Browsing by Author "Bacon, R."
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- ItemALMA spectroscopic survey in the Hubble Ultra Deep Field: Continuum number counts, resolved 1.2-mm extragalactic background, and properties of the faintest dusty star forming galaxies(2016) Bauer, Franz Erik; Aravena, M.; Decarli, R.; Walter, F.; Da Cunha, E.; Carilli, C.; Daddi, E.; Elbaz, D.; Ivison, R.; Riechers, D.; Smail, I.; Weiss, A.; Anguita, T.; Bell, E.; Bertoldi, F.; Bacon, R.
- ItemALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] line and dust emission in 6 < z < 8 galaxies(2016) Aravena, M.; Decarli, R.; Walter, F.; Bouwens, R.; Oesch, P.; Carilli, C.; Bauer, Franz Erik; Da Cunha, E.; Daddi, E.; González, J.; Ivison, R.; Riechers, D.; Smail, I.; Swinbank, A.; Weiss, A.; Anguita, T.; Bacon, R.
- ItemThe ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Constraining the Molecular Content at log (M-*/M-circle dot) ∼ 9.5 with CO Stacking of MUSE-detected z ∼ 1.5 Galaxies(2020) Inami, H.; Decarli, R.; Walter, F.; Weiss, A.; Carilli, C.; Aravena, M.; Boogaard, L.; González López, Jorge; Popping, G.; Bauer, Franz Erik; da Cunha, E.; Bacon, R.; Contini, T.; Cortes, P. C.; Cox, P.; Daddi, E.; Diaz Santos, T.; Kaasinen, M.; Riechers, D. A.; Wagg, J.; van der Werf, P.; Wisotzki, L.
- ItemThe Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) I. Characterisation of extended Lyman-alpha halos and spatial offsets(2022) Claeyssens, A.; Richard, J.; Blaizot, J.; Garel, T.; Kusakabe, H.; Bacon, R.; Bauer, F. E.; Guaita, L.; Jeanneau, A.; Lagattuta, D.; Leclercq, F.; Maseda, M.; Matthee, J.; Nanayakkara, T.; Pello, R.; Thai, T. T.; Tuan-Anh, P.; Verhamme, A.; Vitte, E.; Wisotzki, L.Aims. We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (-23 < M-UV < -14) lensed Lyman-alpha emitters (producing 959 images) with secure spectroscopic redshifts between 2.9 and 6.7. Combining the power of cluster magnification with 3D spectroscopic observations, we were able to reveal the resolved morphological properties of 268 Lyman-alpha emitters.