Stars with GPI. Quinn Konopacky, Bruce Macintosh, Marshall Perrin, Jenny Patience, et al. Stars younger than the primary GPI sample (<10 Myr) represent an interesting population for planet detection with GPI.

137 views • 13 slides

Abstract

Maximizing planet detection zone area Microlensing is unique in its sensitivity to wider-orbit (i.e. cool) planetary-mass bodies .

124 views • 1 slides