  We present the first orbit-integrated self force effects for an IMRI or EMRI
source, specifically the effects of its conservative piece on the orbit and on
the waveform. We consider the quasi-circular motion of a particle in the
spacetime of a Schwarzschild black hole, find the orbit and the corresponding
gravitational waveform, and discuss the importance of the conservative piece of
the self force in detection and parameter estimation. We also show the effect
of the conservative piece of the self force on gauge invariant quantities,
specifically $u^t$ as a function of the angular frequency $\Omega$. For long
templates the inclusion of the conservative piece is crucial for
gravitational-wave astronomy, yet may be ignored for short templates with
little effect on detection rate.
