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A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background from l = 100 to 400

  • Authors: A. D. Miller, R. Caldwell, M. J. Devlin, W. B. Dorwart, T. Herbig, M. R. Nolta, L. A. Page, J. Puchalla, E. Torbet, and H. T. Tran

Miller et al. 1999 The Astrophysical Journal Letters 524 L1.

  • Provider: AAS Journals

Caption: Fig. 1.

Likelihood of the combined D1 and D2 analysis (solid line) as a function of ﹩\delta T^{2}_{l}﹩. The null tests: quadrature (signal with chopper sweeping one direction minus that with the chopper sweeping the other direction; dotted line), fast and slow dither (differences of subsequent 0.5 and 10 s averages, dashed and dash‐doted lines, respectively), and first half minus second half (triple‐dot–dashed line) are also shown. The vertical lines indicate the maximum, ±1 σ, or 95% confidence upper bound.

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