Search results for "Asars"

showing 10 items of 54 documents

Flux and color variations of the quadruply imaged quasar HE 0435-1223

2011

aims: We present VRi photometric observations of the quadruply imaged quasar HE 0435-1223, carried out with the Danish 1.54m telescope at the La Silla Observatory. Our aim was to monitor and study the magnitudes and colors of each lensed component as a function of time. methods: We monitored the object during two seasons (2008 and 2009) in the VRi spectral bands, and reduced the data with two independent techniques: difference imaging and PSF (Point Spread Function) fitting.results: Between these two seasons, our results show an evident decrease in flux by ~0.2-0.4 magnitudes of the four lensed components in the three filters. We also found a significant increase (~0.05-0.015) in their V-R …

Point spread functionCosmology and Nongalactic Astrophysics (astro-ph.CO)FluxFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensing01 natural scienceslaw.inventionTelescopeSettore FIS/05 - Astronomia e AstrofisicaObservatorylaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsgeneral – gravitational lensing; weak – techniques: photometric [quasars]Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsphotometric [Techniques]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasargeneral [Quasars]Spectral bandsSpace and Planetary Scienceastro-ph.COAstrophysics::Earth and Planetary Astrophysicsweak [Gravitational lensing]Astrophysics - Cosmology and Nongalactic Astrophysics
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The ALHAMBRA survey: Discovery of a faint QSO at z = 5.41

2013

[Aims]: We aim to illustrate the potentiality of the Advanced Large, Homogeneous Area, Medium-Band Redshift Astronomical (ALHAMBRA) survey to investigate the high-redshift universe through the detection of quasi stellar objects (QSOs) at redshifts higher than 5. [Methods]: We searched for QSOs candidates at high redshift by fitting an extensive library of spectral energy distributions-including active and non-active galaxy templates, as well as stars-to the photometric database of the ALHAMBRA survey (composed of 20 optical medium-band plus the 3 broad-band JHKs near-infrared filters). [Results]: Our selection over ≈1 square degree of ALHAMBRA data (∼1/4 of the total area covered by the sur…

QSOSAbsolute magnitudeCosmology and Nongalactic Astrophysics (astro-ph.CO)active [Galaxies]Young stellar objectContinuum (design consultancy)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLuminosityhigh-redshift [Galaxies]emission lines [Quasars]Galaxies: distances and redshiftsdistances and redshifts [Galaxies]Astrophysics::Galaxy AstrophysicsPhysicsQuasars: emission linesGalaxies: high-redshiftGalaxies: evolutiongeneral [Quasars]Astronomy and AstrophysicsGalaxies: activeevolution [Galaxies]RedshiftGalaxyQuasars: generalBlack holeSpace and Planetary ScienceAstrophysics - Cosmology and Nongalactic Astrophysics
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The High A(V) Quasar Survey: Reddened quasi-stellar objects selected from optical/near-infrared photometry - II

2014

Quasi-stellar objects (QSOs) whose spectral energy distributions (SEDs) are reddened by dust either in their host galaxies or in intervening absorber galaxies are to a large degree missed by optical color selection criteria like the one used by the Sloan Digital Sky Survey (SDSS). To overcome this bias against red QSOs, we employ a combined optical and near-infrared color selection. In this paper, we present a spectroscopic follow-up campaign of a sample of red candidate QSOs which were selected from the SDSS and the UKIRT Infrared Deep Sky Survey (UKIDSS). The spectroscopic data and SDSS/UKIDSS photometry are supplemented by mid-infrared photometry from the Wide-field Infrared Survey Explo…

QSOSCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectYoung stellar objectgalaxies: activeFOS: Physical sciencesgalaxies: active; quasars: absorption lines; quasars: general; Space and Planetary Science; Astronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPhotometry (optics)quasars: general0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsLarge Magellanic CloudInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshiftGalaxyquasars: absorption linesSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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PKS1830-211 HDO, ND and NH_2_D spectra

2020

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Detection of deuterated molecules, but not of lithium hydride, in the z=0.89 absorber toward PKS 1830-211.' (bibcode: 2020A&A...637A...7M)

Radio astronomyQuasarsRadio spectroscopy
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S5 0836+710 image at 1.6GHz

2012

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'S5 0836+710: An FRII jet disrupted by the growth of a helical instability?' (bibcode: 2012A&A...545A..65P)

Radio sourcesRadio astronomyQuasars
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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MOJAVE. VI. Kinematic analysis of blazar jets

2012

We discuss the jet kinematics of a complete flux-density-limited sample of 135 radio-loud active galactic nuclei (AGNs) resulting from a 13 year program to investigate the structure and evolution of parsec-scale jet phenomena. Our analysis is based on new 2cm Very Long Baseline Array (VLBA) images obtained between 2002 and 2007, but includes our previously published observations made at the same wavelength, and is supplemented by VLBA archive data. In all, we have used 2424 images spanning the years 1994-2007 to study and determine the motions of 526 separate jet features in 127 jets. Cone search capability for table J/AJ/138/1874/agn (AGN sample)

galactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsRadio sourcesAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyCosmologyobservational astronomyBL Lacertae objectsRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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LOFAR images of blazar S5 0836+710

2019

The emission and proper motion of the terminal hotspots of active galactic nucleus (AGN) jets can be used as a powerful probe of the intergalactic medium. However, measurements of hotspot advance speeds in active galaxies are difficult, especially in the young universe, because of the low angular velocities and the low brightness of distant radio galaxies. Our goal is to study the termination of an AGN jet in the young universe and to deduce physical parameters of the jet and the intergalactic medium. We used the LOw Frequency ARray (LOFAR) to image the long-wavelength radio emission of the high-redshift blazar S5 0836+710 on arcsecond scales between 120MHz and 160MHz. The LOFAR image shows…

galactic and extragalactic astronomyAstrophysics and AstronomyRadio sourceshigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyCosmologyobservational astronomyRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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VRi light curves of the lensed QSO HE 0435-1223

2011

We present VRi photometric observations of the quadruply imaged quasar HE0435-1223, carried out with the Danish 1.54m telescope at the La Silla Observatory. Our aim was to monitor and study the magnitudes and colors of each lensed component as a function of time.

galactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsGravitational lensingAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyComputer Science::Digital Librariesobservational astronomyPhotometryAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysical ProcessesNatural SciencesQuasars
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Dynamic SEDs of southern blazars - DSSB

2016

The Dynamic SEDs of southern blazars catalog is based on a TANAMI multiwavelength project that has been monitoring a sample of 22 radio-loud blazars of the southern sky from radio to gamma-ray wavelengths. (4 data files). Simultaneous broadband spectral and temporal studies of blazars are an important tool for investigating active galactic nuclei (AGN) jet physics. Aims. We study the spectral evolution between quiescent and flaring periods of 22 radio-loud AGN through multiepoch, quasi-simultaneous broadband spectra. For many of these sources these are the first broadband studies. Methods. We use a Bayesian block analysis of Fermi/LAT light curves to determine time ranges of constant flux f…

galactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsradio-loud blazarsAstrophysics::Cosmology and Extragalactic AstrophysicsSEDstellar astronomyMultiwavelengthobservational astronomyBL Lacertae objectsNatural SciencesQuasarsAstrophysics::Galaxy AstrophysicsSpectral energy distribution
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