Science with a next-generation Very Large Array

By E. Murphy. 2019

187 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/71eb5c8577037882682a6c129b5cd12e839a4107

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. S. Andrews
2. T. Birnstiel
3. Zhaohuan Zhu
4. D. Wilner
5. C. Dullemond
6. Xue-Ning Bai
7. L. Ricci
8. Jane Huang

Citations in the corpus

• The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science Case and Survey Design (2019, background): “…curve of the event and, more importantly, will allow confirmation of the broad Spectral Energy Distribution (SED) of the radio transient (1–50 GHz), a capability unique to the VLA among radio instruments capable of synoptic surveys (at least until the construction of the ngVLA; Selina et al. 2018).”
• One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering (2019, background): “VLA, ngVLA (Murphy et al. 2018) or SKA (Testi et al. 2015) will be quite powerful in this regard, although these long wavelength observations will get significant contamination from free-free emission from the star or jet.”
• Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620 (2021, background): “…Detector (CHORD; Vanderlinde et al. 2019), 2000 dish Deep Synoptic Array (DSA-2000; Hallinan et al. 2019), and the next-generation Very Large Array (ngVLA; e.g., Chatterjee 2018)—will provide key opportunities in pulsar science with their heightened sensitivity and increased receiver bandwidths.”
• CASA, the Common Astronomy Software Applications for Radio Astronomy (2022, background): “…increase in data rates and volumes that are expected in the era of the next-generation radio telescopes, such as the next-generation VLA (ngVLA; Murphy et al. 2018) and ALMA wideband sensitivity upgrade (Brogan 2019), a next-generation of data processing software needs to be efficient and…”
• Radio Properties of Tidal Disruption Events (2020, unknown): “…at least 15 GHz.7 Radio observations with future facilities such as the SKA and the next generation VLA (ngVLA)8 are expected to produce larger samples of TDEs (hundreds per year) that are also more distant at higher redshifts (Metzger et al. 2015; Donnarumma et al. 2015; van Velzen et al. 2018).”