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UK Astronomy Technology Centre

1998 establishments in Scotland1998 establishments in the United KingdomAstronomy in the United KingdomAstronomy institutes and departmentsResearch institutes established in 1998
Research institutes in EdinburghScience and Technology Facilities CouncilUse British English from August 2017

The UK Astronomy Technology Centre (UK ATC) is based at the Royal Observatory in Edinburgh, Scotland, and is part of the Science and Technology Facilities Council. The UK ATC designs, builds, develops, tests and manages major instrumentation projects in support of UK and international Astronomy. It has design offices, workshops and test facilities for both ground- and space-based instruments, including a suite of test labs capable of handling the largest current and projected instruments.The UK ATC was formed in 1998 in Edinburgh from the technology departments of the Royal Observatory, Edinburgh (ROE), and the Royal Greenwich Observatory, Cambridge (RGO). Its initial "customers" were the then new Gemini Observatory, the former ROE observatories in Hawaii (the James Clerk Maxwell Telescope (JCMT) and the United Kingdom Infrared Telescope (UKIRT)), and a former RGO observatory, the Isaac Newton Group on La Palma, Canary Islands. More recently, collaboration with the European Southern Observatory (ESO) and for the James Webb Space Telescope (JWST) have gained importance. Major projects and collaborations include: Several first-generation instruments for the Gemini Observatory. A mid-infrared spectrometer for the UKIRT and the Gemini Observatory. Data acquisition and reduction software for the UKIRT and the JCMT. The Wide Field Infrared Camera for the UKIRT. The Spectral and Photometric Imaging Receiver of the Herschel Space Observatory. The Visible and Infrared Survey Telescope for UK universities and ESO. A high-sensitivity, wide-field, sub-millimetre camera for the JCMT (SCUBA2). The MIRI (Mid-Infrared Instrument) for the JWST. Observing tool software for the Atacama Large Millimeter Array. Design studies for ESO's European Extremely Large Telescope. An infrared K-band multi-object spectrometer for ESO's Very Large Telescope. The European Union funded Optical Infrared Coordination Network for Astronomy (OPTICON).Following increased government emphasis on knowledge transfer and declining funds for the Science and Technology Facilities Council the UK ATC is increasingly working on projects with astronomical institutions beyond the UK and the EU, with institutions dedicated to science and technology other than astronomy, and with technology-related businesses.

Excerpt from the Wikipedia article UK Astronomy Technology Centre (License: CC BY-SA 3.0, Authors).

UK Astronomy Technology Centre
Observatory Road, City of Edinburgh Blackford

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Wikipedia: UK Astronomy Technology CentreContinue reading on Wikipedia

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N 55.923055555556 ° E -3.1877777777778 °
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Royal Observatory, Edinburgh

Observatory Road
EH9 3HJ City of Edinburgh, Blackford
Scotland, United Kingdom
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roe.ac.uk

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SIRCAMS

The Scottish Instrumentation and Research Centre for Advanced Mass Spectrometry (SIRCAMS) is a facility for ultra-high resolution mass spectrometry of biomolecules. SIRCAMS is based in the University of Edinburgh School of Chemistry.Much of the research activity is focused toward the development and application of mass spectrometry for the analysis of intact peptides, proteins, protein–protein, and protein–RNA/DNA complexes. Recent studies have included: identification of platination sites in peptides (bombesin, substance P, angiotensin, bradykinin) using Infrared multiphoton dissociation (IRMPD), Collision-induced dissociation (CID) and Electron-capture dissociation (ECD), accurate mass measurements on intact proteins (YdaE 6.5kDa, ubiquitin 8.6kDa, trypsinogen 24kDa, carbonic anhydrase 28kDa, beSOD 31kDa, FbpA 33kDa, BSA 66kDa) under native and denaturing conditions, identification of dynamic post-translational modifications in intact human histones using top-down ECD, top-down identification of proteins from complex mixtures, as well as accurate mass analysis of oligonucleotide DNA strands (40 bp). The capital cost of FTICR instruments operating at field strengths higher than 9.4 T are such that few University institutions worldwide can offer access. SIRCAMS offers user access to a 12T Bruker SolariX FTICR mass spectrometer within the facility. By taking advantage of the research expertise that has been developed by staff within the facility, users have access to techniques for accurate mass measurement of intact proteins with isotope peak fitting, top-down protein sequencing from complex mixtures (such as biomarker identification) solution and gas-phase HDX for protein conformational studies, mapping of post-translational modifications in peptides and proteins, and identification of DNA modifications.

