We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …

We report the first detailed measurement of the shape of the CO luminosity function at high
redshift, based on> 320 hr of the NSF's Karl G. Jansky Very Large Array (VLA) observations …

Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

Abstract We use Atacama Large Millimeter Array (ALMA) observations of four submillimeter
galaxies (SMGs) at z∼ 2–3 to investigate the spatially resolved properties of the interstellar …

Single flux density measurements at observed-frame submillimeter and millimeter
wavelengths are commonly used to probe dust and gas masses in galaxies. In this Letter …

Following the success of the Plateau de Bure high-z Blue Sequence Survey (PHIBSS), we
present the PHIBSS2 legacy program, a survey of the molecular gas properties of star …

We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies
between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array …

We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line
deep field targeting CO (1–0) emission from galaxies at z= 1.95–2.85 and CO (2–1) at z …

We present detailed studies of az= 2.12 submillimeter galaxy, ALESS67. 1, using sub-
arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space …