Ethical living and work self efficacy beliefs of academicians of higher education in ASIA: A key determinant of one's belief in one's ability to achieve the desired result in a precise state of affairs
Eigenvalue; Enactive attainment; Factor rotation; Measure of sampling adequacy; Multiple likert scales; Vicarious experience
Ethical academicians are perfectly virtuous. They always strive for greater virtue and follow strictly the moral stands of their profession. The ethical living and self-efficacy are important to them because of being fair and honest in their academics. Determinants of ethics include knowledge, values, attitude and intention. The domain-specific framework developed by Verbeke et al. (2004) has been considered as fundamental for identifying the dimensionality of work Self-efficacy and ethical challenges of academicians. A comprehensive literature review is undertaken regarding the concept of work Self-efficacy to assess workers' confidence and their ethical living in the workplace. This article examines theoretically and analytically the antecedent processes and information cues involved in the formation of work self-efficacy. Theoretical and numerical analysis of the key determinants of work self-efficacy increases the understanding of moral values, truthful fair and honest. Factors which decisively affect ethical living were identified from literature collected from the academicians who are working in the Five Regions of Asia-Central Asia (Tajikistan, Uzbekistan, Kazakhstan, Turkmenistan, Kyrgyzstan) East Asia (China, Mongolia, North Korea, South Korea, Japan, Hong Kong, Taiwan, Macau) South Asia (Sri Lanka, Bangladesh, India, Afghanistan, Pakistan, Bhutan, Nepal, the Maldives) through Google classroom. Methods of Statistical Analysis of self-efficacy data are descriptive statistics, Pearson Correlation Coefficient and Kolmogorov-Smirvnos normality test and KruskalWallis one-way analysis of variance and Principal Component Analysis. Positive, mastery experiences give academicians a sense of accomplishment when they have faced a challenge ethically. Positive Zeal during Academic interaction, vicarious experiences that occur when academician see others succeed and feel an increased sense of their own ability to succeed. Sincere & deeper self, mingling with students, Social persuasion increase a teachers sense of confidence and ability to succeed. A proper plan of action has drawn special attention, and inferences pertaining to future research are discussed at the end of the critique. 2019, Sciedu Press. All rights reserved.
International Journal of Higher Education, Vol-8, No. 6, pp. 203-221.
https://doi.org/10.5430/ijhe.v8n6p203 https://www.scopus.com/inward/record.uri?eid=2-s2.0-85074937312&doi=10.5430%2fijhe.v8n6p203&partnerID=40&md5=458fd539896206795c08bc1b72b91550
Sivarethinamohan R., Christ (Deemed to be University), Hosur Road, Bangalore, 560 029, India; Sujatha S., K. Ramakrishnan College of Technology, Tiruchirappalli, Tamil Nadu, India
Ethical sensitivity of aspiring business leaders: Indian context
Business; Ethical Sensitivity; Ethics Programs; Leadership; University Education; Whole-Person Education
Ethical business leaders can make a huge impact in creating flourishing communities in todays world where Corporations are immensely powerful. In the business context, the first step of ethical decision-making is recognising the ethical dimension of a business problem itself, ethical sensitivity. This study investigates the impact of ethics education in the business program as well as role of early education environment in influencing the ethical sensitivity of business students. It was found that both these variables have significant impact in the ethical sensitivity of the participants of the study. The research has implications in revisiting the ethics education in universities and the role of early education environment in developing ethical business leaders for the sustainable future of our country. 2020 Journal of Dharma: Dharmaram Journal of Religions and Philosophies (DVK, Bangalore).
Journal of Dharma, Vol-45, No. 1, pp. 125-144.
Business ethics; Collaborative partnerships; Ethical considerations; Ethical sourcing; Impact assessment; Labor relations; Regulatory compliance; Responsible consumption; Responsible procurement; SDGs; Suppliers assessment; Sustainable development; Sustainable supply chain management
In an era where sustainable development is a celebrated concept, the notion of ethical sourcing has been explored comprehensively as companies are making a conscious and sustainable effort to gauge their supply chains and examine the sources of procurement of their material and services. This chapter delves deeper into the importance of ethical sourcing, focusing on its benefits and fundamental needs. It also talks about why ethical sourcing is an essential concept in corporate realms, drawing a distinction between sustainable and ethical sourcing. Today, ethical sourcing can be an important tool in the hands of corporations to draw a competitive edge and there would be serious repercussions of indulging in unethical practices. Further, it discusses key principles that act as a beacon of light for sourcing the material ethically, the three levels of ethical sourcing, and how technology can be leveraged to ensure the same. It is crucial to have partnerships and collaborations for sustainable procurement along with robust mechanisms to measure the impact of ethical sourcing. 2026 Elsevier Inc. All rights are reserved, including those for text and data mining, AI training, and similar technologies.
Agrawal, Devika; Kumar, Amit; Kumar, Kishore
International Encyclopedia of Business Management;pp.Vol1:774-Vol1:778
Restricted Access; Hardcopy may be available in the library
https://doi.org/10.1016/B978-0-443-13701-3.00016-5 https://www.scopus.com/pages/publications/105029608468?origin=resultslist
Agrawal D., Institute of Business Management, GLA University, Mathura, India; Kumar A., CHRIST (Deemed to be University) NCR Campus, Ghaziabad, India; Kumar K., School of Management, Bennett University, Greater Noida, India
Ethical Tenets of Stock Price Prediction Using Machine Learning Techniques: A Sustainable Approach
The visible decline of ethics primarily gets reflected in financial markets, as it portrays human actions and sentiments in numerical terms than any sector. Accuracy in Stock market prediction remains inefficient due to many known and unknown variables. Academia and industry recently relied on ML at large to track the market and monetise the movements. The norms of fairness, accuracy, dependability, transparency in financing are left unattended in ML prediction models with assumptions far from reality. This study focuses on the ethical dimension of Machine Learning models and generates a sustainable framework for investors. Specifically, the Sustainable Development goals (SDG) can enhance the prediction models in ML with improved efficiency. Along with SDG, this research broadens the variables' horizon of prediction in ML of computer science domain with concepts of Socially responsible Investing (SRI), Environmental Social and Corporate Governance (ESG), and Carbon footprints. With One hundred fifteen articles reviewed, the proposed framework ensures sustainability in investments at the grassroots level. The Electrochemical Society
ECS Transactions, Vol-107, No. 1, pp. 137-149.
https://doi.org/10.1149/10701.0137ecst https://www.scopus.com/inward/record.uri?eid=2-s2.0-85130550434&doi=10.1149%2f10701.0137ecst&partnerID=40&md5=22066fec368614820c6a6bcdbc43dd87
Vellaiparambill A., Department of Commerce, Christ Deemed to be University, Bangalore, India; Natchimuthu N., Department of Commerce, Christ Deemed to be University, Bangalore, India
The accelerated development of generative artificial intelligence has challenged the principles of creative practice and has laid down them as the established assumptions about the originality, intentions, and cultural significance of humans. This chapter critically discusses the intersection of AI- generated creativity with psychological theories of the agency of humans, social and cultural structures of meaning- making and emerging ethical issues of authorship, ownership and cultural representation. With reference to past and present studies, empirical results and technological advances, the chapter aims to point out the two- sided character of AI as the accelerant of creative possibility and the de- disturbing factor in artistic, economic and cultural ecosystems. It assesses the most notable risks, such as bias, cultural homogenization, deepfakes, labour displacement, and environmental costs, besidesacknowledging the opportunities to democratize, make it more accessible and allow human- machine collaboration. 2026 by IGI Global Scientific Publishing. All rights reserved.
