activity
20172022
most citedThe Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years

181 citations · 1.1k across the 19 of their papers we have counts for

collaborators

47 papers

astro-ph.GA202220 cited

ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background

Jianhang Chen, R. J. Ivison, Martin A. Zwaan +8

Wide, deep, blind continuum surveys at submillimetre/millimetre (submm/mm) wavelengths are required to provide a full inventory of the dusty, distant Universe. However, conducting…

astro-ph.GA2022

Investigating the [C]-to-H conversion factor and the H gas budget of galaxies at with hydrodynamical simulations

David Vizgan, Kasper E. Heintz, Thomas R. Greve +5

One of the most fundamental baryonic matter components of galaxies is the neutral atomic hydrogen (H). At low redshifts, this component can be traced directl…

astro-ph.GA2022

Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models

Gergö Popping, Céline Péroux

The dust abundance of the interstellar medium plays an important role in galaxy physics, the chemical evolution of matter and the absorption and re-emission of stellar light. The l…

astro-ph.GA202224 cited

IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3

Irene Shivaei, Gergö Popping, George Rieke +12

We present results from ALMA 1.2mm continuum observations of a sample of 27 star-forming galaxies at z=2.1-2.5 from the MOSFIRE Deep Evolution Field (MOSDEF) survey. These galaxies…

astro-ph.GA202231 cited

The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift

Prerak Garg, Desika Narayanan, Nell Byler +9

The Baldwin, Philips, & Terlevich diagram of [O III]/H vs. [N II]/H (hereafter N2-BPT) has long been used as a tool for classifying galaxies based on the dominant source of i…

astro-ph.GA202149 cited

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…