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Enabling the next generation of cm-wavelength studies of high-redshift molecular gas with the SKA
J. Wagg, E. Da Cunha, C. L. Carilli +8
The Square Kilometre Array will be a revolutionary instrument for the study of gas in the distant Universe. SKA1 will have sufficient sensitivity to detect and image atomic 21 cm H…
COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS
L. Lentati, J. Wagg, C. L. Carilli +15
The broad spectral bandwidth at mm and cm-wavelengths provided by the recent upgrades to the Karl G. Jansky Very Large Array (VLA) has made it possible to conduct unbiased searches…
The evolution of the cold interstellar medium in galaxies following a starburst
K. Rowlands, V. Wild, N. Nesvadba +4
We present the evolution of dust and molecular gas properties in a sample of 11 starburst to post-starburst (PSB) galaxies selected to span an age sequence from ongoing…
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot +14
Interpreting observations of distant galaxies in terms of constraints on physical parameters - such as stellar mass, star-formation rate (SFR) and dust optical depth - requires spe…
The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared Spectroscopy
Michael V. Maseda, Arjen van der Wel, Hans-Walter Rix +21
We present near-infrared spectroscopy of a sample of 22 Extreme Emission Line Galaxies at redshifts 1.3 < z < 2.3, confirming that these are low-mass (M* = 10^8 - 10^9 M_sun) galax…
A Massive Galaxy in its Core Formation Phase Three Billion Years After the Big Bang
Erica Nelson, Pieter van Dokkum, Marijn Franx +13
Most massive galaxies are thought to have formed their dense stellar cores at early cosmic epochs. However, cores in their formation phase have not yet been observed. Previous stud…