Suchergebnisse

resultado de la primera revolución social del siglo XX fue la Constitución Política de los Estados Unidos Mexicanos, documento que plasmó las aspiraciones de toda una nación, marcando el rumbo de nuestro país hacia la democracia. Gracias a la Carta Magna hoy tenemos garantizados amplios derechos y podemos ejercer plenamente nuestras libertades. Celebro que la Universidad Autónoma del Estado de México conmemore los cien años de nuestra Constitución con la publicación de este libro, elaborado por un grupo multidisciplinario de investigadores, pertenecientes a diversas instituciones educativas del país, que analizan los diferentes artículos de la Constitución de 1917, desde los ámbitos histórico, filosófico, jurídico, educativo y social. Para el Gobierno del Estado de México, un libro conmemorativo de nuestra Carta Magna es invitación a reflexionar sobre las características de nuestras instituciones, así como la conveniencia de mantener o reformar sus artículos para continuar respondiendo a las necesidades de la ciudadanía. En cada propuesta de este libro, desde sus respectivos campos de estudio, los autores analizan los retos de la sociedad actual; además en su lectura e interpretación demuestran que los 136 artículos no son letra muerta, siguen vigentes.

At the international level, gender violence and in particular, violence against women has been part of some sectors of society and has been included in the agendas of public and private entities. In this way, different conventions, resolutions and protocols have been formulated focused on their intervention. One of them is the Convention on the elimination of all forms of discrimination against women CEDAW (1979), which, among many others, deals with the design of equality policies with special and temporary measures to achieve equality between women and men. Likewise, in 1994 the "Belém do Pará" convention was created, which applies to all manifestations of physical, sexual or psychological violence based on gender. In the Political Constitution of Colombia of 1991, in article 43 it is enshrined: "Women and men have equal rights and opportunities. Women may not be subjected to any kind of discrimination ". Likewise, Law 311 of 1996 creates the National Registry of Family Protection and other provisions are issued. In this way, equality between men and women and families are assumed as the responsibility of the State and, therefore, mandatory for its intervention. ; A nivel internacional, la violencia de género y en particular, la violencia contra las mujeres ha formado parte de algunos sectores de la sociedad y ha sido incluida en las agendas de las entidades públicas y privadas. De esta manera, se han formulado diferentes convenciones, resoluciones y protocolos enfocadas a su intervención. Una de ellas es la Convención sobre la eliminación de todas las formas de discriminación contra la mujer CEDAW (1979), la cual, entre otras muchas, trata sobre el diseño de políticas de igualdad con medidas de carácter especial y temporal para alcanzar la igualdad entre mujeres y hombres. Igualmente, en 1994 se crea la convención "Belém do Pará", la cual se aplica a todas las manifestaciones de violencia física sexual o psicológica basada en su género. En la Constitución Política de Colombia de 1991, en el artículo 43 se ...

