COVID Rapid Tests Reliably Detect New Variants : Researchers who “test the tests” say that #COVID rapid tests have kept up with new variants
https://www.scientificamerican.…
Cup-Frust abgebaut - Rapid schickt Red Bull Salzburg mit 2:0 nach Hause #News #Nachrichten
Everything he touches...
Trump loses nearly $2 billion in net worth after Truth Social stock closes at new low - Alternet.org
https://www.alternet.org/trump-loses-net-worth/
Here's the writeup of the new #http2 continuation flood vulnerability from the researcher who discovered it: https://nowotarski.info/http2-continuation-flood-technical-details/…
Another login, and the very first thing at the top of the feed is this one, by @… - https://botsin.space/@blendernation/112207631253190298…
Typisch Rapid! - Aus einem historischen Sieg wird ein großes Drama #News #Nachrichten
JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$
C. T. Donnan, R. J. McLure, J. S. Dunlop, D. J. McLeod, D. Magee, K. Z. Arellano-C\'ordova, L. Barrufet, R. Begley, R. A. A. Bowler, A. C. Carnall, F. Cullen, R. S. Ellis, A. Fontana, G. D. Illingworth, N. A. Grogin, M. L. Hamadouche, A. M. Koekemoer, Feng-Yuan Liu, C. Mason, P. Santini, T. M. Stanton
https://arxiv.org/abs/2403.03171 https://arxiv.org/pdf/2403.03171
arXiv:2403.03171v1 Announce Type: new
Abstract: We present a new determination of the evolving galaxy UV luminosity function (LF) over the redshift range $8.5<15.5$ using a combination of several major Cycle-1 JWST imaging programmes - PRIMER, JADES and NGDEEP. This multi-field approach yields a total of $\simeq370$ sq. arcmin of JWST/NIRCam imaging, reaching (5-$\sigma$) depths of $\simeq30$ AB mag in the deepest regions. We select a sample of 2548 galaxies with a significant probability of lying at high redshift ($p(z>8.5)>0.05$) to undertake a statistical calculation of the evolving UV LF. Our new measurements span $\simeq4$ magnitudes in UV luminosity at $z=9-12.5$, placing new constraints on both the shape and evolution of the LF at early times. We fit our observational data-points with a double-power law (DPL) function and explore the evolution of the DPL parameters. Our UV LF measurements yield a new estimate of the early evolution of cosmic star-formation rate density ($\rho_{\rm{SFR}}$) which confirms the gradual, log-linear decline deduced from early JWST studies, at least out to $z \simeq 12$. Finally we show that the observed early evolution of the galaxy UV LF (and $\rho_{\rm{SFR}}$) can be reproduced in a ${\rm \Lambda}$CDM Universe, with no change in dust properties or star-formation efficiency required out to $z \simeq 12$. Instead, we show that a progressive trend towards younger stellar population ages can reproduce the observations, and we show that the typical ages required at $z \simeq$ 8, 9, 10, and 11 all converge on a time $\simeq 380-330$ Myr after the Big Bang, indicative of a rapid emergence of early galaxies at $z \simeq 12 - 13$. This is consistent with the first indications of a steeper drop-off in the galaxy population we find beyond $z \simeq 13$, possibly reflecting the rapid evolution of the halo mass function at earlier times.
Ausraster gegen Rapid - Heraf: „Meine Familie hat sich bedroht gefühlt“ #News #Nachrichten
Sieben Sperren fix - Derby-Skandal: So hart bestraft die Liga Rapid #News #Nachrichten
Sieben Sperren fix - Derby-Skandal: So hart bestraft die Liga Rapid #News #Nachrichten