Search results for " observations"

showing 10 items of 100 documents

GRB 030227: The first multiwavelength afterglow of an INTEGRAL GRB

2003

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R~23). This OA was seen to decline following a power law decay with index Alpha_R= -0.95 +/- 0.16. The spectral index Beta_opt/NIR yielded -1.25 +/- 0.14. These values may be explained by a relativistic expansion of a fireball (with p = 2.0) in the cooling regime. We also find evidence for inverse Compton scattering in X-rays.

PhysicsSpectral indexBurstsAstrophysics (astro-ph)Gamma raysCompton scatteringbursts [gamma rays]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGamma rays ; Bursts ; Photometric ; Cosmology observationsPhotometricUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsCosmology observationsPower law:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]observations [cosmology]Afterglowphotometric [techniques]Space and Planetary ScienceAstronomy Astrophysics and CosmologyUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Scaling laws in the distribution of galaxies

2004

Research done during the previous century established our Standard Cosmological Model. There are many details still to be filled in, but few would seriously doubt the basic premise. Past surveys have revealed that the large-scale distribution of galaxies in the Universe is far from random: it is highly structured over a vast range of scales. To describe cosmic structures, we need to build mathematically quantifiable descriptions of structure. Identifying where scaling laws apply and the nature of those scaling laws is an important part of understanding which physical mechanisms have been responsible for the organization of clusters, superclusters of galaxies and the voids between them. Find…

PhysicsStructure (mathematical logic)EXTRA-GALACTIC NEBULAEMICROWAVE BACKGROUND-RADIATIONCOSMIC cancer databaseCold dark matterAstrophysics (astro-ph)Cosmic microwave backgroundCAMPANAS REDSHIFT SURVEY2-POINT CORRELATION-FUNCTIONFOS: Physical sciencesGeneral Physics and AstronomyAstrophysicsN-BODY SIMULATIONSAstrophysicsPOINT CORRELATION-FUNCTIONSGalaxyCOLD DARK-MATTERFractalPROBE WMAP OBSERVATIONSDIGITAL SKY SURVEYPEAK-PATCH PICTUREStatistical physicsScalingGalaxy clusterReviews of Modern Physics
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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Observations of molecular hydrogen mixing ratio and stable isotopic composition at the Cabauw tall tower in the Netherlands

2016

AbstractMeasurements of the stable isotopic composition (δD(H2) or δD) of atmospheric molecular hydrogen (H2) are a useful addition to mixing ratio (χ(H2)) measurements for understanding the atmospheric H2 cycle. δD datasets published so far consist mostly of observations at background locations. We complement these with observations from the Cabauw tall tower at the CESAR site, situated in a densely populated region of the Netherlands. Our measurements show a large anthropogenic influence on the local H2 cycle, with frequently occurring pollution events that are characterized by χ(H2) values that reach up to ≈1 ppm and low δD values. An isotopic source signature analysis yields an apparent…

PollutionAtmospheric Science010504 meteorology & atmospheric sciencesMeteorologymedia_common.quotation_subjectCESARGrowing season010501 environmental sciencesAtmospheric sciences01 natural sciencesEnvironmental Science(all)Mixing ratioCabauwAir quality indexStable isotopes0105 earth and related environmental sciencesGeneral Environmental Sciencemedia_commonChemistryStable isotope ratioAtmospheric observationsHydrogen moleculeSampling (statistics)Deuterium13. Climate actionTowerHydrogenAtmospheric Environment
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A K s -band-selected catalogue of objects in the ALHAMBRA survey

2016

The original ALHAMBRA catalogue contained over 400 000 galaxies selected using a synthetic F814W image, to the magnitude limit AB(F814W) ≈ 24.5. Given the photometric redshift depth of the ALHAMBRA multiband data (〈 z〉 = 0.86) and the approximately I-band selection, there is a noticeable bias against red objects at moderate redshift.We avoid this bias by creating a new catalogue selected in the Ks band. This newly obtained catalogue is certainly shallower in terms of apparent magnitude, but deeper in terms of redshift, with a significant population of red objects at z > 1. We select objects using the Ks band images, which reach an approximate AB magnitude limit Ks ≈ 22. We generate masks an…

PopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsApproxSurveys01 natural sciencesPhotometry (optics)Apparent magnitude0103 physical sciencesobservations [Cosmology]education010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysicseducation.field_of_study010308 nuclear & particles physicsCosmology: observationsAstronomyGalaxies: evolutionAstronomy and AstrophysicsAB magnitudeevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyRedshiftSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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NEW IMPORTANT STOP-OVER SITES FOR RUDDY SHELDUCK TADORNA FERRUGINEA PALLAS, 1764 (AVES, ANATIDAE) IN SICILY

