Search results for "observator"

showing 10 items of 410 documents

The performance of the ATHENA X-ray Integral Field Unit

2018

The X-ray Integral Field Unit (X-IFU) is a next generation microcalorimeter planned for launch onboard the Athena observatory. Operating a matrix of 3840 superconducting Transition Edge Sensors at 90 mK, it will provide unprecedented spectro-imaging capabilities (2.5 eV resolution, for a field of view of 5') in the soft X-ray band (0.2 up to 12 keV), enabling breakthrough science. The definition of the instrument evolved along the phase A study and we present here an overview of its predicted performances and their modeling, illustrating how the design of the X-IFU meets its top-level scientific requirements. This article notably covers the energy resolution, count-rate capability, quantum …

Field (physics)X-ray Integral Fiel UnitPhase (waves)Field of viewCondensed Matter Physicmicrocalorimeter01 natural sciencesX-rayMatrix (mathematics)Settore FIS/05 - Astronomia E AstrofisicaObservatory0103 physical sciencesAthenaAerospace engineeringElectrical and Electronic Engineering010306 general physicsPhysics010308 nuclear & particles physicsbusiness.industryElectronic Optical and Magnetic MaterialResolution (electron density)Computer Science Applications1707 Computer Vision and Pattern RecognitionApplied MathematicQuantum efficiencybusinessEnergy (signal processing)performance
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Simeizas teleskopa montāžas gaita Friča Blumbaha fotogrāfijās

2022

Latvijas Universitātes Muzeja F. Candera un Latvijas astronomijas kolekcijas krājumā atrodas latviešu astronoma un metrologa Friča Blumbaha (1864 – 1949) 23 uzņemtās fotoplates un 3 papīra fotogrāfijas, kas atspoguļo viņa līdzdalību Simeizas viena metra teleskopa tapšanā 1922. - 1925. gadā. Tajās redzams F. Blumbahs, teleskopa izgatavotājfirmas Grubb Telescope Company darbinieki un Krievijas pārstāvji, kas bija iesaistīti pasūtījuma veikšanā. Attēlos labi redzamas atsevišķas teleskopa daļas, galvenais spogulis un teleskopa kupols. Tekstā aprakstīta Simeizas teleskopa pasūtīšana, izgatavošana, izmantošana Simeizā un teleskopa bojāeja Otrā pasaules kara laikā.

Fricis Blumbahs:NATURAL SCIENCES::Physics::Astronomy and astrophysics::Astronomy [Research Subject Categories]TeleskopsSimeizas observatorijaAstronomija
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Zvaigžņotā Debess: 2012, Rudens (217)

2012

Saturs: P.Stučkas LVU ieguldījums astronomijas speciālistu sagatavošanā ; Starp "maldugunīm" un zvaigznēm ; A.Alksnis. Dawn kosmosa misija palīdz atklāt asteroīda Vesta noslēpumus ; D.Docenko. Komentārs: Par Higsa bozona atklāšanu ; I.P. Frīdriha Candera 125.dzimšanas dienai Krievijas Pasts izdevis marku ; P.Leckis. Mākoņu pārklātais pavadonis ; D.Kotlere, I.Šmelds. Kosmisko atlūzu novērojumi Ventspils Starptautiskajā radioastronomijas centrā ; Pirmo reizi “ZvD”: Dace Kotlere ; I.P. Divas dienas, godinot Jāni Ikaunieku (28.IV 1912.–27.IV 1969.) ; I.Pundure. Jāņa Ikaunieka devums Latvijas astronomijai ; N.Cimahoviča, Imants Vilks, R.Saveļjeva, T.Millers, A.Krastiņš. Atmiņas par Ikaunieku ; E…

Frīdriham Canderam – 125 (Pastmarkas)LVU astronomijas studenti – 1952. gada diplomandiSfērisks saules pulkstenis (Kocēni)Marss – nolaišanās bez izpletņiemKonkurss skolēniem OdysseusZvaigžņu tēma mākslā – dzeja un zīmējumiJānis IkaunieksLU Astronomiskā observatorija (vēsture):NATURAL SCIENCES::Physics::Astronomy and astrophysics [Research Subject Categories]Dawn misija – asteroīds VestaJauno zinātnieku EXPO 2012 Briselē – sarkano zvaigžņu pētījumiAstronomiskās parādības – 2012.gada rudenīFizikas docents Jānis Kariss (22.06.1927.-22.09.2011.)Higsa bozons – atklāšanaMagnusam Georgam Paukeram – 225Venēras pāriešana – novērojumi Rīgā Jūrmalā Carnikavā Ventspils novadāLatvijas 62. matemātikas olimpiāde – uzdevumiTitānsKosmiskās atlūzas – novērojumi Ventspils Starptautiskajā radioastronomijas centrā
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Zvaigžņotā Debess: 2012, Vasara (216)

2012

Contents: “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: E.Bervalds. From Intention to Reality (abridged) ; A.Egle. Conceptions of Our Ancestry About Heavenly Bodies and Astronomical Phenomena (abridged) ; NEWS: I.Eglītis. Asteroid Discovered at Baldone Observatory Named after Ikaunieks ; A.Alksnis. ALMA Helps to Study Planetary System of Star Fomalhaut ; A.Alksnis. More than Ten Light-Years Long Filament of Cosmic Dust Discovered ; A.Alksnis. Billions of Rocky Planets in the Milky Way ; SPACE RESEARCH and EXPLORATION: M.Sudārs. The Little Secret Space Shuttle Is Flying! ; M.Sudārs. Too Much Litter! Not in Rubbish Dump, but in the Space! ; “ENERĢIJA un PASAULE” VISITS “ZVAIGŽŅOTĀ DEBESS”: Talk with D…

Frīdriham Canderam – 125Asteroīds “Ikaunieks”Viesuļvētra Piena Ceļa binārajā sistēmā IGR J17091 – Čandras atradumsĢeologi par dzīvību uz Zemes – grāmataLVU astronomijas studenti – 1952.gada diplomandi (turpin.)Astronomiskās parādības – 2012.gada vasarāZvaigžņu mākonis LH 88 – Habla Paslēptie dārgumiSeminārs astronomijas skolotājiem7. debess vērotāju salidojums Suntažu observatorijāDalības saules pulksteņiJupitera konjunkcija ar Venēru martā“Enerģija un Pasaule” – “Zvaigžņotā Debess”Marss – slēptie ledājiPlanētu sistēma ap FomalhautuHermanim Ernstam Pflaumam – 150Molekulārais mākonis Vērša zvaigznājāKlinšainās planētas mūsu GalaktikāEzers “Džina krūka” Ziemeļkaukāzā – zemūdens ekspedīcijasZvaigžņu tēma mākslā – dzeja un zīmējumiAtkritumi kosmosā – problēmasLAB seminārs Ērgļa FīSpace Shuttle X-37BFiziķim Jurim Zaķim – 75Par Sauli pirms 100 gadiemDainis Draviņš par astronomiju"Mini planetārijs" Baldones observatorijā
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Zvaigžņotā Debess: 2011, Pavasaris (211)

2011

Contents: “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: A.Alksnis. XIV General Assembly of the International Astronomical Union (abridged) ; H.Strods. Jaunlaicene’s Watchmaker (abridged) ; I.Daube. At the Radioastrophysical Observatory of the Latvian Academy of Sciences (abridged). 50 YEARS SINCE GAGARIN’S SPACE FLIGHT: R.Misa. Dream about Cosmos ; A.Zalcmane. Konstantin Tsiolkovsky Astronautics Museum in Kaluga; E.Bērziņa. Outer Space in Pauls Stradins Museum of History of Medicine. NEWS: A.Alksnis. Different Faces of Whirpool Galaxy ; A.Alksnis. The Kleopatra’s Trio and other Minor Planets Groups. SPACE RESEARCH and EXPLORATION: V.Kalniņš. NASA Preparing Solar Probe Plus to Plunge into Sun's Atmos…

Gagarina kosmiskajam lidojumam – 50Konference “A New Space Policy for Europe”Ilgmārs EglītisStarmus – festivāls debess pētniecībai un mākslaiEižens ĀriņšStarptautiskie kosmiskie lidojumi – pastmarkasAleksandra BriedeTrīskāršais asteroīds (216) KleopatraMarsa polārais ledusSaules aptumsums - 2011.gada 4.janvāris RīgaVirpuļgalaktikas M51 attēliPiepūšamās laivas kosmosāAstronomiskās parādības - 2011Zaigai Kiperei – Artura Balklava balvaCiolkovska Kosmonautikas muzejs KalugāMikrometeorīti – vākšanaKonkurss „Mums pieder debesis 2011”NASA kosmiskais aparāts Stardust un Stardust-NExTLU fizikas docents Egons ZablovskisRīgas Politehnikumam – 150Latvijas atklātā fizikas olimpiādeDabas un vēstures kalendāram – 50Debess demonstrējumi Tokijas observatorijāKosmoss Paula Stradiņa Medicīnas vēstures muzejāNASA zonde Solar Probe PlusSeminārs „Ērgļa ipsilon” - Nereta
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Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

2021

Full list of authors: Abdalla, H.; Abe, H.; Acero, F.; Acharyya, A.; Adam, R.; Agudo, I; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Batista, R. Alves; Amati, L.; Amato, E.; Ambrosi, G.; Anguner, E. O.; Araudo, A.; Armstrong, T.; Arqueros, F.; Arrabito, L.; Asano, K.; Ascasibar, Y.; Ashley, M.; Backes, M.; Balazs, C.; Balbo, M.; Balmaverde, B.; Baquero Larriva, A.; Martins, V. Barbosa; Barkov, M.; Baroncelli, L.; de Almeida, U. Barres; Barrio, J. A.; Batista, P-, I; Becerra Gonzalez, J.; Becherini, Y.; Beck, G.; Tjus, J. Becker; Belmont, R.; Benbow, W.; Bernardini, E.; Berti, A.; Berton, M.; Bertucci, B.; Beshley, V; Bi, B.; Biasuzzi, B.; Biland, A.; Bissaldi, …

Gamma ray AstronomyCherenkov Telescope ArrayaxionsMATÉRIA ESCURAredshift: dependenceAstronomyGamma ray experimentsgamma ray experimentsAstrophysics01 natural sciencesCosmologyObservatorycosmological model: parameter spacegamma ray experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsCherenkov telescopes ; IACT technique ; Gamma rays ; Cosmic raysnew physics4. EducationSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma-ray astronomyviolation: Lorentz3. Good healthobservatoryExtragalactic background lightastro-ph.COaxion-like particlesFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsgamma ray: propagationCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusAxionsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsinvariance: Lorentzjet: relativisticdark matter: halo0103 physical sciencesactive galactic nuclei; gamma ray experiments; axions; extragalactic magnetic fieldsAGNBlazarbackground010308 nuclear & particles physicsFísicaAstronomy and AstrophysicssensitivityCherenkov Telescope Arrayaxionextragalactic magnetic fieldsactive galactic nuclei[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorptionstatisticalBlazarsTelescopes
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First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

2017

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the case of known pulsars a fully coherent search, based on matched filtering, which uses the position and rotational parameters obtained from electromagnetic observations, can be carried out. Matched filtering maximizes the signal-to-noise (SNR) ratio, but a large sensitivity loss is expected in case of even a very small mismatch between the assumed and the true signal parameters. For this reason, {\it narrow-band} analyses methods have been developed, allowing a fully coherent search for gravitational waves from known …

Gravitational-wave observatoryPhysics and Astronomy (miscellaneous)Astronomy01 natural sciencesrotationneutron starsGeneral Relativity and Quantum Cosmologygravitational waves; LIGO; stochastic gravitational-waveLIGOneutron star010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCpulsarQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gravitational Waves neutron stars advanced detectors narrow-band searchDetectorAmplitude[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaasymmetryCoherence (physics)young pulsarinterferometerneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)proper motionadvanced detectorsGravitational wavesPulsar0103 physical sciencesddc:530Gravitational Waves010308 nuclear & particles physicsGravitational wavegravitational radiation530 PhysikLIGOgravitational radiation detectorComputational physicscoherencedetector: sensitivityNeutron starelectromagneticPhysics and AstronomyGravitational waves; Pulsarnarrow-band searchDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]discovery
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The enhanced X-ray Timing and Polarimetry mission—eXTP

2019

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to det…

Gravity (chemistry)Computer sciencespace mission: eXTPX-ray timingPolarimetryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyPhysics and Astronomy (all)Settore FIS/05 - Astronomia E AstrofisicaObservatoryX-ray instrumentation0103 physical sciencesX-ray polarimetryGround segmentAerospace engineering010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)Spacecraftsezelebusiness.industryPayloadGravitational waveAstrophysics::Instrumentation and Methods for Astrophysicsspace mission: eXTP; X-ray instrumentation; X-ray polarimetry; X-ray timing; Physics and Astronomy (all)Space SciencebusinessAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron

2020

We present the detection of VHE gamma-ray emission above 100 TeV from HAWC J2227+610 with the HAWC observatory. Combining our observations with previously published results by VERITAS, we interpret the gamma-ray emission from HAWC J2227+610 as emission from protons with a lower limit in their cutoff energy of 800 TeV. The most likely source of the protons is the associated supernova remnant G106.3+2.7, making it a good candidate for a Galactic PeVatron. However, a purely leptonic origin of the observed emission cannot be excluded at this time.

HAWC - Abteilung HintonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Hydrogen compounds010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLower limitGalaxySpace and Planetary ScienceObservatory0103 physical sciencesSupernova remnantAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences
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Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube

2015

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere dataset consisting primarily of nu_e and nu_tau charged current and neutral current (cascade) neutrino interactions. In the analysis presented here, a data sample of approximately 35,000 muon neutrinos from the Northern sky was extracted from data taken during 659.5 days of livetime recorded between May 2010 and May 2012. While this sample is composed primarily of neutrinos produced by cosmic ray interactions in the Earth's atmosphere, the highest energy events are inconsistent with a hypothesis of …

HIGH-ENERGY NEUTRINOSFLUXESATMOSPHERIC MUONAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesIceCube Neutrino ObservatoryRATIO0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsSolar neutrino problemPhysics and AstronomyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena
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