0000000001102971

AUTHOR

Alejandro Mus

showing 2 related works from this author

ALMA full polarization observations of PKS1830-211 during its record-breaking flare of 2019

2020

We report Atacama Large Millimeter Array (ALMA) Band 6 full-polarization observations of the lensed blazar PKS 1830-211 during its record-breaking radio and gamma-ray flare in the spring of 2019. The observations were taken close to the peak of the gamma activity and show a clear difference in polarization state between the two time-delayed images. The leading image has a fractional polarization about three times lower than the trailing image, implying that significant depolarization occurred during the flare. In addition, we observe clear intra-hour variability of the polarization properties between the two lensed images, with a quasi-linear increase in the differential electric-vector pos…

Astrophysics::High Energy Astrophysical PhenomenaGamma rays: generalgeneral [Gamma rays]FOS: Physical sciencesQuasars: individual: PKS1830-211AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawPolarization0103 physical sciencesindividual: PKS1830-211 [Quasars]Blazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarAtacama Large Millimeter ArrayPolarization (waves)Position angleFractional polarizationSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaFlare
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Polarization calibration techniques for the new-generation VLBI

2020

The calibration and analysis of polarization observations in Very Long Baseline Interferometry (VLBI) requires the use of specific algorithms that suffer from several limitations, closely related to assumptions in the data properties that may not hold in observations taken with new-generation VLBI equipment. Nowadays, the instantaneous bandwidth achievable with VLBI backends can be as high as several GHz, covering several radio bands simultaneously. In addition, the sensitivity of VLBI observations with state-of-the-art equipment may reach dynamic ranges of tens of thousands, both in total intensity and in polarization. In this paper, we discuss the impact of the limitations of common VLBI …

AstrofísicaAstronomyAstrophysics::High Energy Astrophysical PhenomenaPolarimetryFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumInstantaneous bandwidthSoftware0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingPhysicsEvent Horizon Telescope010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsPolarization (waves)Nonlinear systemSpace and Planetary ScienceAstronomiabusinessAstrophysics - Instrumentation and Methods for Astrophysics
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