246 citations · 6k across the 111 of their papers we have counts for
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Exploring the High-Redshift Universe with ALMA
Evanthia Hatziminaoglou, Gergö Popping, Martin Zwaan
The properties of the interstellar medium (ISM) of the highest-redshift galaxies and quasars provide important indications of the complex interplay between the accretion of baryons…
Mapping Obscuration to Reionization with ALMA (MORA): 2mm Efficiently Selects the Highest-Redshift Obscured Galaxies
Caitlin M. Casey, Jorge A. Zavala, Sinclaire M. Manning +24
We present the characteristics of 2mm-selected sources from the largest Atacama Large Millimeter and submillimeter Array (ALMA) blank-field contiguous survey conducted to-date, the…
Revisiting the [C II] line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter
Chandra Shekhar Murmu, Karen P. Olsen, Thomas R. Greve +9
Detecting the line-intensity mapping (LIM) signal from the galaxies of the Epoch of Reionization is an emerging tool to constrain their role in reionization. Ongoing and upcoming e…
Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
L. Y. Aaron Yung, Rachel S. Somerville, Steven L. Finkelstein +5
Active galactic nuclei (AGN) forming in the early universe are thought to be the primary source of hard ionizing photons contributing to the reionization of intergalactic helium. H…
An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift
Shengqi Yang, Gergö Popping, Rachel S. Somerville +3
Sub-millimeter emission lines produced by the interstellar medium (ISM) are strong tracers of star formation and are some of the main targets of line intensity mapping (LIM) survey…
On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
Patrick C. Breysse, Shengqi Yang, Rachel S. Somerville +3
The Millimeter-wave Intensity Mapping Experiment (mmIME) recently reported a detection of excess spatial fluctuations at a wavelength of 3 mm, which can be attributed to unresolved…
The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at
Bade D. Uzgil, Pascal A. Oesch, Fabian Walter +18
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212-272 GHz) covers potential [CII] emission in galaxies at throughout a 2.9 arcm…
SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
Karen Pardos Olsen, Blakesley Burkhart, Mordecai-Mark Mac Low +9
We present an update to the framework called SImulator of GAlaxy Millimeter/submillimeter Emission (SÍGAME). SÍGAME derives line emission in the far-infrared (FIR) for galaxies in…
The dust-continuum size of TNG50 galaxies at : a comparison with the distribution of stellar light, stars, dust and H
Gergö Popping, Annalisa Pillepich, Gabriela Calistro Rivera +6
We present predictions for the extent of the dust-continuum emission of thousands of main-sequence galaxies drawn from the TNG50 simulation between . To this aim, we couple…
The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
J. A. Zavala, C. M. Casey, S. M. Manning +25
We present the first results from the 2mm Mapping Obscuration to Reionization (MORA) survey, the largest ALMA contiguous blank-field survey to-date with a total area of 184 sq. arc…
The prospects for observing [OIII] 52 micron emission from galaxies during the Epoch of Reionization
Shengqi Yang, Adam Lidz, Gergö Popping
The [OIII] 88 m fine structure emission line has been detected into the Epoch of Reionization (EoR) from star-forming galaxies at redshifts with ALMA. These m…