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The aim of this study is to reveal the role of internal organizational communication in motivating employees in public service organizations. Data were collected from 249 surveyed employees, in the mobile telecommunications sector in Kosovo, specifically in the Vala mobile company. The collected data was analyzed by using the SPSS system. The study found that information sharing had the greatest effect on employee motivation, followed by employee involvement in decision-making. This paper can be useful for managers and heads to create an organizational culture that promotes both motivation and performance. This paper is unique as it examines the links between organizational communication, motivation, and performance.

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and admin-istrative staff in Malargtie. We are very grateful to the following agencies and organizations for financial support: Argentina - Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientffica y Tecnologica (ANPCyT) ; Consejo Nacional de Investigaciones Cientfficas y Tecnicas (CONICET) ; Gobierno de la Provincia de Mendoza; Municipalidad de Malargtie; NDM Holdings and Valle Las Leas; in gratitude for their continuing cooperation over land access; Australia - the Australian Research Council; Brazil - Conselho Nacional de Desenvolvi-mento Cientffico e Tecnologico (CNPq) ; Financiadora de Estudos e Projetos (FINEP) ; FundacAo de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ) ; SAo Paulo Research Foundation (FAPESP) Grants No. 2019/101512, No. 2010/07359-6 and No. 1999/054043; Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC) ; Czech Republic - Grant No. MSMT CR LTT18004, LM2015038, LM2018102, CZ.02.1.01/0.0/0.0/16_013/0001402,CZ.02.1.01/0.0/0.0/18_046/0016010 and CZ.02.1.01/0.0/0.0/17_049/0008422; France - Centre de Calcul IN2P3/CNRS; Centre National de la Recherche Scientifique (CNRS) ; Conseil Regional IledeFrance; Departement Physique Nucleaire et Corpusculaire (PNCIN2P3/CNRS) ; Departement Sciences de l'Univers (SDUINSU/CNRS) ; Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63 within the Investissements d'Avenir Programme Grant No. ANR11IDEX000402; Germany - Bundesministerium fur Bildung und Forschung (BMBF) ; Deutsche Forschungsgemeinschaft (DFG) ; Finanzministerium BadenWurttemberg; Helmholtz Alliance for Astroparticle Physics (HAP) ; Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF) ; Min-isterium fur Innovation, Wissenschaft und Forschung des Landes NordrheinWestfalen; Minis-terium fur Wissenschaft, Forschung und Kunst des Landes BadenWurttemberg; Italy - Isti-tuto Nazionale di Fisica Nucleare (INFN) ; Istituto Nazionale di Astrofisica (INAF) ; Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR) ; CETEMPS Center of Excellence; Minis-tero degli Affari Esteri (MAE) ; Mexico - Consejo Nacional de Ciencia y Tecnologia (CONACYT) No. 167733; Universidad Nacional Autonoma de Mexico (UNAM) ; PAPIIT DGAPAUNAM; The Netherlands - Ministry of Education, Culture and Science; Netherlands Organisation for Sci-entific Research (NWO) ; Dutch national e-infrastructure with the support of SURF Cooperative; Poland-Ministry of Science and Higher Education, grant No. DIR/WK/2018/11; National Sci-ence Centre, Grants No. 2013/08/M/ST9/00322, No. 2016/23/B/ST9/01635 and No. HARMONIA 5-2013/10/M/ST9/00062, UMO2016/22/M/ST9/00198; Portugal - Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) ; Romania - Romanian Ministry of Education and Research, the Program Nucleu within MCI (PN19150201/16N/2019 and PN19060102) and project PNIIIP11.2PCCDI20170839/19PCCDI/2018 within PNCDI III; Slovenia - Slovenian Research Agency, grants P10031, P10385, I00033, N10111; Spain - Ministerio de Economia, Industria y Competitividad (FPA2017-85114-P and PID2019104676GBC32, Xunta de Galicia (ED431C 2017/07) , Junta de Andalucia (SOMM17/6104/UGR, P18-FR-4314) Feder Funds, RENATA Red Nacional Tematica de Astroparticulas (FPA2015-68783-REDT) and Maria de Maeztu Unit of Excel-lence (MDM20160692) ; U.S.A. - Department of Energy, Contracts No. DEAC0207CH11359, No. DEFR0204ER41300, No. DE-FG02-99ER41107 and No. DESC0011689; National Sci-ence Foundation, Grant No. 0450696; The Grainger Foundation; Marie CurieIRSES/EPLANET; European Particle Physics Latin American Network; and UNESCO. ; FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system. ; Argentina - Comision Nacional de Energia Atomica ; ANPCyT ; Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET) ; Australian Research Council ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF) ; Financiadora de Inovacao e Pesquisa (Finep) ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio De Janeiro (FAPERJ) ; Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/101512 2010/07359-6 1999/054043 ; Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC) ; Czech Republic Government ; Ministry of Education, Youth & Sports - Czech Republic LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422 IN2P3/CNRS ; Centre National de la Recherche Scientifique (CNRS) ; Region Ile-de-France PNCIN2P3/CNRS ; Institut Lagrange de Paris (ILP) ; LABEX ANR-10-LABX-63 ANR11IDEX000402 ; Federal Ministry of Education & Research (BMBF) ; German Research Foundation (DFG) ; Helmholtz Alliance for Astroparticle Physics (HAP) ; Helmholtz Association ; Min-isterium fur Innovation, Wissenschaft und Forschung des Landes NordrheinWestfalen ; Minis-terium fur Wissenschaft, Forschung und Kunst des Landes BadenWurttemberg; Italy - Isti-tuto Nazionale di Fisica Nucleare (INFN) ; Ministry of Education, Universities and Research (MIUR) ; CETEMPS Center of Excellence ; Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733 ; Universidad Nacional Autonoma de Mexico ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) Universidad Nacional Autonoma de Mexico ; Netherlands Organization for Scientific Research (NWO) DIR/WK/2018/11 ; National Science Centre, Poland 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 5-2013/10/M/ST9/00062 UMO2016/22/M/ST9/00198 ; Portugal - Portuguese national funds ; FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) ; Romania - Romanian Ministry of Education and Research ; Program Nucleu within MCI PN19150201/16N/2019 PN19060102 PNIIIP11.2PCCDI20170839/19PCCDI/2018 ; Slovenian Research Agency - Slovenia P10031 P10385 I00033 N10111 FPA2017-85114-P PID2019104676GBC32 ; Xunta de Galicia European Commission ED431C 2017/07 ; Junta de Andalucia SOMM17/6104/UGR P18-FR-4314 ; European Commission ; RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDT ; Maria de Maeztu Unit of Excel-lence MDM20160692 ; United States Department of Energy (DOE) DEAC0207CH11359 DEFR0204ER41300 DE-FG02-99ER41107 DESC0011689 ; National Science Foundation (NSF) 0450696 ; Grainger Foundation ; European Particle Physics Latin American Network ; UNESCO

