LA COMUNIDAD DE LAS AVES EN TRES HÁBITATS DE LA PLANICIE DE TABASCO, MÉXICO

The wealth and diversity of the bird community in three ecosystems of the Tabasco plain, México, was evaluated, associated to habitats with flood influence (mangrove, arrowroot-tule and floodable grasslands). Four sampling stations were established in each habitat and observations were performed during drought and rainy seasons in 2010 with three sampling days in each station. The sampling method was through fixed-radius observation in eight spots for each season. The data were taken at sunrise, sundown and night. 23,926 individuals of 155 bird species were identified, showing greater wealth and abundance during the rainy season (141 species and 12,595 individuals), of which 123 species were resident, 22 migratory, seven transitory, two local migratory and one summer resident. According to the Clench, there is 89 % completeness in the community. The arrowroot-tule stands showed the highest wealth (122), followed by mangroves (177) and grasslands (110). The first ecosystem was the most diverse (H´=3.69), followed by mangroves (H´=3.58), and in these environments the greatest similarity was observed (S=0.951). Of the species, 13.54% are protected by NOM-059- SEMARNAT-2010. The low zones of the Tabasco plain are very important in maintaining bird communities, in addition to serving as feeding and refuge zones for resident and migratory species.Se evaluó la riqueza y diversidad de la comunidad de aves en tres tipos de ecosistemas de la planicie tabasqueña, asociados a hábitats con influencia de inundación (manglares, popales-tulares y pastizales inundables). Se establecieron 12 estaciones de muestreo, cuatro para cada hábitat. Se trabajó en dos temporadas del año 2010 (secas y lluvias), se muestrearon por tres días en cada estación. El método de muestreo fue por observación de radio fijo en ocho puntos por cada estación. Los datos se tomaron en tres momentos del día (amanecer, atardecer y noche). Se identificaron 23,926 individuos de 155 especies de aves, donde la temporada de lluvias fue más rica y abundante (141 especies y 12,595 individuos) en comparación con la secas. De las cuales 123 especies fueron residentes, 22 migratorias, siete transitorias, dos migrantes locales y una residente de verano. De acuerdo a la Clench la se cuenta con el 89% de la completitud de la comunidad. Los popales-tulares presentaron la mayor riqueza (122), seguida por los manglares (117) y los pastizales (110). Los popales-tulares fueron los más diversos (H´=3.69), seguido por los manglares (H´=3.58). Los popales-tulares y los manglares son los ambientes donde se observó la mayor similitud (S=0.951). El 13.54 % de las especies se encuentra protegida por la NOM-059-SEMARNAT-2010. Las zonas bajas de la planicie de Tabasco, son muy importantes en el mantenimiento de la comunidad de aves, además de poder servir como zonas de alimentación y refugio para especies residentes y migratorias

EFECTO DE TRATAMIENTOS PRE-GERMINATIVOS EN LA CALIDAD DE PLÁNTULAS GUAPINOL (HYMENAEA COURBARIL)

This research has evaluated the effect of five pre-germination treatments on the quality and structure of plant locust (Hymenaea courbaril) due to the high variability in the germination and emergency tillage. Five treatments were evaluated by measuring the rate of Germanization and emergency speed; quality parameters (height and diameter) together with biomass (fresh and dry weight) of seedlings, bringing the Dickson quality index were estimated. Each treatment group contained 50 replicates for 250 plants in the experiment. The data were processed with statistical SPSS V.22.0: variance, standard deviation, variance analysis, obtaining statistical tests of binary correlations, repeated measures analysis and analysis of variance (ANOVA), intra and inter groups, 95% (P-valor 0.05) of confidence. The results show differences between treatments three (hydration) and four (mechanical scarification) regarding treatment one (thermal) and two (chemical) where no statistically significant difference. Treatment five (witness) has less statistical difference with all other evaluated. These same data for determining a positive effect between application of pre germination treatments and increased seedling quality of 93.0%, this translates to a greater chance of survival of the plant to be transplanted in the field. It is tested combination treatments one and three.Esta investigación ha evaluado el efecto que tiene cinco tratamientos pre-germinativos en la calidad y estructura de las planta de guapinol (Hymenaea courbaril) debido a la elevada variabilidad en la germinación y emergencia con la siembra directa. Se evaluaron cinco tratamientos, midiendo el índice de germanización y velocidad de emergencia, parámetros de calidad (altura y diámetro) junto con la de biomasa (peso fresco y seco) de las plántulas, con lo que se estimó el índice de calidad de Dickson. Cada uno de los tratamientos consto de 50 repeticiones para un total de 250 plántulas dentro del experimento. Los datos se procesaron SPSS V.22.0 con los estadísticos: varianza, desviación estándar, análisis de varianza, obteniendo las pruebas estadísticas de correlaciones binarias, análisis de medidas repetidas y análisis de varianza (ANOVA), intra e inter grupos, a un 95% (P-valor 0.05) de confianza. Los resultados muestran diferencia entre los tratamientos tres (hidratación) y cuatro (escarificación mecánica) respecto al tratamiento uno (térmico) y dos (químico) donde no hay diferencia estadísticamente significativa. El tratamiento cinco (testigo) presenta diferencia estadística menor con todos los demás evaluados. Estos mismos datos permiten determinar un efecto positivo entre la aplicación de tratamientos pre-germinativos y el aumento de la calidad de la plántula de un 93.0%, esto se traduce a mayores posibilidades de sobrevivencia de la planta al ser trasplantada en campo. Debe probarse la combinación de los tratamientos uno y tres