36 pages, 12 figures, 1 table ; he tropical Atlantic is home to multiple coupled climate variations covering a wide range of timescales and impacting societally relevant phenomena such as continental rainfall, Atlantic hurricane activity, oceanic biological productivity, and atmospheric circulation in the equatorial Pacific. The tropical Atlantic also connects the southern and northern branches of the Atlantic meridional overturning circulation and receives freshwater input from some of the world's largest rivers. To address these diverse, unique, and interconnected research challenges, a rich network of ocean observations has developed, building on the backbone of the Prediction and Research Moored Array in the Tropical Atlantic (PIRATA). This network has evolved naturally over time and out of necessity in order to address the most important outstanding scientific questions and to improve predictions of tropical Atlantic severe weather and global climate variability and change. The tropical Atlantic observing system is motivated by goals to understand and better predict phenomena such as tropical Atlantic interannual to decadal variability and climate change; multidecadal variability and its links to the meridional overturning circulation; air-sea fluxes of CO2 and their implications for the fate of anthropogenic CO2; the Amazon River plume and its interactions with biogeochemistry, vertical mixing, and hurricanes; the highly productive eastern boundary and equatorial upwelling systems; and oceanic oxygen minimum zones, their impacts on biogeochemical cycles and marine ecosystems, and their feedbacks to climate. Past success of the tropical Atlantic observing system is the result of an international commitment to sustained observations and scientific cooperation, a willingness to evolve with changing research and monitoring needs, and a desire to share data openly with the scientific community and operational centers. The observing system must continue to evolve in order to meet an expanding set of research priorities and operational challenges. This paper discusses the tropical Atlantic observing system, including emerging scientific questions that demand sustained ocean observations, the potential for further integration of the observing system, and the requirements for sustaining and enhancing the tropical Atlantic observing system ; MM-R received funding from the MORDICUS grant under contract ANR-13-SENV-0002-01 and the MSCA-IF-EF-ST FESTIVAL (H2020-EU project 797236). GF, MG, RLu, RP, RW, and CS were supported by NOAA/OAR through base funds to AOML and the Ocean Observing and Monitoring Division (OOMD; fund reference 100007298). This is NOAA/PMEL contribution #4918. PB, MDe, JH, RH, and JL are grateful for continuing support from the GEOMAR Helmholtz Centre for Ocean Research Kiel. German participation is further supported by different programs funded by the Deutsche Forschungsgemeinschaft, the Deutsche Bundesministerium für Bildung und Forschung (BMBF), and the European Union. The EU-PREFACE project funded by the EU FP7/2007–2013 programme (Grant No. 603521) contributed to results synthesized here. LCC was supported by the UERJ/Prociencia-2018 research grant. JOS received funding from the Cluster of Excellence Future Ocean (EXC80-DFG), the EU-PREFACE project (Grant No. 603521) and the BMBF-AWA project (Grant No. 01DG12073C)

Segundo volúmen de la Colección Perspectivas Iberoamericanas sobre la justicia. La Declaración Universal de los Derechos Humanos de las Naciones Unidas cumple, el 10 de diciembre de 2018, setenta años. La simbólica fecha obliga a los investigadores en derechos humanos a reflexionar críticamente sobre los avances y límites de un complejo sistema de normas y, sobre todo, de valores culturales sustentados en la matriz liberal occidental. Desde entonces, ha habido indiscutibles avances institucionales y normativos, como la creación del Consejo de Derechos Humanos, varios pactos y declaraciones complementarias, órganos específicos, tribunales internacionales, jurisprudencia, constituciones estatales, una infinidad de instituciones basadas en esta "ética mínima universal" que, contradictoriamente, no logró evitar un conjunto de catástrofes humanitarias y de vulneración de derechos. La primera década del siglo XX trae un reflejo limitante al consenso de la posguerra, pues la agresividad de los Estados hegemónicos, en alianza con intereses privados transnacionales, pone en jaque la capacidad del sistema protector frente a guerras humanitarias e internacionales. tratados económicos de nueva generación aquellos que excluyen por completo a la democracia del proceso de negociación. ; A Declaração Universal dos Direitos Humanos das Nações Unidas completa, em 10 de diciembre de 2018, setenta años. A data simbólica exige dos pesquisadores em direitos humanos uma reflexão crítica a respeito dos avanços y dos limites de um sistema complexo de normas e, principalmente, de valores culturales apoiados na matriz liberal ocidental. De lá para cá, houve indiscutível avanço institucional e normativo, do qual é exemplo a criação do Conselho de Direitos Humanos, diversos pactos e declarações complementarios, órgão específicos, tribunais internacionais, jurisprudência, constituições dos States, uma infinidade de instituições pautadas nesse "mínimo ético universal" que, contraditoriamente, não conseguiu evitar um conjunto de catástrofes ...

