M. Pannella

The main sequence of star-forming galaxies across cosmic times

The 700 ks <i>Chandra</i> Spiderweb Field

The 700 ks <i>Chandra</i> Spiderweb Field

The VANDELS ESO public spectroscopic survey

Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 ≤ z ≤ 2

Galaxy populations in the most distant SPT-SZ clusters

The main sequence of star-forming galaxies – II. A non-evolving slope at the high-mass end

Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at 1.4 ≲ z ≲ 1.7

GOODS-ALMA: 1.1 mm galaxy survey

“Super-deblended” Dust Emission in Galaxies. I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6

The VANDELS ESO public spectroscopic survey

The main sequence of star-forming galaxies – I. The local relation and its bending

The VANDELS ESO public spectroscopic survey: Observations and first data release

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

VLA AND ALMA IMAGING OF INTENSE GALAXY-WIDE STAR FORMATION IN z ∼ 2 GALAXIES

INFRARED COLOR SELECTION OF MASSIVE GALAXIES AT z &gt; 3

Dust and gas in luminous proto-cluster galaxies at<i>z</i>= 4.05: the case for different cosmic dust evolution in normal and starburst galaxies

Linking the X-ray and infrared properties of star-forming galaxies at z &lt; 1.5★

EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN<i>z</i>∼ 2 DUSTY GALAXIES FROM THE GOODS-<i>HERSCHEL</i>SURVEY