PPT-Microlensing Theory and Observables

Yossi Shvartzvald NPP Fellow JPL Microlensing Geometry       Microlensing Geometry           Microlensing Geometry           Microlensing Geometry. 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-. Microlensing. Planetary Systems.. Scott Gaudi. Matthew Penny. (OSU). WFIRST . Microlensing. Survey.. Microlensing. Survey Dataset. . Properties.. . ~. 3. sq. deg.. ~432 days.. ~80% of the area will have 2 million seconds of integration time.. David . Bennett. University of Notre Dame. WFIRST. Unique Science from Space-based Survey. Exoplanet Survey Question #1: How do planetary systems form and evolve?. complementary to . Kepler. Exoplanet sensitivity down to sub-Earth masses at 0.5 AU - ∞. of . the Standard . Model after . the discovery of an SM-like scalar boson. Andreas Hoecker (CERN). Solvay . workshop . “. Facing . the Scalar . Sector. ”, . May . 29. -. 31, . 2013 . Introduction. 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. -. . D. 0. K. -. Decays at CDF. Karen Gibson. University of Pittsburgh. ICHEP 2008. 08/01/08. CP Asymmetries in B. -. . D. 0. K. -. Decays. CP asymmetries in B. -. . D. 0. K. -. decays can be used to gain information about CKM angle . 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. J.T. . Hoeksema, J. . Schou. , S. . Couvidat. , R.S. Bogart, R.I. Bush, T.L. Duvall, Jr., Y. Liu, A.A. Norton, and P.H. Scherrer. The . Helioseismic. and Magnetic Imager (HMI) acquires sequences of polarized . 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. Daisuke Suzuki. ISAS / JAXA. the MOA collaboration. August . 8. , 2017 . 2017 Sagan Summer Workshop. Microlensing in the Era of WFIRST . a. snow. . = 2.7 (. M. /. M. Sun. ) AU. http://. exoplanet.eu. J.T. . Hoeksema, J. . Schou. , S. . Couvidat. , R.S. Bogart, R.I. Bush, T.L. Duvall, Jr., Y. Liu, A.A. Norton, and P.H. Scherrer. The . Helioseismic. and Magnetic Imager (HMI) acquires sequences of polarized . 6. Extragalactic Microlensing. Wambsganss. . 2001. /sharp caustic crossing. /2,3-pt lens. Local Group vs. Extragalactic Microlensing. =k. Local Group Microlensing – . very very low optical depth. David A. Kosower. Institut. de Physique . Th. é. orique. , CEA–. Saclay. work with. Ben . Maybee. and . Donal. O’Connell (Edinburgh). [arXiv:1811.10950];. by. Ben . Maybee. , . Donal. O’Connell, and Justin Vines [1906.09260]. David Sperzel, MD, MS. August-September 2016. 1. PROJECT GOAL. Analyze and integrate . exiting materials on the . Observables Model. , . Clinical Life Phases. , and . Situations with explicit context .