The Diabolo photometer and the future of ground-based millimetric bolometer devices
/ Authors
F. Désert, A. Benoit, P. Camus, M. Giard, E. Pointecouteau, N. Aghanim, J. Bernard, N. Coron, J. Lamarre, P. Marty
and 2 more authors
/ Abstract
The millimetric atmospheric windows at 1 and 2 mm are interesting targets for cosmological studies. Two broad areas appear leading this field: 1) the search for high redshift star-forming galaxies and 2) the measurement of Sunyaev-Zel’dovich (SZ) effect in clusters of galaxies at all redshifts. The Diabolo photometer is a dual-channel photometer working at 1.2 and 2.1 mm and dedicated to high angular resolution measurements of the Sunyaev-Zel’dovich effect towards distant clusters. It uses 2 by 3 bolometers cooled down to 0.1 K with a compact open dilution cryostat. The high resolution is provided by the IRAM 30 m telescope. The result of several Winter campaigns are reported here, including the first millimetric map of the SZ effect that was obtained by Pointecouteau et al. (2001) [13] on RXJ1347-1145, the non-detection of a millimetric counterpart to the radio decrement towards PC1643+4631 and 2 mm number count upper limits. We discuss limitations in ground-based single-dish millimeter observations, nam...
Journal: arXiv: Astrophysics
DOI: 10.1063/1.1475613