Luca Graziani

Astrophysics with the Laser Interferometer Space Antenna

Cold dust and low [O <scp>iii</scp>]/[C <scp>ii</scp>] ratios: an evolved star-forming population at redshift 7

The ALMA REBELS Survey: the first infrared luminosity function measurement at <i>z</i>  ∼ 7

The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at <i>z</i> <b>=</b> 4–8 revealed by the IRX–β and <i>M</i>⋆ relations

The ALMA Reionization Era Bright Emission Line Survey: The molecular gas content of galaxies at <i>z</i> ~ 7

The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at <i>z</i> = 7.31

Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z &gt; 6.5 Universe

The ALMA REBELS Survey: cosmic dust temperature evolution out to <i>z</i> ∼ 7

The ALMA REBELS survey: the dust content of <i>z</i> ∼ 7 Lyman break galaxies

The ALMA REBELS Survey: dust continuum detections at <i>z</i> &amp;gt; 6.5

The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7

The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at <i>z</i> ≈ 7

The ALMA REBELS Survey : specific star formation rates in the reionization era

The REBELS ALMA Survey: efficient Ly α transmission of UV-bright <i>z</i> ≃ 7 galaxies from large velocity offsets and broad line widths

The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4

The ALMA REBELS Survey: The Cosmic H i Gas Mass Density in Galaxies at z ≈ 7

Exploration of the high-redshift universe enabled by THESEUS

Exploration of the high-redshift universe enabled by THESEUS