Orateur
Apolline CHAPPARD
(Ias)
Description
The QUIJOTE MFI instrument (2012-2018) observed the sky at four frequency bands, namely 11, 13, 17 and 19Ghz, at 1 degree angular resolution. We can use the full database of MFI observations to characterize the correlation properties of the atmospheric signal in those frequency bands. This information will be useful to improve the current sky models at these frequencies, and could be used in further MFI reanalyses, or for the preparation of future observations at these frequencies (e.g. Tenerife Microwave Spectrometer). We will present the preliminary results of these analyses.
| Astrophysics Field | Cosmology |
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Auteur principal
Apolline CHAPPARD
(Ias)
