{"id":808,"date":"2026-11-11T18:58:15","date_gmt":"2026-11-11T17:58:15","guid":{"rendered":"https:\/\/labvector.de\/?page_id=808"},"modified":"2026-11-11T19:10:46","modified_gmt":"2026-11-11T18:10:46","slug":"scientific-instrumentation","status":"publish","type":"page","link":"https:\/\/labvector.de\/de\/engineering-expertise\/scientific-instrumentation\/","title":{"rendered":"Scientific Instrumentation"},"content":{"rendered":"<p>[vc_row][vc_column][vc_column_text]<img src='https:\/\/labvector.de\/wp-content\/uploads\/2026\/11\/lv-photo-instrumentation.jpg' alt='Scientific Instrumentation' style='width:100%;height:auto;border-radius:12px'\/><\/p>\n<p style='font-size:1.15em;margin-top:24px'>We build instruments that measure what others cannot: weak signals, extreme temperatures and very fine positions.<\/p>\n<h2>What we do<\/h2>\n<ul>\n<li>Test and measurement stands for superconducting detectors, including tunnel-junction and SINIS bolometer arrays<\/li>\n<li>Photoresponse measurements of detector samples at 4.2 K and below<\/li>\n<li>Experimental setups for sub-millimetre and millimetre-wave detectors, with optical windows and waveguide inputs<\/li>\n<li>Thin-film process control, including thickness, structure and barrier-layer quality checks<\/li>\n<li>Magnetic-field measurement and calibration setups (see our <a href='\/engineering-expertise\/hall-probe-calibration-european-xfel\/'>XFEL project<\/a>)<\/li>\n<\/ul>\n<h2>Why it matters<\/h2>\n<p>Modern astrophysics and particle physics need detectors that combine high sensitivity, a wide dynamic range and fast response. We know these devices from the inside, so we design measurement setups that let you characterise them reliably and repeatably.<\/p>\n<p style='margin-top:32px'><strong>Have a project in mind? Tell us about it.<\/strong><\/p>\n<p><a href='\/contact\/' style='display:inline-block;padding:12px 24px;background:#0f2133;color:#fff;border-radius:6px;text-decoration:none'>Send a request<\/a><\/p>\n<p>[\/vc_column_text][\/vc_column][\/vc_row]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[vc_row][vc_column][vc_column_text] We build instruments that measure what others cannot: weak signals, extreme temperatures and very fine positions. What we do Test and measurement stands for superconducting detectors, including tunnel-junction and SINIS bolometer arrays Photoresponse measurements of detector samples at 4.2 K and below Experimental setups for sub-millimetre and millimetre-wave detectors, with optical windows and waveguide [&hellip;]<\/p>\n","protected":false},"author":3,"featured_media":0,"parent":807,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-808","page","type-page","status-publish","hentry"],"translation":{"provider":"WPGlobus","version":"3.0.6","language":"de","enabled_languages":["en","de"],"languages":{"en":{"title":true,"content":true,"excerpt":false},"de":{"title":false,"content":false,"excerpt":false}}},"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 5.0.5 - aioseo.com -->\n\t<meta name=\"description\" content=\"We build instruments that measure what others cannot: weak signals, extreme temperatures and very fine positions. 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