Jordan Burn
Jordan Burn

The Jordan Burn, is the name of a stream, now culverted for much of its course, that runs through the Victorian suburb of Morningside in Edinburgh, Scotland, and was until 1856 the southern boundary of the city and county. It is a tributary of the Braid Burn. The Jordan first appears so named on the Roy map of Edinburgh (1753) "in obvious allusion to its position between 'Egypt' and 'Canaan'" (see below). It was originally called the Pow Burn when the Wester Burgh Muir, the area that became Morningside, was first feued by the Edinburgh magistrates in 1586. It was also popularly known in the past as the "Braid Burn", because it marked the northern boundary of the Braid Estate, but should not to be confused with its namesake above which takes a more southerly course. The Jordan rises on Craighouse Hill, then runs eastwards under Myreside Road and along the southern edge of the Royal Edinburgh Hospital grounds, where it is fed by the Comiston Burn from South Morningside, to the end of Maxwell Street. It then flows under Morningside Road between the south side of Jordan Lane and north side of Nile Grove, continuing from there under Woodburn Terrace and through the grounds of the Astley Ainslie Hospital, where it surfaces briefly. It then continues through Blackford until it reaches Mayfield, at which point it becomes known by its old name, the Pow Burn. After leaving Newington, it joins the Braid Burn at Peffermill, where it turns in a north-easterly direction. At Duddingston Mills the name changes again, this time to the Figgate Burn which enters the Firth of Forth at Portobello, having travelled a total distance of approximately ten miles.The name is one of a cluster of biblical names for lands and houses in the Morningside area. These include 'Eden', 'Paradise', 'Jordan', 'Nile', 'Salem', 'Bethel', 'Hebron', 'Goshen', and 'Zion Mount'. They seem connected in origin with a farm called 'Egypt' which stood just south of the burn where present-day Nile Grove and Woodburn Terrace meet. The farm buildings were demolished in the 1890s when the city expanded southwards on the slope of the former Burgh Muir. The farm is first mentioned in the city's Burgh Records of 1585 where it is referred to as "Littill Egypt". Since the leaders of Britain's gypsy communities often styled themselves Kings of 'Little Egypt', it has been surmised that the name indicates a gypsy presence on the muir in the 16th century when "Egyptianis" are mentioned in several official documents from the reign of James V. The lands lying immediately north of the farm, beyond the Jordan Burn, are described as "Canaan", in the Burgh Records of 1661, suggesting the initial spread of names with biblical associations. These appear to have proliferated in the Victorian period, being very likely added by Bible-conscious residents of the expanding suburb of Morningside who wished to perpetuate the tradition; so much so that it contributed to the district's reputation of being the city's "Bible Belt".As late as the mid-1960s, the author of a survey of Edinburgh wrote of the community in Morningside that, ...respect is due to this disciplined if stolid army of South Edinburgh, repairing each week in satins and 'stands' of Sabbath broadcloth to its respective persuasions at 'Holy Corner', (Churchhill) and similar ecclesiastical meccas, and in the pleasant Sunday afternoons making pilgrimages to the large, airy, orderly and flowery cemeteries of Grange, Morningside and Newington. This society sent many of its sons and daughters to settle in New Zealand (among other regions) and to graft the names and cultures of home into places like Dunedin. Its influence has been truly world-wide. So, if an Empire has been lost, this cannot be laid at Morningside's door. Moreover, the influence of its missionary zeal upon the benighted heathen has probably been greater than that of any comparable area on earth.