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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/GkAoN
Repositorysid.inpe.br/iris@1916/2005/06.02.18.40   (restricted access)
Last Update2008:01.10.16.49.03 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/06.02.18.40.08
Metadata Last Update2018:06.05.01.16.03 (UTC) administrator
Secondary KeyINPE-15136-PRE/10043
ISSN0067-0049
1538-4365
Citation KeyODwyerBCFHHLMMMMMNOPSSTVWWW:2005:CoMiBa
TitleThe cosmic microwave background anisotropy power spectrum from the beast experiment
Year2005
MonthMay
Access Date2024, May 06
Secondary TypePRE PI
Number of Files1
Size1075 KiB
2. Context
Author 1 O'Dwyer, I. J.
 2 Bersanelli, M.
 3 Childers, J.
 4 Figueiredo, N.
 5 Halevi, D.
 6 Huey, G.
 7 Lubin, P. M.
 8 Maino, D.
 9 Mandolesi, N.
10 Marvil, J.
11 Meinhold, P. R.
12 Mejia, Jorge
13 Natoli, P.
14 O'Neill, H.
15 Pina, A.
16 Seiffert, M. D.
17 Stebor, N. C.
18 Tello, Camilo
19 Villela Neto, Thyrso
20 Wandelt, B. D.
21 Williams, B.
22 Wuensche, Carlos Alexandre
Resume Identifier 1
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19 8JMKD3MGP5W/3C9JJA6
Group 1 DAS-INPE-MCT-BR
Affiliation 1 Univ Illinois, Dept Astron, Urbana, IL 61801 USA
 2 Univ Milan, Dept Phys, Milan, I-20133 Italy
 3 Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
 4 Univ Fed Itajuba, Dept Quim & Fis, Itajuba, MG BR-50375009 Brazil
 5 Univ Illinois, Dept Phys, Urbana, IL 61801 USA
 6 Univ Calif, White Mt Res Stn, CA 93514 USA
 7 CNR, IASF, Sez Bologna, Bologna, I-40129 Italy
 8 Inst Nacl Pesquisas Espaciais, Div Astrofis, Sao Jose Dos Campos, BR-12245970 Brazil
 9 Univ Roma Tor Vergata, Dipartimento Fis, Rome, I-00173 Italy
10 Univ Roma Tor Vergata, Sez INFN, Rome, I-00173 Italy
11 CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
JournalAstrophysical Journal Supplement Series
Volume158
Number1
Pages93-100
History (UTC)2005-09-02 10:35:28 :: sergio -> administrator ::
2006-09-28 22:29:38 :: administrator -> sergio ::
2008-01-07 12:52:47 :: sergio -> marciana ::
2008-01-10 16:49:03 :: marciana -> administrator ::
2018-06-05 01:16:03 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordscosmic microwave background
cosmology : observations
large-scale structure of universe
AbstractThe Background Emission Anisotropy Scanning Telescope (BEAST) is a 2.2 m off-axis telescope with an eight-element mixed Q-band (38-45 GHz) and Ka-band (26-36 GHz) focal plane, designed for balloon-borne and ground-based studies of the cosmic microwave background (CMB). Here we present the CMB angular power spectrum calculated from 682 hr of data observed with the BEAST instrument. We use a binned pseudo-C-l estimator (the MASTER method). We find results that are consistent with other determinations of the CMB anisotropy for angular wavenumbers l between 100 and 600. We also perform cosmological parameter estimation. The BEAST data alone produce a good constraint on Omega(k) = 1 - Omega(tot) = 0.074 +/- 0.070, consistent with a flat universe. A joint parameter estimation analysis with a number of previous CMB experiments produces results consistent with previous determinations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The cosmic microwave...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target FileO Dwyer - the cosmic microwave.pdf
User Groupadministrator
marciana
sergio
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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