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Fig. 1.

image

Different types of LLAGN in the Palomar Sample (197 sources, classification taken from in Ho et al. 1997). The red (filled with slanted lines) bins represent the new detections reported in this paper, while the cyan (vertical lines) bins represent the earlier observations reported in the literature (compiled in Nagar et al. 2005). The orange (crossed lines) bins depict the number of galaxies that were observed by us but not detected. Finally, the dotted region in green shows the number of galaxies yet to be observed with the highly sensitive VLA.

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