Influence of entrance-channel magicity and isospin on quasi-fission

The role of spherical quantum shells in the competition between fusion and quasi-fission is studied for reactions forming heavy elements. Measurements of fission fragment mass distributions for different reactions leading to similar compound nuclei have been made near the fusion barrier. In general, more quasi-fission is observed for reactions with non-magic nuclei. However, the $^{40}$Ca+$^{208}$Pb reaction is an exception, showing strong evidence for quasi-fission, though both nuclei are doubly magic. Time-dependent Hartree-Fock calculations predict fast equilibration of $N/Z$ in the two fragments early in the collision. This transfer of nucleons breaks the shell effect, causing this reaction to behave more like a non-magic one in the competition between fusion and quasi-fission. Future measurements of fission in reactions with exotic beams should be able to test this idea with larger $N/Z$ asymmetries.Comment: accepted for publication in Physics Letters

Multimessenger astronomy with the Einstein Telescope

Gravitational waves (GWs) are expected to play a crucial role in the development of multimessenger astrophysics. The combination of GW observations with other astrophysical triggers, such as from gamma-ray and X-ray satellites, optical/radio telescopes, and neutrino detectors allows us to decipher science that would otherwise be inaccessible. In this paper, we provide a broad review from the multimessenger perspective of the science reach offered by the third generation interferometric GW detectors and by the Einstein Telescope (ET) in particular. We focus on cosmic transients, and base our estimates on the results obtained by ET's predecessors GEO, LIGO, and Virgo.Comment: 26 pages. 3 figures. Special issue of GRG on the Einstein Telescope. Minor corrections include

Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, \nobreak{$6\times 10^{19}$eV}. The anisotropy was measured by the fraction of arrival directions that are less than $3.1^\circ$ from the position of an active galactic nucleus within 75 Mpc (using the V\'eron-Cetty and V\'eron $12^{\rm th}$ catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is $(38^{+7}_{-6})$, compared with $21$ expected for isotropic cosmic rays. This is down from the early estimate of $(69^{+11}_{-13})$. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation.Comment: Accepted for publication in Astroparticle Physics on 31 August 201

Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

Atmospheric parameters, such as pressure (P), temperature (T) and density, affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ~10% seasonal modulation and ~2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of pressure and density. The former affects the longitudinal development of air showers while the latter influences the Moliere radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory.Comment: 24 pages, 9 figures, accepted for publication in Astroparticle Physic

The exposure of the hybrid detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The "hybrid" detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction.Comment: Paper accepted by Astroparticle Physic

The Fluorescence Detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detector. Finally, we evaluate the detector performance and precision of shower reconstructions.Comment: 53 pages. Submitted to Nuclear Instruments and Methods in Physics Research Section

Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

The advent of the Auger Engineering Radio Array (AERA) necessitates the development of a powerful framework for the analysis of radio measurements of cosmic ray air showers. As AERA performs "radio-hybrid" measurements of air shower radio emission in coincidence with the surface particle detectors and fluorescence telescopes of the Pierre Auger Observatory, the radio analysis functionality had to be incorporated in the existing hybrid analysis solutions for fluoresence and surface detector data. This goal has been achieved in a natural way by extending the existing Auger Offline software framework with radio functionality. In this article, we lay out the design, highlights and features of the radio extension implemented in the Auger Offline framework. Its functionality has achieved a high degree of sophistication and offers advanced features such as vectorial reconstruction of the electric field, advanced signal processing algorithms, a transparent and efficient handling of FFTs, a very detailed simulation of detector effects, and the read-in of multiple data formats including data from various radio simulation codes. The source code of this radio functionality can be made available to interested parties on request.Comment: accepted for publication in NIM A, 13 pages, minor corrections to author list and references in v

Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

We present the results of searches for dipolar-type anisotropies in different energy ranges above $2.5\times 10^{17}$ eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% $C.L.$ for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.Comment: 28 pages, 11 figure