{"id":2,"date":"2022-04-13T12:29:43","date_gmt":"2022-04-13T12:29:43","guid":{"rendered":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/?page_id=2"},"modified":"2022-09-22T08:05:47","modified_gmt":"2022-09-22T08:05:47","slug":"home","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/","title":{"rendered":"Abstract"},"content":{"rendered":"<p>Recent observations of dwarf galaxies have uncovered several tensions with cosmological predictions, such as<br \/>\nan unexpected spatial location around massive galaxies \u2011 the plane\u2011of\u2011satellite problem \u2011, a discrepant dark matter<br \/>\ncontent, and a higher than expected population of globular clusters. They add to other known problems<br \/>\nand challenge the otherwise highly successful \u039b + Cold Dark Matter (\u039bCDM) model of cosmology.<\/p>\n<p>Unfortunately, the detailed studies of dwarf galaxies are hampered by their low luminosities and low surface\u2011brightness<br \/>\nand have so far been limited to a few nearby galaxy groups, including our own Local Group.<br \/>\nUsing the Canada\u2011France\u2011Hawaii Telescope we observed over 200 fields around giant galaxies to an extremely<br \/>\ndeep surface brightness limit. With this data set, we identified an unprecedented number of 2210 dwarf galaxies.<br \/>\nAs follow\u2011up programs, we were granted 87 orbits with the HST in cycle 28 (Oct. 2020 \u2011 Sep. 2021) for a<br \/>\nsubsample of these dwarf galaxies, which represents the largest systematic study of dwarf galaxies with HST<br \/>\nto date. This data set will be accompanied with up to 99 hours of observation time from MUSE mounted at<br \/>\nthe VLT, as part of a snapshot program (Oct. 2020 \u2011 Apr. 2021). With this data set we will answer some pressing<br \/>\nquestions posed in our field of research: Is there a population of dark matter\u2011deficient dwarf galaxies with<br \/>\nextreme globular cluster systems? Do the properties of dwarf galaxies vary with their environment? Is there<br \/>\nmore evidence for co\u2011rotating planes of dwarf galaxies? This new data will increase the study of these objects<br \/>\nfrom a few to a statistically meaningful sample and will test if these challenges to our cosmological model will<br \/>\nremain or vanish.<\/p>\n<p>Our multi\u2011disciplinary team consists of researchers based in Europe (France, Austria, Netherlands, UK), the<br \/>\nUSA, South Africa, and South Korea. At the ISSI in Bern, we aim to bring our team together for the first time<br \/>\nface\u2011to\u2011face for two one\u2011week meetings. Our first planned ISSI meeting will focus on the scientific questions<br \/>\nregarding nearby dwarf galaxies, with a focus on the new HST and VLT data acquired in 2020\/21. The second<br \/>\nmeeting will enlarge the discussions around next-generation surveys, in particular, those to be carried out in<br \/>\nthe near future with Space missions such as Euclid. It will provide the opportunity to use the experience gained<br \/>\nfrom our ground and space\u2011based observations to adjust our strategy to exploit the new surveys and detect<br \/>\ntheir dwarf galaxies and globular cluster populations.<\/p>\n<p>With our project and proposed meetings at ISSI, we aim to get a deeper understanding of dwarf galaxies, combining<br \/>\na statistically significant sample of observed dwarf galaxies and their globular clusters with expertise in<br \/>\ngalaxy formation and cosmological simulations.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Recent observations of dwarf galaxies have uncovered several tensions with cosmological predictions, such as an unexpected spatial location around massive galaxies \u2011 the plane\u2011of\u2011satellite problem \u2011, a discrepant dark matter content, and a higher than expected population of globular clusters. They add to other known problems and challenge the otherwise highly successful \u039b + Cold [&hellip;]<\/p>\n","protected":false},"author":34,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-2","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/users\/34"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":5,"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":17,"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/pages\/2\/revisions\/17"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/obervationdwarfgalaxies\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}