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If the construction of the ngVLA begins in 2026, its sensitivity is expectedto match that of the VLA by late 2029. At that juncture it is anticipated thatopen-skies observing will cease on the VLA and commence on the ngVLA. Wesuggest that during 2026-2029 the VLA be held in a customized finalconfiguration encompassing portions of its standard A, B, C and Dconfigurations. Such a final VLA configuration would (1) help minimize the costof VLA operations and maximize the pace of ngVLA construction andcommissioning; (2) help VLA users pivot to the high-resolution, high-frequencyresearch topics that are projected to headline the ngVLA science program; and(3) help mitigate the effects of source confusion during responses totransients in the era of the Rubin Observatory and LIGO A+.

A Suggested Final Configuration for the Very Large Array