First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon-borne instrument was launched by CNES from the Swedish Esrange base near Kiruna. In addition to the 143 GHz and 217 GHz freq...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Other Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
E D P SCIENCES
2004
|
Subjects: | |
Online Access: | http://hdl.handle.net/11573/362425 https://doi.org/10.1051/0004-6361:20040042 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000224300800024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a http://www.scopus.com/inward/record.url?eid=2-s2.0-4544322654&partnerID=65&md5=d67377a10d32bd95ceca3d3567d154f9 |
id |
ftunivromairis:oai:iris.uniroma1.it:11573/362425 |
---|---|
record_format |
openpolar |
institution |
Open Polar |
collection |
Sapienza Università di Roma: CINECA IRIS |
op_collection_id |
ftunivromairis |
language |
English |
topic |
cosmology : cosmic microwave background cosmology : observation cosmology: cosmic microwave background cosmology: observation ism : dust extinction ism: dust polarization submillimeter |
spellingShingle |
cosmology : cosmic microwave background cosmology : observation cosmology: cosmic microwave background cosmology: observation ism : dust extinction ism: dust polarization submillimeter A. Benoit P. Ade A. Amblard R. Ansari E. Aubourg S. Bargot J. G. Bartlett J. Ph Bernard R. S. Bhatia A. Blanchard J. J. Bock A. Boscaleri F. R. Bouchet A. Bourrachot P. Camus F. Couchot J. Delabrouille F. X. Desert O. Dore M. Douspis L. Dumoulin X. Dupac P. Filliatre P. Fosalba K. Ganga F. Gannaway B. Gautier M. Giard Y. Giraud Heraud R. Gispert L. Guglielmi J. Ch Hamilton S. Hanany S. Henrot Versille J. Kaplan G. Lagache J. M. Lamarre A. E. Lange J. F. Macias Perez K. Madet B. Maffei C. H. Magneville D. P. Marrone F. Mayet A. Murphy F. Naraghi G. Patanchon G. Perrin M. Piat N. Ponthieu S. Prunet J. L. Puget C. Renault C. Rosset D. Santos A. Starobinsky I. Strukov R. V. Sudiwala R. Teyssier M. Tristram C. Tucker J. C. Vanel D. Vibert E. Wakui D. Yvon DE BERNARDIS, Paolo MASI, Silvia NATI, FEDERICO First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
topic_facet |
cosmology : cosmic microwave background cosmology : observation cosmology: cosmic microwave background cosmology: observation ism : dust extinction ism: dust polarization submillimeter |
description |
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon-borne instrument was launched by CNES from the Swedish Esrange base near Kiruna. In addition to the 143 GHz and 217 GHz frequency bands dedicated to CMB; studies, Archeops had one 545 GHz and six 353 GHz bolometers mounted in three polarization-sensitive pairs that were used for Galactic foreground studies. We present maps of the I, Q, U Stokes parameters over 17% of the sky and with a 13 arcmin resolution at 353 GHz (850 mum). They show a significant Galactic large scale polarized emission coherent on the longitude ranges [100, 120] and [180, 200] deg. with a degree of polarization at the level of 4-5%, in agreement with expectations from starlight polarization measurements. Some regions in the Galactic plane (Gem OB 1, Cassiopeia) show an even stronger degree of polarization in the range 10-20%. These findings provide strong evidence for a powerful grain alignment mechanism throughout the interstellar medium and a coherent magnetic field coplanar to the Galactic plane. This magnetic field pervades even some dense clouds. Extrapolated to high Galactic latitude, these results indicate that interstellar dust polarized emission is the major foreground for PLANCK-HFI CMB polarization measurements. |
author2 |
A., Benoit P., Ade A., Amblard R., Ansari E., Aubourg S., Bargot J. G., Bartlett J., Ph Bernard R. S., Bhatia A., Blanchard J. J., Bock A., Boscaleri F. R., Bouchet A., Bourrachot P., Camu F., Couchot DE BERNARDIS, Paolo J., Delabrouille F. X., Desert O., Dore M., Douspi L., Dumoulin X., Dupac P., Filliatre P., Fosalba K., Ganga F., Gannaway B., Gautier M., Giard Y., Giraud Heraud R., Gispert L., Guglielmi J., Ch Hamilton S., Hanany S., Henrot Versille J., Kaplan G., Lagache J. M., Lamarre A. E., Lange J. F., Macias Perez K., Madet B., Maffei C. H., Magneville D. P., Marrone Masi, Silvia F., Mayet A., Murphy F., Naraghi Nati, Federico G., Patanchon |
