High-redshift star formation in the Atacama large millimetre/submillimetre array era

JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

Dusty star-forming galaxies at high redshift

CM Casey, D Narayanan, A Cooray - Physics Reports, 2014 - Elsevier
Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

Detection of lensing substructure using ALMA observations of the dusty galaxy SDP. 81

YD Hezaveh, N Dalal, DP Marrone… - The Astrophysical …, 2016 - iopscience.iop.org
We study the abundance of substructure in the matter density near galaxies using ALMA
Science Verification observations of the strong lensing system SDP. 81. We present a …

The complete redshift distribution of dusty star-forming galaxies from the SPT-SZ survey

C Reuter, JD Vieira, JS Spilker, A Weiss… - The Astrophysical …, 2020 - iopscience.iop.org
Abstract The South Pole Telescope (SPT) has systematically identified 81 high-redshift,
strongly gravitationally lensed, dusty star-forming galaxies (DSFGs) in a 2500 square …

Strong gravitational lensing of explosive transients

M Oguri - Reports on Progress in Physics, 2019 - iopscience.iop.org
Recent rapid progress in time domain surveys makes it possible to detect various types of
explosive transients in the Universe in large numbers, some of which will be gravitationally …

Turbulent Gas in Lensed Planck-selected Starbursts at z∼ 1–3.5

KC Harrington, A Weiss, MS Yun… - The Astrophysical …, 2021 - iopscience.iop.org
Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

The accretion history of AGNs. I. Supermassive black hole population synthesis model

TT Ananna, E Treister, CM Urry, C Ricci… - The Astrophysical …, 2019 - iopscience.iop.org
As matter accretes onto the central supermassive black holes in active galactic nuclei
(AGNs), X-rays are emitted. We present a population synthesis model that accounts for the …

Validation of the equilibrium model for galaxy evolution to z∼ 3 through molecular gas and dust observations of lensed star-forming galaxies

A Saintonge, D Lutz, R Genzel, B Magnelli… - The Astrophysical …, 2013 - iopscience.iop.org
We combine IRAM Plateau de Bure Interferometer and Herschel PACS and SPIRE
measurements to study the dust and gas contents of high-redshift star-forming galaxies. We …

GRAVITATIONAL LENS MODELS BASED ON SUBMILLIMETER ARRAY* IMAGING OF HERSCHEL†-SELECTED STRONGLY LENSED SUB-MILLIMETER …

RS Bussmann, I Pérez-Fournon, S Amber… - The Astrophysical …, 2013 - iopscience.iop.org
Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-
) millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution …

Precise LIGO lensing rate predictions for binary black holes

KKY Ng, KWK Wong, T Broadhurst, TGF Li - Physical Review D, 2018 - APS
We show how LIGO is expected to detect coalescing binary black holes at z> 1 that are
lensed by the intervening galaxy population. Gravitational magnification, μ, strengthens …