The CMBR spectrum: new upper limits for the distortion parameters y and mu

Citation
Es. Battistelli et al., The CMBR spectrum: new upper limits for the distortion parameters y and mu, NEW ASTRON, 5(2), 2000, pp. 77-90
Citations number
20
Categorie Soggetti
Space Sciences
Journal title
NEW ASTRONOMY
ISSN journal
13841092 → ACNP
Volume
5
Issue
2
Year of publication
2000
Pages
77 - 90
Database
ISI
SICI code
1384-1092(20000428)5:2<77:TCSNUL>2.0.ZU;2-P
Abstract
The CMBR Spectrum has been measured by the COBE-FIRAS experiment. Upper lim its only have been found for distortion parameters y and mu: y(up) = 1.5 x 10(-5) and mu(up) = 9 x 10(-5) at 95% of confidence. FIRAS made differentia l measurements between sky and blackbody calibrator The knowledge of its em issivity is important as far as y and mu measurements as concerned. We have re-estimated the XCAL emissivity by using Ray-Tracing techniques. Diffract ion problems have been analyzed by a model based on waveguide approximation : it allowed us to define a propagation function tau inside the XCAL V-groo ve. The emission of the external calibrator distorted with respect to the B lack-Body emission may result in lower upper limits to y and mu. New upper limits for distortion parameters y and mu have been calculated considering the new XCAL emissivity. The results are: y(up) = 3.1 x 10(-5) and mu(up) = 4. x 10(-4) at 95% of confidence. (C) 2000 Elsevier Science B.V. All right s reserved.