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20172021
most citedThe ALMA Spectroscopic Survey in the HUDF: CO emission lines and 3 mm continuum sources

93 citations · 579 across the 12 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.GA2019★ 18 cited

The ALMA Spectroscopic Survey in the HUDF: Constraining cumulative CO emission at with power spectrum analysis of ASPECS LP data from 84 to 115 GHz

Bade Uzgil, Chris Carilli, Adam Lidz +12

We present a power spectrum analysis of the ALMA Spectroscopic Survey Large Program (ASPECS LP) data from 84 to 115 GHz. These data predominantly probe small-scale fluctuations ($k…

astro-ph.GA2019★ 20 cited

Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z=2.2

Drew Brisbin, Manuel Aravena, Emanuele Daddi +5

We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z=2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3), a…

astro-ph.GA2019★ 65 cited

The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy

Leindert A. Boogaard, Roberto Decarli, Jorge González-López +31

We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the de…

astro-ph.GA2019★ 93 cited

The ALMA Spectroscopic Survey in the HUDF: CO emission lines and 3 mm continuum sources

Jorge González-López, Roberto Decarli, Ricardo Pavesi +29

The ALMA SPECtroscopic Survey in the {\it Hubble} Ultra Deep Field is an ALMA large program that obtained a frequency scan in the 3\,mm band to detect emission lines from the molec…

astro-ph.GA2019★ 77 cited

The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM

Gergö Popping, Annalisa Pillepich, Rachel S. Somerville +27

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) provides new constraints for galaxy formation models on the molecular gas properties of galaxies. We compare r…