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 …

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 …

We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

We present the implications for cosmic inflation of the Planck measurements of the cosmic
microwave background (CMB) anisotropies in both temperature and polarization based on …

Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench
star formation in galaxies, although direct observational evidence is still scarce and debated …

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 …

We use deep JWST/NIRSpec R∼ 1000 slit spectra of 113 galaxies at, selected from the
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …

The KMOS3D Survey: Data Release and Final Survey Paper - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

Aims. The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback
(SUPER) aims to trace and characterise ionised gas outflows and their impact on star …

Models and observations suggest that both the power and effects of AGN feedback should
be maximised in hyper-luminous (L Bol> 10 47 erg s-1) quasars, ie objects at the brightest …