{"id":658,"date":"2024-05-25T11:10:08","date_gmt":"2024-05-25T11:10:08","guid":{"rendered":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/?p=658"},"modified":"2024-06-17T09:48:02","modified_gmt":"2024-06-17T09:48:02","slug":"research-assistant-associate-fellow-in-the-lisa-optical-bench-team-at-the-university-of-glasgow","status":"publish","type":"post","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/research-assistant-associate-fellow-in-the-lisa-optical-bench-team-at-the-university-of-glasgow\/","title":{"rendered":"Research Assistant\/ Associate\/ Fellow in the LISA Optical Bench Team at the University of Glasgow"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/my.corehr.com\/pls\/uogrecruit\/erq_jobspec_version_4.display_form\">(Link to Job-Ad)<\/a><\/p>\n\n\n\n<figure class=\"wp-block-table\"><table><tbody><tr><td colspan=\"4\">Research Assistant\/ Associate\/ Fellow<\/td><\/tr><tr><td colspan=\"4\"><strong>Job Purpose<\/strong>The post holder will join the LISA Optical Bench Team at the University of Glasgow.LISA is a European Space Agency (ESA) led mission to launch a gravitational detector in the mid 2030s. The mission has just been adopted by ESA as a flagship scientific mission in the next decade. The LISA instrument consist of 3 satellites in a triangular configuration with 2.5-million-kilometre arms, moving in an Earth-like orbit around the Sun. Gravitational waves from sources throughout the Universe will produce slight oscillations in the arm lengths (smaller than the diameter of an atom). LISA will capture these motions and thus measure the gravitational waves by using laser links to monitor the displacements of test masses free-falling inside the spacecraft. The LISA satellites and their scientific payload are being built by ESA, ESA member nations, and NASA.Each spacecraft carries 2 optical benches which are at the heart of the interferometry system. A joint team from the University of Glasgow and the UK Astronomy Technology Centre (ATC) in Edinburgh are responsible for developing and building these optical benches. The team is funded by the UK Space Agency (UKSA).The optical benches are built&nbsp; on Zerodur, a low expansion glass, with many optical components precision aligned and hydroxy-catalysis bonded to the optical bench base. As part of the optical bench build, a variety of sub-systems such as beam collimators, beam shaping, imaging systems and beam dumps have to be developed, tested and aligned on to the optical bench.You will be involved in the designing, building testing and documenting these systems and processes.Typical investigations might involve some combination of lasers, fibre optics, optical modulators, interferometers, precision manipulators, precision measurement, quadrant photodiodes, home-built electronics, optical beam profiling and data acquisition and control systems.A significant part of the process is liaising with the many different partners in the project \u2013 sub-system suppliers from multiple European countries, ESA, UKSA, ATC, NASA, etc.Please note that for this role, we must comply with a funder\u2019s\/partner\u2019s conditions, namely restrictions on exporting information covered by Export Administration Regulations (EAR). For this reason, there is a genuine occupational requirement that we are unable to consider applications at this time from nationals from countries excluded in the NS2 column in the country list&nbsp;<em>https:\/\/www.bis.doc.gov\/index.php\/documents\/regulations-docs\/2383-supplement-no-1-to-part-738\/file<\/em><\/td><\/tr><\/tbody><\/table><\/figure>\n","protected":false},"excerpt":{"rendered":"<p>(Link to Job-Ad) Research Assistant\/ Associate\/ Fellow Job PurposeThe post holder will join the LISA Optical Bench Team at the University of Glasgow.LISA is a European Space Agency (ESA) led mission to launch a gravitational detector in the mid 2030s. The mission has just been adopted by ESA as a flagship scientific mission in the [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":659,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_monsterinsights_skip_tracking":false,"advanced_seo_description":"","jetpack_seo_html_title":"","jetpack_seo_noindex":false,"jetpack_seo_schema_type":"","_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"_jetpack_feature_clip_id":0,"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_publicize_message":"","jetpack_publicize_feature_enabled":true,"jetpack_social_post_already_shared":false,"jetpack_social_options":{"image_generator_settings":{"template":"highway","default_image_id":0,"font":"","enabled":false},"version":2},"jetpack_post_was_ever_published":false},"categories":[79],"tags":[],"class_list":["post-658","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-employment-opportunities"],"jetpack_publicize_connections":[],"jetpack_featured_media_url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/05\/Unknown.png","jetpack-related-posts":[{"id":945,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/keynote-talk-by-mark-kasevich\/","url_meta":{"origin":658,"position":0},"title":"De Broglie waves and Gravitation","author":"wvk_3vn943","date":"August 21, 2024","format":false,"excerpt":"How do de Broglie waves propagate in gravitational fields?\u00a0 We will present experiments which show that 1) they obey the weak Equivalence Principle to 12 digits in uniform gravitational fields and 2) they exhibit Aharonov-Bohm type phase shifts in suitably non-uniform gravitational fields.