Search results for "observator"

showing 10 items of 410 documents

A next generation Ultra-Fast Flash Observatory (UFFO-100) for IR/optical observations of the rise phase of gamma-ray bursts

2012

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes respond quickly, the number of sub-60 s detections remains small. In mid- to late-2013, the Ultra-Fast Flash Observatory-Pathfinder is to be launched on the Lomonosov spacecraft to investigate early optical GRB emission. This pathfinder mission is necessarily limited in sensitivity and event rate; here we discuss a next generation rapid-response space observatory. We list science topics motivating our instruments, those that require rapid optical-IR GRB response, including: A survey of GRB rise shapes/times, meas…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpacecraftbusiness.industryApertureAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsOrbital mechanicslaw.inventionTelescopeFlash (photography)ObservatorylawbusinessGamma-ray burstAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

2020

In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4$\pi$ steradian field of view and $\sim$99\% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, and to provide valuable insight for other observatories and inform their observing decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these follow up analyses and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analys…

High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysics010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsNeutrino astronomy; High energy astrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesIceCube Neutrino ObservatoryNeutrino astronomySpace and Planetary ScienceObservatory0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High energy astrophysics010303 astronomy & astrophysicsastro-ph.IM0105 earth and related environmental sciencesThe Astrophysical Journal
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LOFT - A large observatory for x-ray timing

2010

The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigations, such as those based on imaging and spectroscopy. Revealing strong gravitational field effects, measuring the mass and spin of black holes and the equation of state of ultradense matter are among the goals of such observations. At present prospects for future, non-focused X-ray timing experiments following the exciting age of RXTE/PCA are uncertain. Technological limitations are unavoidably faced in the conception and development of experiments with effective area of several square meters, as needed in order to…

High Energy Astrophysical Phenomena (astro-ph.HE)sezeleApplied MathematicsSilicon drift chambersFOS: Physical sciencesComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCompact sourcesCompact sources; High energy astrophysics; Silicon drift chambers; Timing; X-rays; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia E AstrofisicaX-raysElectronicTimingOptical and Magnetic MaterialsElectrical and Electronic EngineeringAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)Observatories X-rays Sensors Silicon Physics Polarimetry Electronics Imaging spectroscopyHigh energy astrophysics
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Cosmological waveguides for gravitational waves

1997

We study the linearized equations describing the propagation of gravitational waves through dust. In the leading order of the WKB approximation, dust behaves as a non-dispersive, non-dissipative medium. Taking advantage of these features, we explore the possibility that a gravitational wave from a distant source gets trapped by the gravitational field of a long filament of galaxies of the kind seen in the large scale structure of the Universe. Such a waveguiding effect may lead to a huge magnification of the radiation from distant sources, thus lowering the sensitivity required for a successful detection of gravitational waves by detectors like VIRGO, LIGO and LISA.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGravitational-wave observatoryGravitational waveSpeed of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational accelerationGeneral Relativity and Quantum CosmologyLIGOGravitational energyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldGravitational redshiftPhysical Review D
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Holographic in-situ measurements of the spatial droplet distribution in stratiform clouds

1998

Ground based in-situ measurements on the small-scale structure of low-level stratiform clouds have been performed utilizing the HOlographic Droplet and Aerosol Recording system (HODAR) of the University of Mainz, Germany. 6 holograms recorded during stratus cloud events on the Kleiner Feldberg Taunus Mountain Observatory (Frankfurt, Germany) were reconstructed in the laboratory and analysed by means of an automated data extraction and image processing system. In post-processing, each originally recorded droplet population was subjected to 2 statistical methods: (1) the sub-cell scanning analyses with statistical “Fishing” tests and (2) measurements of inter-droplet distance frequency distri…

In situAtmospheric Scienceeducation.field_of_study010504 meteorology & atmospheric sciencesMeteorologyPopulationHolographyImage processing010501 environmental sciences01 natural sciencesAerosollaw.inventionDistribution (mathematics)ObservatorylawFrequency distributioneducationGeology0105 earth and related environmental sciencesRemote sensingTellus B: Chemical and Physical Meteorology
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La experiencia docente del Observatorio de derechos humanos en la formación de juristas comprometidos

2021

[EN] The Human Rights Observatory is a pilot experience based on the teaching-learning methodology that allows, in an open, dynamic and participatory way. It monitors international current affairs and opens up a space for discussion and debate in the classroom on all those phenomena that, to a greater or lesser extent, condition International Law in the contemporary world. For this purpose, the Observatory will raise questions about issues of interest, highly topical subjects, complex problems, controversial processes and, above all, new approaches that encourage, not only through autonomous work but also through critical reflection, to deepen and complement the theoretical content of the d…

Innovación educativaInnovaciónEducación superiorHuman rightsDerechos humanosEnseñanza superiorTecnologías y educaciónObservatoryInnovationReflexión críticaCritical thinkingObservatorio
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Observatori Astronòmic

2008

Els misteris del cel estan més prop des de la fundació, fa ja un segle, de l'Observatori Astronòmic de la Universitat de València. Actualment, l'Observatori viu una etapa d'expansió. El seu personal desenvolupa diverses línies d'investigació, i al mateix temps realitza tasques de docència i divulgació de l'astronomia en la societat.