Redefining Global Creative Sectors Through AI and Human Augmentation;pp.119-151
https://doi.org/10.4018/979-8-3373-7153-5.ch005 https://www.scopus.com/pages/publications/105032954594?origin=resultslist
Wadhwa M.; Ganguly D.G., School of Business and Management, Christ University, Delhi NCR Campus, India
Digital media; Ethics; Journalists; Professionalism; Technology
Marshall McLuhan proposed that technological changes impact society. Digital media has enabled journalists to reach their audiences instantly with the news. Journalists need more time to decide what to report and how to present it. Ethics is the belief about what is morally correct or acceptable. Traditionally, newspaper reporters devised moral codes to help them in their professional decision-making. There emerged an almost universal set of principles that guided journalists in their profession. Television journalists were compelled to draw up a code of ethics to ward off criticism about sensationalism. Digital media has blurred the distinction between professional and citizen journalists. Twitter allows the man in the street to break the news as it happens. Privacy and copyright are just two of the significant issues that digital journalists must deal with. Digital media throws up these challenges, and this chapter aims to answer them. Is it acceptable to extend the ethical standards of old media to the digital space, or do we need a new set of ethics to guide digital journalists? New principles and ethical standards are being framed to tackle the unique challenges of digital news media. The Author(s), under exclusive license to Springer Nature Singapore Pte Ltd. 2024. All rights reserved.
Handbook of Digital Journalism: Perspectives from South Asia, pp. 545-553.
Naresh Rao H., Department of Media Studies, Christ (Deemed to be University), Bangalore, India
ETHICS OF TECHNOLOGY-ASSISTED NEUROCOGNITIVE REHABILITATION
The integration of invasive, non-invasive, and external technology into healthcare has significantly transformed neurocognitive rehabilitation. It has transformed the relationship between the patients and their care providers, caretakers, and digital agents of care. It can aid the rehabilitating agents at all levels of intervention, stages of patients response, and interactions between them and the patients. While technology can improve the efficiency and effectiveness of neurocognitive rehabilitation, it raises fundamental ethical issues. The three types of technology invasive, noninvasive, and external pose different types of issues that must be addressed by the care providers, caretakers, the digital agents, and the patients. The ethical issues must be balanced against the potential efficiency and effectiveness of the technologies in making intervention decisions. The chapter presents an Ontology of Ethics of Technology-Driven Neurocognitive Rehabilitation as a framework to parse these complex issues clearly, concisely, and comprehensively. It provides a roadmap to address the ethics systemically and systematically. Technology-assisted neurocognitive rehabilitation can deeply affect the mind, body, and spirit of the patient. It is an emerging field and there is little literature on its ethics. The framework can be used to develop a roadmap for research, policies, and practice. 2026 selection and editorial matter, K. Jayasankara Reddy; individual chapters, the contributors. All rights reserved.
Chandra, Ajay; Ramaprasad, Arkalgud; Rangaswamy, Madhavi
The Routledge International Handbook of Neurocognitive Rehabilitation: Practices, Innovations, and Future Directions;pp.269-280
https://doi.org/10.4324/9781003646662-20 https://www.scopus.com/pages/publications/105028463841?origin=resultslist
Chandra A., School of Psychological Sciences, Christ (Deemed to be University), Bengaluru, India, School of Arts, Humanities, and Social Sciences, Chanakya University, Bengaluru, India; Ramaprasad A., Department of Information and Decision Sciences, University of Illinois, Chicago, United States; Rangaswamy M., School of Psychological Sciences, Christ (Deemed to be University), Bengaluru, India
India News, Education, DH Education, Ethics
Choosing the appropriate type of leader that may best be suitable for an academic organisation becomes tricky
Ethics, the compass for academic leadership
But again, with a multitude of leadership styles available, choosing the appropriate type that may best be suitable to the organisation becomes tricky
Ethnic Food: A Solution With Sustainable Food Resources A Study On Consumer Awareness Of Ethnic Food And Its Impact On Consumption Attitude
Food has seen numerous transformations over the centuries and has been a focus of study pertaining to culture and evolution. Besides being a celebration of diversity and a marker of human adaptations, food is also a broad knowledge domain that represents various geographic, cultural and lifestyle outlooks. Ethnic food relates to a heritage or the culture of an ethnic group with them incorporating the local produce and animal sources into their diet. Ethnic food also has a sustainability aspect to it in terms of food miles and carbon emissions since more transportation involved means higher level of GHG released, economic aspect such as with composition changes and food security, and community relationship. This paper finds that when consumer awareness of ethnic food increases, the consumption attitude towards it does, too. This could be of importance in policy implementation and identifying sustainability systems. A connection with the land and a community relationship involving food could help represent more ethnic food, to increase awareness on a global level and also allow more people to experience these vast cultural diversities. If understood well and implemented, ethnic food could be of use as a tourism brochure, sustainability driver, economical promoter and community supporter. The Electrochemical Society
ECS Transactions, Vol-107, No. 1, pp. 13555-13574.
https://doi.org/10.1149/10701.13555ecst https://www.scopus.com/inward/record.uri?eid=2-s2.0-85130535436&doi=10.1149%2f10701.13555ecst&partnerID=40&md5=841f59710fe3c9c178d2da992d98a603
Fukey L.N., Department of Hotel Management, Christ University, Bengaluru, 560029, India; Reddy N.S., Department of Hotel Management, Christ University, Bengaluru, 560029, India; Wankhar V., Department of Hotel Management, Christ University, Bengaluru, 560029, India
In the context of food security, two things are significant. To ensure availability, affordability and accessibility of adequate food to people throughout the country. Also, to promote entrepreneurship for sustainable food production and supply. This paper highlights differences between food security and food insecurity. The global population in 2050 is predicted at 9 billion in which case the output must double considering the dwindling and degrading resources. This may be a challenge for agronomists and policy-makers. Considering that food security must be achieved at individual, household, district, national and global levels, India may need an Integrated Farming System (IFS) to take agriculture further. There are numerous challenges besides the environment that must be considered for this. It is important to ensure that the dignity of the farmer is not compromised while strategizing food security. Currently, private-public partnerships are being introduced in some places as a potential model. However, all stakeholders in food security have their task cut out (1). This paper is a review of existing literature to understand the level of information we have documented. It tries to highlight ways in which consumption of ethnic food could be a way forward in terms of food security and sustainability. The Electrochemical Society
ECS Transactions, Vol-107, No. 1, pp. 13547-13554.
