A High spatial resolution analysis of the MAXIMA-1 cosmic microwave background anisotropy data
Apr, 2001
7 pages
Published in:
- Astrophys.J.Lett. 561 (2001) L1-L6
e-Print:
- astro-ph/0104459 [astro-ph]
DOI:
Experiments:
Citations per year
Abstract: (arXiv)
We extend the analysis of the MAXIMA-1 cosmic microwave background (CMB) data to smaller angular scales. MAXIMA, a bolometric balloon experiment, mapped a 124 deg region of the sky with 10\arcmin resolution at frequencies of 150, 240 and 410 GHz during its first flight. The original analysis, which covered the multipole range , is extended to using data from three 150 GHz photometers in the fully cross-linked central 60 deg of the map. The main improvement over the original analysis is the use of 3\arcmin square pixels in the calculation of the map. The new analysis is consistent with the original for . For , where inflationary models predict a third acoustic peak, the new analysis shows power with an amplitude of \microk at in excess to the average power of \microk in the range .References(20)
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