Author/Authors :
Nolta، M. R. نويسنده , , Devlin، M. J. نويسنده , , Dorwart، W. B. نويسنده , , Miller، A. D. نويسنده , , Page، L. A. نويسنده , , Puchalla، J. نويسنده , , Torbet، E. نويسنده , , Tran، H. T. نويسنده ,
Abstract :
We present a measurement of the angular spectrum of the cosmic microwave background from l = 26 to 225 from the 30 and 40 GHz channels of the MAT/TOCO experiment based on two seasons of observations. At comparable frequencies, the data extend to a lower l than the recent Very Small Array and DASI results. After accounting for known foreground emission in a self-consistent analysis, a rise from the Sachs-Wolfe plateau to a peak of (delta)Tl ~~80 (mu)K near l ~~200 is observed.
Keywords :
scattering , stars , other (Mira) , variables , binaries , symbiotic , individual (V1016 Cygni)