https://doi.org/10.1149/10701.13547ecst https://www.scopus.com/inward/record.uri?eid=2-s2.0-85130524459&doi=10.1149%2f10701.13547ecst&partnerID=40&md5=bc7e6d33cbdbdadcbe608863233d0a08
Reddy N.S., Department of Hotel Management, Christ University, Bengaluru, 560029, India; Fukey L.N., Department of Hotel Management, Christ University, Bengaluru, 560029, India; Wankhar V., Department of Hotel Management, Christ University, Bengaluru, 560029, India
Ethnographic research on primary education of tribals: a scoping review
Cultural inclusiveness; Ethnography; Indigenous people; Multilingual education; Primary education
Ethnographic research offers comprehensive learning outcomes by examining the socio-emotional, economic and cultural components crucial for comprehending marginalized groups experiences. This study aims to examine the methodologies used in studies and the gaps in the literature on the primary education of tribal communities, highlighting the limitations of the current research approaches. Using the preferred reporting items for systematic reviews and meta-analyses (PRISMA) of Arksey and OMalleys six-step framework, the scoping review has considered 19 studies of 406 research articles published from 2015 to 2024 across the databases Scopus, JSTOR, and ERIC. The review highlights that most of these studies used descriptive survey design, mixed-method research design, and ethnographic research design. While the first two document barriers, the ethnographic studies provide richer cultural in-depth also. However, gaps in the literature include a lack of interventions for specific tribes, such as the Mannan community in Kerala, India, and the integration of indigenous knowledge, which is only possible through cultural inclusiveness. The findings suggest that future research should prioritize interdisciplinary collaboration and teacher training in multilingual education (MLE) through ethnographic methods for developing culturally sensitive interventions. These recommendations aim to contribute to developing more culturally inclusive educational practices and policies in the primary education curricula. 2026, Intelektual Pustaka Media Utama. All rights reserved.
Mathew, Jemy Jose; Thomas, Kennedy Andrew
Journal of Education and Learning;Volume;20;Issue;2;pp.1032-1042
All Open Access; Hybrid Gold Open Access
https://doi.org/10.11591/edulearn.v20i2.23687 https://www.scopus.com/pages/publications/105034323963?origin=resultslist
Mathew J.J., Department of Education, CHRIST (Deemed to be University), Bengaluru, India; Thomas K.A., Department of Education, CHRIST (Deemed to be University), Bengaluru, India
Ethylenediamine modified carbon nanospheres from biomass for selective membrane filtration
The present work investigates the antifouling properties dye and antibiotic removal efficiency of PVDF/E-CNS membranes. Carbon nanospheres (CNS) derived from rice husk (RH) were pyrolyzed at 800 C. Further, ethylenediamine functionalized carbon nanospheres (E-CNS) were obtained via in situ decoration of ethylenediamine on acid-functionalized carbon nanospheres (O-CNS). The synthesized E-CNS were characterized by techniques such as XRD, FESEM, Raman spectroscopy, FTIR and BET. The membranes were fabricated by integrating E-CNS at varying loadings (0.10.7 wt%) via a non-solvent induced phase separation (NIPS) technique. The membrane properties were assessed through FESEM, water contact angle measurements, pure water flux, antifouling studies and membrane rejections. In comparison to the other developed membranes, PVDF-2 with 0.3 wt% E-CNS loading displayed optimal performance, pure water flux (PWF) of ?318.90 L m?2 h?1, flux recovery ratio (FRR) > 90% up to three cycles, improved contact angle (80.24 to 68.44) and reduced roughness. Furthermore, PVDF-2 achieved dye rejection of methyl orange (MO 93.2%) and rhodamine B (RB 94.6%), and antibiotic rejection of amoxicillin (AM 93.8%) and tetracycline (TC 94.1%), respectively. These findings demonstrate the integration of E-CNS derived from a bio-source, making them a promising additive to improve PVDF membrane performance. This journal is The Royal Society of Chemistry
Patel, B. G. Maya; Islam, Sk Safikul; Mandal, Samir; Bose, Suryasarathi; Hegde, Gurumurthy
Nanoscale Advances;Volume;7;Issue;24;pp.8074-8084
https://doi.org/10.1039/d5na00661a https://www.scopus.com/pages/publications/105023480507?origin=resultslist
Patel B.G.M., Department of Chemistry, Christ University, Karnataka, Bengaluru, 560029, India, Centre for Advanced Research and Development (CARD), Christ University, Karnataka, Bengaluru, 560029, India; Islam S.S., Innovation and Translational Research Hub (iTRH), Department of Chemistry, School of Engineering, Presidency University, Karnataka, Bengaluru, 560064, India; Mandal S., Department of Materials Engineering, Indian Institute of Science, Karnataka, Bengaluru, 560012, India; Bose S., Department of Materials Engineering, Indian Institute of Science, Karnataka, Bengaluru, 560012, India; Hegde G., Department of Chemistry, Christ University, Karnataka, Bengaluru, 560029, India, Centre for Advanced Research and Development (CARD), Christ University, Karnataka, Bengaluru, 560029, India
Etiology and Advanced Detection Techniques for Fetal Brain Abnormalities: A Comprehensive Study
causes; Fetal brain abnormalities; Fetal MRI; Medical Imaging; Segmentation techniques
In the modern world, women's health deserves greater focus, particularly in a country like India and particularly during pregnancy. The health of mother's as well as baby's is important throw-out this process. According to a survey, three cases out of a thousand have abnormalities in fetal brain. The likelihood of survival of mother and child significantly increased by early identification of these diseases. Several procedures, including fetal ultrasound, MRI, fetal echocardiography etc. must be carried out during pregnancy in order to monitor fetal development. Pregnancyrelated MRI-scans always practiced to identify and treat fetal brain disorders in former stages. It is possible to identify, examin fetal brain problems early on by doing a prenatal MRI examination. The diagnosis of issues with fetal brain MRI imaging involves several crucial procedures. Among these are image segmentation; image analysis, which comprises extracting characteristic characteristics, improving image quality, identifying relevant patterns, and categorising images based on predefined standards. Classification determines if an anomaly is present or not. Analysing pictures can be difficult due to the wide range of shapes, spatial arrangements, and intensities that are present. The primary subjects of this work are the review and comparison of various fetal brain malformations, as well as their causes and commonalities. 2025 IEEE.
2025 10th International Conference on Research in Intelligent Computing in Engineering, RICE 2025;
Institute of Electrical and Electronics Engineers Inc.
https://doi.org/10.1109/RICE67503.2025.11439996 https://www.scopus.com/pages/publications/105037436581?origin=resultslist
Gaikwad N., School of Sciences, CHRIST UNIVERSITY, Department of Computer Science, India; Vijayalakshmi S., School of Sciences, CHRIST UNIVERSITY, Department of Computer Science, India
ETL and Business Analytics Correlation Mapping with Software Engineering
Business analysis; Data science; ETL process; SDLC; Software engineering
Large information approach can't be effectively accomplished utilizing customary information investigation strategies. Rather, unstructured information requires specific information demonstrating methods, apparatuses, and frameworks to separate experiences and data varying by associations. Information science is a logical methodology that applies scientific and measurable thoughts and PC instruments for preparing large information. At present, we all are seeing an exceptional development of data created worldwide and on the web to bring about the idea of large information. Information science is a significant testing zone because of the complexities engaged with consolidating and applying various strategies, calculations, and complex programming procedures to perform insightful investigation in huge volumes of information. Thus, the field of information science has developed from enormous information, or huge information and information science are indistinguishable. In this article we have tried to create bridge between ETL and software engineering. 2021, The Author(s), under exclusive license to Springer Nature Singapore Pte Ltd.
