South Pole Telescope in the Dark
Sector with an LC-130 taking off in the foreground (photo-Chad
Carpenter)
Back
at the Pole for another year
After
being away from the Pole for about two years, working at my job in Rhode Island, I am back at 90o South Latitude for
another year. This time is different
because I am here as a grantee working for the University of Chicago's
Kavli Institute of Cosmological Physics. I will be a
winterover for the South Pole Telescope (SPT). SPT and control room
underneath, attached to the Dark Sector LAB (DSL)
With this large millimeter/submillimeter
wavelength telescope, we will be scanning 40% of the universe, looking
back at the Cosmic Microwave Background (CMB) radiation that was
scattered shortly following the big bang, over 13 billion years ago. It
is anticipated that this data will reveal the nature of galaxy cluster
formation and provide clues to the mystery of dark energy/dark matter
helping to answer questions regarding the physics governing the
expanding
universe. Also, this year is the International Polar Year
(IPY), a multinational effort to study the polar regions.
For more information on SPT, visit: http://spt.uchicago.edu http://spt.uchicago.edu/public
There is also a recent Chicago Tribune article about the SPT program: http://www.chicagotribune.com/news/chi-telescope_31dec31,0,6168513,full.story
The installation of SPT at the Pole was just completed in February, 2007, when it saw "first light" and initial observations were performed between March and October. This austral summer, the SPT team has been busy with improvements in the telescope receiver (sensor) cryostat, characterization of new bolometer (sensor) arrays, as well as upgrades to the various mechanical systems of the telescope. Once the final bolometer wedges are installed and the telescope is reassembled in late January, observations can begin again for 2008.
brad
assembling receiver cryostat
wire bonding
bolometer wedges
joaquin, brad
assemble receiver cone
attaching
receiver cryostat to secondary mirror cryostat
joaquin,
helmuth connect bolometer squid outputs to data acquisition rack
cryostat
pumpdown, cooldown kathryn analyzing
characterization data joaquin, martin
analyzing characterization data dana moving
telescope nils, dana
installing telescope seals nils, dana,
joaquin on roof(warm, its only -20 F) 10 meter (33 ft) diameter
primary mirror SPT and DSL
SPT is sharing the Dark Sector Laboratory (DSL) with the BICEP
telescope. BICEP is smaller Cosmic Microwave Background (CMB) telescope
examining polarization of the CMB. yuki at work
yuki
topping off BICEP with liquid helium
DSL
showing SPT and BICEP (acbar, dasi, quad no longer
operational)
A Real-Time Photo of South Pole Station as Seen
from the ARO
Building (live when satellite is up)
We had a cargo airdrop by a C-17 in December. C-17 drop
close-up of drop (photo by dawg)
The new elevated station is about complete and the outer gun metal grey
cladding is nearing completion. The station dedication is January 12th.
new
elevated station station
side toward skiway
Meanwhile the old dome is now about empty and the front entrance arch
and familiar sign were removed. I will be a bit sad to see the flag
transferred from the dome to the new station at the dedication on January 12th.
removing
dome sign empty dome
It was also nice to be back in Christchurch, New Zealand on my way down
to the Pole at the beginning of December.
christchurch
square
chess in the
square
entertainment
penguin
bus christchurch botanical
gardens
gardens
chc
museum
Finally, a photo of the C-17 that took me from Christchurch to McMurdo
Station where I boarded a ski-equipped LC-130 for the Pole.
C-17
inside
C-17 (photo by yuki
NEXT
MONTH: January... a busy month and more about South Pole Telescope
A
Comprehensive
South Pole Web Site by Bill Spindler
Winterover
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