Slide 1Crew Systems Design Project ENAE 483 October 18, 2012 Rebecca Foust, Shimon Gewirtz, Matthew Rich, and Timothy Russell Slide 2 Mission Itinerary Days 1-3: Voyage to…

Slide 1DustScan Ltd Fine PM – Only Part of the Monitoring Story Oliver Puddle DustScan Ltd 14 March 2013 Slide 2 CONTENTS What is fine particulate matter (PM)? Why do we…

Slide 1 Molecular Gas and Dust in COSMOS Submillimeter Galaxies Caption: Left: 0.3 deg 2 map of a COSMOS field with AzTEC on ASTE at 1.1mm (Scott et al. 2008, MNRAS, 385,…

Slide 1 Star formation Suzanne Ramsay UK Astronomy Technology Centre, Royal Observatory Edinburgh UKIRT+WFCAM infrared image of Orion Slide 2 The Challenge A theory of star…

Slide 1 Sub-arcsecond far-infrared observatory A science imperative Slide 2 Frank Helmich Principal Investigator for Herschel/HIFI Head of SRON´s Low Energy Astrophysics…

Warm Dust in the Most Distant Quasars Ran Wang Department of Astronomy, Peking University, China Introduction Why looking for dust at z~6 The mass of dust in the earliest…

A Systematic Search and Characterization of Dusty Debris Disks M. McElwain, B. Zuckerman (UCLA) Joseph H. Rhee, & I. Song (Gemini Obs.) Photo Credit: T. Pyle (SSC) UCLA…

CONTENTS What is fine particulate matter (PM)? Why do we monitor it? What should PM monitoring achieve? Is fine PM the only emission we can monitor? What is visible ‘nuisance’…

Slide 1 Molecular Gas and Dust in COSMOS Submillimeter Galaxies Caption: Left: 0.3 deg2 map of a COSMOS field with AzTEC on ASTE at 1.1mm (Scott et al. 2008, MNRAS, 385,…

Global and Local Dust over North America Direct questions to Rudolf B. Husar [email protected] Aerosol Types: âDustâ, âSmokeâ and âHazeâ Aerosol are composed of multiple…