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A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400

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arxiv astro-ph/9906421 v4 pith:UIOV3SAG submitted 1999-06-26 astro-ph

A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400

classification astro-ph
keywords approxspectrumangulardatameasurementsamealtiplanoanisotropy
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We report on a measurement of the angular spectrum of the CMB between $l\approx 100$ and $l\approx 400$ made at 144 GHz from Cerro Toco in the Chilean altiplano. When the new data are combined with previous data at 30 and 40 GHz, taken with the same instrument observing the same section of sky, we find: 1) a rise in the angular spectrum to a maximum with $\delta T_l \approx 85~\mu$K at $l\approx 200$ and a fall at $l>300$, thereby localizing the peak near $l\approx 200$; and 2) that the anisotropy at $l\approx 200$ has the spectrum of the CMB.

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  1. DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

    astro-ph.CO 2024-04 accept novelty 7.0

    First-year DESI BAO data are consistent with flat LambdaCDM and, when combined with CMB, show a 2.5-3.9 sigma preference for evolving dark energy (w0 > -1, wa < 0) that strengthens with certain supernova datasets.