Estado de micorrización de árboles truferos en función de su carácter productivo y su edad. Primeros resultados del Subproyecto 1 del Plan de Desarrollo Integral de la Truficultura de Teruel

La truficultura es una actividad con clara dimensión forestal, entre otras razones porque las especies implicadas, tanto el hongo como su árbol simbionte, son de gran valor silvícola. Además, la truficultura y la selvicultura trufera son prácticas que contribuyen a la recuperación de masas forestales y zonas potencialmente boscosas, con el valor añadido de la obtención de las trufas, de modo, en la mayor parte de las ocasiones, totalmente ecológico. El Plan Específico para Teruel (PET) integra varias actuaciones promovidas por el Gobierno Español entre las que se encuentra la ejecución de un Proyecto de Investigación denominado “Desarrollo Integral de la Truficultura de Teruel”, financiado por INIA, en el que se pretende apoyar al sector trufero turolense mediante el conocimiento y la mejora de sus técnicas de cultivo, producción y comercialización. La presente comunicación resume los primeros resultados obtenidos en uno de los 7 subproyectos que lo integran y que afecta al estudio del cortejo micorrícico de los árboles de las plantaciones, productoras o no, y su relación con la producción. La composición micorrícica de los árboles truferos es un factor esencial para realizar predicciones sobre la producción futura. Tanto la ausencia de micorrizas de trufa negra como la detección de otras, capaces de desplazar a la primera de las raíces de los árboles, puede permitir el diagnóstico precoz de fracasos de plantaciones y por lo tanto el ahorro de muchos años de cuidados a la espera de las primeras recolecciones. Para el estudio, se han seleccionado 3 grupos de plantaciones por edad, con 2 localizaciones distintas. Se está desarrollando un inventario periódico de las micorrizas presentes en un total de 48 árboles. Se propone una clasificación de las mismas en función de su capacidad para comprometer la producción de trufa negra, factor que se ha determinado en base al carácter productor o no productor de cada árbol

Effect of Enzyme Addition in the Making of Pedro Ximenez Sweet Wines Using Dynamic Pre-fermentative Maceration

This work evaluated the effect of two commercial pectolytic enzymes on some oenological parameters before andafter enzymatic treatments with pre-fermentative dynamic maceration at room temperature for three hours. Thestudy was conducted on an industrial scale using musts from sun-dried grapes of the Pedro Ximenez variety.Statistical analysis and sensory rating showed that the resulting wines varied significantly in total soluble solids(ºBrix) and in the final sensorial controls. On the other hand, the enzyme treatment had no effect on the contentof total polyphenols (TPI) and other chemical characteristics of the obtained musts. A higher qualitative level wasobserved with regard to aroma and gustative quality compared to the control. The results also demonstrate thattotal juice yield improved after enzyme addition together with dynamic maceration

Erratum to: 36th International Symposium on Intensive Care and Emergency Medicine: Brussels, Belgium. 15-18 March 2016.

[This corrects the article DOI: 10.1186/s13054-016-1208-6.]

MAGIC upper limits on the very high energy emission from GRBs

The fast repositioning system of the MAGIC Telescope has allowed during its first data cycle, between 2005 and the beginning of year 2006, observing nine different GRBs as possible sources of very high energy gammas. These observations were triggered by alerts from Swift, HETE-II, and Integral; they started as fast as possible after the alerts and lasted for several minutes, with an energy threshold varying between 80 and 200 GeV, depending upon the zenith angle of the burst. No evidence for gamma signals was found, and upper limits for the flux were derived for all events, using the standard analysis chain of MAGIC. For the bursts with measured redshift, the upper limits are compatible with a power law extrapolation, when the intrinsic fluxes are evaluated taking into account the attenuation due to the scattering in the Metagalactic Radiation Field (MRF).Comment: 25 pages, 9 figures, final version accepted by ApJ. Changet title to "MAGIC upped limits on the VERY high energy emission from GRBs", re-organized chapter with description of observation, removed non necessaries figures, added plot of effective area depending on zenith angle, added an appendix explaining the upper limit calculation, added some reference

Implementation of the Random Forest Method for the Imaging Atmospheric Cherenkov Telescope MAGIC

