Search results for "Astronomia Aparells i instruments"

showing 2 items of 2 documents

Halo-independent methods for inelastic dark matter scattering

2013

We present halo-independent methods to analyze the results of dark matter direct detection experiments assuming inelastic scattering. We focus on the annual modulation signal reported by DAMA/LIBRA and present three different halo-independent tests. First, we compare it to the upper limit on the unmodulated rate from XENON100 using (a) the trivial requirement that the amplitude of the annual modulation has to be smaller than the bound on the unmodulated rate, and (b) a bound on the annual modulation amplitude based on an expansion in the Earth's velocity. The third test uses the special predictions of the signal shape for inelastic scattering and allows for an internal consistency check of …

AstrofísicaParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesInelastic scattering01 natural sciencesSignalPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsdark matter theory010308 nuclear & particles physicsScatteringdark matter experimentsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsComputational physicsDark matter haloHigh Energy Physics - PhenomenologyAmplitudeModulationHaloAstronomia Aparells i instrumentsAstrophysics - Cosmology and Nongalactic Astrophysics
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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 >-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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