The photoelectron emission time delay τ associated with one-photon absorption, which coincides with half the Wigner delay τ W experienced by an electron scattered off the ionic potential, is a fundamental descriptor of the photoelectric effect. Although it is hard to access directly from experiment, it is possible to infer it from the time delay of two-photon transitions, τ (2) , measured with attosecond pump-probe schemes, provided that the contribution of the probe stage can be factored out. In the absence of resonances, τ can be expressed as the energy derivative of the one-photon ionization amplitude phase, τ = ∂ E arg D Eg , and, to a good approximation, τ = τ (2) − τ cc , where τ cc is associated with the dipole transition between Coulomb functions. Here we show that, in the presence of a resonance, the correspondence between τ and ∂ E arg D Eg is lost. Furthermore, while τ (2) can still be written as the energy derivative of the two-photon ionization amplitude phase,Eg , it does not have any scattering counterpart. Indeed, τ (2) can be much larger than the lifetime of an intermediate resonance in the two-photon process or more negative than the lower bound imposed on scattering delays by causality. Finally, we show that τ (2) is controlled by the frequency of the probe pulse, ω IR , so that by varying ω IR , it is possible to radically alter the photoelectron group delay.