output
20022011
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

5.7k citations

Showing astro-phShow all

413 papers · 1 filter

astro-ph200815 cited

Delayed Recombination and Standard Rulers

Francesco De Bernardis, Rachel Bean, Silvia Galli +3

Measurements of Baryonic Acoustic Oscillations in galaxy surveys have been recognized as a powerful tool for constraining dark energy. However, this method relies on the knowledge…

astro-ph200848 cited

A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2

J. D. Younger, A. Omont, N. Fiolet +6

We present millimetre observations of a sample of 12 high redshift ultraluminous infrared galaxies (ULIRGs) in the Extended Growth Strip (EGS). These objects were initially selecte…

astro-ph2008113 cited

The JCMT Nearby Galaxies Legacy Survey I. Star Forming Molecular Gas in Virgo Cluster Spiral Galaxies

C. D. Wilson, B. E. Warren, F. P. Israel +20

We present large-area maps of the CO J=3-2 emission obtained at the James Clerk Maxwell Telescope for four spiral galaxies in the Virgo Cluster. We combine these data with publishe…

astro-ph2008134 cited

The mass of the black hole in Centaurus A from SINFONI AO-assisted integral-field observations of stellar kinematics

Michele Cappellari, N. Neumayer, J. Reunanen +3

We present a determination of the mass of the supermassive black hole (BH) and the nuclear stellar orbital distribution of the elliptical galaxy Centaurus A (NGC5128) using high-re…

astro-ph200846 cited

Cosmological Systematics Beyond Nuisance Parameters : Form Filling Functions

T. D. Kitching, A. Amara, F. B. Abdalla +2

In the absence of any compelling physical model, cosmological systematics are often misrepresented as statistical effects and the approach of marginalising over extra nuisance syst…

astro-ph2008184 cited

Results from the First Science Run of the ZEPLIN-III Dark Matter Search Experiment

V. N. Lebedenko, H. M. Araujo, E. J. Barnes +35

The ZEPLIN-III experiment in the Palmer Underground Laboratory at Boulby uses a 12kg two-phase xenon time projection chamber to search for the weakly interacting massive particles…