Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL
We investigate local variations of the primordial non-Gaussianity parameter fNL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of fNL. We first improve the needlet bispectrum estimate in ( Rudjord et al. 2009) on the full-sky to fNL = 73±31 usin...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.250.880 2023-05-15T18:22:46+02:00 Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL Øystein Rudjord Frode K. Hansen Xiaohong Lan Michele Liguori Domenico Marinucci Sabino Matarrese The Pennsylvania State University CiteSeerX Archives 2009 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.880 http://arxiv.org/pdf/0906.3232v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.880 http://arxiv.org/pdf/0906.3232v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/0906.3232v1.pdf text 2009 ftciteseerx 2016-01-07T19:44:38Z We investigate local variations of the primordial non-Gaussianity parameter fNL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of fNL. We first improve the needlet bispectrum estimate in ( Rudjord et al. 2009) on the full-sky to fNL = 73±31 using the KQ75 mask on the co-added V+W channel. We find no particular values of fNL estimates close to the galactic plane and conclude that foregrounds are unlikely to affect the estimate of fNL in the V and W bands even for the smaller KQ85 mask. In the Q band however, we find unexpectedly high values of fNL 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 noted that the local fNL 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 fNL = 0 is less than one percent. Text South pole Unknown South Pole |
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We investigate local variations of the primordial non-Gaussianity parameter fNL in the WMAP data, looking for possible influence of foreground contamination in the full-sky estimate of fNL. We first improve the needlet bispectrum estimate in ( Rudjord et al. 2009) on the full-sky to fNL = 73±31 using the KQ75 mask on the co-added V+W channel. We find no particular values of fNL estimates close to the galactic plane and conclude that foregrounds are unlikely to affect the estimate of fNL in the V and W bands even for the smaller KQ85 mask. In the Q band however, we find unexpectedly high values of fNL 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 noted that the local fNL 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 fNL = 0 is less than one percent. |
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The Pennsylvania State University CiteSeerX Archives |
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Text |
author |
Øystein Rudjord Frode K. Hansen Xiaohong Lan Michele Liguori Domenico Marinucci Sabino Matarrese |
spellingShingle |
Øystein Rudjord Frode K. Hansen Xiaohong Lan Michele Liguori Domenico Marinucci Sabino Matarrese Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
author_facet |
Øystein Rudjord Frode K. Hansen Xiaohong Lan Michele Liguori Domenico Marinucci Sabino Matarrese |
author_sort |
Øystein Rudjord |
title |
Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
title_short |
Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
title_full |
Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
title_fullStr |
Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
title_full_unstemmed |
Preprint typeset using L ATEX style emulateapj v. 10/09/06 DIRECTIONAL VARIATIONS OF THE NON-GAUSSIANITY PARAMETER fNL |
title_sort |
preprint typeset using l atex style emulateapj v. 10/09/06 directional variations of the non-gaussianity parameter fnl |
publishDate |
2009 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.880 http://arxiv.org/pdf/0906.3232v1.pdf |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://arxiv.org/pdf/0906.3232v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.880 http://arxiv.org/pdf/0906.3232v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766202184427372544 |