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IR STIG Seminar

Infrared Science and Technology Integration Group

DATE

March 23, 2017

TIME

9:00 am EST

COMMUNITY

IR STIG

TYPE

Seminar

Far-Infrared Next Generation Instrumentation Community Workshop

TitleSpeakerPresentation
Workshop Introduction & ScopeKimberly Ennico[PDF]
What you don't know about SOFIAHal Yorke[PDF]
What may balloons be doing next?Chris Walker[PDF]
Using multiple platforms for Far-IR technology developmentCarl Ferkinhoff[PDF]
Discussion Introduction & Lessons LearnedKimberly Ennico[PDF]
Part 1 - Our Future Are there specific areas that we need to see emphasized in future Far-IR (ROSES, etc.) calls?Moderator: Paul Goldsmith[PDF]
Part 2 - Shaping the Next Generation What do you want your SOFIA Observatory to achieve next? Upcoming ROSES opportunity 
Part 3 - Shaping access above 80,000 feet (24 km) 
Wrap-up and AdjournKimberly Ennico[PDF]

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.