The LOFT (Large Observatory for X-ray Timing) background simulations

The Large Observatory For X-ray Timing (LOFT) is an innovative medium-class mission selected for an assessment phase in the framework of the ESA M3 Cosmic Vision call. LOFT is intended to answer fundamental questions about the behaviour of matter in the very strong gravitational and magnetic fields around compact objects. With an effective area of ~10 m^2 LOFT will be able to measure very fast variability in the X-ray fluxes and spectra. A good knowledge of the in-orbit background environment is essential to assess the scientific performance of the mission and to optimize the instrument design. The two main contributions to the background are cosmic diffuse X-rays and high energy cosmic rays; also, albedo emission from the Earth is significant. These contributions to the background for both the Large Area Detector and the Wide Field Monitor are discussed, on the basis of extensive Geant-4 simulations of a simplified instrumental mass model.Comment: Proceedings of SPIE, Vol. 8443, Paper No. 8443-209, 201

El clima vitícola de las regiones productoras de uvas para vinos de Argentina.

El territorio continental americano de la Argentina está situado entre las latitudes 21° 46’ S y 55° 03’ S y longitudes 53° 38’ O y 73° 34’ O (Instituto Geográfico Militar). Los principales tipos de clima de la Argentina son cuatro: cálido, templado, árido y frío. En la Figura 1A se observa que la extensión del territorio y los accidentes del relieve, principalmente la Cordillera de los Andes, determinan la existencia de variaciones climáticas en cada uno de los tipos citados (Servicio Meteorológico Nacional). En la Argentina, la vitivinicultura orientada a la producción de vinos finos se desarrolla principalmente en la zona pedemontana de la Cordillera de Los Andes desde los 22° hasta los 42° de latitud Sur

Hyper-velocity impact test and simulation of a double-wall shield concept for the Wide Field Monitor aboard LOFT

The space mission LOFT (Large Observatory For X-ray Timing) was selected in 2011 by ESA as one of the candidates for the M3 launch opportunity. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM), based on Silicon Drift Detectors (SDDs). In orbit, they would be exposed to hyper-velocity impacts by environmental dust particles, which might alter the surface properties of the SDDs. In order to assess the risk posed by these events, we performed simulations in ESABASE2 and laboratory tests. Tests on SDD prototypes aimed at verifying to what extent the structural damages produced by impacts affect the SDD functionality have been performed at the Van de Graaff dust accelerator at the Max Planck Institute for Nuclear Physics (MPIK) in Heidelberg. For the WFM, where we expect a rate of risky impacts notably higher than for the LAD, we designed, simulated and successfully tested at the plasma accelerator at the Technical University in Munich (TUM) a double-wall shielding configuration based on thin foils of Kapton and Polypropylene. In this paper we summarize all the assessment, focussing on the experimental test campaign at TUM.Comment: Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91446

Puzzling thermonuclear burst behaviour from the transient low-mass X-ray binary IGR J17473-2721

We investigate the thermonuclear bursting behaviour of IGR J17473-2721, an X-ray transient that in 2008 underwent a six month long outburst, starting (unusually) with an X-ray burst. We detected a total of 57 thermonuclear bursts throughout the outburst with AGILE, Swift, RXTE, and INTEGRAL. The wide range of inferred accretion rates (between <1% and about 20% of the Eddington accretion rate m-dot_Edd) spanned during the outburst allows us to study changes in the nuclear burning processes and to identify up to seven different phases. The burst rate increased gradually with the accretion rate until it dropped (at a persistent flux corresponding to about 15% of m-dot_Edd) a few days before the outburst peak, after which bursts were not detected for a month. As the persistent emission subsequently decreased, the bursting activity resumed with a much lower rate than during the outburst rise. This hysteresis may arise from the thermal effect of the accretion on the surface nuclear burning processes, and the timescale is roughly consistent with that expected for the neutron star crust thermal response. On the other hand, an undetected superburst, occurring within a data gap near the outburst peak, could have produced a similar quenching of burst activity.Comment: 18 pages, 12 figures, 1 table, accepted for publication in MNRA

Aprovechamiento del cardo (Cynara cardunculus L.) para la producción de biomasa lignocelulósica, aceite y forraje verde

Aprovechamiento del cardo (Cynara cardunculus L.) es una especie perteneciente a la familia de las Compuestas (Asteraceae) lo mismo que el cártamo o el girasol. es una especie vivaz gracias a sus yemas de recambio que posee en el cuello de la raíz estando muy bien adaptada a las condiciones del clima mediterráneo de veranos secos y calurosos

Productividad media en tres años de cultivo de diferentes cultivares de pataca en San Esteban de Gormaz (Soria)

La pataca, Helianthus tuberosus L. es una especie de la familia de las Compuestas, de origen americano. Fue introducida en Europa en el siglo XVII y su cultivo fue de tipo local destinado a producir tubérculos como alimento humano y para el ganado. Posteriomente fue desplazado por la patata como alimento humano. En la actualidad se considera como un posible cultivo alternativo para la obtención de furctosa, de mayor poder edulcorante que la sacarosa, y para la obtención de etanol

Correction: Porous monoliths synthesized via polymerization of styrene and divinyl benzene in nonaqueous deep-eutectic solvent-based HIPEs (RSC Advances (2015) 5 (23255-23260) DOI: 10.1039/C5RA02374B)

© 2018 The Royal Society of Chemistry. The authors regret that there was an error in the results and discussion section of the original article. On page 23257, the text read, The surfactant employed here was sorbitan monooleate . This should have read, The surfactant employed here was sorbitan stearate . The Royal Society of Chemistry apologises for these errors and any consequent inconvenience to authors and readers