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20022026
most citedAdvanced capabilities for materials modelling with Quantum ESPRESSO

7.7k citations

Showing 2017 · astro-ph.GAShow all

24 papers · 2 filters

astro-ph.GA201762 cited

The Effect of Filaments and Tendrils on the HI Content of Galaxies

Mary Crone Odekon, Gregory Hallenbeck, Martha P. Haynes +3

We use the ALFALFA HI survey to examine whether the cold gas reservoirs of galaxies are inhibited or enhanced in large-scale filaments. Our sample includes 9947 late-type galaxies…

astro-ph.GA20175 cited

An Infrared Study of the Circumstellar Material Associated with the Carbon Star R Sculptoris

Matthew J. Hankins, Terry L. Herter, Matthias Maercker +2

The asymptotic giant branch (AGB) star R Sculptoris (R Scl) is one of the most extensively studied stars on the AGB. R Scl is a carbon star with a massive circumstellar shell ($M_{…

astro-ph.GA201745 cited

Total Molecular Gas Masses of Planck - Herschel Selected Strongly Lensed Hyper Luminous Infrared Galaxies

K. C. Harrington, M. S. Yun, B. Magnelli +8

We report the detection of CO(1 - 0) line emission from seven Planck and Herschel selected hyper luminous (LIR(8-1000um) > 10^13Lsun) infrared galaxies with the Green Bank Telescop…

astro-ph.GA201749 cited

On the far-infrared metallicity diagnostics: applications to high-redshift galaxies

D. Rigopoulou, M. Pereira-Santaella, G. E. Magdis +5

In an earlier paper we modeled the far-infrared emission from a star-forming galaxy using the photoionisation code CLOUDY and presented metallicity sensitive diagnostics based on f…

astro-ph.GA2017126 cited

Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z~2-4 as probed by multi-J CO lines

C. Yang, A. Omont, A. Beelen +18

(abridged) We present the IRAM-30m observations of multiple-J CO and CI line emission in a sample of redshift ~2-4 Herschel-ATLAS SMGs. A non-negligible effect of differential lens…

astro-ph.GA201755 cited

Dynamical Characterization of Galaxies at z~4-6 via Tilted Ring Fitting to ALMA [CII] Observations

G. C. Jones, C. L. Carilli, Y. Shao +7

Until recently, determining the rotational properties of galaxies in the early universe (z>4, Universe age <1.5Gyr) was impractical, with the exception of a few strongly lensed sys…