Advances in Intelligent Systems and Computing, Vol-1311 AISC, pp. 501-511.
Springer Science and Business Media Deutschland GmbH
Paikaray B.K., Department of CSE, Centurion University of Technology and Management, Bhubaneswar, Odisha, India; Dube M.R., Department of CSE, Vishwakarma Institute of Technology, Pune, India; Swain D., Department of Data Science Department, Christ University, Lavasa, Pune, India
Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster: Detection of parsec-scale star formation within the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
Galaxies: clusters: intracluster medium; Galaxies: evolution; Galaxies: spiral; Galaxies: star formation
Euclid is delivering optical and near-infrared imaging data over 14 000 deg2 on the sky at spatial resolution and surface brightness levels that can be used to understand the morphological transformation of galaxies within groups and clusters. Using the Early Release Observations (ERO) of the Perseus cluster, we demonstrate the capability offered by Euclid in studying the nature of perturbations for galaxies in clusters. Filamentary structures are observed along the discs of two spiral galaxies, UGC 2665 and MCG +07-07-070, with no extended diffuse emission expected from tidal interactions at surface brightness levels of a30 mag arcseca 2. The detected features exhibit a good correspondence in morphology between optical and near-infrared wavelengths, with a surface brightness of a25 mag arcseca 2, and the knots within the features have sizes of a 100 pc, as observed through IE imaging. Using the Euclid, CFHT, UVIT, and LOFAR 144 MHz radio continuum observations, we conducted a detailed analysis to understand the origin of the detected features. We constructed the Euclid IEaYE, YEaHE, and CFHT u ar, g ai colour-colour plane and show that these features contain recent star formation events, which are also indicated by their H? and NUV emissions. Euclid colours alone are insufficient for studying stellar population ages in unresolved star-forming regions, which require multi-wavelength optical imaging data. There are features with red colours that can be explained by dust being stripped along with the gas in these regions. The morphological shape, orientation, and mean age of the stellar population, combined with the presence of extended radio continuum cometary tails can be consistently explained if these features formed during a recent ram-pressure stripping event. This result further confirms the exceptional qualities of Euclid in the study of galaxy evolution in dense environments. 2025 EDP Sciences. All rights reserved.
George, K.; Boselli, A.; Cuillandre, J.-C.; Kmel, M.; Lann, A.; Bellhouse, C.; Saifollahi, T.; Mondelin, M.; Bolzonella, M.; Joseph, P.; Roberts, I.D.; Van Weeren, R.J.; Liu, Q.; Sola, E.; Urbano, M.; Baes, M.; Peletier, R.F.; Klein, M.; Davies, C.T.; Zinchenko, I.A.; Sorce, J.G.; Poulain, M.; Aghanim, N.; Altieri, B.; Amara, A.; Andreon, S.; Auricchio, N.; Baccigalupi, C.; Baldi, M.; Balestra, A.; Bardelli, S.; Battaglia, P.; Biviano, A.; Bonino, D.; Branchini, E.; Brescia, M.; Brinchmann, J.; Camera, S.; Cas-Herrera, G.; Capobianco, V.; Carbone, C.; Carretero, J.; Casas, S.; Castellano, M.; Castignani, G.; Cavuoti, S.; Chambers, K.C.; Cimatti, A.; Colodro-Conde, C.; Congedo, G.; Conselice, C.J.; Conversi, L.; Copin, Y.; Courbin, F.; Courtois, H.M.; Cropper, M.; Da Silva, A.; Degaudenzi, H.; De Lucia, G.; Di Giorgio, A.M.; Dole, H.; Douspis, M.; Dubath, F.; Dupac, X.; Dusini, S.; Escoffier, S.; Farina, M.; Faustini, F.; Ferriol, S.; Fotopoulou, S.; Frailis, M.; Franceschi, E.; Galeotta, S.; Gillis, B.; Giocoli, C.; Gracia-Carpio, J.; Grazian, A.; Grupp, F.; Haugan, S.V.H.; Holmes, W.; Hook, I.M.; Hormuth, F.; Hornstrup, A.; Hudelot, P.; Jahnke, K.; Jhabvala, M.; Keihen, E.; Kermiche, S.; Kiessling, A.; Kubik, B.; Kunz, M.; Kurki-Suonio, H.; Le Brun, A.M.C.; Le Mignant, D.; Ligori, S.; Lilje, P.B.; Lindholm, V.; Lloro, I.; Mainetti, G.; Maino, D.; Maiorano, E.; Mansutti, O.; Marggraf, O.; Markovic, K.; Martinelli, M.; Martinet, N.; Marulli, F.; Massey, R.; Maurogordato, S.; Medinaceli, E.; Mei, S.; Mellier, Y.; Meneghetti, M.; Merlin, E.; Meylan, G.; Mohr, J.J.; Mora, A.; Moresco, M.; Moscardini, L.; Nakajima, R.; Neissner, C.; Nichol, R.C.; Niemi, S.-M.; Nightingale, J.W.; Padilla, C.; Paltani, S.; Pasian, F.; Pedersen, K.; Percival, W.J.; Pettorino, V.; Pires, S.; Polenta, G.; Poncet, M.; Popa, L.A.; Pozzetti, L.; Raison, F.; Rebolo, R.; Renzi, A.; Rhodes, J.; Riccio, G.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Sakr, Z.; Sapone, D.; Sartoris, B.; Schewtschenko, J.A.; Schirmer, M.; Schneider, P.; Secroun, A.; Seidel, G.; Seiffert, M.; Serrano, S.; Sirignano, C.; Sirri, G.; Stanco, L.; Steinwagner, J.; Tallada-Cresp P.; Taylor, A.N.; Tereno, I.; Toft, S.; Toledo-Moreo, R.; Torradeflot, F.; Tutusaus, I.; Valentijn, E.A.; Valenziano, L.; Valiviita, J.; Vassallo, T.; Verdoes Kleijn, G.; Veropalumbo, A.; Wang, Y.; Weller, J.; Zamorani, G.; Zerbi, F.M.; Zucca, E.; Burigana, C.; Gabarra, L.; Mart-Fleitas, J.; Scottez, V.