2018

The Ruddy Shelduck Tadorna ferruginea PALLAS, 1764 is a species widely distributed in Southeast Europe and central Asia (MACKINNON et al., 2000). Records in N and W Europe (including Northern Italy) mainly involve escapes from captivity since this species of duck is commonly kept in wildfowl collection, private gardens and parks. Despite this, actually, in Sicily the Ruddy Shelduck is considered an irregular migratory and wintering species and the observations must be attributed to the presence of wild individuals (CORSO, 2005). From 2009 to 2017, 67 observations were collected and compared with those included in the available bibliography (CORSO, 2005). The species was observed in 7 differ…

Ruddy Shelduck tadorna ferruginea Sicily observations
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Euclid preparation - XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields

2022

Artículo escrito por un elevado núnmero de autores, sólo se referencian el qque aparece en primer lugar, los autores pertenecientes a la UAM y el nombre del grupo de colaboración, si lo hubiere

SAMPLELarge-scale structure of UniverseDATA RELEASEFormationSurveysobservations Dark energy Dark matter Galaxy: formation Large-scale structure of Universe Surveys [Cosmology]kosmologiaAstrophysicsCosmology: observationdark mattergalaksijoukotpimeä ainesurveysDark energyDark matterobservations [Cosmology]dark energyObservationsLEGACY SURVEYAstrophysics of GalaxiesFísicaAstronomy and Astrophysics115 Astronomy Space scienceEVOLUTIONCosmologygalaksitGALAXIESCosmology: observations; Dark energy; Dark matter; Galaxy: formation; Large-scale structure of Universe; SurveysGalaxyformation [Galaxy]Space and Planetary ScienceGalaxy: formationcosmology: observationslarge-scale structure of Universepimeä energiaCosmology and Nongalactic Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The relationship between classroom quality and students' engagement in secondary school

2013

Student engagement has been identified as an influential mediator between classroom interactional quality and adolescent learning outcomes. This study examined the relationship between classroom quality and student behavioural engagement in secondary school classrooms. Three dimensions of classroom quality (emotional, organisational and instructional support) and the dimension of student engagement were observed in nine classrooms using the Classroom Assessment Scoring System. Self-ratings of behavioural engagement were provided by 181 Finnish secondary school students along with their teachers’ ratings of classroom-level student engagement. The results showed, first, that there was variati…

Scoring systemEmotional supportmedia_common.quotation_subjectluokkahuoneen laatuclassroom qualityExperimental and Cognitive PsychologyStudent engagementsitoutuminenEducationOrganisational supportPedagogyobservointiDevelopmental and Educational PsychologyMathematics educationComputingMilieux_COMPUTERSANDEDUCATIONstudent engagementsecondary schoolta516Quality (business)yläkouluPsychologyclassroom observationsComputingMilieux_MISCELLANEOUSmedia_common
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Leaf anatomy in Tamarix arborea var. arborea (Tamaricaceae)

2012

Previously unpublished data on the macro- and micro-morphological features of the leaf of Tamarix arborea var. arborea are provided. Clear differences in salt gland localization and type of venations were observed in the investigated species compared to other Tamarix species, thus emphasizing the taxonomic value of the leaf within this genus.

Settore BIO/01 - Botanica GeneralebiologyGenusBotanyTamarixfood and beveragesMediterranean areaPlant ScienceTamarix arboreaTamaricaceaeTamarix arborea var. arborea Tamaricaceae SEM observations leaf anatomy Mediterranean areabiology.organism_classificationEcology Evolution Behavior and Systematics
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Analysis of the XMM-Newton observations of IC443

2017

We analyze for the first time the full set of archive XMM-Newton EPIC observations of the Galactic Supernova Remnant IC 443. We aim at identifying the contribution of the shocked ejecta and interstellar medium and at the describing the physical and chemical properties of the shocked plasma. We also aim at addressing the presence of overionized plasma and its physical origin. We trace the morphology of Si- and S-rich ejecta with unprecedented spatial resolution, by adopting a novel method to produce maps of equivalent width. We describe in detail the method adopted and the results obtained and present preliminary results of a spatially resolved spectral analysis performed on selected regions…

Settore FIS/05 - Astronomia E AstrofisicaX-ray observations Supernovae remnants interstellar medium
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