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We present a compilation of spectral energy distributions of 35 weak AGNs inLINERs using recent data from the published literature. We make use ofpreviously published compilations of data, after complementing and extendingthem with more recent data. The main improvement in the recent data is affordedby high-spatial resolution observations with the Chandra X-Ray Observatory andhigh-spatial resolution radio observations utilizing a number of facilities. Inaddition, a considerable number of objects have been observed with the HST inthe near-IR through near-UV bands since the earlier compilations werepublished. The data include upper limits resulting from either non-detectionsor observations at low spatial resolution that do not isolate the AGN. For thesake of completeness, we also compute and present a number of quantities fromthe data, such as alpha-ox, bolometric corrections, bolometric luminosities,Eddington ratios, and the average SED. We anticipate that these data will beuseful for a number of applications. In a companion paper, we use a subset ofthese data ourselves to assess the energy budgets of LINERs.

Spectral Energy Distributions of Weak Active Galactic Nuclei Associated With Low-Ionization Nuclear Emission Regions