Noise power spectrum estimation and fast map making for CMB experiments

We present a method designed to estimate the noise power spectrum in the time domain for CMB experiments. The noise power spectrum is extracted from the time ordered data avoiding the contamination coming from sky signal and accounting the pixellisation of the signal and the projection of the noise...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astronomy and astrophysics (Berlin) 2004-04, Vol.417 (3), p.1189-1194
Hauptverfasser: Amblard, A., Hamilton, J.-Ch
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1194
container_issue 3
container_start_page 1189
container_title Astronomy and astrophysics (Berlin)
container_volume 417
creator Amblard, A.
Hamilton, J.-Ch
description We present a method designed to estimate the noise power spectrum in the time domain for CMB experiments. The noise power spectrum is extracted from the time ordered data avoiding the contamination coming from sky signal and accounting the pixellisation of the signal and the projection of the noise when making intermediate sky projections. This method is simple to implement and relies on Monte-Carlo simulations, it runs on a simple desk computer. We also propose a trick for filtering data before making coadded maps in order to avoid ringing due to the presence of signal in the timelines. These algorithms were succesfully tested on Archeops data.
doi_str_mv 10.1051/0004-6361:20034066
format Article
fullrecord <record><control><sourceid>proquest_hal_p</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_in2p3_00024475v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1875850226</sourcerecordid><originalsourceid>FETCH-LOGICAL-c459t-bf90529e809e5a6dfc47b63c8f0ff9a015443198247c9621c382636bb25e25c93</originalsourceid><addsrcrecordid>eNp9kctuFDEQRa0IpAxDfiArb0BIqEn52Ta7pIE8NBCJELG0PI4NJv3C7knC3-PWhMmOhVWy6lTVvVUIHRJ4R0CQIwDglWSSvKcAjIOUe2hBOKMV1Fw-Q4sdsI9e5PyrfClRbIFOvwwxezwO9z7hPHo3pU2HfZ5iZ6c49Nj2NzjYPOHOjuXdxv4HDkPCzecT7B9Gn2Ln-ym_RM-DbbM_eIxLdP3p47fmrFpdnp43x6vKcaGnah00CKq9Au2FlTfB8XotmVMBQtAWiOCcEa0or52WlDimaFG9XlPhqXCaLdHbbd-ftjVjGW7THzPYaM6OVyb2dGRm9sZ5Le5Iod9s6TENvzfFlelidr5tbe-HTTZE1UIJoGXGEr3-P1pLJYSCAtIt6NKQc_JhJ4OAmY8xC-Bm3rX5d4xS9Oqxu83OtiHZ3sX8VCkKLvVsr9pyMU_-YZe36dbImtXCKPhurj5cNRerr8w07C_F65VL</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>17685580</pqid></control><display><type>article</type><title>Noise power spectrum estimation and fast map making for CMB experiments</title><source>Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX</source><source>EDP Sciences</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><creator>Amblard, A. ; Hamilton, J.-Ch</creator><creatorcontrib>Amblard, A. ; Hamilton, J.-Ch</creatorcontrib><description>We present a method designed to estimate the noise power spectrum in the time domain for CMB experiments. The noise power spectrum is extracted from the time ordered data avoiding the contamination coming from sky signal and accounting the pixellisation of the signal and the projection of the noise when making intermediate sky projections. This method is simple to implement and relies on Monte-Carlo simulations, it runs on a simple desk computer. We also propose a trick for filtering data before making coadded maps in order to avoid ringing due to the presence of signal in the timelines. These algorithms were succesfully tested on Archeops data.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>EISSN: 1432-0756</identifier><identifier>DOI: 10.1051/0004-6361:20034066</identifier><identifier>CODEN: AAEJAF</identifier><language>eng</language><publisher>Les Ulis: EDP Sciences</publisher><subject>Astrophysics ; cosmic microwave background ; Cosmology and Extra-Galactic Astrophysics ; cosmology: observations ; large-scale structure of the Universe ; methods: numerical ; Physics ; Sciences of the Universe</subject><ispartof>Astronomy and astrophysics (Berlin), 2004-04, Vol.417 (3), p.1189-1194</ispartof><rights>2004 INIST-CNRS</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c459t-bf90529e809e5a6dfc47b63c8f0ff9a015443198247c9621c382636bb25e25c93</citedby><cites>FETCH-LOGICAL-c459t-bf90529e809e5a6dfc47b63c8f0ff9a015443198247c9621c382636bb25e25c93</cites><orcidid>0000-0002-7820-8405</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,3714,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=15636699$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://in2p3.hal.science/in2p3-00024475$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Amblard, A.</creatorcontrib><creatorcontrib>Hamilton, J.