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Carilli, C.
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Search results
(1 - 24 of 26)
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CO survey of high-z radio galaxies, revisited with the Atacama Large Millimeter/submillimeter Array: jet-cloud alignments and synchrotron brightening by molecular gas in the circumgalactic environment
ALMA 200 pc imaging of a z ~ 7 quasar reveals a compact, disk-like host galaxy
The 700 ks Chandra Spiderweb Field
The 700 ks Chandra Spiderweb Field. I.
The impact of powerful jets on the far-infrared emission of an extreme radio quasar at z~6
The ALMA Spectroscopic Survey in the HUDF
Measuring the average molecular gas content of star-forming galaxies at z = 3-4
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO excitation and atomic carbon in star-forming galaxies at z = 1-3
The ALMA spectroscopic survey large program: the infrared excess of z = 1.5-10 UV-selected galaxies and the implied high-redshift star formation history
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: multiband constraints on line-luminosity functions and the cosmic density of molecular gas
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: constraining the molecular content at log(M*/M) 9.5 with CO stacking of MUSE-detected z >1.5 galaxies
The evolution of the baryons associated with galaxies averaged over cosmic time and space
The ALMA spectroscopic survey in the HUDF: deep 1.2 mm continuum number counts
The ALMA spectroscopic survey in the HUDF: the cosmic dust and gas mass densities in galaxies up to z ~ 3
The ALMA Spectroscopic Survey in the HUDF: the Molecular Gas Content of Galaxies and Tensions with IllustrisTNG and the Santa Cruz SAM
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies
The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources
The evolution of the cosmic molecular gas density
Cold Gas in High-z Galaxies: CO as Redshift Beacon
Cold Gas in High-z Galaxies: The Dense ISM
Cold Gas in High-z Galaxies: The Molecular Gas Budget
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies
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