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Imaging the Early Universe with ACBAR. William Holzapfel NSF 5/3/04. The A rcminute C osmology B olometer A rray R eceiver. Caltech: A.E. Lange M.C. Runyan (now at UC) C. Reichardt. Case-Western: J. Ruhl (co-PI) J. Goldstein. U.C. Berkeley: W.L. Holzapfel (co-PI) - PowerPoint PPT Presentation
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Imaging the Early Universe with ACBAR
William HolzapfelNSF 5/3/04
CMU:J.B. Peterson P. Gomez A.K. Romer
U.C. Berkeley:W.L. Holzapfel (co-PI)C.L. Kuo (now at CIT)M.D. Daub
M. Newcomb (2001/2002)Justus Brevik (2004)
Caltech:A.E. LangeM.C. Runyan(now at UC)C. Reichardt
Cardiff:P.A.R. Ade
Case-Western:J. Ruhl (co-PI)J. Goldstein
JPL:J.J. BockA.D. Turner
The Arcminute Cosmology Bolometer Array Receiver
ACBAR is funded by the NSF Office of Polar Programs
IRAS Dust Emission in the Southern Sky
Observes From South Pole
Viper Telescope: 2.0 meter off-axis
350 m tipper data: atmospheric noiseComparison
Arc
min
ute
Cos
mol
ogy
Bol
omet
ric
Arr
ay R
ecei
ver
Quartiles of PWV at three Sites
At each site, the year is divided into the best and worst 6-month periods.
Bars show quartiles of the PWV distribution at each site.
Because of its cold temperatures (annual average temperature –49 C), the South Pole is considerably drier than either Atacama or Mauna Kea.
SZ
Primary CMB
Atmospheric transmission
ACBAR as configured for 2002 Season
Viper refurbishment 1/2001
ACBAROn Viper
at the beginningof the 2002
winter season
Low z Clusters
1E0657-67 (z=0.299) at 3 frequencies
Decrement at 150, nothing at 220, increment at 275 GHz!
CMB5 FieldWinter 2002Highest S/NMap of the
CMBto date
S/N~100On degree
scale structure
WMAP, ACBAR and CBIBennett et al. astro-ph/0302207
Spergel et al., 2003
What does ACBAR add to parameter estimation from WMAP?
ACBAR and CBI were used as an “ext”ension to the WMAP power spectrum to help break parameter degeneracies.
ACBAR
WMAP
ACBAR
BOOMERanG WMAP
Three Identically processed mapsOf the same ~ 6 deg2 of sky.
Precise cross calibration from theCMB is now a possibility for BOOMERANG and ACBAR.
Cross calibration of ACBAR Boomerang and WMAP
Boom 98 CMB image
ACBAR 02 CMB image
B98 Sky coverage
ACBAR CMB2 Sky coverage
ACBAR Present and Future
•ACBAR is currently observing
•Instrument to be refurbished in summer 2005
•Final year of observations winter 2005
•Future of Viper? Potential for a next generation instrument?
Helium FillAugust 2002Matt Newcomb