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We examine the problem of selecting a small set of linear measurements for reconstructing high-dimensional signals. Well-established methods for optimizing such measurements include principal component analysis …

The structure of compound eyes in arthropods has been the subject of many studies, revealing important biological principles. Until recently, these studies were constrained by the two-dimensional …

Rational computational design is crucial to the pursuit of novel drugs and therapeutic agents. Meso-scale cyclic peptides, which consist of 7-40 amino acid residues, are of …

Decoder-only language models have the ability to dynamically switch between various computational tasks based on input prompts. Despite many successful applications of prompting, there is very limited …

We explore the potential of optical intensity interferometry to extract angularly resolved information from supernova explosions, introducing the "expanding ejecta method" (EEM) as a robust alternative to the …

The Cosmic Dawn Survey Pre-launch (PL) catalogues cover an effective 10.13 deg\(^{2}\) area with uniform deep Spitzer/IRAC data (\(m\sim25\) mag, 5\(\sigma\)), the …

Large language models have been successful at tasks involving basic forms of in-context reasoning, such as generating coherent language, as well as storing vast amounts of knowledge …

We introduce Σ-Attention, a Transformer-based operator-learning framework to address a key computational challenge in correlated materials. Our approach utilizes an Encoder-Only Transformer as an …

A direct solver is introduced for solving overdetermined linear systems involving nonuniform discrete Fourier transform matrices. Such matrices can be transformed into a Cauchy-like form that has …

The properties of a two-dimensional electron gas (2DEG) in a semiconductor host with two valleys related by an underlying \(C_4\) rotational symmetry are studied using Hartree …

We present the most sensitive search to date for light axion-like particles with masses below a micro-eV, using spectropolarimetric data collected from the Lick and Keck …

Monitored quantum circuits in which entangling unitary dynamics compete with projective local measurements can host measurement-induced phase transitions witnessed by entanglement measures at late times. Adding feedback …

Amphipathic helices (AHs) are secondary structures that can facilitate binding of proteins to the membrane by folding into a helix with hydrophobic and hydrophilic faces that interact with …

Amphipathic helices (AHs) are secondary structures that can facilitate binding of proteins to the membrane by folding into a helix with hydrophobic and hydrophilic faces that interact with …

Human perceptual sensitivity often improves with training, a phenomenon known as “perceptual learning.” Another important perceptual dimension is appearance, the subjective sense of stimulus magnitude. Are training-induced …

Germline-soma segregation is crucial for fertility. Primordial germ cells (PGCs) arise early in development and are the very first cells to form in the Drosophila embryo. At …

In this work, we explore two-dimensional attractive Fermi gases at the microscopic level by probing spatial charge and spin correlations in situ. Using atom-resolved continuum quantum …

Type-I disk migration can form a chain of planets engaged in first-order mean-motion resonances (MMRs) parked at the disk inner edge. However, while second- or …

Most black holes (BHs) formed in collapsing stars have low spin, though some are expected to acquire a magnetic accretion disk during the collapse. While such BH disks …

We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hr Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates efficient extragalactic …

We report the confirmation of TOI-6324 b, an Earth-sized (1.059 ± 0.041 R\(_{\oplus}\)) ultra-short-period (USP) planet orbiting a nearby (∼20 pc) M …

We have compiled the ∼4–400 GHz broad spectra of 32 Class II protoplanetary disks (PPDs) in the Taurus-Auriga region, which represents the brightest one-third of …

We present a method to determine the gravitational potential of the Milky Way from measurements of the locations, velocities, and element abundances of stars in the Galactic disk …

Observations of the Milky Way's stellar halo find that it is predominantly comprised of a radially biased population of stars, dubbed the Gaia Sausage–Enceladus, or GSE …

Building on a general relativistic magnetohydrodynamic simulation of a short gamma-ray burst (sGRB) jet with initial magnetization σ\(_{0}\) = 150, propagating through the dynamical ejecta from a …

We present the BoRG-JWST survey, a combination of two JWST Cycle 1 programs aimed at obtaining NIRSpec spectroscopy of representative, UV-bright 7 < z < 10 galaxy candidates …

ΛCDM cosmology predicts the hierarchical formation of galaxies, which build up mass by merger events and accreting smaller systems. The stellar halo of the Milky Way (MW) has …

Stellar streams are one of the most promising tracers of low-mass dark-matter subhalos. Existing frameworks for modeling stream perturbations rely on restrictive assumptions for the Milky …

We introduce the DaRk mattEr and Astrophysics with Machine learning and Simulations (DREAMS) project, an innovative approach to understanding the astrophysical implications of alternative dark matter (DM) models …

We present wide-field mapping at 850 \(\mu\)m and 450 \(\mu\)m of the z = 2.85 protocluster in the HS 1549+19 field using the Submillimetre …

Periodic collisions between a star on an inclined orbit around a supermassive black hole and its accretion disk offer a promising explanation for X-ray "quasiperiodic eruptions" (QPEs …

Dense gas in molecular clouds is an important signature of ongoing and future star formation. We identify and track dense cores in the STARFORGE simulations, following the core …

Although Cherenkov detectors of high-energy neutrinos in ice and water are often optimized to detect teraelectronvolt–petaelectronvolt neutrinos, they may also be sensitive to transient neutrino sources …

We present HIP 8522, a young solar twin with the lowest detected lithium, potentially a field blue straggler or the result of episodic early accretion. Its stellar parameters …

Radiation pressure is a key mechanism by which stellar feedback disrupts molecular clouds and drives H II region expansion. This includes direct radiation pressure exerted by UV photons …

Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of general relativity. We present …

We present the first suite of cosmological hydrodynamical zoom-in simulations of isolated dwarf galaxies for a dark sector that consists of cold dark matter and a strongly …

We present spectral observations of the multiplanet host TOI-1694 during the transit of TOI-1694b, a 26.1 M\(_{\oplus}\) hot Neptune with a 3.77 day …

The sum of neutrino masses can be measured cosmologically, as the sub-eV particles behave as "hot" dark matter whose main effect is to suppress the clustering of …

We propose novel numerical schemes based on the Boris method in curved spacetime, incorporating both hadronic and radiative interactions for the first time. Once the proton has lost …

Electromagnetic fields surrounding pulsars may source coherent ultralight axion signals at the known rotational frequencies of the neutron stars, which can be detected by laboratory experiments (e.g …

After reionization, neutral hydrogen (\({\rm H\, {\small I}}\)) traces the large-scale structure (LSS) of the Universe, enabling \({\rm H\, {\small I}}\) intensity mapping (IM) to capture the …

In this paper we study the filamentary substructure of 3.3 \(\mu\)m PAH emission from JWST/NIRCam observations in the base of the M82 star-burst driven …

We develop a new and simple method to model baryonic effects at the field level relevant for weak lensing analyses. We analyse thousands of state-of-the-art …

So far, even the highest resolution galaxy formation simulations with gravitational softening have failed to reproduce realistic life cycles of star clusters. We present the first star-by …

The inner \(\sim 5\) kiloparsec (kpc) region of the Milky Way is complex. However, unravelling the evolution of the Galaxy requires precise understanding of the formation of this …