A kinetic formalism based on the Vlasov-Maxwell equations is used to investigate properties of the sideband instability for a tenuous, relativistic electron beam propagating through a constant-amplitude helical wiggler magnetic field (wavelength x0 = 2Tr/k 0 , and normalized amplitude aw = w /mc 2 ko). The analysis is carried out for perturbations about an equilibrium BGK state in which the distribution of beam electrons G s(y') and the wiggler magnetic field coexist in quasi-steady equilibrium with a finite-amplitude, circularly polarized, primary A 2 electromagnetic wave (w s,k s) with normalized amplitude as eB/mc ks. Particular emphasis is placed on calculating detailed properties of the sideband instability for the case where a uniform distribution of trapped electrons G (y') is localized near the bottom of the ponderomotive potential moving with velocity vp = os/(k s+k 0) relative to the laboratory frame. For harmonic numbers n > 2, it is found that stable (Imw = 0) sideband oscillations exist for [w-(k+k 0)v p 2 _ n2 Here, (w,k) are the perturbation frequency and wavenumber in the laboratory frame, 0B (aw a sc 2 k' 2/' 2 1 is the bounce frequency, j mc 2 is the maximum energy of the trapped electrons in the ponderomotive frame, and k' and y are defined by k' = (k +k 0)/ p and yP = (1-v /c2)-. On the other hand, for the fundamental (n = 1) mode, instability exists (Imw > 0) over a wide range of system «1ad «1whrr 3 = 2 (2222, parameters B/ck < 1 and r 0 << 1, where r0 = (a w/ 4)(pT/Yp k0)(1+vP/c)(c/vPM 3 and i pT = (47rhnTe /m)1 is the plasma frequency of the trapped electrons. Moreover, the maximum growth rate and bandwidth of the sideband instability for the fundamental (n = 1) mode exhibit a sensitive dependence on the normalized pump strength B /rOk0c.