PRICE OF GRAIN MAIZE AT THE LEVEL OF THE EUROPEAN UNION (2016-2018)

The paper highlights the evolution of the price of grain corn for members of the European Union. The analysed time interval is 2016-2018, emphasizing the short-term price evolution. The price is presented and analysed in the context of the specific conditions of cultivation, for the 28 component states of the European Union, starting from the differences related to climatic factors, the degree of development, capitalization and subsidization of agricultural production. The trading price registered a national multiannual average of 175.22 $/t, with extreme values of 131.90$/t for Croatia (2016) and 251.50 $/t for Greece (2018 - total variation amplitude of 11.96$/t)

Phase noise reveals early category-specific modulation of the event-related potentials

Previous studies have found that the amplitude of the early event-related potential (ERP) components evoked by faces, such as N170 and P2, changes systematically as a function of noise added to the stimuli. This change has been linked to an increased perceptual processing demand and to enhanced difficulty in perceptual decision making about faces. However, to date it has not yet been tested whether noise manipulation affects the neural correlates of decisions about face and non-face stimuli similarly. To this end, we measured the ERPs for faces and cars at three different phase noise levels. Subjects performed the same two-alternative age-discrimination task on stimuli chosen from young–old morphing continua that were created from faces as well as cars and were calibrated to lead to similar performances at each noise-level. Adding phase noise to the stimuli reduced performance and enhanced response latency for the two categories to the same extent. Parallel to that, phase noise reduced the amplitude and prolonged the latency of the face-specific N170 component. The amplitude of the P1 showed category-specific noise dependence: it was enhanced over the right hemisphere for cars and over the left hemisphere for faces as a result of adding phase noise to the stimuli, but remained stable across noise levels for cars over the left and for faces over the right hemisphere. Moreover, noise modulation altered the category-selectivity of the N170, while the P2 ERP component, typically associated with task decision difficulty, was larger for the more noisy stimuli regardless of stimulus category. Our results suggest that the category-specificity of noise-induced modulations of ERP responses starts at around 100 ms post-stimulus

PRIMARY OFFER OF CEREALS IN THE OLT COUNTY (2014-2016)

For agricultural producers in Romania, cereals are a very important group of crops if we take into account only the areas related to them, but also the implications regarding the tradition and the impact on the realized revenues.The area cultivated with cereals in Olt County recorded increases and decreases in the analyzed period (-1.36% in 2015, + 0.18% in 2015), with an average of 265,248.67 ha. In terms of total production, there are significant decreases of 10.20% in 2015 and 15.88% in 2016, so that the average is below the level of 2014 by 8.03% (868.158.33 t compared to 943.924 t in the first year). The average yield per hectare fell from 3,545 kg / ha in 2014 to 3,227 kg / ha in 2015 (-8.93%), to reach 3,047 kg / ha in 2016 (-14.05%)

Altering second-order configurations reduces the adaptation effects on early face-sensitive event-related potential components

The spatial distances among the features of a face are commonly referred to as second-order relations, and the coding of these properties is often regarded as a cornerstone in face recognition. Previous studies have provided mixed results regarding whether the N170, a face-sensitive component of the event-related potential, is sensitive to second-order relations. Here we investigated this issue in a gender discrimination paradigm following long-term (5 s) adaptation to normal or vertically stretched male and female faces, considering that the latter manipulation substantially alters the position of the inner facial features. Gender-ambiguous faces were more likely judged to be female following adaptation to a male face and vice versa. This aftereffect was smaller but statistically significant after being adapted to vertically stretched when compared to unstretched adapters. Event-related potential recordings revealed that adaptation effects measured on the amplitude of the N170 show strong modulations by the second-order relations of the adapter: reduced N170 amplitude was observed, however, this reduction was smaller in magnitude after being adapted to stretched when compared to unstretched faces. These findings suggest early face-processing, as reflected in the N170 component, proceeds by extracting the spatial relations of inner facial features

Evolutionary paths to and from the red sequence: Star formation and HI properties of transition galaxies at z~0

(Abridged) We investigate the properties of galaxies between the blue and the red sequence (i.e., the transition region) by combining UV and NIR imaging to HI line observations for a volume-limited sample of nearby galaxies. We confirm the existence of a tight relation between colour and HI-fraction across all the range of colours, although outside the blue cloud this trend becomes gradually weaker. Transition galaxies are divided into two different families, according to their atomic hydrogen content. HI-deficient galaxies are the majority of transition galaxies in our sample. They are found in high density environments and all their properties are consistent with a quenching of the star formation via gas stripping. However, while the migration from the blue cloud is relatively quick (i.e., <=1 Gyr), a longer amount of time (a few Gyr at least) seems required to completely suppress the star formation and reach the red sequence. At all masses, migrating HI-deficient galaxies are mainly disks, implying that the mechanism responsible for today's migration in clusters cannot have played a significant role in the creation of the red sequence at high-redshift. Conversely, HI-normal transition galaxies are a more heterogeneous population. A fraction of these objects show evidence for accretion/minor-merging events suggesting that at least part of the HI reservoir has an external origin. The detailed evolution of such systems is still unclear, but our analysis suggests that some galaxies might have migrated back from the red sequence after accretion events. Our study clearly shows the variety of evolutionary paths leading to the transition region and suggests that the transition galaxies may not be always associated with systems quickly migrating from the blue to the red sequence.Comment: 19 pages, 11 Figures, 1 Table. MNRAS in press. High resolution version available at http://www.astro.cardiff.ac.uk/pub/Luca.Cortese/papers/mnras09_1159_hires.p

A VLT VIMOS integral field spectroscopic study of perturbed blue compact galaxies: UM 420 and UM 462

We report on optical integral field spectroscopy of two unrelated blue compact galaxies mapped with the 13 x 13 arcsec^2 VIMOS integral field unit at a resolution of 0.33 x 0.33 arcsec^2. Continuum and background subtracted emission line maps in the light of [O III] 5007, H-alpha, and [N II] 6584 are presented. Both galaxies display signs of ongoing perturbation and/or interaction. UM 420 is resolved for the first time to be a merging system composed of two starbursting components with an 'arm-like' structure associated with the largest component. UM 462 which is a disrupted system of irregular morphology is resolved into at least four starbursting regions. Maps of the H-alpha radial velocity and FWHM are discussed. No underlying broad line region was detected from either galaxy as the emission lines are well-fitted with single Gaussian profiles only. Electron temperatures and densities as well as the abundances of helium, oxygen, nitrogen, and sulphur were computed from spectra integrated over the whole galaxies and for each area of recent star formation. Maps of the O/H ratio are presented: these galaxies show oxygen abundances that are ~20 per cent solar. No evidence of substantial abundance variations across the galaxies that would point to significant nitrogen or oxygen self-enrichment is found (<0.2 dex limit). Contrary to previous observations, this analysis does not support the classification of these BCGs as Wolf-Rayet galaxies as the characteristic broad emission line features have not been detected in our spectra. Baldwin-Phillips-Terlevich emission line ratio diagrams which were constructed on a pixel by pixel basis indicate that the optical spectra of these systems are predominantly excited by stellar photoionization.Comment: 19 pages, 14 figure