Spider is a balloon-borne experiment designed to search for primordial gravity waves imprinted on the cosmic microwave background (CMB). Measuring the strength of this signal puts limits on inflationary theory.
The Spider instrument consists of six degree-resolution telescopes cooled to liquid Helium temperature (4 K) which observe at frequencies of 100 GHz, 150 GHz, and 220 GHz (corresponding to wavelengths of 3 mm, 2 mm, and 1.4 mm). Each telescope is coupled to a polarisation-sensitive transition-edge bolometer array cooled to 250 mK.
The first balloon flight of the experiment is planned for 2011 from Alice Springs, Australia. This mid-latitude flight permits mapping of up to half the sky and excellent cross-linking. A second Ultra Long Duration Balloon flight is scheduled for the following season.
The primary science goals include:
- characterization of the curl-free component of the CMB polarization on the largest scales
- searching for the signature of inflationary gravitational waves in the CMB polarization
- characterization of the polarization properties of the emission from our own Milky Way Galaxy
External links
- Spider Homepage at Caltech
- B. P. Crill, et al., "SPIDER: A Balloon-borne Large-scale CMB Polarimeter"
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