The paper describes an application of the tree classification method Random Forest (RF), as used in the analysis of data from the ground-based gamma telescope MAGIC. In such telescopes, cosmic gamma-rays are observed and have to be discriminated against a dominating background of hadronic cosmic-ray particles. We describe the application of RF for this gamma/hadron separation. The RF method often shows superior performance in comparison with traditional semi-empirical techniques. Critical issues of the method and its implementation are discussed. An application of the RF method for estimation of a continuous parameter from related variables, rather than discrete classes, is also discussed.Comment: 16 pages, 8 figure

Unfolding of differential energy spectra in the MAGIC experiment

The paper describes the different methods, used in the MAGIC experiment, to unfold experimental energy distributions of cosmic ray particles (gamma-rays). Questions and problems related to the unfolding are discussed. Various procedures are proposed which can help to make the unfolding robust and reliable. The different methods and procedures are implemented in the MAGIC software and are used in most of the analyses.Comment: Submitted to NIM

First bounds on the very high energy gamma-ray emission from Arp 220

Using the Major Atmospheric Gamma Imaging Cherenkov Telescope (MAGIC), we have observed the nearest ultra-luminous infrared galaxy Arp 220 for about 15 hours. No significant signal was detected within the dedicated amount of observation time. The first upper limits to the very high energy $\gamma$-ray flux of Arp 220 are herein reported and compared with theoretical expectations.Comment: Accepted for publication in Ap

MAGIC observations of very high energy gamma-rays from HESS J1813-178

Recently, the HESS collaboration has reported the detection of gamma-ray emission above a few hundred GeV from eight new sources located close to the Galactic Plane. The source HESS J1813-178 has sparked particular interest, as subsequent radio observations imply an association with SNR G12.82-0.02. Triggered by the detection in VHE gamma-rays, a positionally coincident source has also been found in INTEGRAL and ASCA data. In this Letter we present MAGIC observations of HESS J1813-178, resulting in the detection of a differential gamma-ray flux consistent with a hard-slope power law, described as dN/(dA dt dE) = (3.3+/-0.5)*10^{-12} (E/TeV)^{-2.1+/-0.2} cm^(-2)s^(-1)TeV^(-1). We briefly discuss the observational technique used, the procedure implemented for the data analysis, and put this detection in the perspective of multifrequency observations.Comment: Accepted by ApJ Letter

Constraints on the steady and pulsed very high energy gamma-ray emission from observations of PSR B1951+32/CTB 80 with the MAGIC Telescope

We report on very high energy gamma-observations with the MAGIC Telescope of the pulsar PSR B1951+32 and its associated nebula, CTB 80. Our data constrain the cutoff energy of the pulsar to be less than 32 GeV, assuming the pulsed gamma-ray emission to be exponentially cut off. The upper limit on the flux of pulsed gamma-ray emission above 75 GeV is 4.3*10^-11 photons cm^-2 sec^-1, and the upper limit on the flux of steady emission above 140 GeV is 1.5*10^-11 photons cm^-2 sec^-1. We discuss our results in the framework of recent model predictions and other studies.Comment: 7 pages, 7 figures, replaced with published versio

Discovery of VHE Gamma Radiation from IC443 with the MAGIC Telescope

We report the detection of a new source of very high energy (VHE, E_gamma >= 100GeV) gamma-ray emission located close to the Galactic Plane, MAGIC J0616+225, which is spatially coincident with SNR IC443. The observations were carried out with the MAGIC telescope in the periods December 2005 - January 2006 and December 2006 - January 2007. Here we present results from this source, leading to a VHE gamma-ray signal with a statistical significance of 5.7 sigma in the 2006/7 data and a measured differential gamma-ray flux consistent with a power law, described as dN_gamma/(dA dt dE) = (1.0 +/- 0.2)*10^(-11)(E/0.4 TeV)^(-3.1 +/- 0.3) cm^(-2)s^(-1)TeV^(-1). We briefly discuss the observational technique used and the procedure implemented for the data analysis. The results are put in the perspective of the multiwavelength emission and the molecular environment found in the region of IC443.Comment: Accepted by ApJ Letter