Although less than 1 percent of the baryonic mass budget of a galaxy, cosmic dust profoundly alters the multi-wavelength appearance of galaxies across cosmic time. The (sub)millimeter wavelength regime is uniquely capable of weighing these dust reservoirs, and revealing the total extent of galaxy evolution that remains...
H. Algera, T. Bakx, M. Aravena et al.· 0 citations
MOSAIC is the multi-object fibre spectrograph for ESO's 39-m Extremely Large Telescope (ELT). It offers unique capabilities for a gigantic telescope in terms of multiplexing, wavelength coverage and spectral resolution. MOSAIC covers the visible (0.39-0.95 microns) and NIR (0.95-1.8 microns) wavelength domains, with me...
R. Pelló, M. Puech, M. Rodrigues et al.· Astronomical Telescopes + In...· 10 citations
A comprehensive understanding of galaxy evolution requires a detailed analysis of gas and dust, their distribution, and evolution within galaxies. We analyse spatially resolved (~kpc) rest-frame [CII] and dust continuum ALMA observations together with JWST/NIRSpec IFU data of a sample of galaxies at z~4-5. We focus on...
F. López, M. Relaño, I. de Looze et al.· 0 citations
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