Search
Now showing items 1-3 of 3
GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
(2020-11-02)
In this paper, we extend the source detection in the GOODS-ALMA field (69 arcmin$^2$, rms sensitivity $\sigma$ $\simeq$ 0.18 mJy.beam$^{-1}$), to deeper levels than presented in Franco et al. (2018). Using positional ...
GOODS-ALMA: The slow downfall of star-formation in $z$ = 2-3 massive galaxies
(2020-11-01)
We investigate the properties of a sample of 35 galaxies, detected with ALMA at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin$^2$, resolution = 0.60", RMS $\simeq$ 0.18 mJy beam$^{-1}$). Using the UV-to-radio deep ...
GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
(2020-10-13)
Thanks to its outstanding angular resolution, the Atacama Large Millimeter/submillimeter Array (ALMA) has recently unambiguously identified a population of optically dark galaxies with redshifts greater than z = 3, which ...