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19972025
most citedWhat Powers Ultra-luminous IRAS Galaxies?

1.2k citations · 15.1k across the 198 of their papers we have counts for

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Showing 2017Show all

12 papers · 1 filter

astro-ph.GA2017★ 46 cited

HERUS: The Far-IR/Submm Spectral Energy Distributions of Local ULIRGs & Photometric Atlas

D. L. Clements, C. Pearson, D. Farrah +9

We present the Herschel-SPIRE photometric atlas for a complete flux limited sample of 43 local Ultraluminous Infrared Galaxies (ULIRGs), selected at 60m by IRAS, as part of the…

astro-ph.GA2017★ 49 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.IM2017★ 94 cited

Review: Far-Infrared Instrumentation and Technology Development for the Next Decade

Duncan Farrah, Kimberly Ennico Smith, David Ardila +33

Far-infrared astronomy has advanced rapidly since its inception in the late 1950's, driven by a maturing technology base and an expanding community of researchers. This advancement…

astro-ph.GA2017★ 112 cited

The Origins of [CII] Emission in Local Star-forming Galaxies

Kevin Croxall, J. D. T. Smith, Eric Pellegrini +17

The [CII] 158um fine-structure line is the brightest emission line observed in local star-forming galaxies. As a major coolant of the gas-phase interstellar medium, [CII] balances…

astro-ph.GA2017★ 18 cited

ALMA [NII] 205 micron Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7

Nanyao Lu, Yinghe Zhao, Tanio Diaz-Santos +9

We present the results from Atacama Large Millimeter/submillimeter Array (ALMA) imaging in the [NII] 205 micron fine-structure line (hereafter [NII]) and the underlying continuum o…

astro-ph.GA2017★ 81 cited

Far-infrared metallicity diagnostics: Application to local ultraluminous infrared galaxies

M. Pereira-Santaella, D. Rigopoulou, D. Farrah +2

The abundance of metals in galaxies is a key parameter which permits to distinguish between different galaxy formation and evolution models. Most of the metallicity determinations…