PPT-Gemini Observatory reveals galaxy that is 99.99% dark matter

National Science Foundation Division of Astronomical Sciences Prepared by the Association of Universities for Research in Astronomy SCIENCE PEOPLE TECHNOLOGY Scientists Discover Galaxy that is 9999 Percent Dark Matter. Observations. Josh . Frieman. DES Project Director. Fermilab. and the University of Chicago. Science with a Wide-. Field Infrared Telescope in Space. Pasadena, February. 2012. 2. 2011 Nobel Prize in Physics. Faculty of Geodesy. Ka. č. i. će. va. 26, 10 000 Zagreb. Double Solar Telescope at Hvar. Hvar Observatory - http://. oh.geof.unizg.hr. Double Solar Telescope at Hvar. C. onsists. . of two Carl Zeiss refractors (. near-infrared . photometry . from the . ground for a crowded star cluster. National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . complexity of . starbirth. in unprecedented clarity . to yield evidence . for orphan stars . National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . and Large-Scale Structure. 1. Cora Dvorkin. IAS (Princeton) Harvard (Hubble fellow) . COSMO 2014. August 2014, Chicago. Outline. Dark Matter overview.. Effect of . WIMP Dark Matter . Lisa Randall. Harvard University. @. lirarandall. . What do we know about dark matter?. It has gravitational interactions—of matter!. Gravitational . lensing. Rotation curves in galaxies. Detailed measurements of energy abundances—total and normal matter. Cody . Carr. , Minh Nguyen. December 9. th. , 2014.. Agenda. Motivations (Cosmic & Atomic scales). Dark Matter categories. The Dark Matter Zoo. Neutrinos. Neutralinos. Kaluza. -Klein particles. Summary. February 2016. The UWA Futures Observatory opened in November 2015 to provide a focus for the Centre for Education Futures’ Scholarship and Innovation stream. . Its . purpose is to:. Promote . and encourage UWA’s future thinking . spend visibility . to . public sector and higher education procurement . and finance teams through a . managed service . which includes a . comprehensive. spend data collection and transformation service, an . John . Moffat. Perimeter Institute. Miami 2015 Conference. Fort Lauderdale, December 16, 2015. 2015-12-21. 1. 2. 2015-12-21. 3. https://angel.co/mog. 2015-12-21. Introduction. Observations of the dynamics of galaxies as well as the dynamics. NOAO/. Gemini Data workshop . –. Tucson, 2010. -. 07-20. Marie Lemoine-Busserolle. . Introduction. Hosted by CADC in Victoria, Canada.. Released September 2004. Gemini North data from May 2000. Gemini South data from October 2001. Cosmic Opportunities. . –. 45. th. SLAC Summer Institute. Jonathan . Feng. , UC Irvine. 16 August 2017. INTRODUCTION. We’ve learned a lot about the Universe. Dark . Matter: 23% . ± 4. %. Dark . Gravity . and Light. Black Holes. What is Dark Matter?. Recap. Midterm . Friday . 11/. 1: summary review sheet posted. Canvas homework : . due Wednesday. Lab this week. Using . gravity to measure . masses. Professor Mike Brotherton. Dobson Chapter 19, . Ryden. and Peterson Chapter 20. Galaxies. “My God, they’re full of stars!” (But more dark matter.). Galaxies. Hubble type & characteristics of different types of nearby galaxies; introduction to galaxy clusters.