{"id":608258,"date":"2026-04-26T23:17:34","date_gmt":"2026-04-26T23:17:34","guid":{"rendered":"https:\/\/www.newsbeep.com\/us\/608258\/"},"modified":"2026-04-26T23:17:34","modified_gmt":"2026-04-26T23:17:34","slug":"cosmology-citizen-science-project-with-lmu-participati","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/us\/608258\/","title":{"rendered":"Cosmology: Citizen Science Project with LMU Participati \u2026"},"content":{"rendered":"\n

With the launch of Space Warps<\/a>, a new citizen science project on the Zooniverse platform, you can now join in the search to find rare and elusive strong gravitational lenses in never-before-seen images captured by the European Space Agency\u2019s Euclid space telescope. The project <\/a>aims at shining a light on dark matter in galaxies and providing clues about mysterious dark energy.<\/p>\n

LMU is directly involved in Space Warps; LMU physicist Leon Ecker<\/a> is a member of the ten members research team<\/a>. His research focuses on distant supernovae that are split into multiple images by gravitational lenses, as well as the use of strong gravitational lenses to study dark matter.<\/p>\n

\t\t\t\t\t\"\"<\/p>\n

A compilation of gravitational lenses captured by the Euclid space telescope during its initial observations of the Deep Field regions. Each square shows a different strong gravitational lens in the distant universe. <\/p>\n

\t\t\t\t\u00a9 ESA\/Euclid\/Euclid Consortium\/NASA<\/p>\n

\n\t\t\t\t\tCosmic Atlas: Euclid’s deep insights\n\t\t\t\t<\/p>\n

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\n\t\t\tRead more
\n\t\t<\/a>
\n\t\t\t<\/p>\n

Warps in spacetime do not only show up in science fiction like Star Trek or the film Interstellar. In real life, we can see the warping effect that gravity has on spacetime in the form of gravitational lensing. The enormous gravity of a massive object \u2013 such as a galaxy or a cluster of galaxies \u2013 distorts the shape of spacetime and can bend the light rays coming from a distant galaxy behind. By warping spacetime, the foreground galaxy acts like a magnifying glass.<\/p>\n

Light from the background object that would be obscured doesn\u2019t travel in a straight line anymore. Instead, it curves around the intervening mass, often producing multiple images, stretched arcs, or even a complete ring known as an \u2018Einstein ring\u2019, like the one recently discovered by Euclid. Strong gravitational lenses offer a striking demonstration of Einstein\u2019s theory of general relativity, showing that matter in the Universe can act as a natural telescope, bringing distant objects into sight.<\/p>\n

ESA\u2019s Euclid telescope is revolutionising the studies of strong gravitational lensing by providing very sensitive imaging over large swaths of the sky in unprecedented detail. This is exactly what is needed to identify rare gravitational lenses.<\/p>\n

In March 2025, almost 500 galaxy-galaxy strong lenses were found in the first Quick Data Release (Q1), nestled in just the first 0.04% of Euclid data, most of them previously unknown. This pioneering catalogue was created thanks to the combined effort from citizen scientists, machine learning (ML) \u2013 a subset of what is commonly labelled as artificial intelligence (AI) \u2013 and researchers.<\/p>\n

\tEarly glimpse of new Euclid images<\/p>\n

As Euclid continues its survey, sending around 100 GB of data back to Earth every day, ESA and the Euclid Consortium once again need help from citizen scientists to identify strong gravitational lenses in a large data set.<\/p>\n

To this end, the Space Warps team has launched a citizen science project based on new Euclid images that will be part of the future Euclid Data Release 1 (DR1). While this data is not public yet, by participating in this new citizen science project, you can get an early glimpse of these new images of galaxies captured by the telescope.<\/p>\n

For this project, you will be inspecting new high-quality imaging data from Euclid, in which many previously unknown strong lenses are hiding. About three hundred thousand images pre-selected by AI algorithms will be shown, which are fine-tuned with the results from the initial citizen-science Euclid strong lens search. These are the highest-ranked candidates from a whopping 72 million galaxies in DR1, classified by ML algorithms. Scientists expect that this exquisite, high-quality data will reveal more than 10.000 new lenses.<\/p>\n

