Peculiarities of phases of the WMAP quadrupole
Int.J.Mod.Phys.D17:179-194,2008 We present the analysis on the quadrupole phases of the Internal Linear Combination map, ILC(I) and (III) derived by the WMAP team (1 and 3-year data release). This approach allows us to see the global trend of non-Gaussianity of the quadrupoles for the ILC(III) map t...
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creator | Naselsky, Pavel D Verkhodanov, Oleg V |
description | Int.J.Mod.Phys.D17:179-194,2008 We present the analysis on the quadrupole phases of the Internal Linear
Combination map, ILC(I) and (III) derived by the WMAP team (1 and 3-year data
release). This approach allows us to see the global trend of non-Gaussianity of
the quadrupoles for the ILC(III) map through phase correlations with the
foregrounds. Significant phase correlations is found in between the ILC(III)
quadrupole and the WMAP foregrounds phases for K-W band: the phases of the
ILC(III) quadrupole xi_{2,1}, xi_{2,2} and those of the foregrounds at K-W
bands Phi_{2,1}, Phi_{2,2} display significant symmetry: xi_{2,1}+Phi_{2,1} ~=
xi_{2,2}+Phi_{2,2}, which is a strong indication that the morphology of the
ILC(III) quadrupole is mere reflection of that the foreground quadrupole
through coupling. To clarify this issue we exploit the symmetry of the CMB
power, which is invariant under permutation of the index m=12. By simple
rotation of the ILC(III) phases with the same angle we reach the phases of
foreground quadrupole. We discuss possible sources of phase correlation and
come to the conclusion that the phases of the ILC(III) quadrupole reflect most
likely systematic effects such as changing of the gain factor for the 3-year
data release with respect to the 1-year, rather than manifestation of the
primordial non-Gaussianity. |
doi_str_mv | 10.48550/arxiv.astro-ph/0609409 |
format | Article |
fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_astro_ph_0609409</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>astro_ph_0609409</sourcerecordid><originalsourceid>FETCH-arxiv_primary_astro_ph_06094093</originalsourceid><addsrcrecordid>eNpjYJA3NNAzsTA1NdBPLKrILNNLLC4pytctyNA3MDOwNDGw5GTQC0hNLs3JTCzKLMlMLVbIT1MoyEgshrBKMlIVwn0dAxQKSxNTikoL8nNSeRhY0xJzilN5oTQ3g6qba4izhy7Y_PiCoszcxKLKeLA98QUZ8VB7jIlVBwBGGTiQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Peculiarities of phases of the WMAP quadrupole</title><source>arXiv.org</source><creator>Naselsky, Pavel D ; Verkhodanov, Oleg V</creator><creatorcontrib>Naselsky, Pavel D ; Verkhodanov, Oleg V</creatorcontrib><description>Int.J.Mod.Phys.D17:179-194,2008 We present the analysis on the quadrupole phases of the Internal Linear
Combination map, ILC(I) and (III) derived by the WMAP team (1 and 3-year data
release). This approach allows us to see the global trend of non-Gaussianity of
the quadrupoles for the ILC(III) map through phase correlations with the
foregrounds. Significant phase correlations is found in between the ILC(III)
quadrupole and the WMAP foregrounds phases for K-W band: the phases of the
ILC(III) quadrupole xi_{2,1}, xi_{2,2} and those of the foregrounds at K-W
bands Phi_{2,1}, Phi_{2,2} display significant symmetry: xi_{2,1}+Phi_{2,1} ~=
xi_{2,2}+Phi_{2,2}, which is a strong indication that the morphology of the
ILC(III) quadrupole is mere reflection of that the foreground quadrupole
through coupling. To clarify this issue we exploit the symmetry of the CMB
power, which is invariant under permutation of the index m=1<->2. By simple
rotation of the ILC(III) phases with the same angle we reach the phases of
foreground quadrupole. We discuss possible sources of phase correlation and
come to the conclusion that the phases of the ILC(III) quadrupole reflect most
likely systematic effects such as changing of the gain factor for the 3-year
data release with respect to the 1-year, rather than manifestation of the
