Selective substrate-based inhibitors of mammalian dimethylarginine dimethylaminohydrolase

The enzyme DDAH metabolizes methylarginines that are inhibitors of nitric oxide synthase (NOS). Substrate-based inhibitors of mammalian DDAH have been synthesized, with optimization to give selective inhibition of DDAH with no significant direct effect on NOSs. These are the first examples of reversible DDAH inhibitors with significant activity and selectivity. In vivo administration increases plasma ADMA levels, giving proof of concept that these inhibitors can be used to probe the physiological effects of DDAH inhibition, with potential for pharmaceutical use of DDAH inhibitors in diseases where excess NO production is implicated

Copper (II) mediated arylation with aryl boronic acids for the N-derivatization of pyrazole libraries

Original article can be found at: http://pubs.acs.org/journal/jcchff Copyright American Chemical Society DOI: 10.1021/cc034065k [Full text of this article is not available in the UHRA]A N-derivatized 3-dimethylaminopropyloxypyrazole library was prepared using solution-phase parallel synthesis. The library was designed using physicochemical constraints designed to remove non-membrane-permeable molecules. Cupric acetate-mediated N-arylation with aryl boronic acids proceeded regioselectively to form the N-2-substituted derivatives. The presence of the 3-dimethylaminopropyloxy group was found to completely control the regioselectivity of the arylation. Presence of a dimethylaminoethyloxy or dimethylaminobutyloxy group gave a lesser degree of regioselectivity. The scope of the method as applied to library synthesis is discussed.Peer reviewe

Euclid. I. Overview of the Euclid mission

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance