Tootfinder

🔊 #NowPlaying on #BBCRadio3:
#BBCProms
- 2025
Bill Bailey's Proms debut, Louise Alder sings My Fair Lady & Alison Balsom plays Hummel. Brian May & Roger Taylor join the party to mark the 50th anniversary of Bohemian Rhapsody
Relisten now 👇
https://www.bbc.co.uk/programmes/m002j624

I expect I'm late to the party as usual and everyone's already seen this - but yeah, for once the description of this video is not hyperbole.
The most INSANE Bohemian Rhapsody Flashmob you will ever see!
Not sure about insane but it's very, very impressive. Worth a few minutes of your time and it'll cheer up your day.
#queen #BohemianRhapsody #flashmob

The GAPS programme at TNG XYZ. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
A. S. Bonomo, L. Naponiello, A. Sozzetti, S. Benatti, I. Carleo, K. Biazzo, P. E. Cubillos, M. Damasso, C. Di Maio, C. Dorn, N. Hara, D. Polychroni, M. -L. Steinmeyer, K. A. Collins, S. Desidera, X. Dumusque, A. F. Lanza, B. S. Safonov, C. Stockdale, D. Turrini, C. Ziegler, L. Affer, M. D'Arpa, V. Farde…

The GAPS programme at TNG XYZ. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
Sub-Neptunes with planetary radii of $R_{p} \simeq 2-4 R_{\oplus}$ are the most common planets around solar-type stars in short-period ($P<100$ d) orbits. It is still unclear, however, what their most likely composition is, that is whether they are predominantly gas dwarfs or water worlds. The sub-Neptunes orbiting bright host stars are very valuable because they are suitable for atmospheric characterization, which can break the well-known degeneracy in planet composition from the planet bulk d…

I notice that most people in my circles tend to gravitate toward OpenAI and Anthropic and tend to discount Google when it comes to Gen AI. This is pretty freakin' cool:
https://arstechnica.com/ai/2025/08/google-improves-gemini-ai-image-ed…

Google improves Gemini AI image editing with “nano banana” model
Gemini 2.5 Flash Image is currently atop LMArena’s image-editing leaderboard.

But as much as my mother would bemoan their antics. My aunt… oh my aunt.
She was the most intellectual, the most proud, and the most outspoken person I’ve ever had the privilege of knowing.
My aunt would give them a proper earful about what it meant to live in a society, about how their antics would lead to the entire west looking down on Poland, about how they were letting down their fellow citizen by running such scams.
I miss my aunt. She was a rock star and a role mode …

The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star
F. Manni, L. Naponiello, L. Mancini, S. Vissapragada, K. Biazzo, A. S. Bonomo, D. Polychroni, D. Turrini, D. Locci, A. Maggio, V. D Orazi, M. Damasso, C. Briceno, D. R. Ciardi, C. A. Clark, K. A. Collins, D. W. Latham, N. Law, M. Lopez-Morales, M. B. Lund, L. Malavolta, A. W. Mann, G. Mantovan, D. Nardiello, M. Pinamonti, D. J. Radford, R. P. Schwarz, A. Shporer, A. Sozzetti, C. N., Watki…

The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star
The formation of Neptune planets with orbital periods less than 10\,days remains uncertain. They might have developed similarly to longer-period counterparts, emerged from rare collisions between smaller planets, or could be the remnant cores of stripped giant planets. Characterizing a large number of them is important to advance our understanding of how they form and evolve. We aimed at confirming the planetary nature and characterizing the properties of a close-in Neptune-type transiting exop…