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Providing access to new assets and infrastructure, such as the Engineering Operations Centre and Science Operations Centre, is crucial for supporting the delivery and operation of the SKA MID telescope. The governance framework outlines key documents and obligations, including agreements with SKAO a

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The Einstein Telescope Collaboration has established internal rules and a Code of Conduct to ensure a professional, respectful, and inclusive environment free from discrimination and harassment. All members are expected to adhere to these guidelines to foster a supportive atmosphere for scientific d

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The history of microscopes dates back to the 11th century with the invention of the reading stone, leading to the creation of wearable eyeglasses in the 13th century. The first microscope was developed in the late 16th century by Zacharias Jansen, paving the way for the compound microscope and the t

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This presentation focuses on the design and implementation of a compensator system to reduce deleterious oscillations affecting observations from the Hubble Space Telescope. Utilizing MATLAB for frequency response analysis, the project aims to dampen oscillations occurring at distinct frequencies, e

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Challenge your knowledge of astronomy with these 10 questions from the SAASTA AstroQuiz 2018 Round 4. Test your understanding of telescopes, galaxies, planets, and more in this exciting quiz. Answer questions on various aspects of astronomy, from telescope construction in South Africa to planetary r

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Optical telescopes utilize lenses or mirrors to collect and focus light for imaging celestial objects. The lens-maker's formula is crucial for determining the focal length of lenses, considering factors like index of refraction and radii of curvature. Different lens configurations and materials help

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Delve into the world of observational science with the Einstein Telescope (ET). This comprehensive overview covers the involvement of Flanders researchers, gravitational wave sources, ET's detection capabilities, and its significant contributions to black hole and neutron star properties. Learn abou

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Explore the factors influencing astronomical visibility, such as telescope size, aperture, and light pollution. Learn about the visual systems affecting our ability to see in different lighting conditions and understand concepts like illuminance, luminance, and apparent magnitude in astronomy.

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Discover the challenges faced in radio astronomy due to noise, with the signal often indistinguishable from background noise. Learn about receiver sensitivity issues, minimizing thermal noise, and mitigating atmospheric effects to improve observation quality. Explore the essential elements of telesc

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Construction and setup guide for an optics spectrometer at Rayat Shikshan Sanstha's Veer Wajekar A.S.C. College, including details on the telescope, collimator, and prism table. Instructions cover aligning the telescope, setting up the collimator, and positioning the spectrometer table. Steps are pr

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In preparation for the LSST Commissioning Review in Tucson, the Camera Summit Reverification process led by Travis Lange, an I&T Engineer, involves re-assembling the camera and re-verifying requirements. The schedule, budget, risks, and hazards are outlined, including inherited risks from the I&T ph

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This document provides an overview of the high-level software components involved in the ATST Safety Review conducted on 26th January 2011. It includes details on the Telescope Software Control Systems, Observatory Software Control Systems, and Instrument Software Control Systems, along with respons

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Cutting-edge workflow system designed for effective planning, execution, and management of telescope data flows in astronomical observatories. The system includes modules for image acquisition, data processing, alert management, and real-time data analysis. It provides seamless integration and autom

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Delve into the beauty and mysteries of IC 5067, the Pelican Nebula, located in the Cygnus constellation. Discover its unique features, including emission nebula jets emitted by Herbig-Haro object 555. Follow the imaging process using a Meade LX200 telescope and ST-9XE camera. Uncover the challenges

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Harnessing the power of big data in astronomy, this presentation by Curt Dodds from the Institute for Astronomy at the University of Hawaii, Manoa, delves into the utilization of national cyberinfrastructure to advance artificial intelligence access and foster innovation in the field. The discussion

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The Advanced Virgo (AdV) project involves various activities related to squeezing technology, optical layouts, Faraday isolators, and electronics. The project includes components like the squeezer, clean room, detectors, telescopes, and alignment systems. The installation, commissioning, and status

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In June 2015, progress was reported on the Phased Array Feeds project, highlighting successful tests at the Green Bank Telescope (GBT). The collaboration included advancements in beamforming technology, backend bandwidth expansion, and instrumentation upgrades. Despite some discrepancies between mod

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Total tracks acquired, days of data taking, candidate tracks per day, performance metrics, and duty cycle information for the EEE telescope network up to Run 5, as reported by Fabrizio Coccetti at Centro Fermi Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi in Rome, Italy. The netw

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In the pursuit of sustainable development, the Einstein Telescope (ET) is focusing on minimizing its global carbon footprint. Maria Marsella leads the efforts to evaluate the environmental, societal, and landscape impacts of this strategy, aiming to implement valorization and mitigation actions. By

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PULSE@Parkes is a program where high school students collaborate with professional astronomers to conduct remote observations using the Parkes radio telescope. The program offers hands-on experiences, online modules, and data sessions for students in years 10-12. Students also have the opportunity t

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Fast Radio Bursts (FRBs) are millisecond-duration bursts of radio waves originating from outside our galaxy, offering researchers a unique opportunity to investigate baryon distributions and probe the cold gas clumps in the Universe. Scintillations in radio waves caused by irregularities in the inte

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The Einstein Telescope Collaboration Board Symposium 2022 in Budapest covers various agenda items including membership, elections, discussions on boards, and updating Bylaws. Special guests from ET Directorate and other collaborations are attending. The Collaboration Board is the governing body maki

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Delve into the world of mass, volume, and density as we prepare to launch a telescope into space. Discover the importance of understanding these concepts in selecting materials for space exploration and learn about measuring mass, volume, and density through engaging activities.

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Explore how to estimate the height of lunar mountains by measuring the length of their shadows on the Moon's surface using data from the Liverpool Telescope. Discover the intriguing world of lunar shadows and how they can reveal information about celestial features. See how similar triangles and geo

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Understanding the interfaces between the ET beam pipe and civil infrastructure is vital for successful project implementation. Luigi Scibile shares insights on the connections with roads, buildings, shafts, tunnels, and more at the 2nd Einstein Telescope Annual Meeting in Paris, November 2023. The p

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The report highlights the achievements and initiatives of the Southern African Large Telescope (SALT) project in 2013/14, including outreach statistics, successes with SALT partners, future programs, and suggestions. It covers various activities such as exhibitions, teacher training, robotic telesco

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This network consolidates funding and support for Europe's optical and infrared astronomy facilities, aiming to enhance infrastructure, train new astronomers, and develop cutting-edge technologies. It emphasizes collaboration among national and international agencies, optimizing access to mid-size t

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This lecture covers the concepts of radio telescope sensitivity in detecting small temperature variations from the sky, including factors such as radiometric sensitivity, antenna noise temperature, receiver system noise, and more. Additionally, it touches upon the resolution capabilities of radio te

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