Proporcionalidad y reeducación en la jurisdicción de menores

Esteban, García; David, M; Albentosa, Gutiérrez; Manel, Joan

doi:10.2307/j.ctv1tqcwsr

Cited by 1 publication

(3 citation statements)

References 0 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…We go on to compare our results with the results obtained from the image analysis (see Goddi et al 2021;Albentosa-Ruiz 2021). We get a RM posterior distribution peaked around RM ∼ (0.8-1.6) × 10 5 rad m −2 , consistent with the values obtained from the image analysis.…”

Section: Real Alma Observationssupporting

confidence: 81%

“…On the other hand, values Q, U, and V of the core component are set manually (see Table 1) to simulate a source with greater EVPA rotation compared to M87, thus increasing the RM of our simulated source to ∼0.35 × 10 7 rad m −2 , compared to the value of ∼1.5 × 10 5 rad m −2 for M87*, obtained from the ALMA EHT data (see Goddi et al 2021;Albentosa-Ruiz 2021). Doing so allows us to test the performance and reliability of our method, since the high simulated RM values produce clear imprints in the closure traces.…”

Section: Simulations and Model Parametersmentioning

confidence: 99%

“…Results of the MCMC posterior sampling of the model consisting of three polarized components, fitting two of them (the core and knot A of the M87 AGN+jet structure), for the real ALMA observations. The histogram shows the RM of the core, and the dotted line indicates the expected value, of ∼1.5 × 10 5 rad m −2 , from the image analysis (seeGoddi et al 2021;Albentosa-Ruiz 2021).…”

mentioning

confidence: 99%

See 2 more Smart Citations

Robust analysis of differential Faraday rotation based on interferometric closure observables

Albentosa-Ruiz

Martí-Vidal

2023

A&A

View full text Add to dashboard Cite

Polarization calibration of interferometric observations is a costly procedure and in some cases (e.g., due to limited coverage of paral-lactic angle for the calibrator), it may not be possible to carry out this process. To avoid this worst-case scenario, while extending the possibilities for the exploitation of polarization interferometric observations, the use of a new set of calibration-independent quantities (closure traces) has been proposed. However, these quantities suffer from some degeneracies, so their use in practical situations may be rather limited. In this paper, we explore the use of closure traces on simulated and real observations, showing that (with the proper selection of fitting parameters) it is possible to retrieve information on the source polarization using only closure traces and to constrain spatially resolved polarization. We carried out the first application of closure traces to the brightness modeling of real data, using the ALMA observations of M87 conducted during the April 2017 EHT campaign and quantifying a gradient in the Faraday rotation along the source structure (the M87 jet). This work opens the possibility to apply similar strategies to observations from any kind of interferometer (with a special focus on VLBI), whereby quantities such as the differential rotation measure or the spatially resolved polarization can be retrieved.

show abstract

Section: Real Alma Observationssupporting

confidence: 81%

Section: Simulations and Model Parametersmentioning

confidence: 99%

mentioning

confidence: 99%

See 1 more Smart Citation