output
19922026
Showing 2016 · astro-ph.COShow all

25 papers · 2 filters

astro-ph.CO2016★ 120 cited

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…

astro-ph.CO2016★ 15 cited

Statistical simulations of the dust foreground to CMB polarization

Flavien Vansyngel, François Boulanger, Tuhin Ghosh +6

The characterization of the dust polarization foreground to the Cosmic Microwave Background (CMB) is a necessary step towards the detection of the B-mode signal associated with pri…

astro-ph.CO2016★ 18 cited

Consistency of the Planck CMB data and CDM cosmology

Arman Shafieloo, Dhiraj Kumar Hazra

We test the consistency between Planck temperature and polarization power spectra and the concordance model of Cold Dark Matter cosmology (CDM) within the framework of Cross…

astro-ph.CO2016★ 56 cited

Metastable Dark Energy with Radioactive-like Decay

Arman Shafieloo, Dhiraj Kumar Hazra, Varun Sahni +1

We propose a new class of metastable dark energy (DE) phenomenological models in which the DE decay rate does not depend on external parameters such as the scale factor or the curv…

astro-ph.CO2016★ 60 cited

Calibrating the Planck Cluster Mass Scale with CLASH

M. Penna-Lima, J. G. Bartlett, E. Rozo +5

We determine the mass scale of Planck galaxy clusters using gravitational lensing mass measurements from the Cluster Lensing And Supernova survey with Hubble (CLASH). We have compa…

astro-ph.CO2016★ 178 cited

Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters

Planck Collaboration, N. Aghanim, Y. Akrami +150

The six parameters of the standard CDM model have best-fit values derived from the Planck temperature power spectrum that are shifted somewhat from the best-fit values derived f…