Puebla de Zaragoza, Mexico

The National Institute of Astrophysics, Optics and Electronics is a Mexican science research institute located in Tonantzintla, Puebla. Founded by presidential decree on 11 November 1971, it has over 100 researchers in astrophysics, optics, electronics and computing science, with postgraduate programs in these areas. INAOE is one of 30 public research centers sponsored by the National Council of Science and Technology of Mexico . The Institute, in partnership with the University of Massachusetts Amherst, developed the Large Millimeter Telescope / Gran Telescopio Milimétrico on the Puebla-Veracruz border. Wikipedia.


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Grant
Agency: European Commission | Branch: H2020 | Program: RIA | Phase: ICT-38-2016 | Award Amount: 1.94M | Year: 2016

SmartSDK aims at creating a sustainable FIWARE ecosystem between Europe and Mexico by leveraging on existing FIWARE outcomes and building reference standards for common challenges. To fulfil this goal, SmartSDK will analyse successful FIWARE applications deployed in Europe and derive from these applications a set of FIWARE-based reference service architectures and reference data models to support the agile development of smart solutions for sustainability challenges of today world. In this perspective, SmartSDK will adopt existing Open Standards and Open Source solutions leveraging on results of European and Mexican initiatives based on FIWARE. By standardizing these efforts in a reference Software Development Kit (SDK) for smart applications, SmartSDK will foster a long-term collaboration between Europe and Mexico on FIWARE building on shared societal and economical challenges in Europe and Mexico. The collaboration will promote increased FIWARE adoption in Mexico as ecosystem for developing smart solutions, through the involvement of cities, innovative SMEs and startups. This will insure a wide impact in Mexico and Europe and will support the growth of new FIWARE-based businesses through the direct involvement of a network of around ICT 30 incubators and accelerators with access to more than 1000 ICT Innovative companies and startups and the support of Wayra Mexico (owned by Telefonica), the local branch of the worldwide largest accelerator. The participation of key FIWARE partners in Europe (TID, CREATE-NET) and Mexico (INFOTEC, ITESM), the support of European startups building on FIWARE technology (HOPU, UBI), and Future Internet researchers from Mexico (CECISE, CENIDET, INAOE) under the experienced guide of R&D consultancy specialist and key promoter of FIWARE internationalization (MARTEL) are a unique asset for ensuring SmartSDK success.


Grant
Agency: European Commission | Branch: H2020 | Program: IA | Phase: ICT-20-2015 | Award Amount: 7.28M | Year: 2016

Although online education is a paramount pillar of formal, non-formal and informal learning, institutions may still be reluctant to wager for a fully online educational model. As such, there is still a reliance on face-to-face assessment, since online alternatives do not have the deserved expected social recognition and reliability. Thus, the creation of an e-assessment system that will be able to provide effective proof of student identity, authorship within the integration of selected technologies in current learning activities in a scalable and cost efficient manner would be very advantageous. The TeSLA project provides to educational institutions, an adaptive trust e-assessment system for assuring e-assessment processes in online and blended environments. It will support both continuous and final assessment to improve the trust level across students, teachers and institutions. The system will be developed taking into account quality assurance agencies in education, privacy and ethical issues and educational and technological requirements throughout Europe. It will follow the interoperability standards for integration into different learning environment systems providing a scalable and adaptive solution. The TeSLA system will be developed to reduce the current restrictions of time and physical space in teaching and learning, which opens up new opportunities for learners with physical or mental disabilities as well as respecting social and cultural differences. Given the innovative action of the project, the current gap in e-assessment and the growing number of institutions interested in offering online education, the project will conduct large scale pilots to evaluate and assure the reliability of the TeSLA system. By the nature of the product, dissemination will be performed across schools, higher education institutions and vocational training centres. A free version will be distributed, although a commercial-premium version will be launched on the market.


Alonso M.A.,University of Rochester | Bandres M.A.,National Institute of Astrophysics, Optics and Electronics
Optics Letters | Year: 2012

We introduce nonparaxial spatially accelerating waves whose two-dimensional transverse profiles propagate along semicircular trajectories while approximately preserving their shape. We derive these waves by considering imaginary displacements on spherical fields, leading to simple closed-form expressions. The structure of these waves also allows the closed-form description of pulses. © 2012 Optical Society of America.


Grant
Agency: European Commission | Branch: FP7 | Program: CSA-CA | Phase: ENV.2013.6.5-2 | Award Amount: 1.17M | Year: 2013

The purpose of the EOPOWER project is to create conditions for sustainable economic development through the increased use of Earth observation products and services for environmental applications. This purpose serves the higher goal of effective use of Earth observation for decision making and management of economic and sustainable development processes. This will be achieved through the following activities: 1. Roadshow activities to promote the increased use of EO products and services for environmental applications, including capacity building; 2. Portfolio of potential EO applications for economic development and environmental management; 3. Enhancement of the resource facility on capacity building in the GEO web portal; 4. Establishment of local focal points (nodes) that actively promote and provide capacity building on the use of EO for environmental applications effectively and at low-cost; 5. Explore the establishment of a high-level forum of stakeholders (resource providers, international organizations) that have an interest in EO for economic development and environmental applications; 6. Establishment of a central feedback node that digests and shares information on incubators, innovation, successes, experiences, visibility and provides brokerage and advice on resource mobilization. This will result in the output presented below: 1. Opportunities created for economic development, in particular in developing countries; 2. Key international economic development processes identified that require environmental information and mechanisms to develop them in a sustainable fashion; 3. Local communities and authorities have received capacity building and are able to collaborate with international development programs, use environmental EO information and products, and engage resource providers; 4. Mechanism established to market and exploit EO applications for the creation of new innovative products and support services.


