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Peter A. R. Ade

Researcher at Cardiff University

Publications -  1402
Citations -  147299

Peter A. R. Ade is an academic researcher from Cardiff University. The author has contributed to research in topics: Cosmic microwave background & Telescope. The author has an hindex of 162, co-authored 1387 publications receiving 138051 citations. Previous affiliations of Peter A. R. Ade include Queen Mary's College & Max Planck Society.

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The Atacama Cosmology Telescope: Calibration with the Wilkinson Microwave Anisotropy Probe using cross-correlations

Amir Hajian, +83 more
TL;DR: In this article, a new calibration method based on cross-correlations with the Wilkinson Microwave Anisotropy Probe (WMAP) was proposed and applied to data from the Atacama Cosmology Telescope (ACT).
Proceedings ArticleDOI

An absolute dual beam emission spectrometer

TL;DR: Astronomical spectroscopy at submillimetre wavelengths holds much promise for fields as diverse as the study of planetary atmospheres, molecular clouds and extragalactic sources as mentioned in this paper.
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Measurement of the Sunyaev-Zel'dovich effect toward Abell 2163 at a wavelength of 2.2 millimeters

TL;DR: In this paper, the first significnat detection of the Sunyaev-Zel'dovich (S-Z) effect at millimeter wavelengths was reported, where drift scans of the cluster of galaxies Abell 2163 were performed using a novel bolometric array receiver at a wavelength of 2.2 millimeters.
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PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium

TL;DR: The PILOT balloon project as mentioned in this paper is a test-bed for using multiplexed bolometer arrays for polarization measurements for cosmology cosmology space missions, which aims at characterizing one of these foreground sources, the polarized continuum emission by dust in the diffuse interstellar medium.
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The Blast Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D

TL;DR: In this article, the results from observations of the Vela-D region, covering about 4 deg^2, in which the Balloon-borne Large-Aperture Submillimeter Telescope (BLAST) was used to identify the coldest dense cores possibly associated with the earliest stages of star formation.