\u00a0 In the later experiments, observed phase shifts\u2026","rel":"","context":"In &quot;Keynote Talk&quot;","block_context":{"text":"Keynote Talk","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/conference\/talks\/keynote-talk\/"},"img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":1578,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/philipp-treutlein\/","url_meta":{"origin":658,"position":1},"title":"Philipp Treutlein","author":"wvk_3vn943","date":"August 23, 2024","format":false,"excerpt":"Professor at the University of BaselHead of the Quantum Optics Group Short Biography Philipp Treutlein, born in Reutlingen in 1976, studied physics at the Universities of Konstanz and Stanford in 1996-2002. At Stanford, he worked in the laboratory of Steven Chu on laser cooling and atom interferometry. Back in Konstanz,\u2026","rel":"","context":"In &quot;Invited Speaker&quot;","block_context":{"text":"Invited Speaker","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/conference\/speakers\/invited-speaker\/"},"img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":1100,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/the-past-present-and-future-of-ground-based-laser-interferometric-gravitational-wave-detection\/","url_meta":{"origin":658,"position":2},"title":"The past, present, and future of ground-based laser-interferometric gravitational wave detection","author":"wvk_3vn943","date":"July 31, 2024","format":false,"excerpt":"Mich\u00e8le Heurs Abstract Since the first direct detection of gravitational waves in 2015, we have gained an entirely new observation window to the universe \u2013 now, we not only have electromagnetic telescopes and neutrino detectors to view astrophysical events, but we can also\u00a0listen\u00a0to the cosmos using interferometric gravitational wave detectors\u2026","rel":"","context":"In &quot;Conference Videos&quot;","block_context":{"text":"Conference Videos","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/conference\/presentation-videos\/"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Michele-Heurs-.png?resize=350%2C200&ssl=1","width":350,"height":200,"srcset":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Michele-Heurs-.png?resize=350%2C200&ssl=1 1x, https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Michele-Heurs-.png?resize=525%2C300&ssl=1 1.5x, https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Michele-Heurs-.png?resize=700%2C400&ssl=1 2x"},"classes":[]},{"id":1114,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/grigorios-tsagkatakis\/","url_meta":{"origin":658,"position":3},"title":"Grigorios Tsagkatakis","author":"wvk_3vn943","date":"August 2, 2024","format":false,"excerpt":"Assistant Professor at the Computer Science Department (CSD) of the University of Crete.\u00a0 Associate researcher at the Signal Processing Lab (SPL) of the Institute of Computer Science (ICS), Foundation for Research and Technology Hellas (FORTH).","rel":"","context":"In &quot;Summer School Lecturers&quot;","block_context":{"text":"Summer School Lecturers","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/summer-school\/lecturer\/"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/08\/Grigorios-Tsagkatakis.jpg?resize=350%2C200&ssl=1","width":350,"height":200,"srcset":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/08\/Grigorios-Tsagkatakis.jpg?resize=350%2C200&ssl=1 1x, https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/08\/Grigorios-Tsagkatakis.jpg?resize=525%2C300&ssl=1 1.5x"},"classes":[]},{"id":860,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/carioqa-pmp-towards-a-pathfinder-mission-for-quantum-space-gravimetry\/","url_meta":{"origin":658,"position":4},"title":"CARIOQA-PMP: Towards a Pathfinder Mission for Quantum Space Gravimetry","author":"wvk_3vn943","date":"June 24, 2024","format":false,"excerpt":"Centre National d\u2019Etudes Spatiales, 18 avenue Edouard Belin, 31400 Toulouse, France *for CARIOQA-PMP Consortium The impact of climate change is one of the most severe challenges of the 21st century. It is therefore of high importance to understand the underlying processes and causalities. A powerful tool to gain this vital\u2026","rel":"","context":"In &quot;Invited Talk&quot;","block_context":{"text":"Invited Talk","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/conference\/talks\/invited-talk\/"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/06\/Logo-CARIOQA-PMP.jpg?resize=350%2C200&ssl=1","width":350,"height":200},"classes":[]},{"id":1386,"url":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/magis-100\/","url_meta":{"origin":658,"position":5},"title":"Clock Atom Interferometry for Long-Baseline Atomic Sensors","author":"wvk_3vn943","date":"July 1, 2024","format":false,"excerpt":"Clock atom interferometry makes use of narrow optical clock transitions to metastable excited states are the foundation for the world\u2019s best atomic clocks. Such transitions naturally occur in fermions but are generally strongly forbidden in bosons. We compare and contrast several types of clock atom interferometers and explore their suitability\u2026","rel":"","context":"In &quot;Conference Videos&quot;","block_context":{"text":"Conference Videos","link":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/category\/conference\/presentation-videos\/"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Rudolph-Jan.png?resize=350%2C200&ssl=1","width":350,"height":200,"srcset":"https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Rudolph-Jan.png?resize=350%2C200&ssl=1 1x, https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Rudolph-Jan.png?resize=525%2C300&ssl=1 1.5x, https:\/\/i0.wp.com\/www.matterwaveoptics.eu\/FOMO2024\/wp-content\/uploads\/2024\/07\/Rudolph-Jan.png?resize=700%2C400&ssl=1 2x"},"classes":[]}],"jetpack_sharing_enabled":true,"_links":{"self":[{"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/posts\/658","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/comments?post=658"}],"version-history":[{"count":1,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/posts\/658\/revisions"}],"predecessor-version":[{"id":660,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/posts\/658\/revisions\/660"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/media\/659"}],"wp:attachment":[{"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/media?parent=658"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/categories?post=658"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.matterwaveoptics.eu\/FOMO2024\/wp-json\/wp\/v2\/tags?post=658"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}