Cosmic star-formation history
P Madau, M Dickinson - Annual Review of Astronomy and …, 2014 - annualreviews.org
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
Distant radio galaxies and their environments
G Miley, C De Breuck - The Astronomy and Astrophysics Review, 2008 - Springer
We review the properties and nature of luminous high-redshift radio galaxies (HzRGs, z> 2)
and the environments in which they are located. HzRGs have several distinct constituents …
and the environments in which they are located. HzRGs have several distinct constituents …
The evolution of the IR luminosity function and dust-obscured star formation over the past 13 billion years
JA Zavala, CM Casey, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the first results from the Mapping Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …
The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z= 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History
R Bouwens, J González-López… - The Astrophysical …, 2020 - iopscience.iop.org
We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …
UV luminosity functions at redshifts z∼ 4 to z∼ 10: 10,000 galaxies from HST legacy fields
RJ Bouwens, GD Illingworth, PA Oesch… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The remarkable Hubble Space Telescope (HST) data sets from the CANDELS,
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
The ALPINE-ALMA [CII] survey-The nature, luminosity function, and star formation history of dusty galaxies up to z≃ 6
C Gruppioni, M Béthermin, F Loiacono… - Astronomy & …, 2020 - aanda.org
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
The evolution of the galaxy rest-frame ultraviolet luminosity function over the first two billion years
SL Finkelstein, RE Ryan, C Papovich… - The Astrophysical …, 2015 - iopscience.iop.org
We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity
functions at z= 4–8. We use deep Hubble Space Telescope imaging over the Cosmic …
functions at z= 4–8. We use deep Hubble Space Telescope imaging over the Cosmic …
A model for cosmological simulations of galaxy formation physics
M Vogelsberger, S Genel, D Sijacki… - Monthly Notices of …, 2013 - academic.oup.com
We present a new comprehensive model of the physics of galaxy formation designed for
large-scale hydrodynamical simulations of structure formation using the moving-mesh code …
large-scale hydrodynamical simulations of structure formation using the moving-mesh code …
Full-data results of Hubble frontier fields: UV luminosity functions at z∼ 6–10 and a consistent picture of cosmic reionization
M Ishigaki, R Kawamata, M Ouchi, M Oguri… - The Astrophysical …, 2018 - iopscience.iop.org
We present UV luminosity functions of dropout galaxies at~– z 6 10 with the complete
Hubble Frontier Fields data. We obtain a catalog of∼ 450 dropout-galaxy candidates (350 …
Hubble Frontier Fields data. We obtain a catalog of∼ 450 dropout-galaxy candidates (350 …
Radiative transfer in a clumpy universe. IV. New synthesis models of the cosmic UV/X-ray background
We present improved synthesis models of the evolving spectrum of the UV/X-ray diffuse
background, updating and extending our previous results. Five new main components are …
background, updating and extending our previous results. Five new main components are …