activity
20172021
most citedA Lyman-α protocluster at redshift 6.9

70 citations · 127 across the 4 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021

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…

astro-ph.GA202170 cited

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…

astro-ph.GA2021

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…

astro-ph.GA202130 cited

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…

astro-ph.GA2020

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…

astro-ph.GA2020

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…