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- Massachusetts Institute of TechnologyUS51 papers
- Argonne National LaboratoryUS38 papers
- University of California, Los AngelesUS35 papers
- Michigan State UniversityUS34 papers
- The Ohio State UniversityUS34 papers
- Lawrence Berkeley National LaboratoryUS33 papers
- Texas A&M UniversityUS32 papers
- University of California, DavisUS32 papers
- Carnegie Mellon UniversityUS31 papers
- Purdue University West LafayetteUS31 papers
- University of ChicagoUS31 papers
- Wayne State UniversityUS31 papers
16 papers · 2 filters
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…
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.
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…
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…
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…
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…