1.1k citations · 5.5k across the 56 of their papers we have counts for
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Resolved UV and optical color gradients reveal environmental influence on galaxy evolution at redshift z1.6
William J. Cramer, A. G. Noble, G. Rudnick +13
The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth…
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Daizhong Liu, Amelie Saintonge, Caroline Bot +25
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunitie…
Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: The hidden circumgalactic medium
Minju M. Lee, Alice Schimek, Claudia Cicone +29
Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cos…
Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy
Pamela Klaassen, Alessio Traficante, Maria T. Beltrán +38
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas…
High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
Alice Schimek, Davide Decataldo, Sijing Shen +10
The circumgalactic medium (CGM) is a crucial component of galaxy evolution, but thus far its physical properties are highly unconstrained. As of yet, no cosmological simulation has…
A large-scale kinematic study of molecular gas in high-z cluster galaxies: Evidence for high levels of kinematic asymmetry
W. J. Cramer, A. G. Noble, K. Massingill +14
We investigate the resolved kinematics of the molecular gas, as traced by ALMA in CO (2-1), of 25 cluster member galaxies across three different clusters at a redshift of $z\sim1.6…
Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang
E. F. Jiménez-Andrade, B. Magnelli, A. Karim +23
We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at . We secured CO molecular line detections for the and trans…
ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO
Gergö Popping, Roberto Decarli, Allison W. S. Man +9
We present ALMA detections of the [CI] 1-0, CO J=3-2, and CO J=4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z=2.225, 3D-HST…
ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within
J. E. Geach, D. Narayanan, Y. Matsuda +28
We present new Atacama Large Millimeter/Submillimeter Array (ALMA) 850um continuum observations of the original Lyman-alpha Blob (LAB) in the SSA22 field at z=3.1 (SSA22-LAB01). Th…
Galaxy And Mass Assembly (GAMA): relations of bulges, discs and spheroids
Rebecca Lange, Amanda J. Moffett, Simon P. Driver +25
We perform automated bulge + disc decomposition on a sample of 7500 galaxies from the Galaxy And Mass Assembly (GAMA) survey in the redshift range of 0.002z0.06 using S…
Sub-mm Emission Line Deep Fields: CO and [CII] Luminosity Functions out to z = 6
Gergö Popping, Eelco van Kampen, Roberto Decarli +3
Now that ALMA is reaching its full capabilities, observations of sub-mm emission line deep fields become feasible. We couple a semi-analytic model of galaxy formation with a radiat…
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
Simon P. Driver, Angus H. Wright, Stephen K. Andrews +60
We present the GAMA Panchromatic Data Release (PDR) constituting over 230deg of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data compleme…
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
J. Liske, I. K. Baldry, S. P. Driver +67
The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low-redshift galaxies. Covering an area of ~286 deg^2 (split among five surve…
Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
A. S. G. Robotham, S. P. Driver, L. J. M. Davies +28
We use a highly complete subset of the GAMA-II redshift sample to fully describe the stellar mass dependence of close-pairs and mergers between 10^8 Msun and 10^12 Msun. Using the…