SCIENCE Communication

SCIENCE Communication is a team within the Faculty of Science at the University of Copenhagen. The team's mission is to promote the development of an efficient, coherent, and clearly profiled Faculty whose study programmes and research help to solve the challenges facing society. The team consists of communication officers, special consultants, senior consultants, and a head of section. They are responsible for recruitment of students for Bachelor's and Master's programmes, research communication and press work, web communication (website, intranet, and social media), internal communication (newsletters, management communication, and info screens), coordination of meetings and events, grant administratior Scholarships,\n The team also works closely with the Faculty Secretariat to implement UCPH's strategy for SCIENCE. They manage project management in strategic and interdisciplinary organizational and development projects, service and secretarial assistance for departments and in the Faculty Secretariat, legal advice for departments and the management, coordination of collaboration with key stakeholders including supporting international strategic commitments. The head of section is Lise Walsted Kristiansen. In addition to these responsibilities, SCIENCE Communication is responsible for promoting the Faculty's study programmes and research through popular science events, campus guides, thematic booklets and research communication. They also provide legal advice in relation to contracts and cooperation agreements, GDPR, insurance, public access to documents and general legal issues. The team works with a number of tasks that benefit both operations and development in the entire Faculty.

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Recent Articles

Newly Discovered Galaxies Reveal Early Universe's Star Formation Processes with JWST

Newly Discovered Galaxies Reveal Early Universe's Star Formation Processes with JWST

Broke On: Thursday, 23 May 2024 Scientists discovered three early galaxies using the James Webb Space Telescope, each potentially forming when the universe was 400-600 million years old. Surrounded by suspected hydrogen and helium gas, these galaxies will likely fuel new star formation due to their dense gas. The JWST's sensitive instruments detected this gas, offering insights into early universe star formation processes.