Tootfinder

"Titan Quest 2" angespielt: "Diablo"-Konkurrent, Made in Germany
Das Münchener Entwicklungsstudio Grimlore feiert mit dem Action-Rollenspiel "Titan Quest 2" einen gelungenen Einstieg in die Early-Access-Phase.

Ehrlich gesagt habe etwas Respekt davor, diesen Kraftprotz anzuschneiden.

With moving my calendar away from Google I was looking for a Caldev solution, but ...
Interesting take on CalDev and encryption on Cryptpad's github page.
No chance that that will happen encrypted.
It's waiting for an solution in the Caldev protocol. 😇
[Feature request] Possibility to have CalDAV for the Calendar · Issue #823 · cryptpad/cryptpad

Velle viser sitt sanne ansikt. Han hyllet en hŸyreekstremist som åpenlyst mente det var feil å gi svarte i USA like borgerrettigheter. Som hisset til trakassering og undertrykking av transpersoner. Som var med på arrangere stormingen av Kongressen 6. januar.
Dette var ikke en demokratiforkjemper. Dette var en fascist, som fremmet statlig undertrykkelse av minoriteter.
Og slik viser Velle sitt sanne ansikt.
Det er feil av å le av at en mann blir drept av sin egen retorikk…

SN 2023xgo: Helium rich Type Icn or Carbon-Flash Type Ibn supernova?
Anjasha Gangopadhyay, Jesper Sollerman, Konstantinos Tsalapatas, Keiichi Maeda, Naveen Dukiya, Steve Schulze, Claes Fransson, Nikhil Sarin, Priscila J. Pessi, Mridweeka Singh, Jacob Wise, Tatsuya Nakaoka, Avinash Singh, Raya Dastidar, Miho Kawabata, Yu-Jing Qing, Kaustav K. Das, Daniel Perley, Christoffer Fremling, Kenta Taguchi, K-Ryan Hinds, Ragnhild Lunnan, Rishabh Singh Teja, Monalisa Dubey, Bhavya Ailawadhi, Smar…

SN 2023xgo: Helium rich Type Icn or Carbon-Flash Type Ibn supernova?
We present observations of SN 2023xgo, a transitional Type Ibn/Icn SN, from $-5.6$ to 63 days relative to $r$-band peak. Early spectra show CIII $λ$5696 emission like Type Icn SNe, shifting to Type Ibn features. The He I velocities (1800-10000 km s$^{-1}$) and pseudo-equivalent widths are among the highest in the Ibn/Icn class. The light curve declines at 0.14 mag d$^{-1}$ until 30 days, matching SNe Ibn/Icn but slower than fast transients. SN 2023xgo is the faintest in our SN Ibn sample (M$_{…

Mit den #Tomaten habe ich dieses Jahr etwas Pech. Eine neue Sorte zum Testen trägt leider bei mir nicht. Der #Samen scheint von einer Hybride zu sein. Bisher hat nur eine Pflanze #Früchte angesetzt u…

Ancestral origins of attention to environmental issues
C\'esar Barilla, Palaash Bhargava
https://arxiv.org/abs/2509.09598 https://arxiv.org/pdf/2509.09…

Ancestral origins of attention to environmental issues
How does the climatic experience of previous generations affect today's attention to environmental questions? Using self-reported beliefs and environmental themes in folklore, we show empirically that the realized intensity of deviations from typical climate conditions in ancestral generations influences how much descendants care about the environment. The effect exhibits a U-shape where more stable and more unstable ancestral climates lead to higher attention today, with a dip for intermediate…

Stellar Ancestry Unlocked: Chemical and Orbital Clues Link Metal Poor Stars to Globular Clusters and the Galaxy's Thick Disk
Gizay Yolalan, Timur \c{S}ahin, Sel\c{c}uk Bilir, Olcay Plevne
https://arxiv.org/abs/2506.10400

Stellar Ancestry Unlocked: Chemical and Orbital Clues Link Metal Poor Stars to Globular Clusters and the Galaxy's Thick Disk
This study presents a detailed chemical, kinematic, and orbital dynamic analysis of five metal poor stars in the solar neighborhood: HD 2665, HD 5916, HD 122956, HD 189349, and HD 218857. Using high-resolution spectroscopic data from the ELODIE and ESPaDOnS instruments, we derived elemental abundances for 29 species (25 elements: C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd, and Sm) via LTE based analysis with ATLAS9 model atmospheres. Notably, we re…

Gravitational Waves from Strongly Magnetized Eccentric Neutron Star Binaries
R. Prasad, Anushka Doke, Prayush Kumar
https://arxiv.org/abs/2508.08234 https://

Gravitational Waves from Strongly Magnetized Eccentric Neutron Star Binaries
We study the imprint of magnetic fields on gravitational waves emitted during the inspiral phase of eccentric binary neutron star systems. While observations indicate that neutron stars typically exhibit strong magnetic fields in the range of $10^{14}$-$10^{15}\,\mathrm{G}$, theoretical models allow for fields as high as $ \sim 10^{17-18}\,\mathrm{G}$. In binaries, the fate of these fields depends on the formation pathway: in systems formed through isolated evolution, magnetic fields may decay …

SN 2023uqf: An Interacting Supernova Coincident with a High-Energy Neutrino
Robert Stein, Anna Y. Q. Ho, Anjasha Gangopadhyay, Tomas Ahumada, Mansi M. Kasliwal, Jannis Necker, Simeon Reusch, Marek Kowalski, Anna Franckowiak, Jesper Sollerman, Kohta Murase, Igor Andreoni, Eric C. Bellm, Joshua Bloom, Sean J. Brennan, Liam Connor, Michael W. Coughlin, Richard Dekany, Andrew Drake, Christoffer Fremling, Ariel Goobar, Matthew J. Graham, Steven L. Groom, Theophile Jegou du Laz, Daniel Perle…

SN 2023uqf: An Interacting Supernova Coincident with a High-Energy Neutrino
Astrophysical high-energy (TeV-PeV) neutrinos were first discovered in 2013, but their origin remains largely unknown. Here we present SN 2023uqf, a supernova found in coincidence with high-energy neutrino IC231004A, as part of a systematic optical follow-up program with the Zwicky Transient Facility. SN 2023uqf had a luminous and rapidly-evolving lightcurve, and spectroscopic observations indicated that the source was a Type Ibn supernova. Spectroscopic signatures confirm ongoing interaction b…