875 citations · 2.7k across the 16 of their papers we have counts for
16 papers
The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136
David T. Frayer, Ronald J. Maddalena, R. J. Ivison +3
We present CO(1-0), CO(3-2), and CO(7-6) observations using the Green Bank Telescope (GBT) and the Atacama Large Millimeter Array (ALMA) of the z=2.8 sub-millimeter galaxy SMM J023…
Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift
N. Scoville, N. Lee, P. Vanden Bout +20
ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field.…
ALMA Resolves the Nuclear Disks of Arp 220
Nick Scoville, Lena Murchikova, Fabian Walter +20
We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at mm. The internal gas distribution and kinematics of both galactic nuclei…
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
N. Scoville, K. Sheth, H. Aussel +17
ALMA Cycle 2 observations of the long wavelength dust emission in 145 star-forming galaxies are used to probe the evolution of star-forming ISM. We also develop the physical basis…
The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2
N. Scoville, H. Aussel, K. Sheth +9
The use of submm dust continuum emission to probe the mass of interstellar dust and gas in galaxies is empirically calibrated using samples of local star forming galaxies, Planck o…
The University of Texas Millimeter Wave Observatory
Paul A. Vanden Bout, John H. Davis, Robert B. Loren
This is an account of the Millimeter Wave Observatory, a 4.9 meter diameter antenna facility that pioneered continuum observations of planets and interstellar molecular spectroscop…