93 citations · 579 across the 12 of their papers we have counts for
12 papers
The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at
Bade D. Uzgil, Pascal A. Oesch, Fabian Walter +18
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212-272 GHz) covers potential [CII] emission in galaxies at throughout a 2.9 arcm…
A Lyman-α protocluster at redshift 6.9
Weida Hu, Junxian Wang, Leopoldo Infante +21
Protoclusters, the progenitors of the most massive structures in the Universe, have been identified at redshifts of up to 6.6. Besides exploring early structure formation, searchin…
ALMA Lensing Cluster Survey: Bright [CII] 158 m Lines from a Multiply Imaged Sub- Galaxy at
Seiji Fujimoto, Masamune Oguri, Gabriel Brammer +31
We present bright [CII] 158 m line detections from a strongly magnified and multiply-imaged () sub- ( = ) Lyman-break gal…
ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at 6
N. Laporte, A. Zitrin, R. S. Ellis +20
We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift 6.07 viewed through the cluster MACSJ0600.1-2008 (=0.46). A $\sim…
The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts
Jorge González-López, Mladen Novak, Roberto Decarli +19
We present the results from the 1.2 mm continuum image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS). The 1.2 mm continuum image has a s…
The ALMA Spectroscopic Survey in the HUDF: A model to explain observed 1.1 and 0.85 millimeter dust continuum number counts
Gergö Popping, Fabian Walter, Peter Behroozi +17
We present a new semi-empirical model for the dust continuum number counts of galaxies at 1.1 millimeter and 850 \micron. Our approach couples an observationally motivated model fo…
The ALMA Spectroscopic Survey in the HUDF: Constraining cumulative CO emission at with power spectrum analysis of ASPECS LP data from 84 to 115 GHz
Bade Uzgil, Chris Carilli, Adam Lidz +12
We present a power spectrum analysis of the ALMA Spectroscopic Survey Large Program (ASPECS LP) data from 84 to 115 GHz. These data predominantly probe small-scale fluctuations ($k…
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…
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…
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…
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…
ALMA resolves the molecular gas in a young low-metallicity starburst galaxy at z=1.7
Jorge González-López, L. Felipe Barrientos, M. D. Gladders +6
We present Atacama Large Millimeter/submillimeter Array observations of CO lines and dust continuum emission of the source RCSGA 032727--132609, a young low-metallicity sta…