len() > 99 { break; } } } } } } for path in wallpapers { if let Some(value) = load_image_with_thumbnail(&mut buffer, path).await { let _res = tx.send(value).await; } } wallpapers }); rx if let Ok(wallpapers) = wallpapers.await { use futures_util::StreamExt; let future...
linux (4.18.0-12.13) cosmic; urgency=medium * linux: 4.18.0-12.13 -proposed tracker (LP: #1802743) * [FEAT] Guest-dedicated Crypto Adapters (LP: #1787405) - s390/zcrypt: Add ZAPQ inline function. - s390/zcrypt: Review inline assembler constraints. - s390/zcrypt: Integrate ap_asm.h...
We review results from cosmic X-ray surveys of active galactic nuclei (AGNs) over the past\(\approx 15\)years that have dramatically improved our understanding of growing supermassive black holes in the distant universe. First, we discuss the utility of such surveys for AGN investigations and t...
WEAVE [101] and CLAMATO [102] to help isolate and constrain the impact of Lyman-αemitters on their environment, as well as to improve BAO measurements [99]. A particularly interesting prospect is to combine LIM of a CO line by a LIM mission with tomographic Lyman-αforest from the ...
where H 0 is the Hubble parameter at the present epoch, G is Newton’s gravitational constant, and c is the velocity of light), must be equal to unity, Ω = ε ε c = 1 , i.e., much larger than the measured value of the mass-density parameter, Ω M = ρ ρ c = 0.302 ±...
Such a reduction explains, depending on the preprocessing method adopted, between 98%98% and 99%99% of the total variance in our dataset. We decided to adopt such a number of dimensions because it allowed us to more easily manipulate the value of 𝜖ϵ in (4), which must be ...