Introduction: In response to the necessity of concise,accurate and practical information to supportclinical decision making, the Colombian government,in partnership with universities and scientificsocieties, has heavily invested in the developmentof clinical practice guidelines (CPG). Objectives:To develop a Web portal for the dissemination andcommunication of CPG and its clinical recommendations.Methodology: Development of the ColombianGPC web portal based on the principlesof adult learning, learning development in medicinebased on the Web and improvement of webdevelopment for medical education, using variousinformatic tools. Results: A Web portal that fulfillsthe purpose of disseminating the recommendationsof the GPC, using various alternatives for the presentationof content, as well as to create channelsof communication between developers and users ofthe CPG Portal. ; Introducción: En respuesta a la necesidad de información concisa, veraz y práctica para sustentar la toma de decisiones clínicas, el Gobierno colombiano, en alianza con diversas universidades y sociedades científicas, ha hecho una gran inversión en el desarrollo de guías de práctica clínica (GPC). Objetivos: Desarrollar un portal web para la difusión y comunicación de las GPC y las recomendaciones clínicas consignadas en las guías. Metodología: Desarrollo del portal web colombiano de GPC basado en los principios de aprendizaje para adultos, desarrollo de aprendizaje en medicina basado en web (e-learning) y mejoramiento de desarrollo web en educación médica, utilizando diversas herramientas informáticas. Resultados: El portal web cumple con el propósito de difundir las recomendaciones de las GPC, utilizando diversas alternativas para la presentación de los contenidos, así como para la creación de canales de comunicación entre los desarrolladores de las GPC y sus usuarios

El presente libro aporta al campo de los estudios sociales de la ciencia, la tecnología y la innovación, mediante el análisis comparado de los Planes de Ciencia Tecnología e Innovación (PCTI), tratando de superar el enfoque dominante que privilegia los casos nacionales independientes que ha limitado el debate académico. Considera tanto estudios sobre las dinámicas de su institucionalización, el papel de los diversos actores, las contribuciones del campo a la concepción de las políticas y los desafíos que se presentan a las PCTI para responder a los imperativos de democratización, inclusión y sustentabilidad.

This paper addresses the evolution of archives in the Mexican context under four axes of analysis, archive institutions, legislation, professional training, and professional associations. A transverse and parallel chronological review of the facts is performed within this framework, which has marked the development of the discipline and shows the emerging presence of the national archives through the actions to be undertaken and made visible to the discipline. The successive, natural and unstructured during the beginning to the middle of the past century, have been the basis for building the scaffolding that through the education offered by universities on the one hand and,to the other hand the self-development of the profession through the integration of Information Technology and Communication and its regulation through a legal framework have been developing National Archives which has resulted in an embryonic professional association more or less organized. ; El presente trabajo aborda la evolución archivística en el contexto mexicano bajo cuatro ejes de análisis: las instituciones archivísticas, la legislación, la formación profesional y las asociaciones profesionales. Se hace una revisión cronológica de manera transversal y paralela con los hechos -dentro de este marco- que han marcado el devenir de la disciplina y evidencian la incipiente presencia de la archivística nacional a través de las acciones que se han emprendido y han hecho visible a la disciplina. El empalme sucesivo, natural y poco estructurado de principios a mediados del siglo pasado, ha servido de base para construir el andamiaje en el que, a través de la oferta educativa de carreras a nivel superior por un lado y, por otro, el desarrollo propio de la profesión mediante la inserción de Tecnologías de la Información y la Comunicación y su regulación a través de un marco legal, han ido gestando una Archivística nacional que ha incidido en un gremio profesional embrionario y más o menos organizado.

