No one can trust Red Bull, obviously, but yes, that is the rumour.

But this is one of those situations where I hope both sides lose (the team's other personnel is the sad collateral damage, which sucks). So if RBR can be in the low midfield next season and then both Horner and Marko get the sack, that would be splendid.

The exodus continues. Behind the smiles and jokes in the press conferences, the atmosphere must be horrendously bad for top, middle, and bottom people be heading for the exits as if the ship is sinking.

Low-key hoping next year is humbling for Horner and Marko. A pity for everyone else that works there, but those two really needs a swift kick in the arse.

Python package called FastF1.

Excellent haul!

The king of malicious compliance. And one of the best Brooklyn 99 guest stars.

I love it. Malicious compliance is the best form of protest. To hell with MbS (both of them, actually).

https://imgur.com/a/t6XU07H

Even put VER as driver_1 because it feels wrong putting him as driver_3. So both versions are there. Thank you for the feedback again, they are MUCH more useful this way.

Thank you for the feedback. Was a bit pressed for time and could not change the code to change the colours, but will do. Not usual to have Williams and TR along with Red Bull....

Hard to do any worse... Even Latifi beat Albon once.

I think one of the issues he was adamant about was no 1 year deal. So I would guess he is at least 2 years.

But Audi has a vacant seat...

PER finally beats VER in qualy!!!

Plus, Williams helped ALB get beaten for the first time as well.

I love when this kind of thing happens. SAI sets the FL with no purple sectors, VER does the 2nd best with 2 purple sectors.

https://tenor.com/view/formula1-f1-i-am-stupid-stupid-gif-15825263

The Brake Magic race alone is a huge swing between them, as VER was getting 25 and ended up with zero that day.

Yeah, me neither. I knew PER had a good record there, but best of everyone? Unexpected.

Let's see what he can do this weekend. It is a good time for the supposed street track specialist to deliver, with 2 of them coming up.

Average of points scored

Not comparable because not everyone in the UK was going to be paid millions and millions while doing it. Also, that was hyperbole, sorry if it was not explicit.

I uprooted my family for five years and it was a brilliant experience for everyone. My kid speaks four languages, we learned a bunch of new ways of thinking and living, and expanded ourselves quite a bit. It has tough moments no doubt, but it is worth it, especially for the kids.

He would design a car for Satan if Lawrence still paid 30 million, gave him shares, gave him authority over his dept. and some people who tried to run away from him (Fallows CANNOT be happy), allowed him to remain at home, etc.

Lance is no all-time great, but it 100% beats designing cars at Williams for better drivers with a much shittier infrastructure. Or having to move to Italy (which anyone not willing to do is clearly insane, but that's another matter) when he does not want to, having to play office politics at Ferrari, etc.

Last part of the paper:

For stellar models, the remarkably high 𝜉ion is untenable 27,36 under common initial mass functions (IMFs). Since this quantity is directly sensitive to the hottest stars, its extreme value may be ascribed to an extension of the IMF to very massive stars 37,38. The high average ionising-photon energy of a 𝑇 = 105 K blackbody moreover yields a 2× higher ratio of Lyα to LyC photons than standard case-B recombination24, thereby bringing the required 𝜉ion more closely in agreement with the theoretical maximum for such stars 39. Whilst at such high 𝜉ion (and relatively low 𝑓esc, LyC) a UV turnover could be produced by a prominent nebular continuum40, the extremely blue UV continuum (𝛽UV ≲ −2.7) appears incompatible with a 2𝛾- dominated spectrum. One explanation is to invoke an ISM density upwards of 𝑛 ≈ 104 cm−3, as may be expected from the compactness of JADES-GS-z13-1-LA. Considering nebular continuum would be reddened further by the free-bound contribution, however, it may again indicate significant LyC leakage, corroborating the suggestion that JADES-GS-z13-1-LA is located inside an ionised bubble.

One particularly intriguing class of objects predicted to radiate up to 40% of their bolometric luminosity as Lyα are entirely metalfree Population III (Pop III) stars 41–43 thought to reach significantly higher masses and effective temperatures than subsequent metal-4 enriched stellar populations. However, the absolute UV magnitude of JADES-GS-z13-1-LA, 𝑀UV ≈ −18.7 mag, would require a stellar mass of 𝑀∗ ≈ 106 M⊙ as a pure Pop III system, somewhat higher than typical predictions 44. We further note the absence of strong He ii 𝜆 1640 Å emission (Methods) may argue against the Pop III scenario45, although its strength rapidly evolves a few Myr after a star formation burst 42,43. A high LyC escape fraction would also suppress He ii, yet still leaves the UV turnover to be explained.

Whatever the origin of the Lyα emission of JADES-GS-z13-1-LA may be, it reveals the rather extreme character of one of the earliest galaxies known, despite having been found in a modest survey area 16 probing a comoving volume of 50 000 Mpc3 between 𝑧 = 11 and 𝑧 = 15. At just 330 Myr after the Big Bang, JADES-GS-z13-1-LA indicates the profound marks left on the IGM by the first generation of galaxies through the creation of reionised regions. Furthermore, it provides tangible evidence for the Wouthuysen-Field coupling of the spin temperature of neutral hydrogen to that of the gas via the emission of Lyα photons, the global evolution of which is anticipated to be uncovered soon by H i 21 cm experiments 46,47 to provide a complementary view of Cosmic Dawn.

Sadly, no mention of the obvious reason for this: aliens!

That is my fear too. Especially because that is what usually happens, especially with such a complete revolution of the regulations.

It will be a pity, just as this set of regs is becoming super competitive...