We experimentally demonstrate an all-diffractive optical setup for digital lensless holographic microscopy with easy wavelength line selection and micrometric resolution. In the proposed system, an ultrashort laser pulse is focused with a diffractive lens (DL) onto a pinhole of diameter close to its central wavelength to achieve a highly spatially coherent illumination cone as well as a spectral line with narrow width. To scan the complete spectrum of the light source the DL is displaced with respect to the pinhole plane. The proposed microscopy setup allows us to spectrally separate contributions from different sections of a sample, which may be attractive for several applications in life sciences. In this context, multispectral imaging has become a tool of increasing use, i.e., as a way to discriminate among several components (e.g., proteins or genes) or functions within the cell [9], or to enlarge the range of application of phase-based digital holographic techniques [10]. In DLHM multispectral illumination has been achieved not only with coherent sources like a tunable He-Ne laser [11] or a set of lasers that emit at different wavelength lines [12], but also with incoherent light-emitting diodes [8]. However, the above implementations allow only a discrete set of wavelength lines with full width at half-maximum (FWHM), typically on the order of some tens of nanometers. In contrast, it is well known that the ability to separate spectral contributions from multiple components of a sample depends largely on the number of images collected at different wavelength bands as well as on the width of these wavelength bands. In terms of the spectral image cube or lambda stack, it means that the finer the spectral slicing of the available broadband spectral source the better.In this Letter, we show an extremely compact and simple optical setup for all-diffractive multispectral DLHM with complete spectral tuning over the whole spectrum of the light source. The optical setup is based on the substitution of the microscopy objective given in most typical in-line DLHM geometries [1,12] by a kinoform DL. Here, it should be pointed out that a DL can be regarded as an optical element that focuses the light by diffraction. Its focal length Fλ varies inversely with the wavelength of the incident light as Fλ F 0 λ 0 ∕λ, where F 0 is the main focal length for the wavelength λ 0 . In our proposal, the pinhole that is placed at a given focal plane of the DL has a dual role. On one hand, it acts as a spatial filter of the light, removing higherorder aberrations and phase-front distortions, thus providing a secondary illuminating spherical wave. On the other hand, moving the DL with respect to the pinhole plane allows us to select very narrow wavelength bands within the spectrum of the incident light. The combination of a DL (or a Fresnel zone plate) with a small pinhole can be thought as a linear spectrometer whose resolving power R, for our experimental conditions (pinhole diameter not larger than the diameter of the Airy disc), can...