Astronomy and Astrophysics;Volume;701;Issue;;Article No.;A40;
All Open Access; Gold Open Access; Green Open Access
https://doi.org/10.1051/0004-6361/202554836 https://www.scopus.com/pages/publications/105015302152?origin=resultslist
George K., University Observatory, LMU, Faculty of Physics, Scheinerstrasse 1, Munich, 81679, Germany; Boselli A., Aix-Marseille Universite, CNRS, CNES, LAM, Marseille, France; Cuillandre J.-C., UniversitParis-Saclay, UniversitParis Cite, CEA, CNRS, AIM, Gif-sur-Yvette, 91191, France; Kmel M., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany; Lann A., Universitde Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, Strasbourg, 67000, France; Bellhouse C., School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, United Kingdom; Saifollahi T., Universitde Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, Strasbourg, 67000, France; Mondelin M., UniversitParis-Saclay, UniversitParis Cite, CEA, CNRS, AIM, Gif-sur-Yvette, 91191, France; Bolzonella M., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Joseph P., Indian Institute of Astrophysics, Koramangala II Block, Bangalore, 560034, India, Department of Physics and Electronics, CHRIST (Deemed to Be University), Bangalore, 560029, India; Roberts I.D., Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, N2L 3G1, ON, Canada; Van Weeren R.J., Leiden Observatory, Leiden University, Einsteinweg 55, Leiden, 2333 CC, Netherlands; Liu Q., Leiden Observatory, Leiden University, Einsteinweg 55, Leiden, 2333 CC, Netherlands; Sola E., Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom; Urbano M., Universitde Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, Strasbourg, 67000, France; Baes M., Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, Gent, 9000, Belgium; Peletier R.F., Kapteyn Astronomical Institute, University of Groningen, PO Box 800, Groningen, 9700 AV, Netherlands; Klein M., Ludwig-Maximilians-University, Schellingstrasse 4, Munich, 80799, Germany; Davies C.T., Ludwig-Maximilians-University, Schellingstrasse 4, Munich, 80799, Germany; Zinchenko I.A., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany; Sorce J.G., Univ. Lille, CNRS, Centrale Lille, UMR 9189, CRIStAL, Lille, 59000, France, UniversitParis-Saclay, CNRS, Institut da Astrophysique Spatiale, Orsay, 91405, France; Poulain M., Space Physics and Astronomy Research Unit, University of Oulu, Pentti Kaiteran katu 1, Oulu, FI-90014, Finland; Aghanim N., UniversitParis-Saclay, CNRS, Institut da Astrophysique Spatiale, Orsay, 91405, France; Altieri B., ESAC/ESA, Camino Bajo Del Castillo, s/n., Urb. Villafranca del Castillo, Villanueva de la Cada, Madrid, 28692, Spain; Amara A., School of Mathematics and Physics, University of Surrey, Guildford, Surrey, GU2 7XH, United Kingdom; Andreon S., INAF, Osservatorio Astronomico di Brera, Via Brera 28, Milano, 20122, Italy; Auricchio N., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Baccigalupi C., IFPU, Institute for Fundamental Physics of the Universe, Via Beirut 2, Trieste, 34151, Italy, INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy, INFN, Sezione di Trieste, Via Valerio 2, TS, Trieste, 34127, Italy, SISSA, International School for Advanced Studies, Via Bonomea 265, TS, Trieste, 34136, Italy; Baldi M., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, Dipartimento di Fisica e Astronomia, Universitdi Bologna, Via Gobetti 93/2, Bologna, 40129, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy; Balestra A., INAF-Osservatorio Astronomico di Padova, Via della Osservatorio 5, Padova, 35122, Italy; Bardelli S., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Battaglia P., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Biviano A., IFPU, Institute for Fundamental Physics of the Universe, Via Beirut 2, Trieste, 34151, Italy, INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Bonino D., INAF, Osservatorio Astrofisico di Torino, Via Osservatorio 20 (TO), Pino Torinese, 10025, Italy; Branchini E., INAF, Osservatorio Astronomico di Brera, Via Brera 28, Milano, 20122, Italy, Dipartimento di Fisica, Universitdi Genova, Via Dodecaneso 33, Genova, 16146, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, Genova, 16146, Italy; Brescia M., Department of Physics E. Pancini, University Federico II, Via Cinthia 6, Napoli, 80126, Italy, INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, Napoli, 80131, Italy; Brinchmann J., Instituto de Astrofica e Ciencias Do Espa, Universidade Do Porto, CAUP, Rua das Estrelas PT4150-762, Porto, Portugal, Faculdade de Ciencias, Universidade Do Porto, Rua do Campo de Alegre, Porto, 4150-007, Portugal; Camera S., INAF, Osservatorio Astrofisico di Torino, Via Osservatorio 20 (TO), Pino Torinese, 10025, Italy, Dipartimento di Fisica, UniversitDegli Studi di Torino, Via P. Giuria 1, Torino, 10125, Italy, INFN-Sezione di Torino, Via P. Giuria 1, Torino, 10125, Italy; Cas-Herrera G., Leiden Observatory, Leiden University, Einsteinweg 55, Leiden, 2333 CC, Netherlands, European Space Agency, ESTEC, Keplerlaan 1, Noordwijk, 2201 AZ, Netherlands, Institute Lorentz, Leiden University, Niels Bohrweg 2, Leiden, 2333 CA, Netherlands; Capobianco V., INAF, Osservatorio Astrofisico di Torino, Via Osservatorio 20 (TO), Pino Torinese, 10025, Italy; Carbone C., INAF-IASF Milano, Via Alfonso Corti 12, Milano, 20133, Italy; Carretero J., Centro de Investigaciones Energicas, Medioambientales y Tecnolicas (CIEMAT), Avenida Complutense 40, Madrid, 28040, Spain, Port da InformaciCientica, Campus UAB, C. Albareda s/n, Bellaterra, Barcelona, 08193, Spain; Casas S., Institute for Theoretical Particle Physics and Cosmology (TTK), RWTH, Aachen University, Aachen, 52056, Germany; Castellano M., INAF-Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone, 00078, Italy; Castignani G., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Cavuoti S., INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, Napoli, 80131, Italy, INFN Section of Naples, Via Cinthia 6, Napoli, 80126, Italy; Chambers K.C., Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, 96822, HI, United States; Cimatti A., Dipartimento di Fisica e Astronomia Augusto Righi, Alma Mater Studiorum Universita di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy; Colodro-Conde C., Instituto de Astrofica de Canarias, Via Ltea, La Laguna, Tenerife, 38205, Spain; Congedo G., Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom; Conselice C.J., Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom; Conversi L., ESAC/ESA, Camino Bajo Del Castillo, s/n., Urb. Villafranca del Castillo, Villanueva de la Cada, Madrid, 28692, Spain, European Space Agency, ESRIN, Largo Galileo Galilei 1, Frascati, Roma, 00044, Italy; Copin Y., UniversitClaude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France; Courbin F., Institut de Cicies Del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Marti Franqu 1, Barcelona, 08028, Spain, InstituciCatalana de Recerca i Estudis Avants (ICREA), Passeig de Llu Companys 23, Barcelona, 08010, Spain; Courtois H.M., UCB Lyon 1, CNRS, IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, Villeurbanne, 69622, France; Cropper M., Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, RH5 6NT, United Kingdom; Da Silva A., Departamento de Fica, Faculdade de Ciencias, Universidade de Lisboa, Edifio C8, Campo Grande, Lisboa, PT1749-016, Portugal, Instituto de Astrofica e Ciencias Do Espa, Faculdade de Ciencias, Universidade de Lisboa, Campo Grande, Lisboa, 1749-016, Portugal; Degaudenzi H., Department of Astronomy, University of Geneva, ch. da Ecogia 16, Versoix, 1290, Switzerland; De Lucia G., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Di Giorgio A.M., INAF, Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere, 100, Roma, 00100, Italy; Dole H., UniversitParis-Saclay, CNRS, Institut da Astrophysique Spatiale, Orsay, 91405, France; Douspis M., UniversitParis-Saclay, CNRS, Institut da Astrophysique Spatiale, Orsay, 91405, France; Dubath F., Department of Astronomy, University of Geneva, ch. da Ecogia 16, Versoix, 1290, Switzerland; Dupac X., ESAC/ESA, Camino Bajo Del Castillo, s/n., Urb. Villafranca del Castillo, Villanueva de la Cada, Madrid, 28692, Spain; Dusini