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ); São Paulo Research Foundation (FAPESP) Grants No. 2010/07359-6 and No. 1999/05404-3; Ministério de Ciência e Tecnologia (MCT); Czech Republic – Grant No. MSMT CR LG15014, LO1305, LM2015038 and CZ.02.1.01/0.0/0.0/16_013/0001402; France – Centre de Calcul IN2P3/CNRS; Centre National de la Recherche Scientifique (CNRS); Conseil Régional Ile-de-France; Département Physique Nucléaire et Corpusculaire (PNCIN2P3/CNRS); Département Sciences de l'Univers (SDU-INSU/CNRS); Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63 within the Investissements d'Avenir Programme Grant No. ANR-11-IDEX-0004-02; Germany – Bundesministerium für Bildung und Forschung (BMBF); Deutsche Forschungsgemeinschaft (DFG); Finanzministerium Baden-Württemberg; Helmholtz Alliance for Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF); Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Ministerium für Wissenschaft, Forschung und Kunst des Landes Baden-Württemberg; Italy – Istituto Nazionale di Fisica Nucleare (INFN); Istituto Nazionale di Astrofisica (INAF); Ministero dell'Istruzione, dell'Universitá e della Ricerca (MIUR); CETEMPS Center of Excellence; Ministero degli Affari Esteri (MAE); Mexico – Consejo Nacional de Ciencia y Tecnología (CONACYT) No. 167733; Universidad Nacional Autónoma de México (UNAM); PAPIIT DGAPA-UNAM; The Netherlands – Ministerie van Onderwijs, Cultuur en Wetenschap; Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO); Stichting voor Fundamenteel Onderzoek der Materie (FOM); Poland – National Centre for Research and Development, Grants No. ERA-NET-ASPERA/01/11 and No. ERA-NET-ASPERA/02/11; National Science Centre, Grants No. 2013/08/M/ST9/00322, No. 2013/08/M/ST9/00728 and No. HARMONIA 5–2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198; Portugal – Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia (COMPETE); Romania – Romanian Authority for Scientific Research ANCS; CNDI-UEFISCDI partnership projects Grants No. 20/2012 and No.194/2012 and PN 16 42 01 02; Slovenia – Slovenian Research Agency; Spain – Comunidad de Madrid; Fondo Europeo de Desarrollo Regional (FEDER) funds; Ministerio de Economía y Competitividad; Xunta de Galicia; European Community 7th Framework Program Grant No. FP7-PEOPLE-2012-IEF- 328826; USA – Department of Energy, Contracts No. DE-AC02-07CH11359, No. DEFR02-04ER41300, No. DE-FG02-99ER41107 and No. DE-SC0011689; National Science Foundation, Grant No. 0450696; The Grainger Foundation; Marie CurieIRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Program, Grant No. PIRSES-2009-GA-246806; European Union's Horizon 2020 research and innovation programme (Grant No. 646623); and UNESCO. ; Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies observed in nature. Clues to their origin come from studying the distribution of their arrival directions. Using 3×104 cosmic rays above 8×1018 electron volts, recorded with the Pierre Auger Observatory from a total exposure of 76,800 square kilometers steradian year, we report an anisotropy in the arrival directions. The anisotropy, detected at more than the 5.2σ level of significance, can be described by a dipole with an amplitude of 6.5+1.3−0.9% towards right ascension αd=100±10 degrees and declination δd=−24+12−13 degrees. That direction indicates an extragalactic origin for these ultra-high energy particles.

This paper aims to explain the legal, political and moral obligation of the European Union institutions in the promotion, advancement, respect, and implementation of human rights and freedoms as a universal value, and above all as binding legal- political principles during their efforts in relations with actors both inside and outside the EU. This research work simultaneously analyzes and interprets international legal rules that regulate human rights. Moreover, the cases and means in promoting the human rights used by the European Union in different cultural regions have been compared and analyzed as well as the possibility of changing the approach of EU policy towards countries where the highest level of resistance exist in the accepting of such values.

The contract of sale represents one of the most important contracts on internal and external circulation of goods. This contract is considered one of the oldest and it has the same purpose in all the countries worldwide. With this contract, the seller is obliged to deliver the goods he sells to the buyer, in order for him to gain the right of ownership, whereas the buyer is obliged to pay the price as per the contract. validity conditions, resolution and consequences of resolution, etc.In some occasions, the contracts are subjects of different conflicts which reach the only solution through courts. Given the fact that there are different types of the contracts of sale, it is important that we make efforts in order to study them, difficulties we encounter with regards to the circulation of goods and money.