El presente trabajo aborda la evolución archivística en el contexto mexicano bajo cuatro ejes de análisis: las instituciones archivísticas, la legislación, la formación profesional y las asociaciones profesionales. Se hace una revisión cronológica de manera transversal y paralela con los hechos -dentro de este marco- que han marcado el devenir de la disciplina y evidencian la incipiente presencia de la archivística nacional a través de las acciones que se han emprendido y han hecho visible a la disciplina. El empalme sucesivo, natural y poco estructurado de principios a mediados del siglo pasado, ha servido de base para construir el andamiaje en el que, a través de la oferta educativa de carreras a nivel superior por un lado y, por otro, el desarrollo propio de la profesión mediante la inserción de Tecnologías de la Información y la Comunicación y su regulación a través de un marco legal, han ido gestando una Archivística nacional que ha incidido en un gremio profesional embrionario y más o menos organizado. ; This paper addresses the evolution of archives in the Mexican context under four axes of analysis, archive institutions, legislation, professional training, and professional associations. A transverse and parallel chronological review of the facts is performed within this framework, which has marked the development of the discipline and shows the emerging presence of the national archives through the actions to be undertaken and made visible to the discipline. The successive, natural and unstructured during the beginning to the middle of the past century, have been the basis for building the scaffolding that through the education offered by universities on the one hand and,to the other hand the self-development of the profession through the integration of Information Technology and Communication and its regulation through a legal framework have been developing National Archives which has resulted in an embryonic professional association more or less organized.

We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67μeV mass range. A radio frequency cavity consisting of 5 sub-cavities coupled by inductive irises took physics data inside the CAST dipole magnet for the first time using this filter-like haloscope geometry. An exclusion limit with a 95% credibility level on the axion-photon coupling constant of gaγ & 4 × 10−13 GeV−1 over a mass range of 34.6738μeV < ma < 34.6771μeV is set. This constitutes a significant improvement over the current strongest limit set by CAST at this mass and is at the same time one of the most sensitive direct searches for an axion dark matter candidate above the mass of 25μeV. The results also demonstrate the feasibility of exploring a wider mass range around the value probed by CAST-RADES in this work using similar coherent resonant cavities ; We wish to thank our colleagues at CERN, in particular Marc Thiebert from the coating lab, as well as the whole team of the CERN Central Cryogenic Laboratory for their support and advice in speci c aspects of the project. We thank Arefe Abghari for her contributions as the project's summer student during 2018. This work has been funded by the Spanish Agencia Estatal de Investigacion (AEI) and Fondo Europeo de Desarrollo Regional (FEDER) under project FPA-2016-76978-C3-2-P and PID2019-108122GB-C33, and was supported by the CERN Doctoral Studentship programme. The research leading to these results has received funding from the European Research Council and BD, JG and SAC acknowledge support through the European Research Council under grant ERC-2018-StG-802836 (AxScale project). BD also acknowledges fruitful discussions at MIAPP supported by DFG under EXC-2094 { 390783311. IGI acknowledges also support from the European Research Council (ERC) under grant ERC-2017-AdG-788781 (IAXO+ project). JR has been supported by the Ramon y Cajal Fellowship 2012-10597, the grant PGC2018-095328-B-I00(FEDER/Agencia estatal de investigaci on) and FSE-GA2017-2019-E12/7R (Gobierno de Aragón/FEDER) (MINECO/FEDER), the EU through the ITN \Elusives" H2020-MSCA-ITN-2015/674896 and the Deutsche Forschungsgemeinschaft under grant SFB-1258 as a Mercator Fellow. CPG was supported by PROMETEO II/2014/050 of Generalitat Valenciana, FPA2014-57816-P of MINECO and by the European Union's Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreements 690575 and 674896. AM is supported by the European Research Council under Grant No. 742104. Part of this work was performed under the auspices of the US Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344.