Investigació Astronomia Observatori Astronòmic
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The THESEUS space mission concept: science case, design and expected performances

2018

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing …

IonizationAtmospheric Sciencecosmological modelCherenkov Telescope Array[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyDark ageMASSIVE SINGLE STARSStar formation rates Gamma ray01 natural sciencesCosmology: observationlocalizationlaw.inventionAstrophysicEinstein Telescopeobservational cosmologylawObservational cosmologyRe-ionizationCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionizationLIGOobservations [Cosmology]Telescope010303 astronomy & astrophysicsHigh sensitivityHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMulti-wavelengthenergy: highsezelegamma-ray burstsCosmology: observationsCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionization; Aerospace Engineering; Space and Planetary ScienceAstrophysics::Instrumentation and Methods for Astrophysicsimagingstar: formationburst [Gamma-ray]observatoryGeophysicsDark agesX rays Cosmology: observationAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenasignatureStarTIDAL DISRUPTIONGamma-ray: burstAstrophysics::High Energy Astrophysical PhenomenaSIMILAR-TO 6Socio-culturaleFOS: Physical sciencesAerospace EngineeringGamma-ray: burstsobservation [Cosmology]galaxy: luminosityX-ray astronomy: instrumentation7 CANDIDATE GALAXIESAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burst114 Physical sciencesSettore FIS/03 - Fisica della MateriaTelescopeX-raybursts [Gamma-ray]FIS/05 - ASTRONOMIA E ASTROFISICASettore FIS/05 - Astronomia e AstrofisicaFirst star0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]KAGRAInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsFirst starsLIGHT CURVESEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and Astrophysics115 Astronomy Space scienceCherenkov Telescope ArrayredshiftsensitivityRedshiftNEUTRON-STAR MERGERmessengerVIRGOelectromagneticLUMINOSITY FUNCTIONSpace and Planetary ScienceBLACK-HOLEGeneral Earth and Planetary SciencesGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Zvaigžņotā Debess: 2017, Vasara (236)

2017

Contents: In MEMORIAM of ANDREJS ALKSNIS: Curriculum Vitae of Andrejs Alksnis (1928-2017) ; Condolences and Parting Words ; List of Publications by Professor Andrejs Alksnis ; “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: J.Francmanis. Enigma of Saturn’s Rings Brightness (abridged) ; E.Mūkins. Crater on Mercury Named After Rainis (abridged) ; Ā.Alksne. The Starry Sky in the Summer of 1977 (abridged) ; DEVELOPMENTS in SCIENCE: K.Schwartz. Early Universe Through the Eyes of Telescopes ; DISCOVERIES: K.Schwartz. Dwarf Galaxy Henize 2-10 with a Massive Black Hole ; J.Kuzmanis. Hot Topic – FRB 121102 ; SPACE RESEARCH and EXPLORATION: J.Kalvāns. Are Earth's Oceans of Interstellar Origin? ; J.Jaunbergs. ‘D…

Johanam Brocem – 275LU Astronomijas institūtam – 20Saturns – gredzenu sistēmaLatvijas 67.matemātikas olimpiāde – 3.posma uzdevumiPundurgalaktika Henize 2-10 masīvs melnais caurumsZvaigžņu nosaukumi – standartizācijaAstronomijas amatieru salidojums StarParty #17:NATURAL SCIENCES::Physics::Astronomy and astrophysics [Research Subject Categories]In memoriam Andrejs Alksnis (1928-2017) – dzīvesgaitas apraksts līdzjūtības atvadu vārdiTeleskopi – agrīnais VisumsHabla kosmiskais teleskops HST – HST 27.gadadienas attēlsMarsa visurgājējs Opportunity – intervija ar Dž.KallasuLielzeltiņu observatorijaLU Astronomijas institūts 2016Staņislavam Vasiļevskim – 110Debess spīdekļi – 2017.gada vasaraKosmiskā infrastruktūra – tendencesZemes okeāni – starpzvaigžņu izcelsmeZvaigžņotais visums grafikas mākslā – Dzidra EzergaileMīkla – mākslas darbsFrīdriham Canderam – 130A.Alkšņa zinātnisko darbu saraksts (1952-1980)FRB 121102 – milisekunžu radiostarojuma impulsi
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Zvaigžņotā Debess: 2008/09, Ziema

2008

Latvijas Zinātņu akadēmija, Latvijas Universitāte

Juris ŽagarsKrustvārdu mīklaNorises uz SaulesZiemeļvalstu-Baltijas vasaras skola 2008 (Lietuva Moletai)Mēness mobiļi – projekts ATHLETEKomisks fakts no NASA (radiomodemi bez garantijas)Visuma tēma filatēlijāLU fizikas profesors Fridrihs Treijs (1887-1965)VSRC sekmīgs eksperimentsBaldones observatorijas atklājums – asteroīds 2008 OS9Pasaules filosofijas kongress (22. kongress Seula)Astronomu jokiLU Astronomijas institūts - 10 gadiAleksandrs MičulisSpace Ship 2 un pasažieri kosmosāHeliobiologs Aleksandrs Čiževskis (1897-1964)Eiropas SWEETS autobuss RīgāZMP skaits un to iespējamās sadursmesESA/NASA Ulysses misija un Saules sistēmas vairogsKosmiskās difūzās plazmas spektroskopijaAntimatērijas dzinējsMarsa polārā ainavaAstronomiskās parādības - 2009Latvijas atklātā fizikas olimpiādeUNESCO un IAU Memorands par astronomisko pasaules mantojumuStarptautiskā matemātikas olimpiādeNestabilā dubultzvaigzne Kuģa Ķīļa EtaJurijs FrancmanisIndijas pilotējamo kosmisko misiju programmaJaunākie ieguvumi “Zvaigžņotās Debess” bibliotēkāPlanētu redzamības kompleksā diagramma 2009„Bēglis” B tipa milzis HD 271791Zvaigžņotā debess 2008./09. gada ziemāStarptautiskais Astronomijas gads - 2009Profesore Alla Masēviča (1918-2008)Daļējs Saules aptumsums - 2008.gada 1.augusts Saulkrasti
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