The Balloon-borne Anisotropy Measurement (BAM): Status and Future Prospects

Details The Balloon-borne Anisotropy Measurement (BAM): Status and Future Prospects The Balloon-borne Anisotropy Measurement (BAM): Status and Future Prospects

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.564t&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

BAM is designed to measure the cosmic microwave background (CMB) anisotropy at medium angular scales. BAM is unique in the filed, using a cryogenic differential Fourier transform spectrometer couple dto a lightweight off-axis telescope. The first flight of BAM found evidence of anisotropy in the microwave sky. We will present preliminary results from the second flight of BAM and discuss plans for a long duration balloon flight.

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