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- W2024080803 abstract "We predict the emission line luminosity functions (LFs) of the first 10 rotational transitions of 12C16O in galaxies at redshift z = 0 to z = 10. This prediction relies on a recently presented simulation of the molecular cold gas content in ∼3 × 107 evolving galaxies based on the Millennium Simulation. We combine this simulation with a model for the conversion between molecular mass and CO-line intensities, which incorporates the following mechanisms: (1) molecular gas is heated by the cosmic microwave background (CMB), starbursts (SBs), and active galactic nuclei (AGNs); (2) molecular clouds in dense or inclined galaxies can overlap; (3) compact gas can attain a smooth distribution in the densest part of disks; (4) CO luminosities scale with metallicity changes between galaxies; and (5) CO luminosities are always detected against the CMB. We analyze the relative importance of these effects and predict the cosmic evolution of the CO-LFs. The most notable conclusion is that the detection of regular galaxies (i.e., no AGN, no massive SB) at high z ≳ 7 in CO emission will be dramatically hindered by the weak contrast against the CMB, in contradiction to earlier claims that CMB heating will ease the detection of high-redshift CO. The full simulation of extragalactic CO lines and the predicted CO-LFs at any redshift can be accessed online (http://s-cubed.physics.ox.ac.uk/, go to S3-SAX) and they should be useful for the modeling of CO-line surveys with future telescopes, such as the Atacama Large Millimeter/submillimeter Array or the Square Kilometre Array." @default.
- W2024080803 created "2016-06-24" @default.
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- W2024080803 date "2009-08-20" @default.
- W2024080803 modified "2023-10-01" @default.
- W2024080803 title "A HEURISTIC PREDICTION OF THE COSMIC EVOLUTION OF THE CO-LUMINOSITY FUNCTIONS" @default.
- W2024080803 cites W1643121850 @default.
- W2024080803 cites W1954033364 @default.
- W2024080803 cites W1965359410 @default.
- W2024080803 cites W1967305001 @default.
- W2024080803 cites W1970038401 @default.
- W2024080803 cites W1971343676 @default.
- W2024080803 cites W1972155987 @default.
- W2024080803 cites W1973939397 @default.
- W2024080803 cites W1987836177 @default.
- W2024080803 cites W1988790306 @default.
- W2024080803 cites W1995286441 @default.
- W2024080803 cites W2001663399 @default.
- W2024080803 cites W2013759984 @default.
- W2024080803 cites W2013979799 @default.
- W2024080803 cites W2014170433 @default.
- W2024080803 cites W2015182320 @default.
- W2024080803 cites W2016723001 @default.
- W2024080803 cites W2020736183 @default.
- W2024080803 cites W2022651322 @default.
- W2024080803 cites W2022914110 @default.
- W2024080803 cites W2032205063 @default.
- W2024080803 cites W2040322225 @default.
- W2024080803 cites W2042240341 @default.
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- W2024080803 cites W2067857092 @default.
- W2024080803 cites W2074529843 @default.
- W2024080803 cites W2075478923 @default.
- W2024080803 cites W2075884494 @default.
- W2024080803 cites W2078583702 @default.
- W2024080803 cites W2080364106 @default.
- W2024080803 cites W2089078596 @default.
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- W2024080803 cites W2098914923 @default.
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- W2024080803 cites W2107833181 @default.
- W2024080803 cites W2109146631 @default.
- W2024080803 cites W2118265220 @default.
- W2024080803 cites W2124307094 @default.
- W2024080803 cites W2132646102 @default.
- W2024080803 cites W2138729205 @default.
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- W2024080803 cites W2170689655 @default.
- W2024080803 cites W2599301852 @default.
- W2024080803 cites W2996433497 @default.
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- W2024080803 cites W3099033475 @default.
- W2024080803 cites W3099415545 @default.
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- W2024080803 cites W3099564527 @default.
- W2024080803 cites W3099573144 @default.
- W2024080803 cites W3099686650 @default.
- W2024080803 cites W3100805745 @default.
- W2024080803 cites W3101004763 @default.
- W2024080803 cites W3101869526 @default.
- W2024080803 cites W3102225801 @default.
- W2024080803 cites W3102757339 @default.
- W2024080803 cites W3102937302 @default.
- W2024080803 cites W3103357491 @default.
- W2024080803 cites W3103471601 @default.
- W2024080803 cites W3126143209 @default.
- W2024080803 cites W34289084 @default.
- W2024080803 cites W4250001863 @default.
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- W2024080803 doi "https://doi.org/10.1088/0004-637x/702/2/1321" @default.
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