Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-19T12:14:13.924Z Has data issue: false hasContentIssue false
  • English
  • Français

Cosmic Microwave Background science from Dome C

Published online by Cambridge University Press:  24 December 2009

L. Spinoglio ,
N. Epchtein ,
P. de Bernardis ,
D. Barbosa ,
Y. Giraud-Héraud ,
M. Gervasi ,
E. Kreysa ,
B. Maffei ,
S. Masi  and
P. Mauskopf
...Show all authors
P. de Bernardis
Affiliation:
Dipartimento di Fisica, Universitá di Roma La Sapienza, Italy
D. Barbosa
Affiliation:
Grupo de RadioAstronomia, Instituto de Telecomunicações, Aveiro, Portugal
Y. Giraud-Héraud
Affiliation:
APC Paris, France
M. Gervasi
Affiliation:
Dipartimento di Fisica, Universitá di Milano Bicocca, Italy
E. Kreysa
Affiliation:
Max Planck Radioastronomie, Bonn, Germany
B. Maffei
Affiliation:
University of Manchester, UK
S. Masi
Affiliation:
Dipartimento di Fisica, Universitá di Roma La Sapienza, Italy
P. Mauskopf
Affiliation:
Department of Physics and Astronomy, University of Cardiff, UK
F. Pajot
Affiliation:
IAS Orsay, France
L. Verde
Affiliation:
Institute of Space Sciences, Bellaterra, Spain
Get access

Abstract

We summarize the results of the Cosmic Microwave Background (CMB) working group of the ARENA project. The focus has been on precision measurements of CMB polarization (looking for the echoes of cosmological inflation) and high angular resolution CMB measurements (looking for Sunyaev Zeldovich effect in distant clusters of Galaxies, to probe the evolution of the Universe, Dark Matter and Dark Energy). For both projects the Dome C site represents the best choice worldwide.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 40: 3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica) , 2010 , pp. 391 - 398
Copyright
© EAS, EDP Sciences, 2010

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Battistelli, E.S., et al., 2002, Astrophys. J., 580, L101 CrossRef
Baumann, D., et al. [astro-ph/0811.3919]
Calisse, P.G., Ashley, M.C.B., Burton, M.G., et al., 2004, PASA, 21, 256 CrossRef
Calvo, M., et al., 2008, Mem. S. A. It., 75, 282
Carlstrom, J., Holder, G., & Reese, E., 2002, Ann. Rev. Astron. Astrophys., 40, 643 CrossRef
Chiang, H.C., et al., 2009, ApJ, submitted [astro-ph/0906.1181]
Colafrancesco, S., et al., 2007, Astron. Astrophy., 467, 1, L1-L5 CrossRef
de Bernardis, P., et al., 2009, Exper. Astron., 23, 5 [astro-ph/0808.1881] CrossRef
de Korte, P., 2009, Astrophysics Detector Workshop 2008, P. Kern ed., EAS Publ. Series, 37, 19–22 CrossRef
Doyle, S., et al., 2008, J. Low Temp. Phys., 151, 530 CrossRef
Hamilton, J.C., et al., 2008, Astron. Astrophys., in press [astro-ph/0807.0438]
Hanany, S., & Rosenkranz P. [astro-ph/0307052]
Hincks, A.D., et al., 2009, ApJ, submitted [astro.ph/0907.0461]
Masi, S., et al., 2006, Astron. Astrophys., 458, 687 CrossRef
Polenta, G., et al., 2007, New Astron. Rev., 51, 256 CrossRef
Ruhl, J., et al., 2004, Proc. SPIE, 5498, 11 CrossRef
Staniszewski, Z., et al., 2008, ApJ, submitted [astro-ph/0810.1578]
Stark, A., 2003 [astro-ph/0309005]
Valenziano, L., & Dall' Oglio, G., 1999, Publ. Astron. Soc. Aust., 16, 167 CrossRef