Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Surveying the distant Universe
Artikel i vetenskaplig tidskrift, 2024

During the most active period of star formation in galaxies, which occurs in the redshift range 1 < z < 3, strong bursts of star formation result in significant quantities of dust, which obscures new stars being formed as their UV/optical light is absorbed and then re-emitted in the infrared, which redshifts into the mm/sub-mm bands for these early times. To get a complete picture of the high- z galaxy population, we need to survey a large patch of the sky in the sub-mm with sufficient angular resolution to resolve all galaxies, but we also need the depth to fully sample their cosmic evolution, and therefore obtain their redshifts using direct mm spectroscopy with a very wide frequency coverage. This requires a large single-dish sub-mm telescope with fast mapping speeds at high sensitivity and angular resolution, a large bandwidth with good spectral resolution and multiplex spectroscopic capabilities. The proposed 50-m Atacama Large Aperture Submillimeter Telescope (AtLAST) will deliver these specifications. We discuss how AtLAST allows us to study the whole population of high-z galaxies, including the dusty star-forming ones which can only be detected and studied in the sub-mm, and obtain a wealth of information for each of these up to z ∼ 7: gas content, cooling budget, star formation rate, dust mass, and dust temperature. We present worked examples of surveys that AtLAST can perform, both deep and wide, and also focused on galaxies in proto-clusters. In addition we show how such surveys with AtLAST can measure the growth rate f σ 8 and the Hubble constant with high accuracy, and demonstrate the power of the line-intensity mapping method in the mm/sub-mm wavebands to constrain the cosmic expansion history at high redshifts, as good examples of what can uniquely be done by AtLAST in this research field.

galaxy formation

cluster galaxies

cosmology

sub-mm galaxies

galaxy surveys

Författare

E. van Kampen

European Southern Observatory (ESO)

Tom Bakx

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

C. De Breuck

European Southern Observatory (ESO)

C. C. Chen

Academia Sinica

H. Dannerbauer

Instituto de Astrofísica de Canarias

Universidad de la Laguna

Benjamin Magnelli

Université Paris-Saclay

F.M. Montenegro-Montes

European Southern Observatory (ESO)

IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos)

Teppei Okumura

Academia Sinica

Sy Yin Pu

National Tsing Hua University

Academia Sinica

M. Rybak

Netherlands Institute for Space Research (SRON)

Universiteit Leiden

TU Delft

Amélie Saintonge

Max-Planck-Gesellschaft

University College London (UCL)

C. Cicone

Universitetet i Oslo

E. Hatziminaoglou

Universidad de la Laguna

Instituto de Astrofísica de Canarias

European Southern Observatory (ESO)

Juliëtte Hilhorst

Yale University

Universiteit Leiden

Pamela Klaassen

Royal Observatory

Minju Lee

Danmarks Tekniske Universitet (DTU)

Cosmic Dawn Center (DAWN)

Christopher C. Lovell

University of Portsmouth

A. Lundgren

Laboratoire d'Astrophysique de Marseille

Luca Di Mascolo

IFPU - Institute for Fundamental Physics of the Universe

Laboratoire Joseph-Louis Lagrange

Universita degli Studi di Trieste

Osservatorio Astronomico di Trieste

Tony Mroczkowski

European Southern Observatory (ESO)

Laura Sommovigo

Flatiron Institute

M. Booth

Royal Observatory

M. A. Cordiner

NASA Goddard Space Flight Center

R. J. Ivison

ARC Centre of Excellence for All-sky Astrophysics

European Southern Observatory (ESO)

University of Edinburgh

Dublin Institute for Advanced Studies

D. Johnstone

National Research Council Canada

University of Victoria

Daizhong Liu

Chinese Academy of Sciences

Max-Planck-Gesellschaft

T. J. Maccarone

Texas Tech University at Lubbock

M. W.L. Smith

Cardiff University

Alexander Thelen

California Institute of Technology (Caltech)

S. Wedemeyer

Universitetet i Oslo

Open Research Europe

27325121 (eISSN)

Vol. 4 122

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.12688/openreseurope.17445.1

Mer information

Senast uppdaterat

2024-10-28