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Narrow-band surveys for very high redshift Lyman-alpha emitters
(EDP SCIENCES S A, 2007)
Context. Many current and future surveys aim to detect the highest redshift ( z greater than or similar to 7) sources through their Lyman-alpha (Ly alpha) emission, using the narrow- band imaging method. However, to date ...
AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale Structure
(Monthly Notices of the Royal Astronomical Society, 2012)
VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
(Oxford University Press, 2017)
We present an extragalactic survey using observations from the Atacama Large Millimeter/ submillimeter Array (ALMA) to characterize galaxy populations up to z = 0.35: the Valparaiso ALMA Line Emission Survey (VALES). We ...
The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]–SFR relation over the last 13 Gyr
(European Southern Observatory, 2020)
The [C ii] 158 m line is one of the strongest IR emission lines, which has been shown to trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z 2. Whether this is also the case at higher ...
The ALPINE-ALMA [CII] Survey: A Triple Merger at z ~ 4.56
(Royal Astronomical Society, 2020)
We report the detection of [C II] λ158 μm emission from a system of three closely separated sources in the Cosmic Evolution Survey (COSMOS) field at z ∼ 4.56 , as part of the Atacama Large Millimeter/submillimeter Array ...
ON THE NATURE OF THE FIRST GALAXIES SELECTED AT 350 mu m
(IOP PUBLISHING LTD, 2009)
We present constraints on the nature of the first galaxies selected at 350 mu m. The sample includes galaxies discovered in the deepest blank-field survey at 350 mu m (in the Bootes Deep Field) and also later serendipitous ...
On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
(Wiley-blackwell Publishing, Inc, 2013-11)
A population of galaxies is simulated in a cosmological box in order to analyse generic trends for the stellar, baryonic and halo mass assembly of low-mass galax- ies (M∗ 3 × 1010M⊙) as a function of their present halo ...