output
20022009
most citedCharge insensitive qubit design derived from the Cooper pair box

3.4k citations

Showing 2008 · astro-phShow all

16 papers · 2 filters

astro-ph2008303 cited

CMBPol Mission Concept Study: Probing Inflation with CMB Polarization

Daniel Baumann, Mark G. Jackson, Peter Adshead +56

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measu…

astro-ph2008

Calculation of Solar P-mode Oscillation Frequency Splittings Based on a Two-dimensional Solar Model

Linghuai Li, Sarbani Basu, Sabatino Sofia +1

We compute the p-mode oscillation frequencies and frequency splittings that arise in a two-dimensional model of the Sun that contains toroidal magnetic fields in its interior.

astro-ph20082 cited

Neutrinos and Future Concordance Cosmologies

Peter Adshead, Richard Easther

We review the free parameters in the concordance cosmology, and those which might be added to this set as the quality of astrophysical data improves. Most concordance parameters en…

astro-ph2008380 cited

Photometric redshift and classification for the XMM-COSMOS sources

M. Salvato, G. Hasinger, O. Ilbert +40

We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our…

astro-ph2008141 cited

The evolution of the specific star formation rate of massive galaxies to z ~ 1.8 in the E-CDFS

Maaike Damen, Ivo Labbe, Marijn Franx +3

We study the evolution of the star formation rate (SFR) of mid-infrared (IR) selected galaxies in the extended Chandra Deep Field South (E-CDFS). We use a combination of U-K GaBoDS…

astro-ph2008

Stability of Galactic Gaseous Disks and the Formation of Massive Clusters

Andres Escala, Richard B. Larson

We study gravitational instabilities in disks, with special attention to the most massive clumps that form because they are expected to be the progenitors of globular-type clusters…