primordial non-Gaussianity.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0609409</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2006-09</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0609409$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0609409$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1142/S0218271808011936$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Naselsky, Pavel D</creatorcontrib><creatorcontrib>Verkhodanov, Oleg V</creatorcontrib><title>Peculiarities of phases of the WMAP quadrupole</title><description>Int.J.Mod.Phys.D17:179-194,2008 We present the analysis on the quadrupole phases of the Internal Linear
Combination map, ILC(I) and (III) derived by the WMAP team (1 and 3-year data
release). This approach allows us to see the global trend of non-Gaussianity of
the quadrupoles for the ILC(III) map through phase correlations with the
foregrounds. Significant phase correlations is found in between the ILC(III)
quadrupole and the WMAP foregrounds phases for K-W band: the phases of the
ILC(III) quadrupole xi_{2,1}, xi_{2,2} and those of the foregrounds at K-W
bands Phi_{2,1}, Phi_{2,2} display significant symmetry: xi_{2,1}+Phi_{2,1} ~=
xi_{2,2}+Phi_{2,2}, which is a strong indication that the morphology of the
ILC(III) quadrupole is mere reflection of that the foreground quadrupole
through coupling. To clarify this issue we exploit the symmetry of the CMB
power, which is invariant under permutation of the index m=1<->2. By simple
rotation of the ILC(III) phases with the same angle we reach the phases of
foreground quadrupole. We discuss possible sources of phase correlation and
come to the conclusion that the phases of the ILC(III) quadrupole reflect most
likely systematic effects such as changing of the gain factor for the 3-year
data release with respect to the 1-year, rather than manifestation of the
primordial non-Gaussianity.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA3NNAzsTA1NdBPLKrILNNLLC4pytctyNA3MDOwNDGw5GTQC0hNLs3JTCzKLMlMLVbIT1MoyEgshrBKMlIVwn0dAxQKSxNTikoL8nNSeRhY0xJzilN5oTQ3g6qba4izhy7Y_PiCoszcxKLKeLA98QUZ8VB7jIlVBwBGGTiQ</recordid><startdate>20060914</startdate><enddate>20060914</enddate><creator>Naselsky, Pavel D</creator><creator>Verkhodanov, Oleg V</creator><scope>GOX</scope></search><sort><creationdate>20060914</creationdate><title>Peculiarities of phases of the WMAP quadrupole</title><author>Naselsky, Pavel D ; Verkhodanov, Oleg V</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_astro_ph_06094093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Naselsky, Pavel D</creatorcontrib><creatorcontrib>Verkhodanov, Oleg V</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Naselsky, Pavel D</au><au>Verkhodanov, Oleg V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Peculiarities of phases of the WMAP quadrupole</atitle><date>2006-09-14</date><risdate>2006</risdate><abstract>Int.J.Mod.Phys.D17:179-194,2008 We present the analysis on the quadrupole phases of the Internal Linear
Combination map, ILC(I) and (III) derived by the WMAP team (1 and 3-year data
release). This approach allows us to see the global trend of non-Gaussianity of
the quadrupoles for the ILC(III) map through phase correlations with the
foregrounds. Significant phase correlations is found in between the ILC(III)
quadrupole and the WMAP foregrounds phases for K-W band: the phases of the
ILC(III) quadrupole xi_{2,1}, xi_{2,2} and those of the foregrounds at K-W
bands Phi_{2,1}, Phi_{2,2} display significant symmetry: xi_{2,1}+Phi_{2,1} ~=
xi_{2,2}+Phi_{2,2}, which is a strong indication that the morphology of the
ILC(III) quadrupole is mere reflection of that the foreground quadrupole
through coupling. To clarify this issue we exploit the symmetry of the CMB
power, which is invariant under permutation of the index m=1<->2. By simple
rotation of the ILC(III) phases with the same angle we reach the phases of
foreground quadrupole. We discuss possible sources of phase correlation and
come to the conclusion that the phases of the ILC(III) quadrupole reflect most
likely systematic effects such as changing of the gain factor for the 3-year
data release with respect to the 1-year, rather than manifestation of the
primordial non-Gaussianity.</abstract><doi>10.48550/arxiv.astro-ph/0609409</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
title | Peculiarities of phases of the WMAP quadrupole |
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