-Ch</creatorcontrib><title>Noise power spectrum estimation and fast map making for CMB experiments</title><title>Astronomy and astrophysics (Berlin)</title><description>We present a method designed to estimate the noise power spectrum in the time domain for CMB experiments. The noise power spectrum is extracted from the time ordered data avoiding the contamination coming from sky signal and accounting the pixellisation of the signal and the projection of the noise when making intermediate sky projections. This method is simple to implement and relies on Monte-Carlo simulations, it runs on a simple desk computer. We also propose a trick for filtering data before making coadded maps in order to avoid ringing due to the presence of signal in the timelines. These algorithms were succesfully tested on Archeops data.</description><subject>Astrophysics</subject><subject>cosmic microwave background</subject><subject>Cosmology and Extra-Galactic Astrophysics</subject><subject>cosmology: observations</subject><subject>large-scale structure of the Universe</subject><subject>methods: numerical</subject><subject>Physics</subject><subject>Sciences of the Universe</subject><issn>0004-6361</issn><issn>1432-0746</issn><issn>1432-0756</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><recordid>eNp9kctuFDEQRa0IpAxDfiArb0BIqEn52Ta7pIE8NBCJELG0PI4NJv3C7knC3-PWhMmOhVWy6lTVvVUIHRJ4R0CQIwDglWSSvKcAjIOUe2hBOKMV1Fw-Q4sdsI9e5PyrfClRbIFOvwwxezwO9z7hPHo3pU2HfZ5iZ6c49Nj2NzjYPOHOjuXdxv4HDkPCzecT7B9Gn2Ln-ym_RM-DbbM_eIxLdP3p47fmrFpdnp43x6vKcaGnah00CKq9Au2FlTfB8XotmVMBQtAWiOCcEa0or52WlDimaFG9XlPhqXCaLdHbbd-ftjVjGW7THzPYaM6OVyb2dGRm9sZ5Le5Iod9s6TENvzfFlelidr5tbe-HTTZE1UIJoGXGEr3-P1pLJYSCAtIt6NKQc_JhJ4OAmY8xC-Bm3rX5d4xS9Oqxu83OtiHZ3sX8VCkKLvVsr9pyMU_-YZe36dbImtXCKPhurj5cNRerr8w07C_F65VL</recordid><startdate>20040401</startdate><enddate>20040401</enddate><creator>Amblard, A.</creator><creator>Hamilton, J.-Ch</creator><general>EDP Sciences</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-7820-8405</orcidid></search><sort><creationdate>20040401</creationdate><title>Noise power spectrum estimation and fast map making for CMB experiments</title><author>Amblard, A. ; Hamilton, J.-Ch</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c459t-bf90529e809e5a6dfc47b63c8f0ff9a015443198247c9621c382636bb25e25c93</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Astrophysics</topic><topic>cosmic microwave background</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>cosmology: observations</topic><topic>large-scale structure of the Universe</topic><topic>methods: numerical</topic><topic>Physics</topic><topic>Sciences of the Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Amblard, A.</creatorcontrib><creatorcontrib>Hamilton, J.-Ch</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Amblard, A.</au><au>Hamilton, J.-Ch</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Noise power spectrum estimation and fast map making for CMB experiments</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2004-04-01</date><risdate>2004</risdate><volume>417</volume><issue>3</issue><spage>1189</spage><epage>1194</epage><pages>1189-1194</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><coden>AAEJAF</coden><abstract>We present a method designed to estimate the noise power spectrum in the time domain for CMB experiments. The noise power spectrum is extracted from the time ordered data avoiding the contamination coming from sky signal and accounting the pixellisation of the signal and the projection of the noise when making intermediate sky projections. This method is simple to implement and relies on Monte-Carlo simulations, it runs on a simple desk computer. We also propose a trick for filtering data before making coadded maps in order to avoid ringing due to the presence of signal in the timelines. These algorithms were succesfully tested on Archeops data.</abstract><cop>Les Ulis</cop><pub>EDP Sciences</pub><doi>10.1051/0004-6361:20034066</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-7820-8405</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-6361
ispartof Astronomy and astrophysics (Berlin), 2004-04, Vol.417 (3), p.1189-1194
issn 0004-6361
1432-0746
1432-0756
language eng
recordid cdi_hal_primary_oai_HAL_in2p3_00024475v1
source Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals
subjects Astrophysics
cosmic microwave background
Cosmology and Extra-Galactic Astrophysics
cosmology: observations
large-scale structure of the Universe
methods: numerical
Physics
Sciences of the Universe
title Noise power spectrum estimation and fast map making for CMB experiments
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T13%3A33%3A44IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_hal_p&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Noise%20power%20spectrum%20estimation%20and%20fast%20map%20making%20for%20CMB%20experiments&rft.jtitle=Astronomy%20and%20astrophysics%20(Berlin)&rft.au=Amblard,%20A.&rft.date=2004-04-01&rft.volume=417&rft.issue=3&rft.spage=1189&rft.epage=1194&rft.pages=1189-1194&rft.issn=0004-6361&rft.eissn=1432-0746&rft.coden=AAEJAF&rft_id=info:doi/10.1051/0004-6361:20034066&rft_dat=%3Cproquest_hal_p%3E1875850226%3C/proquest_hal_p%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=17685580&rft_id=info:pmid/&rfr_iscdi=true