Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …

We present specific star formation rates (sSFRs) for 40 ultraviolet (UV)-bright galaxies at z∼
7–8 observed as part of the Reionization Era Bright Emission Line Survey (REBELS) …

The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …

We present our new Atacama Large Millimeter/Submillimeter Array (ALMA) observations
targeting [O iii] 88 μm,[C ii] 158 μm,[N ii] 122 μm, and dust-continuum emission for three …

We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …

We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158
μm emission in a large sample of normal star-forming galaxies at 4< z< 6 from the ALMA …

The [C II] 158 μm line is one of the strongest IR emission lines, which has been shown to
trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z∼ 2 …

We report on the detection of the [C ii] 157.7 μ m emission from the Lyman break galaxy
(LBG) MACS0416_Y1 at z= 8.3113, by using the Atacama Large Millimeter/submillimeter …