format |
Article in Journal/Newspaper |
author |
A. Benoit P. Ade A. Amblard R. Ansari E. Aubourg S. Bargot J. G. Bartlett J. Ph Bernard R. S. Bhatia A. Blanchard J. J. Bock A. Boscaleri F. R. Bouchet A. Bourrachot P. Camus F. Couchot J. Delabrouille F. X. Desert O. Dore M. Douspis L. Dumoulin X. Dupac P. Filliatre P. Fosalba K. Ganga F. Gannaway B. Gautier M. Giard Y. Giraud Heraud R. Gispert L. Guglielmi J. Ch Hamilton S. Hanany S. Henrot Versille J. Kaplan G. Lagache J. M. Lamarre A. E. Lange J. F. Macias Perez K. Madet B. Maffei C. H. Magneville D. P. Marrone F. Mayet A. Murphy F. Naraghi G. Patanchon G. Perrin M. Piat N. Ponthieu S. Prunet J. L. Puget C. Renault C. Rosset D. Santos A. Starobinsky I. Strukov R. V. Sudiwala R. Teyssier M. Tristram C. Tucker J. C. Vanel D. Vibert E. Wakui D. Yvon DE BERNARDIS, Paolo MASI, Silvia NATI, FEDERICO |
author_facet |
A. Benoit P. Ade A. Amblard R. Ansari E. Aubourg S. Bargot J. G. Bartlett J. Ph Bernard R. S. Bhatia A. Blanchard J. J. Bock A. Boscaleri F. R. Bouchet A. Bourrachot P. Camus F. Couchot J. Delabrouille F. X. Desert O. Dore M. Douspis L. Dumoulin X. Dupac P. Filliatre P. Fosalba K. Ganga F. Gannaway B. Gautier M. Giard Y. Giraud Heraud R. Gispert L. Guglielmi J. Ch Hamilton S. Hanany S. Henrot Versille J. Kaplan G. Lagache J. M. Lamarre A. E. Lange J. F. Macias Perez K. Madet B. Maffei C. H. Magneville D. P. Marrone F. Mayet A. Murphy F. Naraghi G. Patanchon G. Perrin M. Piat N. Ponthieu S. Prunet J. L. Puget C. Renault C. Rosset D. Santos A. Starobinsky I. Strukov R. V. Sudiwala R. Teyssier M. Tristram C. Tucker J. C. Vanel D. Vibert E. Wakui D. Yvon DE BERNARDIS, Paolo MASI, Silvia NATI, FEDERICO |
author_sort |
A. Benoit |
title |
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
title_short |
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
title_full |
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
title_fullStr |
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
title_full_unstemmed |
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops |
title_sort |
first detection of polarization of the submillimetre diffuse galactic dust emission by archeops |
publisher |
E D P SCIENCES |
publishDate |
2004 |
url |
http://hdl.handle.net/11573/362425 https://doi.org/10.1051/0004-6361:20040042 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000224300800024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a http://www.scopus.com/inward/record.url?eid=2-s2.0-4544322654&partnerID=65&md5=d67377a10d32bd95ceca3d3567d154f9 |
long_lat |
ENVELOPE(21.117,21.117,67.883,67.883) ENVELOPE(64.483,64.483,-70.200,-70.200) |
geographic |
Arctic Esrange Kiruna Starlight |
geographic_facet |
Arctic Esrange Kiruna Starlight |
genre |
Arctic Kiruna |
genre_facet |
Arctic Kiruna |
op_relation |
info:eu-repo/semantics/altIdentifier/wos/WOS:000224300800024 volume:424 issue:2 firstpage:571 lastpage:582 numberofpages:12 journal:ASTRONOMY & ASTROPHYSICS http://hdl.handle.net/11573/362425 doi:10.1051/0004-6361:20040042 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-4544322654 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000224300800024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a http://www.scopus.com/inward/record.url?eid=2-s2.0-4544322654&partnerID=65&md5=d67377a10d32bd95ceca3d3567d154f9 |
op_doi |
https://doi.org/10.1051/0004-6361:20040042 |
_version_ |
1792045202020499456 |
spelling |
