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First results from the Very Small Array - IV. Cosmological parameter estimation
British Library Online Contents | 2003| -
Lines in the cosmic microwave background spectrum from the epoch of cosmological helium recombination
Free accessEDP Sciences | 2008| -
On the presence of thermal Sunyaev--Zel'dovich induced signal in the first-year WMAP temperature maps
Oxford University Press | 2004| -
Constraining the regular Galactic Magnetic Field with the 5-year WMAP polarization measurements at 22 GHz
Free accessArXiv | 2010| -
Constraining the regular Galactic magnetic field with the 5-year WMAP polarization measurements at 22 GHz
Free accessEDP Sciences | 2010| -
Lines in the cosmic microwave background spectrum from the epoch of cosmological helium recombination
Free accessArXiv | 2007| -
On the Presence of Thermal SZ Induced Signal in the First Year WMAP Temperature Maps
Free accessArXiv | 2003| -
Discriminating between unresolved point sources and 'negative' Sunyaev-Zel'dovich clusters in cosmic microwave background maps
Oxford University Press | 2003| -
Lines in the Cosmic Microwave Background Spectrum from the Epoch of Cosmological Hydrogen Recombination
Free accessArXiv | 2006| -
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
Free accessArXiv | 2002| -
Cosmological hydrogen recombination: populations of the high level sub-states
Free accessArXiv | 2006| -
Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018
Free accessArXiv | 2022| -
Testing the conditional mass function of dark matter halos against numerical N-body simulations
Free accessArXiv | 2017| -
An Overview of the MOS Capabilities of the 4-10 m Telescopes at La Palma Observatory for Investigating Galaxy Clusters
British Library Conference Proceedings | 2016|
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