activity
19972020
most citedWilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization

940 citations · 2k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2020★ 14 cited

CMB-HD: Astro2020 RFI Response

Neelima Sehgal, Simone Aiola, Yashar Akrami +45

CMB-HD is a proposed ultra-deep (0.5 uk-arcmin), high-resolution (15 arcseconds) millimeter-wave survey over half the sky that would answer many outstanding questions in both funda…

astro-ph.CO2014★ 94 cited

Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos

Mathew Madhavacheril, Neelima Sehgal, Rupert Allison +40

We present evidence of the gravitational lensing of the cosmic microwave background by solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology T…

astro-ph.CO2011★ 664 cited

The Primordial Inflation Explorer (PIXIE): A Nulling Polarimeter for Cosmic Microwave Background Observations

A. Kogut, D. J. Fixsen, D. T. Chuss +9

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission to measure the gravity-wave signature of primordial inflation through its distinctive imprint on the linear p…

astro-ph2008★ 142 cited

The Wilkinson Microwave Anisotropy Probe (WMAP) Source Catalog

E. L. Wright, X. Chen, N. Odegard +18

We present the list of point sources found in the WMAP 5-year maps. The technique used in the first-year and three-year analysis now finds 390 point sources, and the five-year sour…

astro-ph2007★ 140 cited

Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization

A. Kogut, J. Dunkley, C. L. Bennett +14

We present a full-sky model of polarized Galactic microwave emission based on three years of observations by the Wilkinson Microwave Anisotropy Probe (WMAP) at frequencies from 23…

astro-ph2003★ 940 cited

Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization

A. Kogut, D. N. Spergel, C. Barnes +10

The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the full sky in Stokes I, Q, and U parameters at frequencies 23, 33, 41, 61, and 94 GHz. We detect correlations between t…