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The evolution of the star-forming interstellar medium across cosmic time
LJ Tacconi, R Genzel, A Sternberg - Annual Review of …, 2020 - annualreviews.org
Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
Star-forming galaxies at cosmic noon
NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …
star-formation history, which culminated around; this period is often nicknamed “cosmic …
A dusty compact object bridging galaxies and quasars at cosmic dawn
Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …
become a major challenge, since it was discovered that luminous quasars existed only 700 …
The Herschel view of the dominant mode of galaxy growth from z= 4 to the present day
We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …
The coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary universe
TM Heckman, PN Best - Annual Review of Astronomy and …, 2014 - annualreviews.org
We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …
physics and phenomenology of the processes that link the formation and evolution of …
The Illustris simulation: the evolving population of black holes across cosmic time
We study the properties of black holes and their host galaxies across cosmic time in the
Illustris simulation. Illustris is a large-scale cosmological hydrodynamical simulation which …
Illustris simulation. Illustris is a large-scale cosmological hydrodynamical simulation which …
What drives the growth of black holes?
DM Alexander, RC Hickox - New Astronomy Reviews, 2012 - Elsevier
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
massive galaxies in the local Universe. Recent years have seen remarkable advances in …
Cosmological simulations of black hole growth: AGN luminosities and downsizing
M Hirschmann, K Dolag, A Saro… - Monthly Notices of …, 2014 - academic.oup.com
In this study, we present a detailed, statistical analysis of black hole growth and the evolution
of active galactic nuclei (AGN) using cosmological hydrodynamic simulations run down to z …
of active galactic nuclei (AGN) using cosmological hydrodynamic simulations run down to z …
The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations
B Magnelli, P Popesso, S Berta, F Pozzi… - Astronomy & …, 2013 - aanda.org
We present results from the deepest Herschel-Photodetector Array Camera and
Spectrometer (PACS) far-infrared blank field extragalactic survey, obtained by combining …
Spectrometer (PACS) far-infrared blank field extragalactic survey, obtained by combining …
The KMOS3D survey: demographics and properties of galactic outflows at z= 0.6–2.7
NMF Schreiber, H Übler, RL Davies… - The Astrophysical …, 2019 - iopscience.iop.org
We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …