Search results for "Declination"

showing 10 items of 16 documents

Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

2016

Using high-resolution radio imaging with VLBI techniques, the TANAMI program has been observing the parsec-scale radio jets of southern (declination south of -30{\deg}) gamma-ray bright AGN simultaneously with Fermi/LAT monitoring of their gamma-ray emission. We present the radio and gamma-ray properties of the TANAMI sources based on one year of contemporaneous TANAMI and Fermi/LAT data. A large fraction (72%) of the TANAMI sample can be associated with bright gamma-ray sources for this time range. Association rates differ for different optical classes with all BL Lacs, 76% of quasars and just 17% of galaxies detected by the LAT. Upper limits were established on the gamma-ray flux from TAN…

AstrofísicaBrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationRadio continuum: galaxies0103 physical sciencesVery-long-baseline interferometryGalaxies; Interferometry; Luminance; Radio astronomy; Temperature Galaxies : active; Galaxies: nuclei; Galaxies:jets; Gamma rays: galaxies; Radio continuum: galaxies Gamma rays; Galaxies: active; Galaxies: jets; Galaxies: nuclei; Gamma rays: galaxies; Radio continuum: galaxiesRadio astronomyBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxies: nuclei0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGalaxies : activeGalaxies:jetsGamma raysTemperatureGamma rayAstronomy and AstrophysicsQuasarGalaxies: activeGalaxiesGalaxyGamma rays: galaxiesInterferometryLuminanceGalaxies: jetsSpace and Planetary ScienceAstronomiaComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeAstronomy & Astrophysics
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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Geometry/Time Measurement/Sundials Graphical Resolution via Algorithmic and Parametric Processes

2018

Every people, in every historical period, developed methods to measure Time both at a daily scale and at a yearly scale. Some of them constructed sundials to represent the apparent trajectory of the Sun around the Earth, by using and developing tools from descriptive and projective Geometry, mainly. This subject acquired a great multidisciplinary interest since ancient times, also for Science of Representation applications. This study presents the first results of an ongoing research concerning some aspects related to Time Measurement. The geometric-spatial setting of the Sun-Earth system is described and is structured parametrically via algorithms, following the known conventions shared an…

CollocationScale (ratio)Computer science05 social sciences0211 other engineering and technologies021107 urban & regional planning02 engineering and technologyDeclinationGnomonic projectionHour angleGeometry of curves and surface Sundials Algorithmic modeling0502 economics and businessSettore ICAR/17 - DisegnoRepresentation (mathematics)SundialAlgorithm050203 business & managementProjective geometry
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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TANAMI: tracking active galactic nuclei with austral milliarcsecond interferometry

2010

We introduce the TANAMI program (Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry) which is monitoring an initial sample of 43 extragalactic jets located south of -30 degrees declination at 8.4 GHz and 22 GHz since 2007. All aspects of the program are discussed. First epoch results at 8.4 GHz are presented along with physical parameters derived therefrom. We present first epoch images for 43 sources, some observed for the first time at milliarcsecond resolution. Parameters of these images as well as physical parameters derived from them are also presented and discussed. These and subsequent images from the TANAMI survey are available at http://pulsar.sternwarte.uni…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsBrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusEpoch (astronomy)FOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsDeclinationGalaxyRedshiftInterferometrySpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomy and Astrophysics
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Establishing a high-resolution surface sediment chronology with multiple dating methods – Testing 137Cs determination with Nurmijärvi clastic-biogeni…

2017

Abstract The uppermost 50 cm of sediments from the 23 m deep lacustrine basin of Nurmijarvi, a lake in south-central Finland, are composed of the clastic-biogenic type of varves. We use multiple dating methods to render a sediment chronology that is as precise and accurate as possible for future paleoenvironmental research on this high-fidelity sedimentary archive. The 250-year-long varve chronology contains a chronological error of ±2%, as estimated based on repeated varve counts. The varve-based chronology was verified with the vertical distribution of 137Cs by comparing variations in the paleomagnetic relative declination of the surface sediments with instrumental observations and a calc…

