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20062026
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 20.7k across the 287 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.GA2018★ 55 cited

The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last 10 Gyr

Alfred L. Tiley, A. M. Swinbank, C. M. Harrison +16

We analyse maps of the spatially-resolved nebular emission of 1500 star-forming galaxies at - from deep KMOS and MUSE observations to measure the average…

astro-ph.GA2018★ 123 cited

A Survey of Atomic Carbon [C I] in High-redshift Main-Sequence Galaxies

F. Valentino, G. E. Magdis, E. Daddi +15

We present the first results of an ALMA survey of the lower fine structure line of atomic carbon [C I] in far infrared-selected galaxies on the main sequence a…

astro-ph.GA2018★ 42 cited

KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since

A. L. Tiley, M. Bureau, L. Cortese +27

We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One…

astro-ph.GA2018★ 57 cited

PAHs as tracers of the molecular gas in star-forming galaxies

I. Cortzen, J. Garrett, G. Magdis +12

[Abridged] We combine new CO(1-0) line observations of 24 intermediate redshift galaxies (0.03 < z < 0.28) along with literature data of galaxies at 0<z<4 to explore scaling relati…

astro-ph.GA2018★ 54 cited

The molecular gas content and fuel efficiency of starbursts at z ~ 1.6 with ALMA

J. Silverman, W. Rujopakarn, E. Daddi +17

We present an analysis of the molecular gas properties, based on CO(2 - 1) emission, of twelve starburst galaxies at z~1.6 selected by having a boost (>~4x) in their star formation…

astro-ph.GA2018★ 19 cited

Concurrent starbursts in molecular gas disks within a pair of colliding galaxies at z = 1.52

J. Silverman, E. Daddi, W. Rujopakarn +20

We report on the discovery of a merger-driven starburst at z = 1.52, PACS-787, based on high signal-to-noise ALMA observations. CO(5-4) and continuum emission (850um) at a spatial…