This is a deeper question than you may have intended. There is no unique way of defining what "now" is in the Universe (not even locally!) and hence there is no way of uniquely answering your question. Even if you do take a definition of now, you then have to define what you mean by such a thing as "the time since Big Bang". The time corresponding to an observer arriving to the "now" will generally depend both on your definition of "now" and the history of how the observer has moved.
With those caveats, in cosmology there are some standard assumptions. One of them is that the Universe is isotropic and homogeneous. This in itself actually singles out a particular definition of "now", namely the "now" that makes the Universe isotropic and homogeneous. It also singles out a particular type of observer, namely observers that actually observe the Universe as isotropic and homogeneous, e.g., do not move relative to the CMB. Such observers are called comoving observers because they do not move relative to the background. Now, when cosmologists talk about the "age of the Universe", what they are referring to is the time elapsed since the Big Bang that would be measured by a comoving observer. By definition, this time is the same everywhere in the same "now" (again, with the definition of "now" from above).