@libreitalia founder, @libreoffice lover, mad goalkeeper, geeko @suse, minion @UyuniProject. she/her. Tweets are my own opinions

Munich, Bavaria
Joined November 2010
Package maintainers are not necessarily software engineers. Inversely software engineers are not necessarily package maintainers. I wouldn't confuse the two.
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SUSE Multi-Linux Manager 5.2 Announcement Launch! 🚀Enabling Operational Sovereignty and Agentic AI Across Mixed Linux Estates suse.com/c/suse-multi-linux-… @SUSE #Linux #LinuxManagement #Ops #SysArmy
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Marina Latini @[email protected] retweeted
SUSE Multi‑Linux Manager 5.2 is here 🚀 Operational sovereignty, AI-assisted ops, OVAL-based CVE precision, FIPS support - all in one independent control plane for 16+ Linux distros. A practical modernization on‑ramp for real‑world, mixed Linux estates. 👉 Learn more: okt.to/sBge4Y #SUSE #Linux #OpenSource #AI #Security #InfraOps #DigitalSovereignty
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Uyuni 2026.06 is now available, featuring a container base OS upgrade to openSUSE Leap 16.0, support for in-place product migrations to SLES 16.0, deployments on FIPS-enabled host OSes, and several CVE fixes! Check the release notes for the full details. uyuni-project.org/pages/stab…
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Where is #openSUSE Conference 2027 going to take place? 🥁🥁🥁🥁🥁
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A BIG THANK YOU to all the speakers, supports, sponsors and viewers of this year's #openSUSE Conference. A HUGE Thx to the openSUSE Video #Team. #C3voc and the wonderful volunteers who helped make the event a success. Cya in #Prague for #oSC27. #OpenSource #Linux
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Happy Birthday, The Document Foundation, the nonprofit home of #LibreOffice. 14 years ago, the entity was incorporated in Berlin. It provides a safe, stable, enduring and independent home to the leading free office suite and all the fantastic people contributing to it.
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Today we celebrate "I Love Free Software Day" and the heroes behind it: the #Maintainers! #IloveFS #SUSECares @SUSE @tdforg @LibreOffice @fsfe fsfe.org/activities/ilovefs/…
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URLs break. Code disappears. The #SWHID is the cryptographically strong, decentralized tech that guarantees persistence. Compute it yourself. (Plus, it's now an ISO standard.) softwareheritage.org/2025/11… #CodeRescue
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Missed the #Uyuni Community Hours today? 🎥 Don't panic! 😱 The recording is already up and waiting for you. Catch up on all the latest community updates and discussions here: 👉 youtu.be/bglyjOtfL5Y #OpenSource #Linux #SystemsManagement #DevOps
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A bright spiral galaxy of the northern sky, Messier 63 is nearby, about 30 million light-years distant toward the loyal constellation Canes Venatici. Also cataloged as NGC 5055, the majestic island universe is nearly 100,000 light-years across, about the size of our own Milky Way. Its bright core and majestic spiral arms lend the galaxy its popular name, The Sunflower Galaxy. This exceptionally deep exposure also follows faint loops and curling star streams far into the galaxy's halo. Extending nearly 180,000 light-years from the galactic center, the star streams are likely remnants of tidally disrupted satellites of M63. Other satellite galaxies of M63 can be spotted in the remarkable wide-field image, including dwarf galaxies, which could contribute to M63's star streams in the next few billion years. Image Credit & Copyright: Alberto Pisabarro
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The most massive young star cluster in the Small Magellanic Cloud is NGC 346, embedded in our small satellite galaxy's largest star forming region some 210,000 light-years distant. Of course the massive stars of NGC 346 are short lived, but very energetic. Their winds and radiation sculpt the edges of the region's dusty molecular cloud triggering star-formation within. The star forming region also appears to contain a large population of infant stars. A mere 3 to 5 million years old and not yet burning hydrogen in their cores, the infant stars are strewn about the embedded star cluster. This spectacular infrared view of NGC 346 is from the James Webb Space Telescope's NIRcam. Emission from atomic hydrogen ionized by the massive stars' energetic radiation as well as molecular hydrogen and dust in the star-forming molecular cloud is detailed in pink and orange hues. Webb's sharp image of the young star-forming region spans 240 light-years at the distance of the Small Magellanic Cloud. Science - NASA, ESA, CSA, Olivia C. Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA) Processing - Alyssa Pagan (STScI), Nolan Habel (USRA), Laura Lenkić (USRA), Laurie E. U. Chu (NASA Ames)
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