Church et al. (1997 [SuZIE94], in preparation [SuZIE98]) use 140 GHz
data from the ground-based SuZIE (Sunyaev-Zel'dovich Infrared
Experiment) experiment on Mauna Kea to constrain CMBR anisotropy.
Ganga et al. (1997b) summarize the SuZIE94 experiment.
The FWHM of the beams, assumed to be gaussian, are
(SuZIE94) and (SuZIE98). The zero-lag window
function of the smooth-scan, two-beam experiment is
The first column in the window function file
is , which runs from
2 to 15000. The second and third columns are the SuZIE94 and SuZIE98
The quoted bandtemperature values for SuZIE94 are from Ganga et al. (1997b).
They were computed assuming a flat bandpower spectrum and, following Ganga
et al. (1997a), account for the SuZIE absolute calibration uncertainty of 8%.
The SuZIE98 results are preliminary and account for the calibration uncertainty
by adding it in quadrature to the statistical 1 error bars.
Ganga et al. (1997b) and Ratra et al. use the SuZIE94 data to constrain
Link to the experiment webpage.
S.E. Church, K.M. Ganga, P.A.R. Ade, W.L. Holzapfel, P.D. Mauskopf, T.M.
Wilbanks, and A.E. Lange, ``An Upper Limit to Arcminute-Scale Anisotropy
in the Cosmic Microwave Background Radiation at 142 GHz", Astrophys. J.
484, 523 (1997).
K. Ganga, B. Ratra, S.E. Church, N. Sugiyama, P.A.R. Ade, W.L. Holzapfel,
P.D. Mauskopf, and A.E. Lange, ``Using Sunyaev-Zeldovich Infrared Experiment
(SuZIE) Arcminute-Scale Cosmic Microwave Background Anisotropy Data to Probe
Open and Flat Cold Dark Matter Cosmogonies",Astrophys. J.
484, 517 (1997b).
K. Ganga, B. Ratra, J.O. Gundersen, and N. Sugiyama, ``UCSB South Pole 1994
Cosmic Microwave Background Anisotropy Measurement Constraints on Open and
Flat- Cold Dark Matter Cosmogonies", Astrophys. J. 484,
B. Ratra, R. Stompor, K. Ganga, G. Rocha, N. Sugiyama, and K.M. Górski, ``Cosmic Microwave Background Anisotropy Constraints on Open and Flat- Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data", Astrophys. J. 517, 549 (1999).