A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data

Bibcode
2013AdAst2013E...9M
DOI
10.1155/2013/780407
Macías-Pérez, J. F.; Davies, R. D.; Watson, R.; Gutierrez, C. M. ; Rebolo, R.
Referencia bibliográfica

Advances in Astronomy, vol. 2013, id. 780407

Fecha de publicación:
8
2013
Número de autores
5
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
The Anomalous microwave emission (AME) has been proved to be an important component of the Galactic diffuse emission in the range from 20 to 60 GHz. To discriminate between different models of AME low frequency microwave data from 10 to 20 GHz are needed. We present here a re-analysis of published and un-published Tenerife data from 10 to 33 GHz at large angular scales (from 5 to 15 degrees). We cross-correlate the Tenerife data to templates of the main Galactic diffuse emissions: synchrotron, free-free and thermal dust. We find evidence of dust correlated emission in the Tenerife data that could be explained as spinning dust grain emission.
Tipo
Con árbitro

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