S., INFN-Padova, Via Marzolo 8, Padova, 35131, Italy; Escoffier S., Aix-Marseille Universite, CNRS, IN2P3, CPPM, Marseille, France; Farina M., INAF, Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere, 100, Roma, 00100, Italy; Faustini F., INAF-Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone, 00078, Italy, Space Science Data Center, Italian Space Agency, Via del Politecnico snc, Roma, 00133, Italy; Ferriol S., UniversitClaude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France; Fotopoulou S., School of Physics, HH Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL, United Kingdom; Frailis M., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Franceschi E., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Galeotta S., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Gillis B., Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom; Giocoli C., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy; Gracia-Carpio J., Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Grazian A., INAF-Osservatorio Astronomico di Padova, Via della Osservatorio 5, Padova, 35122, Italy; Grupp F., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Haugan S.V.H., Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, Oslo, 0315, Norway; Holmes W., Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109, CA, United States; Hook I.M., Department of Physics, Lancaster University, Lancaster, LA1 4YB, United Kingdom; Hormuth F., Felix Hormuth Engineering, Goethestr. 17, Leimen, 69181, Germany; Hornstrup A., Technical University of Denmark, Elektrovej 327, Kgs. Lyngby, 2800, Denmark, Cosmic Dawn Center (DAWN), Denmark; Hudelot P., Institut da Astrophysique de Paris, UMR 7095, CNRS, Sorbonne Universite, 98 bis boulevard Arago, Paris, 75014, France; Jahnke K., Max-Planck-Institut f Astronomie, Konigstuhl 17, Heidelberg, 69117, Germany; Jhabvala M., NASA, Goddard Space Flight Center, Greenbelt, 20771, MD, United States; Keihen E., Department of Physics, Helsinki Institute of Physics, University of Helsinki, Gustaf Hlstrin katu 2, 00014, Finland; Kermiche S., Aix-Marseille Universite, CNRS, IN2P3, CPPM, Marseille, France; Kiessling A., Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109, CA, United States; Kubik B., UniversitClaude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France; Kunz M., Universitde Gene, Dartement de Physique Theorique, Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, Geneve 4, CH-1211, Switzerland; Kurki-Suonio H., Department of Physics, University of Helsinki, P.O. Box 64, 00014, Finland, Helsinki Institute of Physics, University of Helsinki, Gustaf Hallstrin katu 2, Helsinki, Finland; Le Brun A.M.C., Laboratoire da Etude de la Univers et des Phenomenes EXtremes, Observatoire de Paris, UniversitPSL, Sorbonne Universite, CNRS, Meudon, 92190, France; Le Mignant D., Aix-Marseille Universite, CNRS, CNES, LAM, Marseille, France; Ligori S., INAF, Osservatorio Astrofisico di Torino, Via Osservatorio 20 (TO), Pino Torinese, 10025, Italy; Lilje P.B., Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, Oslo, 0315, Norway; Lindholm V., Department of Physics, University of Helsinki, P.O. Box 64, 00014, Finland, Helsinki Institute of Physics, University of Helsinki, Gustaf Hallstrin katu 2, Helsinki, Finland; Lloro I., SKA Observatory, Jodrell Bank, Lower Withington, Macclesfield, Cheshire, SK11 9FT, United Kingdom; Mainetti G., Centre de Calcul de La, IN2P3, CNRS, 21 avenue Pierre de Coubertin, Cedex, Villeurbanne, 69627, France; Maino D., INAF-IASF Milano, Via Alfonso Corti 12, Milano, 20133, Italy, Dipartimento di Fisica Aldo Pontremoli, UniversitDegli Studi di Milano, Via Celoria 16, Milano, 20133, Italy, Via Celoria 16, Milano, 20133, Italy; Maiorano E., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Mansutti O., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Marggraf O., Universit Bonn, Argelander-Institut fur Astronomie, Auf dem Hel 71, Bonn, 53121, Germany; Markovic K., Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109, CA, United States; Martinelli M., INAF-Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone, 00078, Italy, INFN, Sezione di Roma, C/o Dipartimento di Fisica, Piazzale Aldo Moro, 2 , Edificio G. Marconi, Roma, 00185, Italy; Martinet N., Aix-Marseille Universite, CNRS, CNES, LAM, Marseille, France; Marulli F., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy, Dipartimento di Fisica e Astronomia Augusto Righi, Alma Mater Studiorum, Universita di Bologna, Via Piero Gobetti 93/2, Bologna, 40129, Italy; Massey R., Department of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, United Kingdom; Maurogordato S., UniversitCote da Azur, Observatoire de la Cote da Azur, CNRS, Laboratoire Lagrange, Bd de la Observatoire, CS 34229, cedex 4, Nice, 06304, France; Medinaceli E., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Mei S., UniversitParis Cite, CNRS, Astroparticule et Cosmologie, Paris, 75013, France, CNRS-UCB, International Research Laboratory, Centre Pierre Binetruy, IRL2007, CPB-IN2P3, Berkeley, United States; Mellier Y., Institut da Astrophysique de Paris, UMR 7095, CNRS, Sorbonne Universite, 98 bis boulevard Arago, Paris, 75014, France, Institut da Astrophysique de Paris, 98bis Boulevard Arago, Paris, 75014, France; Meneghetti M., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy; Merlin E., INAF-Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone, 00078, Italy; Meylan G., Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fale de Lausanne (EPFL), Observatoire de Sauverny, Versoix, 1290, Switzerland; Mohr J.J., University Observatory, LMU, Faculty of Physics, Scheinerstrasse 1, Munich, 81679, Germany; Mora A., Aurora Technology for European Space Agency (ESA), Camino Bajo Del Castillo, s/n, Urbanizacion Villafranca del Castillo, Villanueva de la Canada, Madrid, 28692, Spain; Moresco M., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, Dipartimento di Fisica e Astronomia Augusto Righi, Alma Mater Studiorum, Universita di Bologna, Via Piero Gobetti 93/2, Bologna, 40129, Italy; Moscardini L., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy, Dipartimento di Fisica e Astronomia Augusto Righi, Alma Mater Studiorum, Universita di Bologna, Via Piero Gobetti 93/2, Bologna, 40129, Italy; Nakajima R., Universit Bonn, Argelander-Institut fur Astronomie, Auf dem Hel 71, Bonn, 53121, Germany; Neissner C., Port da InformaciCientica, Campus UAB, C. Albareda s/n, Bellaterra, Barcelona, 08193, Spain, Institut de Fica da Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, Bellaterra, Barcelona, 08193, Spain; Nichol R.C., School of Mathematics and Physics, University of Surrey, Guildford, Surrey, GU2 7XH, United Kingdom; Niemi S.-M., European Space Agency, ESTEC, Keplerlaan 1, Noordwijk, 2201 AZ, Netherlands; Nightingale J.W., School of Mathematics Statistics and Physics, Newcastle University, Herschel Building, Newcastle-upon-Tyne, NE1 7RU, United Kingdom; Padilla C., Institut de Fica da Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, Bellaterra, Barcelona, 08193, Spain; Paltani S., Department of Astronomy, University of Geneva, ch. da Ecogia 16, Versoix, 1290, Switzerland; Pasian F., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Pedersen K., DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, Copenhagen, 2200, Denmark; Percival W.J., Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, N2L 3G1, ON, Canada, Department of Physics and Astronomy, University of Waterloo, Waterloo, N2L 3G1, ON, Canada, Perimeter Institute for Theoretical Physics, Waterloo, N2L 2Y5, ON, Canada; Pettorino V., European Space Agency, ESTEC, Keplerlaan 1, Noordwijk, 2201 AZ, Netherlands; Pires S., UniversitParis-Saclay, UniversitParis Cite, CEA, CNRS, AIM, Gif-sur-Yvette, 91191, France; Polenta G., Space Science Data Center, Italian Space Agency, Via del Politecnico snc, Roma, 00133, Italy; Poncet M., Centre National da Etudes Spatiales, Centre Spatial de Toulouse, 18 avenue Edouard Belin Cedex 9, Toulouse, 31401, France; Popa L.A., Institute of Space Science, Str. Atomistilor, nr. 409 MA gurele, Ilfov, 077125, Romania; Pozzetti L., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Raison F., Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Rebolo R., Instituto de Astrofica de Canarias, Via Ltea, La Laguna, Tenerife, 38205, Spain, Consejo Superior de Investigaciones Cientificas, Calle Serrano 117, Madrid, 28006, Spain, Universidad de la Laguna, Departamento de Astrofica, La Laguna, Tenerife, 38206, Spain; Renzi A., INFN-Padova, Via Marzolo 8, Padova, 35131, Italy, Dipartimento di Fisica e Astronomia G. Galilei, Universitdi Padova, Via Marzolo 8, Padova, 35131, Italy; Rhodes J., Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109, CA, United States; Riccio G., INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, Napoli, 80131, Italy; Romelli E., INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Roncarelli M., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Rossetti E., Dipartimento di Fisica e Astronomia, Universitdi Bologna, Via Gobetti 93/2, Bologna, 40129, Italy; Saglia R., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Sakr Z., Institut f Theoretische Physik, University of Heidelberg, Philosophenweg 16, Heidelberg, 69120, Germany, Institut de Recherche en Astrophysique et Planologie (IRAP), Universitde Toulouse, CNRS, UPS, CNES, 14 Av. Edouard Belin, Toulouse, 31400, France, UniversitSt Joseph, Faculty of Sciences, Beirut, Lebanon; Sapone D., Departamento de Fica, FCFM, Universidad de Chile, Blanco Encalada, Santiago, 2008, Chile; Sartoris B., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany, INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Schewtschenko J.A., Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom; Schirmer M., Max-Planck-Institut f Astronomie, Konigstuhl 17, Heidelberg, 69117, Germany; Schneider P., Universit Bonn, Argelander-Institut fur Astronomie, Auf dem Hel 71, Bonn, 53121, Germany; Secroun A., Aix-Marseille Universite, CNRS, IN2P3, CPPM, Marseille, France; Seidel G., Max-Planck-Institut f Astronomie, Konigstuhl 17, Heidelberg, 69117, Germany; Seiffert M., Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109, CA, United States; Serrano S., Institut da Estudis Espacials de Catalunya (IEEC), Edifici RDIT, Campus UPC, Castelldefels, Barcelona, 08860, Spain, Satlantis, University Science Park, Sede Bld, Leioa, Bilbao, 48940, Spain, Institute of Space Sciences, ICE, CSIC, Campus UAB, Carrer de Can Magrans, s/n, Barcelona, 08193, Spain; Sirignano C., INFN-Padova, Via Marzolo 8, Padova, 35131, Italy, Dipartimento di Fisica e Astronomia G. Galilei, Universitdi Padova, Via Marzolo 8, Padova, 35131, Italy; Sirri G., INFN-Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, 40127, Italy; Stanco L., INFN-Padova, Via Marzolo 8, Padova, 35131, Italy; Steinwagner J., Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Tallada-CrespP., Centro de Investigaciones Energicas, Medioambientales y Tecnolicas (CIEMAT), Avenida Complutense 40, Madrid, 28040, Spain, Port da InformaciCientica, Campus UAB, C. Albareda s/n, Bellaterra, Barcelona, 08193, Spain; Taylor A.N., Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom; Tereno I., Departamento de Fica, Faculdade de Ciencias, Universidade de Lisboa, Edifio C8, Campo Grande, Lisboa, PT1749-016, Portugal, Instituto de Astrofica e Ciencias Do Espa, Faculdade de Ciencias, Universidade de Lisboa, Tapada da Ajuda, Lisboa, 1349-018, Portugal; Toft S., Cosmic Dawn Center (DAWN), Denmark, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, Copenhagen, 2200, Denmark; Toledo-Moreo R., Universidad Politnica de Cartagena, Departamento de Electrica y Tecnologia de Computadoras, Plaza del Hospital 1, Cartagena, 30202, Spain; Torradeflot F., Centro de Investigaciones Energicas, Medioambientales y Tecnolicas (CIEMAT), Avenida Complutense 40, Madrid, 28040, Spain, Port da InformaciCientica, Campus UAB, C. Albareda s/n, Bellaterra, Barcelona, 08193, Spain; Tutusaus I., Institut de Recherche en Astrophysique et Planologie (IRAP), Universitde Toulouse, CNRS, UPS, CNES, 14 Av. Edouard Belin, Toulouse, 31400, France; Valentijn E.A., Kapteyn Astronomical Institute, University of Groningen, PO Box 800, Groningen, 9700 AV, Netherlands; Valenziano L., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy, INFN-Bologna, Via Irnerio 46, Bologna, 40126, Italy; Valiviita J., Department of Physics, University of Helsinki, P.O. Box 64, 00014, Finland, Helsinki Institute of Physics, University of Helsinki, Gustaf Hallstrin katu 2, Helsinki, Finland; Vassallo T., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany, INAF, Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, Trieste, 34143, Italy; Verdoes Kleijn G., Kapteyn Astronomical Institute, University of Groningen, PO Box 800, Groningen, 9700 AV, Netherlands; Veropalumbo A., INAF, Osservatorio Astronomico di Brera, Via Brera 28, Milano, 20122, Italy, Dipartimento di Fisica, Universitdi Genova, Via Dodecaneso 33, Genova, 16146, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, Genova, 16146, Italy; Wang Y., Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, 91125, CA, United States; Weller J., Universits-Sternwarte Mchen, Fakult f Physik, Ludwig-Maximilians-Universit Mchen, Scheinerstrasse 1, Mchen, 81679, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, Garching, 85748, Germany; Zamorani G., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Zerbi F.M., INAF, Osservatorio Astronomico di Brera, Via Brera 28, Milano, 20122, Italy; Zucca E., INAF, Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Piero Gobetti 93/3, Bologna, 40129, Italy; Burigana C., INFN-Bologna, Via Irnerio 46, Bologna, 40126, Italy, INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, Bologna, 40129, Italy; Gabarra L., Department of Physics, Oxford University, Keble Road, Oxford, OX1 3RH, United Kingdom; Mart-Fleitas J., Aurora Technology for European Space Agency (ESA), Camino Bajo Del Castillo, s/n, Urbanizacion Villafranca del Castillo, Villanueva de la Canada, Madrid, 28692, Spain; Scottez V., Institut da Astrophysique de Paris, 98bis Boulevard Arago, Paris, 75014, France, ICL, Junia, UniversitCatholique de Lille, LITL, Lille, 59000, France
EUI: A Novel Underwater Image Enhancement Network
illumination levels; Low-light image enhancement techniques; underwater image enhancement
The use of optical imaging cameras on underwater vehicles has been increasingly common in recent years. These cameras are increasingly being utilized for the purpose of assisting with the search for aquatic items and the gathering of images. The past ten years have seen the publication of a number of techniques that have been utilized to enhance underwater images. These techniques include enhancing the signal-to-noise ratio and decreasing the amount of backscattered noise at the receiving end. Nevertheless, the development of these algorithms was driven by the need to find a solution to the problem of improving photographs of underwater environments when they are exposed to daylight. The accuracy of these, on the other hand, will not be known until they have been tested on photographs taken underwater in low light conditions. As a result of the fact that dark underwater scene photos typically have an exceptionally low quality and the presence of a great deal of noise, it is simple for artifacts to arise during the process of improvement. In order to fill this need, we conduct an in-depth analysis of the most recent deep learning-based algorithms for the enhancement of underwater images. A novel underwater image augmentation network that is capable of handling the severe decrease in underwater image quality that is induced by low illumination is that which we propose as our last suggestion. Our approach allows for the possibility of ULPs avoiding both low-light damage and scattering at the same time. Additionally, the results of our tests suggest that our method continues to be trustworthy even when exposed to different levels of illumination, which has allowed it to be applied to a wider range of applications. When compared to some of the most cutting-edge strategies for improving underwater pictures that are already in use, as well as techniques for improving low-light images, our method has shown to be superior in terms of performance in a variety of low-light underwater situations. 2025 IEEE.
