10.6k citations
- University of GenevaCH144 papers
- Centre National de la Recherche ScientifiqueFR127 papers
- University of CambridgeGB121 papers
- University College LondonGB120 papers
- University of ManchesterGB112 papers
- California Institute of TechnologyUS111 papers
- Princeton UniversityUS111 papers
- University of California, BerkeleyUS111 papers
- Lawrence Berkeley National LaboratoryUS110 papers
- Imperial College LondonGB107 papers
- National Institute for AstrophysicsIT104 papers
- University of HelsinkiFI104 papers
52 papers · 1 filter
Planck intermediate results. LII. Planet flux densities
Planck Collaboration, Y. Akrami, M. Ashdown +147
Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100-857 GH…
ZFIRE: Similar Stellar Growth in H-emitting Cluster and Field Galaxies at z~2
Kim-Vy H. Tran, Leo Y. Alcorn, Glenn G. Kacprzak +13
We compare galaxy scaling relations as a function of environment at with our ZFIRE survey where we have measured H fluxes for 90 star-forming galaxies selected from a m…
Epoch of Reionisation 21cm Forecasting From MCMC-Constrained Semi-Numerical Models
Sultan Hassan, Romeel Dave, Kristian Finlator +1
The recent low value of Planck (2016) integrated optical depth to Thomson scattering suggests that the reionization occurred fairly suddenly, disfavoring extended reionization scen…
Symmetry Energy III: Isovector Skins
Pawel Danielewicz, Pardeep Singh, Jenny Lee
Isoscalar density is a sum of neutron and proton densities and isovector is a normalized difference. Here, we report on the experimental evidence for the displacement of the isovec…
Cold gas stripping in satellite galaxies: from pairs to clusters
Toby Brown, Barbara Catinella, Luca Cortese +6
In this paper we investigate environment driven gas depletion in satellite galaxies, taking full advantage of the atomic hydrogen (HI) spectral stacking technique to quantify the g…
Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
P. S. Corasaniti, S. Agarwal, D. J. E. Marsh +1
We use state-of-art measurements of the galaxy luminosity function (LF) at z=6, 7 and 8 to derive constraints on warm dark matter (WDM), late-forming dark matter (LFDM) and ultra-l…