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Next Generation Very Large Array Memo No. 6, Science Working Group 1: The Cradle of Life
Andrea Isella, Charles L. H. Hull, Arielle Moullet +33
This paper discusses compelling science cases for a future long-baseline interferometer operating at millimeter and centimeter wavelengths, like the proposed Next Generation Vary L…
Next Generation Very Large Array Memo No. 5: Science Working Groups -- Project Overview
C. L. Carilli, M. McKinnon, J. Ott +17
We summarize the design, capabilities, and some of the priority science goals of a next generation Very Large Array (ngVLA). The ngVLA is an interferometric array with 10x larger e…
Next Generation Very Large Array Memo No. 8 Science Working Group 3: Galaxy Assembly through Cosmic Time
Caitlin M. Casey, Jacqueline A. Hodge, Mark Lacy +14
The Next-Generation Very Large Array (ngVLA) will be critical for understanding how galaxies are built and evolve at the earliest epochs. The sensitivity and frequency coverage wil…
(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - II. The spatial extent of the radio-emitting regions
Oskari Miettinen, Mladen Novak, Vernesa Smolčić +9
Radio emission at cm wavelengths from highly star-forming galaxies, such as SMGs, is dominated by synchrotron radiation arising from supernova activity. Using deep, high-resolution…
Imaging the cold molecular gas in SDSS J1148 + 5251 at z = 6.4
Irina I. Stefan, Chris L. Carilli, Jeff Wagg +7
We present Karl G. Jansky Very Large Array (VLA) observations of the CO () line emission towards the quasar SDSS J (J$1148+5251…
Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies
Chris J. Willott, Chris L. Carilli, Jeff Wagg +1
We present Atacama Large Millimeter Array (ALMA) detections of atomic carbon line and dust continuum emission in two UV-luminous galaxies at redshift 6. The far-infrared (FIR) lumi…