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20182021
most citedPlanck 2018 results. IX. Constraints on primordial non-Gaussianity

159 citations · 191 across the 3 of their papers we have counts for

collaborators

15 papers

astro-ph.CO202116 cited

CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation

K. Kiiveri, D. Gruen, A. Finoguenov +19

The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sample of X-ray clusters at . It was selected from ROSAT data in the…

astro-ph.CO2020

Planck intermediate results. LVII. Joint Planck LFI and HFI data processing

Planck Collaboration, Y. Akrami, K. J. Andersen +136

We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High…

astro-ph.CO2020

Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

Planck Collaboration, Y. Akrami, M. Ashdown +126

The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularl…

astro-ph.GA202016 cited

Kinematic unrest of low mass galaxy groups

G. Gozaliasl, A. Finoguenov, H. G. Khosroshahi +6

In an effort to better understand the formation of galaxy groups, we examine the kinematics of a large sample of spectroscopically confirmed X-ray galaxy groups in the Cosmic Evolu…

astro-ph.CO2019

CODEX clusters. The Survey, the Catalog, and Cosmology of the X-ray Luminosity Function

A. Finoguenov, E. Rykoff, N. Clerc +17

Large area catalogs of galaxy clusters constructed from ROSAT All Sky Survey provide the base for our knowledge on the population of clusters thanks to the long-term multiwavelengt…

astro-ph.CO2019

Planck 2018 results. V. CMB power spectra and likelihoods

Planck Collaboration, N. Aghanim, Y. Akrami +165

This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementin…