Search results for "1510*"

showing 10 items of 80 documents

Fra kristen trosopplæring til pluralistisk religionsundervisning

2003

Tradisjonelt har religionsfaget stått sentralt i formidlingen av skolens kristne verdigrunnlag, men med KRL-faget er ikke dette lenger så selvsagt. På grunn av samfunnsutviklingen står både opplæringslovens kristne verdiforankring og skolens religionsundervisning i dag under debatt. I det følgende vil jeg se nærmere på den historiske utviklingen som har ført oss frem til dagens omdiskuterte religionsfag, kristendoms-, religions- og livssynskunnskap.

VDP::Humanities: 000::Theology and religious science: 150::Theology: 151VDP::Social science: 200::Education: 280::Subject didactics: 283
researchProduct

MORA, Albert (dir.); DE LUCAS, Javier; GONZÁLEZ, Mª Eugenia; SOLANES, Ángeles; VÁZQUEZ, Ana Isabel (2017): Informe jurídico-social sobre la situación…

2019

VÁZQUEZGONZÁLEZ1137-7038 8537 Arxius de sociologia 525290 2019 40 7038149 MORAMª Eugenia:SOCIOLOGÍA [UNESCO]Javier2017 Caturla BastitUniversitat de ValènciaSOLANESÁngelesInforme jurídico-social sobre la situación de las personas inmigrantes en la Comunitat Valenciana. Instituto de Derechos Humanos [Ana Isabel (2017)]DE LUCASUNESCO::SOCIOLOGÍAMª del Mar 151 154Ana Isabel (2017): Informe jurídico-social sobre la situación de las personas inmigrantes en la Comunitat Valenciana. Instituto de Derechos HumanosAlbert (dir.)
researchProduct

GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

2017

On August 14, 2017 at 10 30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of 1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5-3.0+5.7M and 25.3-4.2+2.8M (at the 90% credible level). The luminosity distance of the source is 540-210+130 Mpc, corresponding to a redshift of z=0.11-0.04+0.03. A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible regio…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyCredible regionsGeneral Physics and Astronomyadvanced ligoADVANCED LIGOAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationVIRGO detectorFilter signalsGW170814TOOLLIGOInterferometerGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)010303 astronomy & astrophysicsQCchoiceQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectstoolFalse alarm rateCHOICEAntenna responseGravitational-wave signalsDetector networks[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenagravitational radiation: polarizationSignal processingAstrophysics::High Energy Astrophysical Phenomenablack hole: binary: coalescenceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionGravitational-wave astronomy[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]General Relativity and Quantum CosmologyPhysics and Astronomy (all)Binary black hole0103 physical sciencesGW151226ddc:530KAGRASTFCGw150914GW170814 Virgo LIGO010308 nuclear & particles physicsGravitational wavePhysiqueVirgogravitational radiationAstronomyRCUKMatched filtersblack hole: massStarsLIGOgravitational radiation detectorBlack holeradiationVIRGOPhysics and AstronomyTesting Relativistic Gravitygravitationgravitational radiation: emissionStellar-mass black holesRADIATIONStellar black holeHigh Energy Physics::ExperimentAntennasDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Une mariophanie martiale à Dijon

2015

The ”delivrance de Dijon” in 1513 is an ambiguous event that mixes original procession, memorial procession, votive tapestry and historiographical interpretation. This paper studies, in this ”millefeuille”, the uses of martial miracle of the Virgin Mary in favor of Dijon inhabitants. What is the role of these invocation-purposed processions in the panic context of war and in the Marian piety of the Burgundian renaissance ? The Mariophany of the delivrance must not be interpreted in the light of negotiations between the city and the besiegers and a treaty that saves the city and its inhabitants, but sees Louis XII unhappy ? Finally, doesn’t divine intervention result from the power of the im…

[ SHS.HIST ] Humanities and Social Sciences/Historymariophanie[SHS.HIST] Humanities and Social Sciences/History1513culte des imagesNotre-Dame de Bon-Espoir[SHS.HIST]Humanities and Social Sciences/Historydélivrance de Dijon
researchProduct

Faire monument / Que faire du monument ? Une interrogation à propos de l'institution patrimoniale de deux villes lorraines

2015

Actes du colloque de Montréal, 16-18 avril 2012; International audience

[SHS.ANTHRO-SE] Humanities and Social Sciences/Social Anthropology and ethnologyUrbanisme[ SHS.ANTHRO-SE ] Humanities and Social Sciences/Social Anthropology and ethnologyProtection[SHS.SOCIO]Humanities and Social Sciences/Sociology[SHS.SOCIO] Humanities and Social Sciences/SociologyVilles[ SHS.SOCIO ] Humanities and Social Sciences/SociologyPatrimoine culturelHT151. S249.2015[SHS.ANTHRO-SE]Humanities and Social Sciences/Social Anthropology and ethnologyPériurbanisationAménagement du territoire
researchProduct

Hyvinvointi-, hius- ja kauneusalan ammatteihin opiskelevat kriittisinä nettilukijoina

2023

Tutkimuksessa selvitettiin ammatillisen koulutuksen opiskelijoiden (hyvinvointi-, hius- ja kauneusala) kriittistä nettilukutaitoa. Lisäksi tarkasteltiin aikaisemman tiedon, tekstien lukemisjärjestyksen ja perustelutaitojen yhteyttä siihen, kuinka hyvin opiskelijat osasivat arvioida luotettavia (varmentaminen) ja epäluotettavia (kyseenalaistaminen) nettitekstejä sekä erottaa luotettavat tekstit epäluotettavista. Tutkimukseen osallistui 82 opiskelijaa, joista valtaosa oli 15–18-vuotiaita. Opiskelijat lukivat ja arvioivat kaksi luotettavaa ja kaksi epäluotettavaa tekstiä sokerin vaikutuksista. Opiskelijat arvioivat kirjoittajan asiantuntijuutta, tarkoitusperiä, julkaisupaikkaa ja evidenssin la…

ammatillinen koulutustekstitaitoluotettavuus [http://www.yso.fi/onto/yso/p1629]medialukutaito [http://www.yso.fi/onto/yso/p14048]516 KasvatustieteetlähdekritiikkiGeneral Medicineinformaatiolukutaito [http://www.yso.fi/onto/yso/p15108]kriittinen lukutaitoverkkojulkaisutammatillinen koulutus [http://www.yso.fi/onto/yso/p9700]arviointi [http://www.yso.fi/onto/yso/p7413]informaatiolukutaitoammattikoululaisetArtikkelitmedialukutaito
researchProduct

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
researchProduct

"Figure 3" of "Nuclear modification of psi^prime, chi_c and J/psi production in d+Au collisions at sqrt(s_NN) = 200 GeV"

2023

The $\psi^{\prime}$ nuclear modification factor, $R_{dAu}$, as a function of $N_{coll}$. Also included is the previously measured $J/\psi$ $R_{dAu}$ as a function of $N_{coll}$.

ppg151nuclear modification$\psi^\prime$ suppressionmidrapidity200.0$d$ Au --> CHARGED X
researchProduct

"Figure 2" of "Nuclear modification of psi^prime, chi_c and J/psi production in d+Au collisions at sqrt(s_NN) = 200 GeV"

2023

The $\psi^{\prime}$, $\chi_c$, and $J/\psi$ $R_{dAu}$ for minimum bias centrality integrated $d$+Au collisions as a function of the quarkonia binding energy, where $J/\psi$ $R_{dAu}$ has been corrected for the effects of $\psi^{\prime}$ and $\chi_c$ feed-down.

ppg151nuclear modification$\psi^\prime$ suppressionmidrapidity200.0$d$ Au --> CHARGED X
researchProduct

"Figure 4" of "Nuclear modification of psi^prime, chi_c and J/psi production in d+Au collisions at sqrt(s_NN) = 200 GeV"

2023

The $\psi^{\prime}$ nuclear modification factor, $R_{dAu}$, as a function of proper time in nucleus. Also included is the previously measured $J/\psi$ $R_{dAu}$ as a function of $N_{coll}$.

ppg151nuclear modification$\psi^\prime$ suppressionmidrapidity200.0$d$ Au --> CHARGED X
researchProduct