Listar Departamento de Ingeniería de Computadores, Automática y Robótica por financiación

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      Financiación
      Taif University, Taif, Saudi Arabia TURSP-2020/125 [1]
      TecNM-15340.22-P [1]
      TecNM-5654.19-P [1]
      The Consolidated Research Group MATHMODE (IT1456-22) [1]
      The article processing charge (APC) was funded by the Research Group “Ingeniería Cartográfica” (Grant No. PAIDI-TEP-164 from the Regional Government of Andalucía) from the University of Jaén. [1]
      The authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contractANR-15- CE31-0020 ), Centre National de la Recherche Scientifique (CNRS) , Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF) , IdEx program and UnivEarthS Labex programatSorbonneParisCité( ANR-10-LABX-0023 and ANR-11-IDEX-0 0 05-02 ), France; Deutsche Forschungsgemeinschaft (DFG) , Germany; The General Secretariat of Research and Technol- ogy (GSRT) , Greece; Istituto Nazionale di Fisica Nucleare (INFN) , Ministero dell’Istruzione, dell’Universitàedella Ricerca(MIUR) , Italy; Ministry of Higher Education , Scientific Research and Professional Training, Morocco; Nederlandse organisatie voor Weten- schappelijk Onderzoek (NWO) , the Netherlands; The National Science Centre , Poland ( 2015/18/E/ST2/00758 ); National Authority for Scientific Research (ANCS) , Romania; Plan Estatal de Investigación (refs. FPA2015-65150-C3-1-P , -2-P and -3-P , ( MINECO /FEDER)), Severo Ochoa Centre of Excellence program ( MINECO ), Red Consolider MultiDark, (ref. FPA2017-90566-REDC , MINECO ) and Prometeo and Grisolía programs ( Generalitat Valenciana ), Spain. [1]
      The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), France; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell’Universitàe della Ricerca (MIUR), Italy; Agence de l’Oriental and CNRST, Morocco; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandseorganisatie voor Wetenschappelijk Onderzoek (NWO), The Netherlands; National Authority for Scientific Research (ANCS), Romania; Plan Estatal de Investigación (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolía programs (Generalitat Valenciana), Spain. The KM3NeT collaboration has received funding from the European Community Sixth Framework Programme under Contract 011937 and the Seventh Framework Programme under Grant Agreement 212525. [1]
      The authors also want to acknowledge received funding from the European Union’s Horizon 2020 research and innovation programme under Grant Agreement #769553 [1]
      The authors thank Ana Palomares for revising their English text. This work has been supported by the National Grant (AP2007-00275), the projects ARC-VISION (TEC2010-15396), ITREBA (TIC-5060), and the EU project TOMSY (FP7-270436). [1]
      The EGIA project (KK-2022/00119 [1]
      The Parkes radio telescope and the Australia Telescope Compact Array are part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. The GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. VLAis run by theNational Radio Astronomy Observatory (NRAO). NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work was performed on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Government’s Education Investment Fund. This work is also based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org. Funding from the European Research Council under the European Union’s Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement n. 617199 (EP). Access to the Lovell Telescope is supported through an STFC consolidated grant. The 100-m telescope in Effelsberg is operation by the Max- Planck-Institut für Radioastronomie with funds of the Max-Planck Society. The Sardinia Radio Telescope (SRT) is funded by the Department of University and Research (MIUR), the Italian Space Agency (ASI), and the Autonomous Region of Sardinia (RAS) and is operated as National Facility by the National Institute for Astrophysics (INAF). TB and RWW are grateful to the STFC for financial support (grant reference ST/P000541/1). Research support to IA is provided by the Australian Astronomical Observatory. The ANTARES authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10- LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR- 11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001- 02), Région Île-de-France (DIM-ACAV), Région Alsace (contrat CPER), Région Provence-Alpes-Côte d’Azur, Département du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium für Bildung und Forschung (BMBF), Germany; IstitutoNazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economía y Competitividad (MINECO): Plan Estatal de Investigación (refs. FPA2015- 65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolía programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory’s High Energy Astrophysics Division. This work is based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. This paper makes use of software developed for the Large Synoptic Survey Telescope. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org. RPE/MK gratefully acknowledges support from ERC Synergy Grant "BlackHoleCam" Grant Agreement Number 610058 [1]
      The publication of this article was supported by projects TIN2015-71873-R and P12-TIC 2082. [1]
      The research leading to these results has received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 604102 (Human Brain Project) and from the European Unions Horizon 2020 Research and Innovation Programme under Grant Agreement No. 720270 (HBP SGA1). [1]
      The study was approved by The Research Ethics Committee of the University of Granada (3582/CEIH/2023) [1]
      This research received fund by the Ibero-American Postgraduate University Association (AUIP). [1]
      This research was funded by [Ministry of Economy and Competitiveness (Spain)] grant number [TIN2015-67020P], [Ministry of Economy and Competitiveness (Spain)] grant number [DPI2015-69098-REDT], [Junta of Andalucia (Spain)] grant number [P11-TIC-7983], [Spanish National Youth Guarantee Implementation Plan] grant number [Research contract], [Nicolo Association for the R+D in neurotechnologies for disability] grant number [Research support], and [Orden Hospitalaria San Juan de Dios] grant number [Beca investigacion]. [1]
      This research was funded by University of Naples Federico II through the Finanziamento della Ricerca di Ateneo (FRA) 2020 (CUP: E69C20000380005) and has been partially supported by the ”Programa de ayuda para Estancias Breves en Centros de Investigación de Calidad” of the University of Málaga and the research project BIA2016-79270-P, the Spanish Ministry of Science, Innovation and Universities and the European Regional Development Fund-ERDF (Fondo Europeo de Desarrollo Regional-FEDER) under project PGC2018-096156-B-I00 Recuperación y Descripción de Imágenes mediante Lenguaje Natural usando Técnicas de Aprendizaje Profundo y Computación Flexible and the Andalusian Government under Grant P18-RT-2248. [1]
      This research was partly funded by the research project “Progress in Computer Architectures for Automatic Learning using Heterogeneous Sources: Health and Well-Being Applications” (TIN2015-71873-R). [1]
      This research was supported by an Institute for Information & Communications Technology Promotion (IITP) grant funded by the Korean government (MSIT) (No. 2017-0-00655). This research was supported by the MSIT (Ministry of Science and ICT), Korea, under the ITRC (Information Technology Research Center) support program (IITP-2017-0-01629) supervised by the IITP (Institute for Information & communications Technology Promotion). This research was supported by the MIST (Ministry of Science and ICT), Korea, under the National Program for Excellence in SW supervised by the IITP (Institute for Information & communications Technology Promotion) (2017-0-00093). [1]
      This study was funded by the Helmholtz Alliance for Systems Biology (Germany), grant to MAA-N, and the Government of Andalusia (Spain), Project P09-TIC-175476. [1]