Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

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 …

We present Atacama Large Millimeter/submillimeter Array (ALMA) sub-kiloparsec-to
kiloparsec-scale resolution observations of the [C II], CO (9–8), and OH+(1 1–0 1) lines …

We present a high-resolution kinematic study of the massive main-sequence star-forming
galaxy (SFG) SDSS J090122. 37+ 181432.3 (J0901) at z= 2.259, using∼ 0 farcs 36 …

The vast quantity of strong galaxy–galaxy gravitational lenses expected by future large-scale
surveys necessitates the development of automated methods to efficiently model their mass …

We present a sub-kpc resolved study of the interstellar medium properties in SDP. 81, a=
3.042 strongly gravitationally lensed, dusty star-forming galaxy, based on high-resolution …

We report on the internal distribution of star formation efficiency in IRAS 08339+ 6517
(hereafter IRAS08), using∼ 200 pc resolution CO (2− 1) observations from NOEMA. The …

Exploiting the sensitivity of the IRAM NOrthern Extended Millimeter Array (NOEMA) and its
ability to process large instantaneous bandwidths, we have studied the morphology and …

We present a high-resolution study of the cold molecular gas as traced by CO (1-0) in the
unlensed z∼ 3.4 submillimeter galaxy SMM J13120+ 4242, using multiconfiguration …