521 citations · 11.4k across the 211 of their papers we have counts for
14 papers · 2 filters
Galaxy growth in a massive halo in the first billion years of cosmic history
D. P. Marrone, J. S. Spilker, C. C. Hayward +34
According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…
The ALMA Frontier Fields Survey - IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
A. M. Muñoz Arancibia, J. González-López, E. Ibar +15
[abridged] Characterizing the number counts of faint, dusty star-forming galaxies is currently a challenge even for deep, high-resolution observations in the FIR-to-mm regime. They…
Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang
E. F. Jiménez-Andrade, B. Magnelli, A. Karim +23
We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at . We secured CO molecular line detections for the and trans…
An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
Drew Brisbin, Oskari Miettinen, Manuel Aravena +28
We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N5 with an average continuum RMS of 150 Jy. These fiel…
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…
An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
Oskari Miettinen, Ivan Delvecchio, Vernesa Smolčić +25
We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of mm, and followed up at $λ_{\rm o…