A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data
Joint Authors
Davies, R. D.
Gutierrez, C. M.
Watson, R.
Rebolo, R.
Macías-Pérez, J. F.
Source
Issue
Vol. 2013, Issue 2013 (31 Dec. 2013), pp.1-15, 15 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2013-03-11
Country of Publication
Egypt
No. of Pages
15
Main Subjects
Abstract EN
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We present here a reanalysis of published and unpublished Tenerife data from 10 to 33 GHz at large angular scales (from 5 to 15 degrees).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.
American Psychological Association (APA)
Macías-Pérez, J. F.& Davies, R. D.& Watson, R.& Gutierrez, C. M.& Rebolo, R.. 2013. A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data. Advances in Astronomy،Vol. 2013, no. 2013, pp.1-15.
https://search.emarefa.net/detail/BIM-497413
Modern Language Association (MLA)
Macías-Pérez, J. F.…[et al.]. A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data. Advances in Astronomy No. 2013 (2013), pp.1-15.
https://search.emarefa.net/detail/BIM-497413
American Medical Association (AMA)
Macías-Pérez, J. F.& Davies, R. D.& Watson, R.& Gutierrez, C. M.& Rebolo, R.. A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data. Advances in Astronomy. 2013. Vol. 2013, no. 2013, pp.1-15.
https://search.emarefa.net/detail/BIM-497413
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-497413
