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19982026
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 8.3k across the 91 of their papers we have counts for

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Showing 2014 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2014★ 67 cited

ALMA Observations of Warm Dense Gas in NGC 1614 --- Breaking of Star Formation Law in the Central kpc

C. K. Xu, C. Cao, N. Lu +20

We present ALMA Cycle-0 observations of the CO (6-5) line emission and of the 435um dust continuum emission in the central kpc of NGC 1614, a local luminous infrared galaxy (LIRG)…

astro-ph.GA2014★ 94 cited

High-Resolution Radio Continuum Measurements of the Nuclear Disks of Arp 220

Loreto Barcos-Muñoz, Adam K. Leroy, Aaron S. Evans +16

We present new Karl G. Jansky Very Large Array radio continuum images of the nuclei of Arp 220, the nearest ultra-luminous infrared galaxy. These images have both the angular resol…

astro-ph.GA2014★ 32 cited

Radio continuum properties of luminous infrared galaxies. Identifying the presence of an AGN in the radio

E. Vardoulaki, V. Charmandaris, E. J. Murphy +7

Luminous infrared galaxies are systems enshrouded in dust, which absorbs most of their optical/UV emission and re-radiates it in the mid- and far-infrared. Radio observations are l…

astro-ph.GA2014★ 81 cited

Extended [CII] Emission in Local Luminous Infrared Galaxies

T. Diaz-Santos, L. Armus, V. Charmandaris +20

We present Herschel/PACS observations of extended [CII]157.7μm line emission detected on ~ 1 - 10 kpc scales in 60 local luminous infrared galaxies (LIRGs) from the Great Observato…

astro-ph.GA2014★ 55 cited

Warm Molecular Gas in Luminous Infrared Galaxies

N. Lu, Y. Zhao, C. K. Xu +18

We present our initial results on the CO rotational spectral line energy distribution (SLED) of the to 1 transitions from up to from Herschel SPIRE spectroscop…

astro-ph.GA2014★ 41 cited

ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34

C. K. Xu, C. Cao, N. Lu +17

We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435 dust continuum emission in the nuclear region of NGC 34,…