Search results for " luminosity"

showing 2 items of 42 documents

The ALHAMBRA survey: B -band luminosity function of quiescent and star-forming galaxies at 0.2 ≤  z  < 1 by PDF analysis

2016

[Aims]: Our goal is to study the evolution of the B-band luminosity function (LF) since z ∼ 1 using ALHAMBRA data. [Methods]: We used the photometric redshift and the I-band selection magnitude probability distribution functions (PDFs) of those ALHAMBRA galaxies with I ≤ 24 mag to compute the posterior LF. We statistically studied quiescent and star-forming galaxies using the template information encoded in the PDFs. The LF covariance matrix in redshift - magnitude - galaxy type space was computed, including the cosmic variance. That was estimated from the intrinsic dispersion of the LF measurements in the 48 ALHAMBRA sub-fields. The uncertainty due to the photometric redshift prior is also…

luminosity function mass function [Galaxies]Galaxies: statisticsAstrophysics::High Energy Astrophysical PhenomenaPopulationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminositystatistics [Galaxies]0103 physical scienceseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhotometric redshiftLuminosity function (astronomy)Physicseducation.field_of_study010308 nuclear & particles physicsGalaxies: luminosity function mass functionGalaxies: evolutionAstronomy and AstrophysicsCosmic varianceB bandevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesRedshiftGalaxy[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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Measurement of Solar pp-neutrino flux with Borexino: results and implications

2015

International audience; Measurement of the Solar pp-neutrino flux completed the measurement of Solar neutrino fluxes from the pp-chain of reactions in Borexino experiment. The result is in agreement with the prediction of the Standard Solar Model and the MSW/LMA oscillation scenario. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10(5) years time scale, and sets a strong limit on the power production by the unknown energy sources in the Sun.

model: solarHistoryneutrino: solarSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaluminosity: solarSolar luminosity[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyneutrino: fluxEducationLuminosityNuclear physicsPhysics and Astronomy (all)SEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsDETECTORBorexinoMSW effectPhysicsStandard solar modelSolar energetic particles010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyphotonAstronomySolar neutrino problemstabilityoscillationComputer Science Applicationsp p13. Climate actionPhysics::Space PhysicsBorexinoAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental results
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