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Nabila Aghanim

Researcher at Université Paris-Saclay

Publications -  450
Citations -  110271

Nabila Aghanim is an academic researcher from Université Paris-Saclay. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 137, co-authored 416 publications receiving 100914 citations. Previous affiliations of Nabila Aghanim include University of Paris-Sud & University of Paris.

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Journal Article

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Asantha Cooray, +249 more
TL;DR: The Herschel-SPIRE Legacy Survey (HSLS) as mentioned in this paper is a large-scale survey of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA.
Journal ArticleDOI

High-resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations

TL;DR: In this article, the authors investigate the angular redshift fluctuations (ARF), which probe the information contained in the projected redshift distribution of galaxies, and show how ARF will provide complementary cosmological information compared to traditional angular galaxy clustering.
Journal ArticleDOI

Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data

TL;DR: In this paper, a new all-sky Compton parameter map (y-map) of the thermal Sunyaev-Zel'dovich (tSZ) effect from the 100 to 857 GHz frequency channel maps delivered within the Planck data release 4.
Journal ArticleDOI

High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations

TL;DR: In this article, the authors investigate the angular redshift fluctuations (ARF), which probe the information contained in the projected redshift distribution of galaxies, and show how ARF will provide complementary cosmological information compared to traditional angular galaxy clustering.