ftunivromairis:oai:iris.uniroma1.it:11573/362425 2024-02-27T08:38:17+00:00 First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops A. Benoit P. Ade A. Amblard R. Ansari E. Aubourg S. Bargot J. G. Bartlett J. Ph Bernard R. S. Bhatia A. Blanchard J. J. Bock A. Boscaleri F. R. Bouchet A. Bourrachot P. Camus F. Couchot J. Delabrouille F. X. Desert O. Dore M. Douspis L. Dumoulin X. Dupac P. Filliatre P. Fosalba K. Ganga F. Gannaway B. Gautier M. Giard Y. Giraud Heraud R. Gispert L. Guglielmi J. Ch Hamilton S. Hanany S. Henrot Versille J. Kaplan G. Lagache J. M. Lamarre A. E. Lange J. F. Macias Perez K. Madet B. Maffei C. H. Magneville D. P. Marrone F. Mayet A. Murphy F. Naraghi G. Patanchon G. Perrin M. Piat N. Ponthieu S. Prunet J. L. Puget C. Renault C. Rosset D. Santos A. Starobinsky I. Strukov R. V. Sudiwala R. Teyssier M. Tristram C. Tucker J. C. Vanel D. Vibert E. Wakui D. Yvon DE BERNARDIS, Paolo MASI, Silvia NATI, FEDERICO A., Benoit P., Ade A., Amblard R., Ansari E., Aubourg S., Bargot J. G., Bartlett J., Ph Bernard R. S., Bhatia A., Blanchard J. J., Bock A., Boscaleri F. R., Bouchet A., Bourrachot P., Camu F., Couchot DE BERNARDIS, Paolo J., Delabrouille F. X., Desert O., Dore M., Douspi L., Dumoulin X., Dupac P., Filliatre P., Fosalba K., Ganga F., Gannaway B., Gautier M., Giard Y., Giraud Heraud R., Gispert L., Guglielmi J., Ch Hamilton S., Hanany S., Henrot Versille J., Kaplan G., Lagache J. M., Lamarre A. E., Lange J. F., Macias Perez K., Madet B., Maffei C. H., Magneville D. P., Marrone Masi, Silvia F., Mayet A., Murphy F., Naraghi Nati, Federico G., Patanchon 2004 STAMPA http://hdl.handle.net/11573/362425 https://doi.org/10.1051/0004-6361:20040042 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000224300800024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a http://www.scopus.com/inward/record.url?eid=2-s2.0-4544322654&partnerID=65&md5=d67377a10d32bd95ceca3d3567d154f9 eng eng E D P SCIENCES info:eu-repo/semantics/altIdentifier/wos/WOS:000224300800024 volume:424 issue:2 firstpage:571 lastpage:582 numberofpages:12 journal:ASTRONOMY & ASTROPHYSICS http://hdl.handle.net/11573/362425 doi:10.1051/0004-6361:20040042 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-4544322654 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000224300800024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a http://www.scopus.com/inward/record.url?eid=2-s2.0-4544322654&partnerID=65&md5=d67377a10d32bd95ceca3d3567d154f9 cosmology : cosmic microwave background cosmology : observation cosmology: cosmic microwave background cosmology: observation ism : dust extinction ism: dust polarization submillimeter info:eu-repo/semantics/article 2004 ftunivromairis https://doi.org/10.1051/0004-6361:20040042 2024-01-31T17:47:12Z We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon-borne instrument was launched by CNES from the Swedish Esrange base near Kiruna. In addition to the 143 GHz and 217 GHz frequency bands dedicated to CMB; studies, Archeops had one 545 GHz and six 353 GHz bolometers mounted in three polarization-sensitive pairs that were used for Galactic foreground studies. We present maps of the I, Q, U Stokes parameters over 17% of the sky and with a 13 arcmin resolution at 353 GHz (850 mum). They show a significant Galactic large scale polarized emission coherent on the longitude ranges [100, 120] and [180, 200] deg. with a degree of polarization at the level of 4-5%, in agreement with expectations from starlight polarization measurements. Some regions in the Galactic plane (Gem OB 1, Cassiopeia) show an even stronger degree of polarization in the range 10-20%. These findings provide strong evidence for a powerful grain alignment mechanism throughout the interstellar medium and a coherent magnetic field coplanar to the Galactic plane. This magnetic field pervades even some dense clouds. Extrapolated to high Galactic latitude, these results indicate that interstellar dust polarized emission is the major foreground for PLANCK-HFI CMB polarization measurements. Article in Journal/Newspaper Arctic Kiruna Sapienza Università di Roma: CINECA IRIS Arctic Esrange ENVELOPE(21.117,21.117,67.883,67.883) Kiruna Starlight ENVELOPE(64.483,64.483,-70.200,-70.200) |