The design and construction of CARMENES has been presented at previous SPIE conferences. It is a next-generation radial-velocity instrument at the 3.5m telescope of the Calar Alto Observatory, which was built by a consortium of eleven Spanish and German institutions. CARMENES consists of two separate échelle spectrographs covering the wavelength range from 0.52 to 1.71¿m at a spec-tral resolution of R < 80,000, fed by fibers from the Cassegrain focus of the telescope. CARMENES saw ¿First Light¿ on Nov 9, 2015. During the commissioning and initial operation phases, we established basic performance data such as throughput and spectral resolution. We found that our hollow-cathode lamps are suitable for precise wavelength calibration, but their spectra contain a number of lines of neon or argon that are so bright that the lamps cannot be used in simultaneous exposures with stars. We have therefore adopted a calibration procedure that uses simultaneous star / Fabry Pérot etalon exposures in combination with a cross-calibration between the etalons and hollow-cathode lamps during daytime. With this strategy it has been possible to achieve 1-2 m/s precision in the visible and 5-10 m/s precision in the near-IR; further improvements are expected from ongoing work on temperature control, calibration procedures and data reduction. Comparing the RV precision achieved in different wavelength bands, we find a ¿sweet spot¿ between 0.7 and 0.8¿m, where deep TiO bands provide rich RV information in mid-M dwarfs. This is in contrast to our pre-survey models, which predicted comparatively better performance in the near-IR around 1¿m, and explains in part why our near-IR RVs do not reach the same precision level as those taken with the visible spectrograph. We are now conducting a large survey of 340 nearby M dwarfs (with an average distance of only 12pc), with the goal of finding terrestrial planets in their habitable zones. We have detected the signatures of several previously known or suspected planets and also discovered several new planets. We find that the radial velocity periodograms of many M dwarfs show several significant peaks. The development of robust methods to distinguish planet signatures from activity-induced radial velocity jitter is therefore among our priorities. Due to its large wavelength coverage, the CARMENES survey is generating a unique data set for studies of M star atmospheres, rotation, and activity. The spectra cover important diagnostic lines for activity (H alpha, Na I D1 and D2, and the Ca II infrared triplet), as well as FeH lines, from which the magnetic field can be inferred. Correlating the time series of these features with each other, and with wavelength-dependent radial velocities, provides excellent handles for the discrimination between planetary companions and stellar radial velocity jitter. These data are also generating new insight into the physical properties of M dwarf atmospheres, and the impact of activity and flares on the habitability of M star planets. © 2018 SPIE. ; CARMENES is an instrument for the Centro Astronomico Hispano-Aleman de Calar Alto (CAHA, Almeria, Spain). CARMENES is funded by the German Max-Planck-Gesellschaft (MPG), the Spanish Consejo Superior de Investigaciones Cientificas (CSIC), the European Union through FEDER/ERF FICTS-2011-02 funds, and the members of the CARMENES Consortium (Max-Planck-Institut fur Astronomie, Instituto de Astrofisica de Andalucia, Landessternwarte Konigstuhl, Institut de Ciencies de l'Espai, Insitut fur Astrophysik Gottingen, Universidad Complutense de Madrid, Thuringer Landessternwarte Tautenburg, Instituto de Astrofisica de Canarias, Hamburger Sternwarte, Centro de Astrobiologia and Centro Astronomico Hispano-Aleman), with additional contributions by the Spanish Ministry of Science, the German Science Foundation through the Major Research Instrumentation Program and DFG Research Unit FOR2544 "Blue Planets around Red Stars", the Klaus Tschira Stiftung, the states of Baden-Wurttemberg and Niedersachsen, and by the Junta de Andalucia.

