Line-intensity mapping: theory review with a focus on star-formation lines
Line-intensity mapping (LIM) is an emerging approach to survey the Universe, using
relatively low-aperture instruments to scan large portions of the sky and collect the total …
relatively low-aperture instruments to scan large portions of the sky and collect the total …
Neutrino mass ordering from oscillations and beyond: 2018 status and future prospects
PF De Salas, S Gariazzo, O Mena… - Frontiers in Astronomy …, 2018 - frontiersin.org
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor
physics, and its determination may provide the key to establish the relationship among the …
physics, and its determination may provide the key to establish the relationship among the …
The Simons Observatory: science goals and forecasts
The Simons Observatory (SO) is a new cosmic microwave background experiment being
built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the …
built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the …
[HTML][HTML] Planck intermediate results-XLVII. Planck constraints on reionization history
R Adam, N Aghanim, M Ashdown, J Aumont… - Astronomy & …, 2016 - aanda.org
We investigate constraints on cosmic reionization extracted from the Planck cosmic
microwave background (CMB) data. We combine the Planck CMB anisotropy data in …
microwave background (CMB) data. We combine the Planck CMB anisotropy data in …
Hydrogen epoch of reionization array (HERA)
Abstract The Hydrogen Epoch of Reionization Array (HERA) is a staged experiment to
measure 21 cm emission from the primordial intergalactic medium (IGM) throughout cosmic …
measure 21 cm emission from the primordial intergalactic medium (IGM) throughout cosmic …
Unveiling secrets with cosmological data: Neutrino masses and mass hierarchy
Using some of the latest cosmological data sets publicly available, we derive the strongest
bounds in the literature on the sum of the three active neutrino masses, M ν, within the …
bounds in the literature on the sum of the three active neutrino masses, M ν, within the …
Fundamental physics with the square kilometre array
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal
J Park, A Mesinger, B Greig… - Monthly Notices of the …, 2019 - academic.oup.com
The properties of the first galaxies, expected to drive the Cosmic Dawn and the Epoch of
Reionization, are encoded in the 3D structure of the cosmic 21-cm signal. Parameter …
Reionization, are encoded in the 3D structure of the cosmic 21-cm signal. Parameter …
Planck intermediate results-XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
R Adam, PAR Ade, N Aghanim, M Arnaud… - Astronomy & …, 2016 - aanda.org
The polarized thermal emission from diffuse Galactic dust is the main foreground present in
measurements of the polarization of the cosmic microwave background (CMB) at …
measurements of the polarization of the cosmic microwave background (CMB) at …
CMB-S4 science book
This book lays out the scientific goals to be addressed by the next-generation ground-based
cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated …
cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated …