Jason Glenn

TL;DR: In this paper, the authors present 350 micron photometry of all 17 galaxy candidates in the Lockman Hole detected in a 1.1 mm Bolocam survey, and find that the far-infrared to radio relation for star-forming ULIRGs systematically overpredicts the radio luminosities and overestimates redshifts on the order of Delta z ~ 1, whereas redshifting based on either on submillimeter data alone or the 1.6 micron stellar bump and PAH features are more accurate.

TL;DR: In this paper, the ALMA cycle 3 observations of CO and SiO were compared to non-LTE radiative transfer models created using the Line Modeling Engine (LIME) for simple gas dynamics to gain insight into how physical parameters, such as rotational velocity, turbulent velocity, gas temperature, dust temperature, and gas mass can reproduce the observed kinematic and spatial features.

TL;DR: In this paper, spectrally resolved CO J = 5-4 to J = 8-7 lines from Herschel Space Observatory HIFI observations are combined with ground-based observations and high-J Herschel SPIRE observations to decompose the nuclear and putative outflow velocity components and to model the molecular gas to quantify its properties.

TL;DR: It is shown how KIDs can meet the sensitivity target, focusing on two existing architectures that together demonstrate the key necessary attributes, and a straightforward combination of the elements of these already-demonstrated devices points to a low-volume design that is expected to meet the Origins sensitivity targets.

TL;DR: The Galaxy Evolution Probe (GEP) as mentioned in this paper is a mid and far-infrared space observatory designed to survey sky for star-forming galaxies from redshifts of z = 0 to beyond z = 4.