Cities play a major role in tackling the COVID-19 pandemic as many measures are adopted at the scale of cities and involve adjustments to the way urban areas operate. Drawing from case studies across the globe, this book explores how the pandemic and the policies it has prompted have caused changes in the ways cities function. The contributors examine the advancing social inequality brought on by the pandemic and suggest policies intended to contain contagion whilst managing the economy in these circumstances. Offering crucial insights for reforming cities to be more resilient to future crises, this is an invaluable resource for scholars and policy makers alike

We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample of 117 stars to classify their behaviour regarding variability and place them in the Hertzsprung-Russell diagram using Gaia DR2 data. Included within our sample are the eponymous members of two pulsator classes, γ Doradus and SX Phoenicis. Our sample of pulsating intermediate-mass stars observed by TESS also allows us to confront theoretical models of pulsation driving in the classical instability strip for the first time and show that mixing processes in the outer envelope play an important role. We derive an empirical estimate of 74 per cent for the relative amplitude suppression factor as a result of the redder TESS passband compared to the Kepler mission using a pulsating eclipsing binary system. Furthermore, our sample contains many high-frequency pulsators, allowing us to probe the frequency variability of hot young δ Scuti stars, which were lacking in the Kepler mission data set, and identify promising targets for future asteroseismic modelling. The TESS data also allow us to refine the stellar parameters of SX Phoenicis, which is believed to be a blue straggler. © 2019 The Author(s) ; We thank the referee for useful comments and discussions. This paper includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA Explorer Program. Funding for the TESS Asteroseismic Science Operations Centre is provided by the Danish National Re-search Foundation (Grant agreement no.: DNRF106), ESA PRODEX (PEA 4000119301), and Stellar Astrophysics Centre (SAC) at Aarhus University. We thank the TESS and TASC/TASOC teams for their support of this work. This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-2655. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant agreement no.: DNRF106). MC was supported by FCT -Fundacao para a Ciencia e a Tecnologia through national funds and by FEDER through COMPETE2020 -Programa Operacional Competitividade e Internacionalizacao by these grants: UID/FIS/04434/2019, PTDC/FIS-AST/30389/2017, and POCI-01-0145-FEDER-030389. MC is supported in the form of work contract funded by national funds through FCT (CEECIND/02619/2017). JDD acknowledges support from the Polish National Science Center (NCN), grant no. 2018/29/B/ST9/02803. AGH acknowledges funding support from Spanish public funds for research under projects ESP201787676-2-2 and ESP2015-65712-C5-5-R of the Spanish Ministry of Science and Education. FKA gratefully acknowledges funding through grant 2015/18/A/ST9/00578 of the Polish National Science Centre (NCN). JPe acknowledges funding support from the NSF REU program under grant number PHY-1359195. APi and KK acknowledge support provided by the Polish National Science Center (NCN) grant No. 2016/21/B/ST9/01126. This project has been supported by the Lendulet Program of the Hungarian Academy of Sciences, project No. LP2018-7/2018, and by the support provided from the National Research, Development and Innovation Fund of Hungary, financed under the K16 funding scheme, project No. 115709. JCS acknowledges funding support from Spanish public funds for research under projects ESP2017-87676-2-2 and ESP2015-65712-C5-5-R, and from project RYC2012-09913 under the 'Ramon y Cajal' program of the Spanish Ministry of Science and Education. The research leading to these results has (partially) received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement N.670519: MAMSIE), from the KULeuven Research Council (grant C16/18/005: PARADISE), from the Research Foundation Flanders (FWO) under grant agreement G0H5416N (ERC Runner Up Project), as well as from the BELgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO. SBF acknowledges support by the Spanish State Research Agency (AEI) through project No. 'ESP2017-87676-C5-1-R' and No MDM-2017-0737 Unidad de Excelencia `Maria de Maeztu'-Centro de Astrobiolog ' ia (CSICINTA). ZsB acknowledges the support provided from the National Research, Development and Innovation Fund of Hungary, financed under the PD1717 funding scheme, project no. PD-123910. DLB acknowledges support from the Whitaker Foundation. SC gratefully acknowledges funding through grant 2015/18/A/ST9/00578 of the Polish National Science Centre (NCN). CCL gratefully acknowledges support from the Natural Sciences and Engineering Research Council of Canada. GMM acknowledges funding by the STFC consolidated grant ST/R000603/1. RMO, SC, and DR were supported in this work by the 'Programme National de Physique Stellaire' (PNPS) of CNRS/INSU co-funded by CEA and CNES. IS acknowledges the partial support of projects DN 08-1/2016 and DN 18/13-12.12.2017. PS acknowledges financial support by the Polish NCN grant 2015/18/A/ST9/00578. MS acknowledges the Postdoc@MUNI project CZ.02.2.69/0.0/0.0/16-027/0008360. JPG, JRR, and MLM acknowledge funding support from Spanish public funds for research under project ESP2017-87676-C5-5-R and from the State Agency for Research of the Spanish MCIU through the 'Center of Excellence Severo Ochoa' award for the Instituto de Astrofisica de Andalucia (SEV-2017-0709). JAE acknowledges STFC for funding support (reference ST/N504348/1). LFM acknowledges the financial support from the DGAPA-UNAM under grant PAPIIT IN100918. DMk acknowledges his work as part of the research activity of the National Astronomical Research Institute of Thailand (NARIT), which is supported by the Ministry of Science and Technology of Thailand. MR acknowledges the support of the French Agence Nationale de la Recherche (ANR), under grant ESRR (ANR-16-CE31-0007-01). We acknowledge the International Space Science Institute (ISSI) for supporting the SoFAR international team http://www.issi.unibe.ch/teams/sofar/.TW acknowledges the NSFC of China (Grant Nos. 11873084 and 11521303) and YunnanApplied Basic Research Projects (GrantNo. 2017B008). IS acknowledges for a partial support of DN 08-1/2016 funded by the Bulgarian NSF. This work hasmade use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, ht tps://www.cosmos.esa.int/web/gaia/dpac/consortium).Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. The research leading to these results has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No. 670519: MAMSIE) and from the Fonds Wetenschappelijk Onderzoek - Vlaanderen (FWO) under the grant agreement G0H5416N (ERC Opvangproject). This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI:10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Soicety © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved ; We present results of the first dynamical stream fits to the recently discovered Tucana III stream. These fits assume a fixed Milky Way potential and give proper motion predictions, which can be tested with the upcoming Gaia Data Release 2 (DR2). These fits reveal that Tucana III is on an eccentric orbit around the Milky Way and, more interestingly, that Tucana III passed within 15 kpc of the Large Magellanic Cloud (LMC) approximately 75 Myr ago. Given this close passage, we fit the Tucana III stream in the combined presence of the Milky Way and the LMC. We find that the predicted proper motions depend on the assumed mass of the LMC and that the LMC can induce a substantial proper motion perpendicular to the stream track. A detection of this misalignment will directly probe the extent of the LMC's influence on our Galaxy, and has implications for nearly all methods which attempt to constraint the Milky Way potential. Such a measurement will be possible with the upcoming Gaia DR2, allowing for a measurement of the LMC's mass. ; DE and VB acknowledge that the research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007- 2013) / ERC Grant Agreement no. 308024. EB acknowledges financial support from the European Research Council (StG-335936). ABP acknowledges generous support from the George P. and Cynthia Woods Institute for Fundamental Physics and Astronomy at Texas A&M University. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro- Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundacâo Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnología e Inovacâo, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey

