The Dark Energy Survey: more than dark energy–an overview
Dark Energy Survey Collaboration:… - Monthly Notices of …, 2016 - academic.oup.com
This overview paper describes the legacy prospect and discovery potential of the Dark
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …
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∼ …
A JWST/NIRSpec First Census of Broad-line AGNs at z= 4–7: Detection of 10 Faint AGNs with M BH∼ 106–108 M⊙ and Their Host Galaxy Properties
We present the first statistical sample of faint type 1 AGNs at z> 4 identified by
JWST/NIRSpec deep spectroscopy. Among the 185 galaxies at z spec= 3.8–8.9 confirmed …
JWST/NIRSpec deep spectroscopy. Among the 185 galaxies at z spec= 3.8–8.9 confirmed …
First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
GA-NIFS: A massive black hole in a low-metallicity AGN at z∼ 5.55 revealed by JWST/NIRSpec IFS
H Übler, R Maiolino, E Curtis-Lake… - Astronomy & …, 2023 - aanda.org
We present rest-frame optical data of the compact z= 5.55 galaxy GS_3073 obtained using
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …
Simulating galaxy formation with black hole driven thermal and kinetic feedback
The inefficiency of star formation in massive elliptical galaxies is widely believed to be
caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas …
caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas …
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 …
AGN wind scaling relations and the co-evolution of black holes and galaxies
Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …
the main mechanism responsible for regulating star formation in active galactic nucleus …
Theoretical challenges in galaxy formation
T Naab, JP Ostriker - Annual review of astronomy and …, 2017 - annualreviews.org
Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …
evolution. Over the decades the field has made significant progress. It is now possible to …
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 …