Actas de la XIII Reunión Española sobre Criptología y Seguridad de la Información RECSI XIII : Alicante, 2-5 de septiembre de 2014

Si tuviéramos que elegir un conjunto de palabras clave para definir la sociedad actual, sin duda el término información sería uno de los más representativos. Vivimos en un mundo caracterizado por un continuo flujo de información en el que las Tecnologías de la Información y Comunicación (TIC) y las Redes Sociales desempeñan un papel relevante. En la Sociedad de la Información se generan gran variedad de datos en formato digital, siendo la protección de los mismos frente a accesos y usos no autorizados el objetivo principal de lo que conocemos como Seguridad de la Información. Si bien la Criptología es una herramienta tecnológica básica, dedicada al desarrollo y análisis de sistemas y protocolos que garanticen la seguridad de los datos, el espectro de tecnologías que intervienen en la protección de la información es amplio y abarca diferentes disciplinas. Una de las características de esta ciencia es su rápida y constante evolución, motivada en parte por los continuos avances que se producen en el terreno de la computación, especialmente en las últimas décadas. Sistemas, protocolos y herramientas en general considerados seguros en la actualidad dejarán de serlo en un futuro más o menos cercano, lo que hace imprescindible el desarrollo de nuevas herramientas que garanticen, de forma eficiente, los necesarios niveles de seguridad. La Reunión Española sobre Criptología y Seguridad de la Información (RECSI) es el congreso científico español de referencia en el ámbito de la Criptología y la Seguridad en las TIC, en el que se dan cita periódicamente los principales investigadores españoles y de otras nacionalidades en esta disciplina, con el fin de compartir los resultados más recientes de su investigación. Del 2 al 5 de septiembre de 2014 se celebrará la decimotercera edición en la ciudad de Alicante, organizada por el grupo de Criptología y Seguridad Computacional de la Universidad de Alicante. Las anteriores ediciones tuvieron lugar en Palma de Mallorca (1991), Madrid (1992), Barcelona (1994), Valladolid (1996), Torremolinos (1998), Santa Cruz de Tenerife (2000), Oviedo (2002), Leganés (2004), Barcelona (2006), Salamanca (2008), Tarragona (2010) y San Sebastián (2012)

Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe

We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median $z\sim 0.03$). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between $z\sim 0.6$ and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call "Marvin." The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data

A922 Sequential measurement of 1 hour creatinine clearance (1-CRCL) in critically ill patients at risk of acute kidney injury (AKI)

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Robust estimation of bacterial cell count from optical density

Optical density (OD) is widely used to estimate the density of cells in liquid culture, but cannot be compared between instruments without a standardized calibration protocol and is challenging to relate to actual cell count. We address this with an interlaboratory study comparing three simple, low-cost, and highly accessible OD calibration protocols across 244 laboratories, applied to eight strains of constitutive GFP-expressing E. coli. Based on our results, we recommend calibrating OD to estimated cell count using serial dilution of silica microspheres, which produces highly precise calibration (95.5% of residuals <1.2-fold), is easily assessed for quality control, also assesses instrument effective linear range, and can be combined with fluorescence calibration to obtain units of Molecules of Equivalent Fluorescein (MEFL) per cell, allowing direct comparison and data fusion with flow cytometry measurements: in our study, fluorescence per cell measurements showed only a 1.07-fold mean difference between plate reader and flow cytometry data

Baile del Juicio de Paris: Edizione di una pieza breve attribuita a Antonio Zamora a partire dal ms. della Biblioteca Nacional de Madrid

Edizione di una piéce poco conosciuta in cui confluiscono due tradizioni letterarie auree, il travestimento burlesco e il baile dramático, la cui fortuna si stava all’epoca esaurendo lasciando spazio a forme distinte: la «parodia mista» e i sainetes costumbristas dei quali questo baile, come testo di transizione, anticipa il sapore locale.Edizione di una piéce poco conosciuta in cui confluiscono due tradizioni letterarie auree, il travestimento burlesco e il baile dramático, la cui fortuna si stava all’epoca esaurendo lasciando spazio a forme distinte: la «parodia mista» e i sainetes costumbristas dei quali questo baile, come testo di transizione, anticipa il sapore locale

Dramaticos posteriores a Lope de Vega : Coleccion escogida y ordenada, con un discurso, apuntes biográficos y críticos de los autores, noticias bibliográficos y catálogos /

1. Estudios críticos / por J. Amador de los Rios y A. Gil de Zárate -- 2. Apuntes biográficos y críticos.Mode of access: Internet

Images of Earth and Space: SC97 Edition

The entire narrated Images video made for Supercomputing 97 Educational levels: Undergraduate lower division, Undergraduate upper division, Graduate or professional

Images of Earth and Space II

This videotape tours the Solar System and outer space using scientific visualizations from Goddard Space Flight Center, Jet Propulsion Laboratory, and the HPCC Earth and Space Sciences Project. At the Sun, simulations investigate processes that create magnetic field and release energetic particles. Earth science begins with the Pacific Ocean, studying the 1997-98 El Nino and Cyclone Susan. Crossing the globe, visualizations trace North Americas East Coast and ocean currents in the North Atlantic Ocean. The lights of the worlds cities then show human impact. Next, two models probe nearby-space phenomena, fluid behavior in microgravity conditions and an asteroid collision. A jaunt to Mars explores the mountains and trenches of its dry, rocky exterior. The video concludes at a binary neutron star system, where two city-sized objects with the Suns mass merge in a titanic explosion. Educational levels: Undergraduate lower division, Undergraduate upper division, Graduate or professional