Ritter G.X.,University of Florida | Urcid G.,National Institute of Astrophysics, Optics and Electronics
Information Sciences | Year: 2011

In this manuscript we propose a method for the autonomous determination of endmembers in hyperspectral imagery based on recent theoretical advancements on lattice auto-associative memories. Given a hyperspectral image, the lattice algebra approach finds in a single-pass all possible candidate endmembers from which various affinely independent sets of final endmembers may be derived. In contrast to other endmember detection methods, the endmembers found using two dual canonical lattice matrices are geometrically linked to the data set spectra. The mathematical foundation of the proposed method is first described in some detail followed by application examples that illustrate the key steps of the proposed lattice based method. © 2010 Elsevier Inc. All rights reserved.


Silich S.,National Institute of Astrophysics, Optics and Electronics | Tenorio-Tagle G.,National Institute of Astrophysics, Optics and Electronics
Astrophysical Journal | Year: 2013

The impact of radiation pressure on the dynamics of the gas in the vicinity of young stellar clusters is thoroughly discussed. The radiation over the thermal/ram pressure ratio time evolution is calculated explicitly and the crucial roles of the cluster mechanical power, the strong time evolution of the ionizing photon flux, and the bolometric luminosity of the exciting cluster are stressed. It is shown that radiation has only a narrow window of opportunity to dominate the wind-driven shell dynamics. This may occur only at early stages of the bubble evolution and if the shell expands into a dusty and/or a very dense proto-cluster medium. The impact of radiation pressure on the wind-driven shell always becomes negligible after about 3 Myr. Finally, the wind-driven model results allow one to compare the model predictions with the distribution of thermal pressure derived from X-ray observations. The shape of the thermal pressure profile then allows us to distinguish between the energy and the momentum-dominated regimes of expansion and thus conclude whether radiative losses of energy or the leakage of hot gas from the bubble interior have been significant during bubble evolution. © 2013. The American Astronomical Society. All rights reserved.


Rodriguez-Lara B.M.,National Institute of Astrophysics, Optics and Electronics
Journal of the Optical Society of America B: Optical Physics | Year: 2014

We study an intensity-dependent quantum Rabi model that can be written in terms of SU(1, 1) group elements and is related to the Buck-Sukumar model for the Bargmann parameter k = 1/2. The spectrum seems to present avoided crossings for all valid parameter sets and, thus, may be integrable. For a degenerate qubit, the model is soluble, and we construct an unbroken supersymmetric partner for it. We discuss the classical simulation of the general model in photonic lattices and show that it presents quasi-periodic reconstruction for a given initial state and parameter set. © 2014 Optical Society of America.


Bandres M.A.,National Institute of Astrophysics, Optics and Electronics | Rodriguez-Lara B.M.,National Institute of Astrophysics, Optics and Electronics
New Journal of Physics | Year: 2013

Diffraction is one of the universal phenomena of physics, and a way to overcome it has always represented a challenge for physicists. In order to control diffraction, the study of structured waves has become decisive. Here, we present a specific class of nondiffracting spatially accelerating solutions of the Maxwell equations: the Weber waves. These nonparaxial waves propagate along parabolic trajectories while approximately preserving their shape. They are expressed in an analytic closed form and naturally separate in forward and backward propagation. We show that the Weber waves are self-healing, can form periodic breather waves and have a well-defined conserved quantity: the parabolic momentum. We find that our Weber waves for moderate to large values of the parabolic momenta can be described by a modulated Airy function. Because the Weber waves are exact time-harmonic solutions of the wave equation, they have implications for many linear wave systems in nature, ranging from acoustic, electromagnetic and elastic waves to surface waves in fluids and membranes. © IOP Publishing and Deutsche Physikalische Gesellschaft.


Ostrovsky A.S.,Autonomous University of Puebla | Rickenstorff-Parrao C.,Autonomous University of Puebla | Arrizon V.,National Institute of Astrophysics, Optics and Electronics
Optics Letters | Year: 2013

We introduce the concept of the perfect optical vortex whose dark hollow radius does not depend on the topological charge. It is shown analytically and experimentally that such a vortex can be approximately generated in the Fourier transforming optical system with a computer-controlled liquid-crystal spatial light modulator. © 2013 Optical Society of America.


Torres-Torres R.,National Institute of Astrophysics, Optics and Electronics
Electronics Letters | Year: 2011

A method to determine the characteristic impedance of transmission lines considering the substrate loss is presented. The extracted data shows that at microwave frequencies the finite loss tangent parameter impacts the characteristic impedance even in a low-loss substrate. © 2011 The Institution of Engineering and Technology.

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