PPT-Very Long Baseline Interferometry

Very Long Baseline Interferometry Very Long Baseline Interferometry time   θ   t Very Long Baseline Interferometry Moving Sources             0             What is the signal made of. measurements: . One physicist’s crooked . path from quantum optics to quantum information. Introduction . Squeezed states and optical . interferometry. Ramsey . interferometry. and cat states. Quantum information perspective. Berlin/. Zeuthen. ;. . May 2010. Dainis Dravins & . Hannes. Jensen. Lund Observatory, Sweden. www.astro.lu.se. /~dainis. HUNDRED TIMES SHARPER THAN . HUBBLE !. Intensity Interferometry with. Steps 1 & 2: Identify & Select. Steps. Identify. . - . what digital content do you have? . Select - . what portion of that content will be preserved? . Store - . what issues are there for long term storage? . limits on . dark . energy. Jun. 17. 2011. Geena Kim. P. Hamilton, D. Schlippe, and H. Mueller. University of California, Berkeley. Paul Hamilton. Müller group. University of California at Berkeley. . Clare Burrage. University of Nottingham. Clare.Burrage@nottingham.ac.uk. Outline:. Chameleon dark energy. A . review of atom interferometry. Dark energy in the laboratory. Solutions to the Cosmological Constant Problem. [1]. ICHIKAWA . Ryuichi. , . [2]. ISHII . Atsutoshi. , . [3]. TAKIGUCHI Hiroshi, . KIMURA . Moritaka. , . [1]. SEKIDO Mamoru, . [1]. TAKEFUJI Kazuhiro,. [1]. UJIHARA Hideki, . [1]. HOBIGER Thomas, . [1]. Jonathan Singh . (. jonathan.singh@ed.ac.uk. ). A Curtis, I Main, A . Cartwright-Taylor, I . B . Butler, M Chapman, F . Fusseis. Outline. What is the Velocity?. CWI for Monitoring Velocity Change. Experimental Rock Physics Applications. Material for this talk: A.M.S. Richards, T.W.B.Muxlow, N.J.Jackson (JBCA Manchester); . R.A.Laing (ESO Garching); I. Marti-Vidal (OSO, Onsala); R. Perley (NRAO Socorro) and Wikipedia. Summary. Radio astronomy – key aspects. Dainis Dravins, . Hannes. Jensen . Lund Observatory, Sweden. Stephan LeBohec, Paul D.. . Nuñez. . The University of Utah, Salt Lake City. STELLAR INTENSITY INTERFEROMETRY. . Astrophysical targets for sub-. during the last decade. Olivier CHESNEAU. delivered and distorted by John . Monnier. 2. 3. Albert A. Michelson (1852-1931). 1974: I2T. 4. . MIDI . First direct recombination (2T) in the mid-IR (8-13. Harmonised Technical Guidance for eCTDSubmissions in the EU A baseline submission is a compiledsubmission of the current status of the dossier, i.e. resubmission CMDHBest Practice Guide he Use he Ele Achuta . Kadambi. , Jamie . Schiel. and Ramesh . Raskar. , IEEE CVPR16 . An interferometric 3D camera for multipath imaging for meter scale scenes. Swept Frequency Electronic Interferometry. Take-home message:. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics, Northwestern University. NPS Colloquium. February 1, 2019 . Conceptual overview of atom interferometry. Motivation for gravitational wave detection in the “mid-band” frequency range of ~ 0.1 Hz to 10 Hz. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics (CFP), Northwestern University. CPAD 2021. Brief overview of atom interferometry. Enabling technology advances for large-area/long-baseline atom interferometry demonstrated with 10-meter baselines.