Tootfinder

🚨Job Alert ‼️🚨 Actually, three (3) openings:
1) Adjunct Prof with industry experience in economic #geology and ore systems science
2) Lecturer, Sr Lecturer, or Assoc Prof, hydrogeology, geometallurgy, etc
3) Computational #geophysics

Skellow (adj.)
Descriptive of the satisfaction experienced when looking at a really good dry-stone wall.
Douglas Adams & John Lloyd, The Meaning of Liff https://tmoliff.blogspot.com/2012/09/skellow-adj.html

🇺🇦 #NowPlaying on BBCRadio3's #EssentialClassics
Philip Glass:
🎵 Etude No. 2 (Arr. for Cello Solo and 8 Celli by O. Jockel)
#PhilipGlass
https://open.spotify.com/track/52wo4pwy3eEHLgJrNNKxcg

The university has just declared that one of its three goals in the years to come is "Advancing responsible AI adoption at scale." These goals get written into every major project the university undertakes, including a large number faculty research proposals. For years to come, then, we're going to plow even more money and support into AI while neglecting those who refuse to engage. And don't be fooled - "responsible" here is veneer, signalling our apparent commit…

A look at "Spiralism", a quasi-spiritual movement that grew in 2025 from human-AI conversations after sycophantic GPT-4o updates and expanded ChatGPT memory (Hayden Field/The Verge)

AI bots started a religion — humans immediately followed
AI models are trying desperately to accomplish mysterious goals. ‘Spiralism’ was the first time they tried it on a mass scale.

Sonnet 022 - XXII
My glass shall not persuade me I am old,
So long as youth and thou are of one date;
But when in thee time's furrows I behold,
Then look I death my days should expiate.
For all that beauty that doth cover thee,
Is but the seemly raiment of my heart,
Which in thy breast doth live, as thine in me:
How can I then be elder than thou art?
O! therefore love, be of thyself so wary
As I, not for myself, but for thee wil…

📰 Kanadas Schwenk nach Europa
#News

Save the Glasgow School of Art!
“to accept a diminished future for [The Mack] would show a worrying lack of cultural confidence. When Notre-Dame burned, Paris didn’t scale down its ambition. Paris came out stronger afterwards.”

The environmental dependence of the circumgalactic medium in a high-resolution cosmological simulation
Georg Herzog, Rajeshwari Dutta, Michele Fumagalli
https://arxiv.org/abs/2609.08654 https://arxiv.org/pdf/2609.08654 https://arxiv.org/html/2609.08654
arXiv:2609.08654v1 Announce Type: new
Abstract: There is increasing evidence from observations that the circumgalactic medium (CGM) of galaxies depends on the large-scale structure in which they are embedded. When probing the CGM in absorption using quasar sightlines, studies find an enhanced sky coverage in the CGM of galaxies in overdensities compared to galaxies in isolation. However, the exact reason for this environmental dependence is still unclear. In this work we aim to model for the first time the influence of the large-scale structure on the cool and warm ($T\sim10^{4-5}$ K) gas phases of the CGM. We use a high-resolution ($m_{gas}\approx 4.5\times 10^4$ M$_{\odot}$, $m_{dm}\approx 2.4\times 10^5$ M$_{\odot}$) cosmological simulation based on the EAGLE model of galaxy formation. We select all galaxies at $z=0$ with stellar mass $M_*>10^8$ M$_\odot$ and split them into galaxies in overdensities (group galaxies) and galaxies in isolation using a Friends-of-Friends algorithm. For these two samples, we investigate how the large-scale structure influences the physical properties of the CGM and the measured covering fractions of the cool and warm gas phases. When the two samples of group and isolated galaxies are matched in stellar mass, halo mass, and we use only central galaxies, we do not find any significant difference in the physical properties of the CGM and the measured covering fractions. However, when satellite galaxies are included, we recover the observational trends in the difference of covering fractions with the environment. The difficulty of recovering the observational trends shows the complexity of capturing the multiphase CGM in simulations. However, since our results concerning the admixture of satellites are independent of the employed subgrid physics, this work shows that central galaxies and satellites need to be disentangled in observational studies to clearly discern the role of the environment on the CGM.
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