Observing the dust
in our galaxy with
BLAST-TNG
Gabriele Coppi
University of Pennsylvania
07/07/2019
Properties of dust in the ISM
From Sharif, PhD Thesis, 2015
Dusty galaxies
Andromeda
How to create stars
Gravitational Energy
Kinetic Energy
Magnetic Field
Pillars of creation
Eagle Nebula
Dust as CMB foreground
Due to its polarization effect, dust is also a strong contaminant for extragalactic sub-mm observations
BK-2014
BK/Planck -2015
BLAST-TNG
NRAO
University of California
Cardiff University
University of Pennsylvania
NIST
Northwestern University
ASU
Università Milano Bicocca
Balloon Large Aperture Submillimeter Telescope - The Next generation
BLAST-TNG in numbers
Why BLAST-TNG
2010
2019
Planck
View from a balloon
View from SPIDER
Why BLAST-TNG on a balloon
Why Antarctica
Why Antarctica
BLASTPol flight path
Telescope
BLAST-TNG Camera
BLAST in the Media
Thanks for listening
and
Enjoy your beer(s)