\t\t\t\tThe current DR1 data set now benefits from that refinement, which helped avoid overlooking a considerable number of potential strong lensing detections.
\n\t\t\t\tLeon Ecker, PhD student at LMU<\/p>\n

\tPr\u00e4zise Vorauswahl gegen die Datenflut<\/p>\n

Scientists from LMU and the Max Planck Institute for Extraterrestrial Physics (MPE) in Garching near Munich, Germany, were strongly involved in selecting data that were fed into the Space Warps sample. In order to capture galaxies, Euclid must peer through the Milky Way, our home galaxy. Therefore, multiple other objects, such as stars, nebulae, and other phenomena, must be identified and removed from the catalogue before focusing on the lensing candidates.<\/p>\n

\u201cDuring the first attempt using the Q1 data, this step reduced 29 million objects to only one million that went into closer scrutiny via ML, followed by human inspection,\u201d LMU PhD student Leon Ecker explains. However, Ecker, together with Maximilian Fabricius, Stella Seitz, and Roberto Saglia (all from LMU and MPE), found that the initial selection was too broad. They refined the procedure and identified 27,000 additional candidates, which, in the end, yielded another 72 strong-lensing objects the initial approach missed \u2013 14 percent of the complete sample of almost 600. \u201cThe current DR1 data set now benefits from that refinement, which helped avoid overlooking a considerable number of potential strong lensing detections,\u201d Ecker adds.<\/p>\n

\tWelche Erkenntnisse liefern starke Gravitationslinsen?<\/p>\n

The Euclid mission explores how the Universe has expanded and how its structure has changed through cosmic history using mainly two methods: weak lensing and baryonic acoustic oscillations. From this, scientists can learn more about the role of gravity and the nature of dark matter and dark energy. Strong gravitational lenses can also provide insights into these central questions. For example, strong lensing features can \u2018weigh\u2019 individual galaxies and galaxy clusters. This reveals the total matter (whether dark or light) and traces the distribution of dark matter. By studying strong lenses across cosmic time, scientists can trace the expansion of the Universe and its apparent acceleration. This will provide additional insight into the role of dark energy.<\/p>\n

\u201cWe\u2019ve already seen the success of combining AI with visual inspection by citizen volunteers and scientists on Space Warps, efficiently finding hundreds of high\u2011probability lens candidates in an initial small Euclid search in 2024\u201d, explains Aprajita Verma, Space Warps\u2019 co-founder and project lead at the University of Oxford, UK. \u201cIn this brand new DR1 data, 30 times larger than the initial search and together with our improved algorithms, we are expecting to find more than 10,000 high-quality lens candidates. This is more than four times the number of lenses that we have been able to find since the first gravitational lens was discovered nearly 50 years ago.\u201d<\/p>\n

This step-change is made possible by Euclid. The mission can map large areas of the sky with unprecedented sharpness, an ideal combination for finding rare objects such as strong gravitational lenses.<\/p>\n

\tAdditional Informations<\/p>\n

Citizen Science: Space Warps<\/p>\n

https:\/\/www.zooniverse.org\/projects\/aprajita\/space-warps-esa-euclid<\/a><\/p>\n

The most important questions about participation are answered here <\/a>on the Space Warps website.<\/p>\n","protected":false},"excerpt":{"rendered":"With the launch of Space Warps, a new citizen science project on the Zooniverse platform, you can now…\n","protected":false},"author":2,"featured_media":608259,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[49],"tags":[144811,264280,97048,2496,199,1728,79,43104,6671],"class_list":{"0":"post-608258","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-physics","8":"tag-lmu","9":"tag-ludwig-maximilians-universitat","10":"tag-munchen","11":"tag-munich","12":"tag-physics","13":"tag-research","14":"tag-science","15":"tag-universitat","16":"tag-university"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts\/608258","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/comments?post=608258"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/posts\/608258\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/media\/608259"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/media?parent=608258"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/categories?post=608258"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/us\/wp-json\/wp\/v2\/tags?post=608258"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}