Here's one possible setup, involving "standard configuration" of a primed and unprimed frame:
In the primed frame, a spectrometer remains at rest at the origin while a light-source moving parallel to the ##x^\prime##-axis [edit: in the
negative ##x^\prime##-direction, as per standard configuration] briefly sends a monochromatic light wave directly toward the spectrometer. The unprimed frame is the light-source's rest frame.
The goal is to find an expression for the wavelength (and ultimately the frequency) of the light as measured in the primed frame. Steps:
- Use time dilation to express the wave's primed period in terms of its unprimed wavelength.
- Express the (primed) distance the light travels during the primed period in terms of the unprimed wavelength.
- Express the (primed) radial component of the light-source's displacement during the primed period in terms of the unprimed wavelength. (This will involve the cosine of the primed angle between the light's velocity vector and the positive ##x^\prime##-direction.)
- Sum the previous two results—that's your primed wavelength in terms of the unprimed wavelength and the aforementioned primed angle. You may also Lorentz-transform the primed angle to the
equivalent corresponding [edited] unprimed angle (aberration).