activity
19972023
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 30.5k across the 119 of their papers we have counts for

collaborators

119 papers

astro-ph.GA2023★ 1 cited

MIDIS: The Relation between Strong (Hb+[OIII]) Emission, Star Formation and Burstiness Around the Epoch of Reionization

Karina I. Caputi, Pierluigi Rinaldi, Edoardo Iani +25

We investigate the properties of strong (Hb+[OIII]) emitters before and after the end of the Epoch of Reionization from z=8 to z=5.5. We make use of ultra-deep JWST/NIRCam imaging…

astro-ph.GA2023★ 28 cited

Uncovering the stellar structure of the dusty star-forming galaxy GN20 at z=4.055 with MIRI/JWST

L. Colina, A. Crespo Gómez, J. Álvarez-Márquez +35

Luminous infrared galaxies at high redshifts (>4) include extreme starbursts that build their stellar mass over short periods of time (>100 Myr). These galaxies are considered t…

astro-ph.GA2019★ 14 cited

Investigating the physical properties of galaxies in the Epoch of Reionization with MIRI/JWST spectroscopy

J. Álvarez-Márquez, L. Colina, R. Marques-Chaves +14

The James Webb Space Telescope will provide deep imaging and spectroscopy for sources at redshifts above 6, covering the Epoch of Reionization (EoR, 6 < z < 10). The Mid-IR instrum…

astro-ph.CO2019★ 1.1k cited

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…

astro-ph.GA2019★ 14 cited

Statistical stellar mass corrections for high-z galaxies observed with JWST broad-band filters due to template degeneracies

L. Bisigello, K. I. Caputi, L. Colina +6

Stellar masses in future James Webb Space Telescope (JWST) deep blank-fields will be mainly derived fitting the spectral energy distribution with theoretical galaxy templates. We i…

astro-ph.CO2018★ 2 cited

Confirmation of the detection of B-modes in the Planck polarization maps

H. U. Nørgaard-Nielsen

One of the main problems for extracting the Cosmic Microwave Background (CMB) from submm/mm observations is to correct for the Galactic components, mainly synchrotron, free - free…