Tootfinder

Nun stand ein Ausflug nach #Osaka an. Zunächst ging es dort am Bahnhof auf das Umeda Sky Building. Die Aussichtsplattform ist zwischen zwei Gebäude gehängt - ebenso wie Fahrstuhl und Rolltreppen dorthin. Man hat eine weite Aussicht auf große Teile Osakas und der Umgebung. #UmedaSkyBuilding

In #Osaka Den Den Town gibt es einen Escape Room mit Anime-Themen. Darunter zu #Dandadan. Coole Sache, aber aus nem japanischen Escape Room würden wir wohl nie herausfinden. :blobcatsweat:
#DonInJapan

In the #China Pavilion at the Osaka #Expo, robots dance and #AI sings. But on closer look, these companies on display are the same ones sanctioned by the US for trade, human rights, and geopolitical reasons.

I booked an Air Serbia flight through Air Canada to Shanghai with the intention of booking a second connecting flight to Osaka but I don't want to book that connecting flight until I get a confirmation from Air Serbia ... and it has been a few days.

Back in 2018, I took the Maglev between Longyang Road and Pudong Airport. The route was so short that the train was only able to get to it's top speed for something like a minute before it had to start slowing down again. The new Chuo Shinkansen is supposed to go from Tokyo to Osaka and be faster than the Shanghai Maglev. I think that's really cool.
#Trains #Maglev #Japan

Second Discovery of GeV-TeV Connection from the Globular Cluster UKS 1
Jiwon Shin (Chungnam National University), C. Y. Hui (Chungnam National University), Sangin Kim (Chungnam National University), Kwangmin Oh (Michigan State University), Ellis R. Owen (RIKEN, Osaka University)
https://arxiv.org/abs/2510.11215

Second Discovery of GeV-TeV Connection from the Globular Cluster UKS 1
Using 16 years of data collected by Fermi Large Area Telescope and 1523 days of survey data from High Altitude Water Cherenkov (HAWC) Observatory, we discovered the long-sought second GeV-TeV connection towards the globular cluster (GC) UKS 1 (Shin et al. 2025). Gamma-ray spectroscopy suggests that the GeV emission can be attributed to both the pulsar magnetosphere and inverse Compton scattering (ICS) by the pulsar wind. In particular, the TeV peak is displaced from the cluster center by severa…