We present complete near infrared (0.85-2.45 μm), low-resolution (˜100) spectra of a sample of 26 disk L-dwarfs with reliable optical spectral type classification. The observations have been obtained with a prism-based optical element (the Amici device) that provides a complete spectrum of the source on the detector. Our observations show that low

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V and I images of the nearby dIrr galaxies Sextans A and Sextans B were searched for the clusters. The cadidates were selected, from a sample of non-stellar objects, on the basis of their morphology, their integrated colors and magnitudes. One of the candidates in Sextans A shows a few resolved stars whose location in the color-magnitude diagram

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