Crinoids are the most common and diverse group of echinoderms in the Silurian of the British Isles. This guide describes examples of all nominal crinoid groups recognized from this interval and region (48 genera, about 100 species). In contrast, coronate, edrioasteroid, mitrate and cyclocystoid echinoderms are rare, the first three higher taxonomic groups being represented by a single species each, and the last by two species. Of 145 species of echinoderms in the Silurian of the British Isles, 74 are known from the Much Wenlock Limestone Formation of Wenlock age at Dudley in the West Midlands. For comparison, the most diverse faunas from the Llandovery Series (North Esk Inlier, Pentland Hills, Scotland) and Ludlow Series (Lower Leintwardine Formation, Leintwardine, Herefordshire) consist of only 16 and 17 species, respectively. If the echinoderm-rich succession at Dudley was unknown, the three older series of the Silurian, the Llandovery, Wenlock and Ludlow, would each include about 30 known species of echinoderm. It is the extreme diversity of the Much Wenlock Limestone Formation at Dudley that makes the echinoderm diversities of the Llandovery and Ludlow appear depauperate. (BMNH), but also in those of the British Geological Survey, Keyworth (BGS GSM), the James Mitchell Museum, University College Galway (JMM), the Geological Museum, University of Copenhagen (MGUH), the National Museum of Wales, Cardiff (NMW), and the Sedgwick Museum, Cambridge (SM). Individual taxa are illustrated in Figures 1-15. In order to keep the survey of crinoids to a manageable length, systematic descriptions are mainly at the hierarchical level of genus. This entails examination of 48 genera, including about 100 species (Donovan et al. 2008, tables 16.1-16.3). Where a taxon is monospecific in the study area, it is referred to under the specific epithet. Taxa are listed within the major groups of Palaeozoic crinoids (Simms & Sevastopulo 1993), that is, diplobathrid and monobathrid camerates, cladids, sagenocrinid and taxocrinid flexibles, and disparids. The descriptions are based on the personal observations of the authors, supported by Ramsbottom (1954), Moore & Teichert (1978), Widdison (2001a) and other references as indicated. Unless stated otherwise, columns are assumed to be holomeric.