Institute for Advanced Study Informal Astrophysics Seminar
A Pilot for a Very Large Array HI deep Field
ABSTRACT: Neutral atomic hydrogen is by far the most abundant element in
galaxies. Although reasonably complete images of the HI sky exist out
to redshifts of 0.08, we know surprisingly little about the HI
properties of galaxies at larger redshifts. This will change
dramatically with the pending completion of the upgrade of the VLA and
the construction of SKA pathfinders MeerKAT and ASKAP. Soon it will be
possible to make in HI deep pencil beam surveys out to z=0.5. To prepare
for these new opportunities we have performed a pilot for an EVLA HI
Deep Field, probing in one pointing (0.5 square degrees) all the HI at
redshifts from 0 to 0.2. I will motivate the science, present
preliminary results and
discuss future possibilities.
Date & Time
May 09, 2013 | 11:00am – 12:00pm
Location
Bloomberg Hall, Astrophysics LibrarySpeakers
Jacqueline van Gorkom
Affiliation
Columbia University