activity
20092025
most citedPlanck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters

178 citations · 462 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

5 papers · 1 filter

astro-ph.CO2025★ 1 cited

Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution

Euclid Collaboration, J. Bel, S. Gouyou Beauchamps +281

We investigate the non-Gaussian features in the distribution of the matter power spectrum multipoles. Using the COVMOS method, we generate 100\,000 mock realisations of dark matter…

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…

astro-ph.CO2015★ 40 cited

Planck 2015 results. I. Overview of products and scientific results

Planck Collaboration, R. Adam, P. A. R. Ade +352

The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submilli…

astro-ph.CO2014★ 73 cited

Cosmic expansion histories in massive bigravity with symmetric matter coupling

Jonas Enander, Adam R. Solomon, Yashar Akrami +1

We study the cosmic expansion history of massive bigravity with a viable matter coupling which treats both metrics on equal footing. We derive the Friedmann equation for the effect…

astro-ph.CO2009★ 84 cited

Direct Constraints on Minimal Supersymmetry from Fermi-LAT Observations of the Dwarf Galaxy Segue 1

Pat Scott, Jan Conrad, Joakim Edsjö +3

The dwarf galaxy Segue 1 is one of the most promising targets for the indirect detection of dark matter. Here we examine what constraints 9 months of Fermi-LAT gamma-ray observatio…