Cosmic microwave background science from Dome C

P. De Bernardis; D. Barbosa; Y. Giraud-Héraud; M. Gervasi; E. Kreysa; B. Maffei; S. Masi; P. Mauskopf; F. Pajot; L. Verde

doi:10.1051/eas/1040054

Cosmic microwave background science from Dome C

P. De Bernardis
, D. Barbosa
, Y. Giraud-Héraud
, M. Gervasi
, E. Kreysa
, B. Maffei
, S. Masi
, P. Mauskopf
, F. Pajot
, L. Verde

Research output: Chapter in Book/Conference proceeding › Conference contribution › peer-review

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. © 2010 EAS, EDP Sciences.

Original language	English
Title of host publication	EAS Publications Series\|EAS Publ. Ser.
Pages	391-398
Number of pages	7
Volume	40
DOIs	https://doi.org/10.1051/eas/1040054
Publication status	Published - 2010
Event	EAS Publications Series - Duration: 1 Jan 1824 → … http://adsabs.harvard.edu/abs/2010EAS....40..391D

Conference

Conference	EAS Publications Series
Period	1/01/24 → …
Internet address	http://adsabs.harvard.edu/abs/2010EAS....40..391D

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10.1051/eas/1040054

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@inproceedings{981ca75e49bb4ab195121bff1e1344ae,

title = "Cosmic microwave background science from Dome C",

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. {\textcopyright} 2010 EAS, EDP Sciences.",

author = "\{De Bernardis\}, P. and D. Barbosa and Y. Giraud-H{\'e}raud and M. Gervasi and E. Kreysa and B. Maffei and S. Masi and P. Mauskopf and F. Pajot and L. Verde",

note = "Spinoglio, L. 40 391-398 DOI: 10.1051/eas/1040054; EAS Publications Series ; Conference date: 01-01-1824",

year = "2010",

doi = "10.1051/eas/1040054",

language = "English",

volume = "40",

pages = "391--398",

booktitle = "EAS Publications Series|EAS Publ. Ser.",

url = "http://adsabs.harvard.edu/abs/2010EAS....40..391D",

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TY - GEN

T1 - Cosmic microwave background science from Dome C

AU - De Bernardis, P.

AU - Barbosa, D.

AU - Giraud-Héraud, Y.

AU - Gervasi, M.

AU - Kreysa, E.

AU - Maffei, B.

AU - Masi, S.

AU - Mauskopf, P.

AU - Pajot, F.

AU - Verde, L.

N1 - Spinoglio, L. 40 391-398 DOI: 10.1051/eas/1040054

PY - 2010

Y1 - 2010

N2 - 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. © 2010 EAS, EDP Sciences.

AB - 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. © 2010 EAS, EDP Sciences.

U2 - 10.1051/eas/1040054

DO - 10.1051/eas/1040054

M3 - Conference contribution

VL - 40

SP - 391

EP - 398

BT - EAS Publications Series|EAS Publ. Ser.

T2 - EAS Publications Series

Y2 - 1 January 1824

ER -

Cosmic microwave background science from Dome C

Abstract

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