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dc.date.accessioned | 2019-01-22T20:50:35Z | |
dc.date.available | 2019-01-22T20:50:35Z | |
dc.date.issued | 2018 | |
dc.identifier.issn | 1860-7179 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/149061 | |
dc.description.abstract | © 2018 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim This is, to our knowledge, the most comprehensive analysis to date based on generative topographic mapping (GTM) of fragment-like chemical space (40 million molecules with no more than 17 heavy atoms, both from the theoretically enumerated GDB-17 and real-world PubChem/ChEMBL databases). The challenge was to prove that a robust map of fragment-like chemical space can actually be built, in spite of a limited (≪105) maximal number of compounds (“frame set”) usable for fitting the GTM manifold. An evolutionary map building strategy has been updated with a “coverage check” step, which discards manifolds failing to accommodate compounds outside the frame set. The evolved map has a good propensity to separate actives from inactives for more than 20 external structure–activity sets. It was proven to properly accommodate the entire collection of 40 m compounds. Next, it served as a library comparison tool to highlight biases of real-world molecules (PubChem and ChEMBL) versus the universe of all possible species represented by FDB-17, a fragment-like subset of GDB-17 containing 10 million molecules. Specific patterns, proper to some libraries and absent from others (diversity holes), were highlighted. | |
dc.relation.ispartofseries | ChemMedChem | |
dc.subject | computer chemistry | |
dc.subject | generative topographic mapping | |
dc.subject | library comparison | |
dc.subject | molecular diversity | |
dc.subject | structure analysis | |
dc.title | Mapping of the Available Chemical Space versus the Chemical Universe of Lead-Like Compounds | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 6 | |
dc.relation.ispartofseries-volume | 13 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 540 | |
dc.source.id | SCOPUS18607179-2018-13-6-SID85041137519 |