2nd International Conference on Electronics, Computing, Communication and Control Technology, ICECCC 2025;
https://doi.org/10.1109/ICECCC65144.2025.11063831 https://www.scopus.com/pages/publications/105012021630?origin=resultslist
Sumalatha A., School of Engineering and Technology, CHRIST (Deemed to be University), Department of Computer Science and Engineering, Bengaluru, India; Aruna S.K., School of Engineering and Technology, CHRIST (Deemed to be University), Department of Computer Science and Engineering, Bengaluru, India
European VLBI Network observations of the peculiar radio source 4C 35.06 overlapping with a compact group of nine galaxies
galaxies: active; galaxies: clusters: general; galaxies: formation; galaxies: jets; galaxies: nuclei; radio continuum: galaxies
Context. According to the hierarchical structure formation model, brightest cluster galaxies (BCGs) evolve into the most luminous and massive galaxies in the Universe through multiple merger events. The peculiar radio source 4C 35.06 is located at the core of the galaxy cluster Abell 407, overlapping with a compact group of nine galaxies. Low-frequency radio observations have revealed a helical, steep-spectrum, kiloparsec-scale jet structure and inner lobes with less steep spectra, compatible with a recurring active galactic nucleus (AGN) activity scenario. However, the host galaxy of the AGN responsible for the detected radio emission remained unclear. Aims. We aim to identify the host of 4C 35.06 by studying the object at high angular resolution and thereby confirm the recurrent AGN activity scenario. Methods. To reveal the host of the radio source, we carried out very long baseline interferometry (VLBI) observations with the European VLBI Network of the nine galaxies in the group at 1.7 and 4.9 GHz. Results. We detected compact radio emission from an AGN located between the two inner lobes at both observing frequencies. In addition, we detected another galaxy at 1.7 GHz, whose position appears more consistent with the principal jet axis and is located closer to the low-frequency radio peak of 4C 35.06. The presence of another radio-loud AGN in the nonet sheds new light on the BCG formation and provides an alternative scenario in which not just one but two AGNs are responsible for the complex large-scale radio structure. The Authors 2024.
Veres P.M.; Gabyi K.; Frey S.; Paragi Z.; An T.; Bagchi J.; Bogd ; Biju K.G.; Kun E.; Jacob J.; Adebahr B.
All Open Access; Green Open Access; Hybrid Gold Open Access
Veres P.M., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary; Gabyi K., Department of Astronomy, Institute of Physics and Astronomy, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary, HUN-RENELTE Extragalactic Astrophysics Research Group, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary; Frey S., Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, Institute of Physics and Astronomy, ELTE Ev Lord University, Pmy Per sy 1/A, Budapest, 1117, Hungary; Paragi Z., Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, Dwingeloo, 7991 PD, Netherlands; An T., Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China, Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, 100101, China; Bagchi J., Department of Physics and Electronics, CHRIST (Deemed to be University, Hosur Road, Bangalore, 560029, India; Bogd , Center for Astrophysics, Harvard and Smithsonian, 60 Garden Street, Cambridge, 02138, MA, United States; Biju K.G., W.M.O. Arts and Science College, Muttil, Kerala, Wayanad, 673122, India; Kun E., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, CSFK, MTA Centre of Excellence, Konkoly Thege Mikl 15-17, Budapest, 1121, Hungary, Theoretical Physics IV, Faculty for Physics and Astronomy, Ruhr University Bochum, Universitsstr. 150, Bochum, 44780, Germany, Ruhr Astroparticle And Plasma Physics Center, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44780, Germany; Jacob J., Newman College, Kerala, Thodupuzha, 685584, India; Adebahr B., Astronomisches Institut, Ruhr-Universit Bochum, Universitsstr. 150, Bochum, 44801, Germany
EV Service Stations for Future Smart Cities
batteries; Charging Infrastructure; Electric Vehicles; Training; workforce
The market for electric vehicles (EVs) has been growing at a fast pace in recent years. It is expected to continue growing at a much faster pace in the coming decades. The emerging EV technology is increasingly gaining a high demand for continued good transport connections in smart cities. Most of the Smart Cities' charging infrastructure and future growth revolve around its public transport network, especially an EV service station. New technologies, therefore, need to be complemented with new and versatile charging options to cater to different types of charging options available for charging Li-ion Batteries with newer materials and charging capacity. Building an EV service station in the ongoing scenario anticipates smart engineering knowledge to complement innovative charging methods. An EV service station needs hardware, software, and test equipment before charging, during charge, and post-charge states. It is expected to inform the user of available options to choose and select from. This paper investigates the challenges and suggests solutions to meet the EV service station support for EV vehicles in present and future smart cities. It also highlights the demand for a skilled workforce to maintain these service stations, including updating their skills. Examples of a few smart cities in developed as well as developing countries have been quoted. These developments will contribute to the transport infrastructure needed for future smart cities. The paper paves the way for future research in this area. The Institution of Engineering & Technology 2023.
IET Conference Proceedings, Vol-2023, No. 44, pp. 463-466.
Institution of Engineering and Technology
https://doi.org/10.1049/icp.2024.0968 https://www.scopus.com/inward/record.uri?eid=2-s2.0-85194252113&doi=10.1049%2ficp.2024.0968&partnerID=40&md5=85c876b67c387c81ffe4df36d4a3bcdd
Vishwakarma S., BC Hydro, Vancouver, Canada; Chaurasia A., School of Commerce Finance Accountancy, Christ University, Ghaziabad, India; Tyagi R., Asian Institute of Technology, Thailand