Reproduced with permission of AAS ; We present chemical abundance measurements of three stars in the ultrafaint dwarf galaxy Horologium I, a Milky Way satellite discovered by the Dark Energy Survey. Using high-resolution spectroscopic observations, we measure the metallicity of the three stars, as well as abundance ratios of several α-elements, iron-peak elements, and neutron-capture elements. The abundance pattern is relatively consistent among all three stars, which have a low average metallicity of [Fe/H] ∼ -2.6 and are not α-enhanced ([α/Fe] ∼ 0.0). This result is unexpected when compared to other low-metallicity stars in the Galactic halo and other ultrafaint dwarfs and suggests the possibility of a different mechanism for the enrichment of Hor I compared to other satellites. We discuss possible scenarios that could lead to this observed nucleosynthetic signature, including extended star formation, enrichment by a Population III supernova, and or an association with the Large Magellanic Cloud ; Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The DES data management system is supported by the National Science Foundation under grant nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015-71825, ESP2015-88861, FPA2015-68048, SEV- 2012-0234, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (FP7/2007- 2013), including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project no. CE110001020

La transparencia en México ha tenido un sinuoso camino, para garantizar que las instituciones y los funcionarios públicos den a conocer la información sobre sus actividades de interés para los ciudadanos. En ese sentido, las organizaciones de la sociedad civil como el Colectivo por Municipios Transparentes (CIMTRA), académicos y universidades son un espacio de discusión que busca impulsar y promover este derecho consagrado en la Constitución. Además, para garantizar la rendición de cuentas se ha estimulado el combate a la corrupción y doctrinas políticas como el gobierno abierto, que promulgan la colaboración y participación ciudadana a fin de hacer accesible la información de las organizaciones e instituciones públicas. Ese importante análisis, innovador y actual, formulado por especialistas e investigadores sobre los alcances y limitaciones de estos temas es abordado en esta obra, para mover a la reflexión y análisis críticos y, sobre todo, para impulsar acciones a favor de políticas públicas que mejoren la función sustantiva del gobierno: garantizar a los ciudadanos bienestar. ; 11Presentación Felipe José Hevia de Jara 15Introducción José Antonio Meyer Rodríguez José Luis Estrada Rodríguez José Ojeda Bustamante 17Capítulo I Calidad de la democracia para la fiscalización, control y seguimiento de los recursos públicos José Luis Estrada Rodríguez Lorenzo Antonio Portilla Vásquez 35Capítulo II Deliberación pública y participación ciudadana, primordial sustento para el Gobierno Abierto y la rendición de cuentas José Antonio Meyer Rodríguez Jorge Luis Castillo Durán Alejandra Rodríguez Estrada 47Capítulo III Midiendo al Gobierno Abierto en México: los portales estatales de transparencia durante el periodo 2015-2016 Rodrigo Sandoval Almazán 67Capítulo IV Transparencia y contraloría social en la generación de Gobierno Abierto en el ámbito subnacional María Gabriela Martínez Tiburcio 87Capítulo V Discurso presidencial y corrupción en México. Una aproximación desde el Análisis Crítico del Discurso Carlos Enrique Ahuactzin Martínez Jorge Luis Castillo Durán Bárbara Torres Romero 113 Capítulo VI Retos y sensibilización hacia la transparencia en la Ciudad de México Dulce Maribel Corona Rojas María Luisa Rubio González Víctor Alejandro Villegas Corona 129 Capítulo VII Partidos Políticos en México: los Intocables de la transparencia y rendición de cuentas Hugo Sánchez Gudiño 149 Capítulo VIII Gobierno Abierto en el contexto subnacional José de Jesús Sosa López 169 Capítulo IX Capacidades institucionales para la transparencia presupuestal en la frontera norte de México Ramón Fernández Mejía 189 Capítulo X Comprender y transparentar a la legislatura en Puebla: una agenda ciudadana José Luis Mendoza Tablero 201 Capítulo XI Práctica exitosa en la implementación y ejecución del modelo de Gobierno Abierto: caso Zacatecas Norma Julieta del Río Venegas 223 Capítulo XII La educación cívica como condición para la transparencia y rendición de cuentas Rafael Caballero Álvarez Alma Verónica Méndez Pacheco 243 Capítulo XIII Transparencia y sujetos obligados: análisis de los juicios presentados al IAIP de Tlaxcala (2015-2016) María Magdalena Sam Bautista 267 Capítulo XIV Hacia una nueva agenda de transparencia, acceso a la información y rendición de cuentas en el ámbito local en México Ricardo Joel Jiménez González 299 Capítulo XV Gobierno Abierto: retos y avances en Veracruz Yolli García Alvarez Angélica Mendieta Ramírez 321 Capítulo XVI Análisis sobre los indicadores de impunidad y corrupción en Puebla Juan Antonio Le Clercq Ortega 339 Capítulo XVII Las ampliaciones de la Unión Europea hacia Europa del Este, impacto político en transparencia y gobernanza Pedro Manuel Rodríguez Suárez 361 Capítulo XVIII El Sistema Nacional Anticorrupción en México: análisis de sus alcances y limitaciones Jairo Garzón Montaño 385 Capítulo XIX Gobierno de opacidad vs Gobierno Abierto: comité local de Gobierno Abierto subnacional José Ojeda Bustamante Yadira del Carmen Rosales Ruiz Georgina Alducin González 405 Sobre los autores