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(1 - 16 of 16)
The wide-field, multiplexed, spectroscopic facility WEAVE
Resolved CO(1-0) emission and gas properties in luminous dusty star-forming galaxies at z = 2-4
Characterisation of Herschel-selected strong lens candidates through HST and sub-mm/mm observations
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies
An ultradeep multiband very large array survey of the faint radio sky (COSMOS-XS)
The bright extragalactic ALMA redshift survey (BEARS) I
The 700 ks Chandra Spiderweb Field
The 700 ks Chandra Spiderweb Field. I.
Cooperation and trust across societies during the Covid-19 pandemic
Intergenerational conflicts of interest and prosocial behavior during the COVID-19 pandemic
Close-up view of a luminous star-forming galaxy at z = 2.95
COALAS
The infrared-radio correlation of star-forming galaxies is strongly M*-dependent but nearly redshift-invariant since z ~ 4
NOEMA redshift measurements of bright Herschel galaxies