246 citations · 6k across the 111 of their papers we have counts for
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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…
A solar metallicity galaxy at 7? Possible detection of the [N II] 122 m and [O III] 52 m lines
Meghana Killi, Darach Watson, Seiji Fujimoto +9
We present the first detection of the [N II] 122 m and [O III] 52 m lines for a reionisation-epoch galaxy. Based on these lines and previous [C II] 158 m and [O III] 88 $μ…
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…
Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
L. Y. Aaron Yung, Rachel S. Somerville, Steven L. Finkelstein +11
The Nancy Grace Roman Space Telescope, NASA's next flagship observatory, will redefine deep-field galaxy survey with a field of view two orders of magnitude larger than Hubble and…
To see or not to see a galaxy, that is the question
Melanie Kaasinen, Joshiwa van Marrewijk, Gergö Popping +7
Determining when the first galaxies formed remains an outstanding goal of modern observational astronomy. Theory and current stellar population models imply that the first galaxies…
An upper limit on [OIII] 88 m and 1.2 mm continuum emission from a JWST galaxy candidate with ALMA
Gergö Popping
A number of new galaxy candidates have recently been identified based on public James Webb Space Telescope (JWST) NIRCam observations. Spectroscopic confirmation of these ca…
Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
L. Y. Aaron Yung, Rachel S. Somerville, Henry C. Ferguson +6
In anticipation of the new era of high-redshift exploration marked by the commissioning of the James Webb Space Telescope (JWST), we present two sets of galaxy catalogues that are…
The strongest cool core in REXCESS: Missing X-ray cavities in RXC J2014.8-2430
Tony Mroczkowski, Megan Donahue, Joshiwa van Marrewijk +8
We present a multiwavelength study of RXC J2014.8-2430, the most extreme cool-core cluster in the Representative Cluster Structure Survey (REXCESS), using X-…
CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at
Ryan L. Sanders, Alice E. Shapley, Tucker Jones +9
We present observations of CO(3-2) in 13 main-sequence star-forming galaxies at that span a wide range in metallicity (O/H) based on res…
The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon
Gergö Popping, Irene Shivaei, Ryan L. Sanders +6
We aim to quantify the relation between the dust-to-gas mass ratio (DTG) and gas-phase metallicity of 2.1-2.5 luminous galaxies and contrast this high-redshift relation against…
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…
Tracing Molecular Gas in z 6 Galaxies with [C]
David Vizgan, Thomas R. Greve, Karen P. Olsen +7
We investigate the fine-structure [C] line at m as a molecular gas tracer by analyzing the relationship between molecular gas mass () and…
The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2
Irene Shivaei, Leindert Boogaard, Tanio Díaz-Santos +10
The UV bump is a broad absorption feature centered at 2175Å that is seen in the attenuation/extinction curve of some galaxies, but its origin is not well known. Here, we use a samp…
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…
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…