Lake Nurmijärvi010506 paleontologyPaleomagnetism010504 meteorology & atmospheric sciences137CsStratigraphyta1171GeochemistryStructural basin01 natural sciencesDeclinationEarth and Planetary Sciences (miscellaneous)varveslakeGeomorphologyFinland0105 earth and related environmental sciencesVarvepaleomagnetismSedimentGeologychronologysedimentClastic rockSedimentary rockGeologyChronologyQuaternary Geochronology
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A new sample of large angular size radio galaxies I. The radio data

2001

We present a new sample of 84 large angular size radio galaxies selected from the NRAO VLA Sky Survey. Radio sources with declination above +60 degrees, total flux density greater than 100 mJy at 1.4 GHz and angular size larger than 4 arcmin have been selected and observed with the VLA at 1.4 and 4.9 GHz. The radio observations attempt to confirm the large angular size sources and to isolate the core emission for optical identification. In this paper, the first of a series of three, we present radio maps of 79 sources from the sample and discuss the effects of the selection criteria in the final sample. 37 radio galaxies belong to the class of giants, of which 22 are reported in this paper …

NRAO VLA Sky SurveyPhysicsActive galaxies ; Nuclei ; Radio continuumActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsSample (graphics)DeclinationNuclei:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Radio continuumSpace and Planetary ScienceAngular diameterActive galaxiesUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astrophysics::Galaxy Astrophysics
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Three Peculiar Objects From a New Sample of Radio Galaxies

2001

We have constructed a new sample of 84 large angular size radio galaxies selected from the NRAO VLA Sky Survey (NVSS). Radio sources with declination above +60°, total flux density greater than 100 mJy at 1.4 GHz and angular size larger then 4′ have been selected and observed with the VLA at 1.4 and 4.9 GHz. A number of peculiar radio galaxies have been discovered, of which we present here results on J1835+620, J2114+820 and J2157+664.

NRAO VLA Sky SurveyPhysicsLuminous infrared galaxyX-shaped radio galaxyAngular diameterRadio galaxyAstrophysicsSample (graphics)Declination
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A sample of weak blazars at milli-arcsecond resolution

2015

We started a follow-up investigation of the Deep X-ray Radio Blazar Survey objects with declination &gt;-10 deg. We undertook a survey with the EVN at 5GHz to make the first images of a complete sample of weak blazars, aiming at a comparison between high- and low-power samples of blazars. All of the 87 sources observed were detected. Point-like sources are found in 39 cases, and 48 show core-jet structure. According to the spectral indices previously obtained, 58 sources show a flat spectral index, and 29 sources show a steep spectrum or a spectrum peaking at a frequency around 1-2 GHz. Adding to the DXRBS objects we observed those already observed with ATCA in the southern sky, we found th…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AstrofísicaSpectral indexmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of GalaxiesDeclinationLuminosity13. Climate actionSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)ROSATAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy Astrophysicsmedia_commonAstronomia Aparells i instruments
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A new sample of large angular size radio galaxies II. The optical data

2001

We constructed and presented in the first paper of this series a new sample of 84 large angular size radio galaxies by selecting from the NRAO VLA Sky Survey objects with angular size &gt; 4', declination above +60 degrees and total flux density at 1.4 GHz &gt; 100 mJy. In this paper we present optical spectra and images of those galaxies associated with the radio emission for which no redshift was known prior to our observations. Optical counterparts have been identified for all (but one) members of the sample. After our observations, a reliable spectroscopic redshift is available for 67 objects (80%) from the sample. This paper, second of a series of three, contributes to increase the num…

PhysicsNRAO VLA Sky Survey3D optical data storageRadio galaxyAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysicsSample (graphics)DeclinationGalaxyRedshiftSpace and Planetary ScienceAngular diameterAstrophysics::Galaxy Astrophysics
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