Abstract
The COBE Differential Microwave Radiometer (DMR) experiment will measure the anisotropy of the cosmic microwave background radiation (CMBR). The initial phase of data analysis uses a ‘sparse matrix’ algorithm to convert the differential temperature data into sky maps. The sky maps are then fitted to a ‘fast’ multipole expansion in spherical harmonics. Since the CMBR anisotropy is very weak, powerful techniques are used to extract the angular unevenness of the sky from the low signal-to-noise data. Instrument signature and other systematic errors are subtracted by fitting models of these effects. Test results are presented.
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© 1989 Plenum Press, New York
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Torres, S. et al. (1989). Cosmic Background Explorer (COBE) Satellite Anisotropy Experiment Data Analysis Techniques. In: Di Gesù, V., Scarsi, L., Crane, P., Friedman, J.H., Levialdi, S., Maccarone, M.C. (eds) Data Analysis in Astronomy III. Ettore Majorana International Science Series, vol 40. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-5646-2_32
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DOI: https://doi.org/10.1007/978-1-4684-5646-2_32
Publisher Name: Springer, Boston, MA
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