ngVLA Update

By Erik Rosolowsky (U Alberta), Joan Wrobel (NRAO)
(Cassiopeia – Spring 2024)

ngVLA development is continuing apace with ongoing science plan and technology planning in Canada and other engaged nations including Germany, Japan, Mexico, and Taiwan. There are two upcoming conferences that could be of interest to the Canadian ngVLA community.

Follow the Monarchs: A Journey to Explore the Cosmos at (Sub)milliarcsecond Scales with the ngVLA

Conference poster for “Follow the Monarchs: A Journey to Explore the Cosmos at (Sub)milliarcsecond Scales with the ngVLA” (credit: IRyA/NRAO/AUI/NSF)

This ngVLA international science conference will be held November 11-14 in person in the UNESCO World Heritage site of Morelia, Mexico. The conference will highlight and explore the novel scientific opportunities that will unfold with the unprecedented angular resolution and sensitivity capabilities offered by this new flagship facility. The conference will coincide with the Monarch butterflies completing their migration journey from Canada and the US to the mountains surrounding Morelia. Registration and abstract submission will open on April 1.

A variety of oral presentations and posters will be featured, with a special focus on the new science that will be possible at high angular resolution. The ngVLA will allow, for the first time, the detection of thermal emission at 1 mas angular scales, as well as unprecedented high fidelity imaging of non-thermal emission on scales less than 1 mas. Researchers within and beyond radio astronomy expertise are invited to engage in discussions, share insights, and start to plan the groundbreaking science that the ngVLA will make possible. We particularly encourage the participation of early career scientists, who will be the major users of this observatory.

A Coherent View of Atomic and Molecular Gas from Infrared to Radio Wavelengths

This IAU Focus Meeting 2 will be held August 6-7 in person in Cape Town, South Africa. The meeting will explore how the work taking place at existing facilities is shaping our understanding of the interstellar medium structure and feedback in our own Milky Way and external galaxies, and how this work is re-framing the science that will be addressed by the remarkable capabilities of future radio observatories. Contributed speakers will be announced on April 8.

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