246 citations · 447 across the 3 of their papers we have counts for
8 papers · 1 filter
A dense, solar metallicity ISM in the z=4.2 dusty star-forming galaxy SPT0418-47
Carlos De Breuck, Axel Weiss, Matthieu Bethermin +16
We present a study of six far-infrared fine structure lines in the z=4.225 lensed dusty star-forming galaxy SPT0418-47 to probe the physical conditions of its InterStellar Medium (…
Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z 3
Sreevani Jarugula, Joaquin D. Vieira, Justin S. Spilker +17
Water (), one of the most ubiquitous molecules in the universe, has bright millimeter-wave emission lines easily observed at high-redshift with the current generation o…
The [CII]/[NII] ratio in 3 < z < 6 sub-millimetre galaxies from the South Pole Telescope survey
D. J. M. Cunningham, S. C. Chapman, M. Aravena +19
We present Atacama Compact Array and Atacama Pathfinder Experiment observations of the [N II] 205 m fine-structure line in 40 sub-millimetre galaxies lying at redshifts z = 3 to…
Imaging the Molecular Interstellar Medium in a Gravitationally Lensed Star-forming Galaxy at z=5.7
Yordanka Apostolovski, Manuel Aravena, Timo Anguita +17
Aims: We present and study spatially resolved imaging obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) of multiple CO(65, 87 and 98) and tw…
Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe
J. S. Spilker, M. Aravena, M. Bethermin +20
Galaxies grow inefficiently, with only a few percent of the available gas converted into stars each free-fall time. Feedback processes, such as outflowing winds driven by radiation…
A massive core for a cluster of galaxies at a redshift of 4.3
T. B. Miller, S. C. Chapman, M. Aravena +35
Massive galaxy clusters are now found as early as 3 billion years after the Big Bang, containing stars that formed at even earlier epochs. The high-redshift progenitors of these ga…