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Anthony Lasenby

Researcher at University of Cambridge

Publications -  651
Citations -  117889

Anthony Lasenby is an academic researcher from University of Cambridge. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 143, co-authored 630 publications receiving 105090 citations. Previous affiliations of Anthony Lasenby include University of Manchester.

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Planck intermediate results. XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck

Fermi Collaborations, +197 more
TL;DR: In this paper, the authors used observations of the nearby Chamaeleon clouds in gamma rays with the Fermi Large Area Telescope and in thermal dust emission with Planck and IRAS to map the gas column densities in different phases and at the dark neutral medium (DNM) transition between the HI-bright and CO-bright media; constrain the CO-to-H_2$ conversion factor, $X_{CO}$; and probe the dust properties per gas nucleon in each gas phase and spatially across the clouds.
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Planck 2013 results. V. LFI calibration

Nabila Aghanim, +218 more
TL;DR: In this article, the authors used a combination of the orbital dipole plus the solar dipole to estimate the signal generated by the dipole in the CMB rest frame of the Planck spacecraft.
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Cosmic microwave background anisotropies in the CDM model: a covariant and gauge-invariant approach

TL;DR: In this paper, a fully covariant and gauge-invariant calculation of the evolution of anisotropies in the cosmic microwave background (CMB) radiation has been presented.
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Planck 2015 results. IV. Low Frequency Instrument beams and window functions

Peter A. R. Ade, +201 more
TL;DR: In this paper, the beam normalization and beam window functions for the Planck Low Frequency Instrument (LFI) were characterized and the uncertainties in the beam window function were analyzed.
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Planck intermediate results: I. Further validation of new Planck clusters with XMM-Newton

Nabila Aghanim, +210 more
TL;DR: In this article, the authors present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5 < S/N < 5.3 in the same 10-month survey maps used in the construction of the Early SZ sample.