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A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density
F. Walter, R. Decarli, M. Sargent +19
We present direct constraints on the CO luminosity function at high redshift and the resulting cosmic evolution of the molecular gas density, (z), based on a blind mole…
A deep search for molecular gas in two massive Lyman break galaxies at z=3 and 4: vanishing CO-emission due to low metallicity?
Qinghua Tan, Emanuele Daddi, Mark T. Sargent +14
We present deep IRAM Plateau de Bure Interferometer (PdBI) observations, searching for CO-emission toward two massive, non-lensed Lyman break galaxies (LBGs) at z=3.216 and 4.058.…
The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared
Matthieu Béthermin, Lingyu Wang, Olivier Doré +5
[Abridged] Recent studies revealed a strong correlation between the star formation rate (SFR) and stellar mass of star-forming galaxies, the so-called star-forming main sequence. A…
Regularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate plane
Mark T. Sargent, E. Daddi, M. Béthermin +6
Star-forming galaxies (SFGs) display a continuous distribution of specific star formation rates (sSFR) which can be approximated by the superposition of two log-normal distribution…
On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observations
Elisabete da Cunha, Brent Groves, Fabian Walter +11
Modern (sub-)millimeter interferometers enable the measurement of the cool gas and dust emission of high-redshift galaxies (z>5). However, at these redshifts the cosmic microwave b…
Empirical predictions for (sub-)millimeter line and continuum deep fields
Elisabete da Cunha, Fabian Walter, Roberto Decarli +11
[abridged] Modern (sub-)millimeter/radio interferometers will enable us to measure the dust and molecular gas emission from galaxies that have luminosities lower than the Milky Way…