PPT-T he Mass Function of Planets Measured from Microlensing

Daisuke Suzuki ISAS JAXA the MOA collaboration August 8 2017 2017 Sagan Summer Workshop Microlensing in the Era of WFIRST a snow 27 M M Sun AU http exoplaneteu. only 2 50-day observing windows per year. The bulge must be observed whenever it can be. Significant “edge effect” penalties for regular interruptions. 0.5 year . SNe. program. Must sample high-. temperature both . in . situ. (a) and . ex situ . (b).. Understanding depoling behavior through property and structure measurements of Fe-doped NBT. Permittivity and loss measured . as a function of . Heck. is. . . Metrics. ?. Metrics is the Language of Science. By measuring, scientists can express their observations more precisely and communicate more information about what they observe.. Metrics is worldwide. A PHOTOMETRIC TRANSIT SEARCH FOR PLANETS AROUND COOL STARS . FROM THE ITALIAN ALPS: RESULTS FROM A FEASIBILITY STUDY. A. . Bernagozzi. . (1),. E. . Bertolini. . (1),. P. . Calcidese. . (1),. . M. . Figure of Merit . David . Bennett. University of Notre Dame. WFIRST. WFIRST Microlensing Figure of Merit. Primary FOM1 - # of planets detected for a particular mass and separation range. Cannot be calculated analytically – must be simulated. . Yossi Shvartzvald NPP Fellow @ JPL. . Microlensing . Geometry.  .  .  . Microlensing . Geometry.  .  .  .  .  . Microlensing . Geometry.  .  .  .  .  . Microlensing . Geometry. in Globular Clusters. Margarita . Safonova. . Ancient Greeks knew that light travels in a straight line... Or you wouldn’t be able to cross the road!. Gravitational . Lensing. —. Astronomical Mirages. E.ST.05.21. Describe the motion of planets and moons in terms of. rotation on axis and . orbits.. Advanced Note-Taking Practice 101! . Every time you see something typed in . YELLOW. …you need to write it down. . and a fly’s-eye ‘. evryscope. ’. at Antarctica. Philip . Yock. , Auckland, New Zealand. 20th Microlensing Workshop . Institut. . d'Astrophysique. de Paris. 13-15 January 2016 . Twenty years ago. The Ohio State University. (with the WFIRST SDTs and on behalf of the WFIRST . μSIT. ). Completing the Census of . Exoplanetary. Systems . with WFIRST.. 21. st. International . Microlnesing. Conference. On the Giant Drop on the Gold Coast, passengers fall 120 . metres. (39 . storeys. ) in 5 seconds, reaching speeds up to 135 km/h! . A . magnetic braking system stops them just before they hit the ground. . Sergei . popov. Sizes and masses. 1312.3323. Radius vs. mass. 1604.07558. Results of modeling.. Old (relaxed) planets.. Colors correspond to . different fractions . of light elements.. Light elements contribution. Neal Evans. The University of Texas at Austin and . KASI. The Long and Winding Road. Core to Star + Disk. The idea of a Core. Some simple theory. Evolutionary Stages and SED Classes. Dense Cores. Observations find regions of strongly enhanced density, decreased turbulence. Jennifer Yee. &. Etienne . Bachelet. Big Picture. Using simulated WFIRST light curves, explore the kinds of . microlensing. planets WFIRST will find.. Goals. Identify planetary perturbations in light curves.