Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …

ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS
OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD - IOPscience …

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 …

THE EVOLUTION OF INTERSTELLAR MEDIUM MASS PROBED BY DUST EMISSION: ALMA
OBSERVATIONS AT z = 0.3–2 - IOPscience Skip to content IOP Science home Accessibility …

THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD:
CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND …

Abstract Using the Australia Telescope Compact Array, we conducted a survey of CO J= 1−
0 and J= 2− 1 line emission towards strongly lensed high-redshift dusty star-forming …

ABSTRACT We present FIR [50–300 μm]− CO luminosity relations (ie, $\log L_ {\rm
FIR}=\alpha\log L^{\prime} _ {\rm CO}+\beta $) for the full CO rotational ladder from J= 1–0 …

We analyze the interstellar medium properties of a sample of 16 bright CO line emitting
galaxies identified in the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field …

Using the NSF's Karl G. Jansky Very Large Array (VLA), we report six detections of CO (J=
1→ 0) emission and one upper limit in z= 2–3 galaxies originally detected in higher-J CO …