- Centre National de la Recherche ScientifiqueFR568 papers
- University of OxfordGB500 papers
- University of CambridgeGB477 papers
- University of EdinburghGB451 papers
- Royal ObservatoryGB428 papers
- California Institute of TechnologyUS350 papers
- Durham UniversityGB342 papers
- European Southern ObservatoryCL334 papers
- University College LondonGB329 papers
- National Institute for AstrophysicsIT318 papers
- Imperial College LondonGB312 papers
- Leiden UniversityNL297 papers
273 papers · 1 filter
Excitation energies from G{ö}rling-Levy perturbation theory along the range-separated adiabatic connection
Elisa Rebolini, Andrew M. Teale, Trygve Helgaker +2
A G{ö}rling-Levy (GL)-based perturbation theory along the range-separated adiabatic connection is assessed for the calculation of electronic excitation energies. In comparison with…
Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups
Wentao Luo, Xiaohu Yang, Tianhuan Lu +10
As the second paper of a series on studying galaxy-galaxy lensing signals using the Sloan Digital Sky Survey Data Release 7 (SDSS DR7), we present our measurement and modelling of…
Band structure of CuMnAs probed by optical and photoemission spectroscopy
M. Veis, J. Minar, G. Steciuk +19
Tetragonal phase of CuMnAs progressively appears as one of the key materials for antiferromagnetic spintronics due to efficient current-induced spin-orbit torques whose existence c…
The second Herschel-ATLAS Data Release - III: optical and near-infrared counterparts in the North Galactic Plane field
Cristina Furlanetto, S. Dye, N. Bourne +8
This paper forms part of the second major public data release of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). In this work, we describe the identification of o…
Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE
J. Greenslade, D. L. Clements, T. Cheng +19
By determining the nature of all the Planck compact sources within 808.4 deg^2 of large Herschel surveys, we have identified 27 candidate proto-clusters of dusty star forming galax…
Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…