Directional Variations of the Non-Gaussianity Parameter f_NL
We investigate local variations of the primordial non-Gaussianity parameter f NL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of f NL. We first improve the needlet bispectrum estimate in Rudjord et al. on the full sky to f NL = 73 ± 31 using t...
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ftunivpadovairis:oai:www.research.unipd.it:11577/2426104 2024-02-27T08:45:32+00:00 Directional Variations of the Non-Gaussianity Parameter f_NL RUDJORD O HANSEN F. K LAN X MARINUCCI D LIGUORI, MICHELE MATARRESE, SABINO Rudjord, O HANSEN F., K Lan, X Liguori, Michele Marinucci, D Matarrese, Sabino 2010 STAMPA http://hdl.handle.net/11577/2426104 https://doi.org/10.1088/0004-637X/708/2/1321 eng eng info:eu-repo/semantics/altIdentifier/wos/WOS:000273021000029 volume:708 firstpage:1321 lastpage:1325 numberofpages:5 journal:THE ASTROPHYSICAL JOURNAL http://hdl.handle.net/11577/2426104 doi:10.1088/0004-637X/708/2/1321 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-77950289617 info:eu-repo/semantics/article 2010 ftunivpadovairis https://doi.org/10.1088/0004-637X/708/2/1321 2024-01-31T17:47:51Z We investigate local variations of the primordial non-Gaussianity parameter f NL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of f NL. We first improve the needlet bispectrum estimate in Rudjord et al. on the full sky to f NL = 73 ± 31 using the KQ75 mask on the co-added V + W channel. We find no particular values of f NL estimates close to the galactic plane and conclude that foregrounds are unlikely to affect the estimate of f NL in the V and W bands even for the smaller KQ85 mask. In the Q band, however, we find unexpectedly high values of f NL in local estimates close to the galactic mask, as well as significant discrepancies between Q-band estimates and V/W-band estimates. We therefore conclude that the Q band is too contaminated to be used for non-Gaussianity studies even with the larger KQ75 mask. We further note that the local f NL estimates on the V + W channel are positive on all equatorial bands from the north to the south pole. The probability for this to happen in a universe with f NL = 0 is less than 1%. Article in Journal/Newspaper South pole Padua Research Archive (IRIS - Università degli Studi di Padova) South Pole The Astrophysical Journal 708 2 1321 1325 |
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Open Polar |
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Padua Research Archive (IRIS - Università degli Studi di Padova) |
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ftunivpadovairis |
language |
English |
description |
We investigate local variations of the primordial non-Gaussianity parameter f NL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of f NL. We first improve the needlet bispectrum estimate in Rudjord et al. on the full sky to f NL = 73 ± 31 using the KQ75 mask on the co-added V + W channel. We find no particular values of f NL estimates close to the galactic plane and conclude that foregrounds are unlikely to affect the estimate of f NL in the V and W bands even for the smaller KQ85 mask. In the Q band, however, we find unexpectedly high values of f NL in local estimates close to the galactic mask, as well as significant discrepancies between Q-band estimates and V/W-band estimates. We therefore conclude that the Q band is too contaminated to be used for non-Gaussianity studies even with the larger KQ75 mask. We further note that the local f NL estimates on the V + W channel are positive on all equatorial bands from the north to the south pole. The probability for this to happen in a universe with f NL = 0 is less than 1%. |
author2 |
Rudjord, O HANSEN F., K Lan, X Liguori, Michele Marinucci, D Matarrese, Sabino |
format |
Article in Journal/Newspaper |
author |
RUDJORD O HANSEN F. K LAN X MARINUCCI D LIGUORI, MICHELE MATARRESE, SABINO |
spellingShingle |
RUDJORD O HANSEN F. K LAN X MARINUCCI D LIGUORI, MICHELE MATARRESE, SABINO Directional Variations of the Non-Gaussianity Parameter f_NL |
author_facet |
RUDJORD O HANSEN F. K LAN X MARINUCCI D LIGUORI, MICHELE MATARRESE, SABINO |
author_sort |
RUDJORD O |
title |
Directional Variations of the Non-Gaussianity Parameter f_NL |
title_short |
Directional Variations of the Non-Gaussianity Parameter f_NL |
title_full |
Directional Variations of the Non-Gaussianity Parameter f_NL |
title_fullStr |
Directional Variations of the Non-Gaussianity Parameter f_NL |
title_full_unstemmed |
Directional Variations of the Non-Gaussianity Parameter f_NL |
title_sort |
directional variations of the non-gaussianity parameter f_nl |
publishDate |
2010 |
url |
http://hdl.handle.net/11577/2426104 https://doi.org/10.1088/0004-637X/708/2/1321 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
info:eu-repo/semantics/altIdentifier/wos/WOS:000273021000029 volume:708 firstpage:1321 lastpage:1325 numberofpages:5 journal:THE ASTROPHYSICAL JOURNAL http://hdl.handle.net/11577/2426104 doi:10.1088/0004-637X/708/2/1321 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-77950289617 |
op_doi |
https://doi.org/10.1088/0004-637X/708/2/1321 |
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The Astrophysical Journal |
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708 |
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2 |
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1321 |
op_container_end_page |
1325 |
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