@article{19067,
  abstract     = {Modern experimental methods enable the creation of self-assembly building blocks with tunable interactions, but optimally exploiting this tunability for the self-assembly of desired structures remains an important challenge. Many studies of this inverse problem start with the so-called fully addressable limit, where every particle in a target structure is different. This leads to clear design principles that often result in high assembly yield, but it is not a scalable approach—at some point, one must grapple with “reusing” building blocks, which lowers the degree of addressability and may cause a multitude of off-target structures to form, complicating the design process. Here, we solve a key obstacle preventing robust inverse design in the “semiaddressable regime” by developing a highly efficient algorithm that enumerates all structures that can be formed from a given set of building blocks. By combining this with established partition-function-based yield calculations, we show that it is almost always possible to find economical semiaddressable designs where the entropic gain from reusing building blocks outweighs the presence of off-target structures and even increases the yield of the target. Thus, not only does our enumeration algorithm enable robust and scalable inverse design in the semiaddressable regime, our results demonstrate that it is possible to operate in this regime while maintaining the level of control often associated with full addressability.},
  author       = {Hübl, Maximilian and Goodrich, Carl Peter},
  issn         = {1079-7114},
  journal      = {Physical Review Letters},
  number       = {5},
  publisher    = {American Physical Society},
  title        = {{Accessing semiaddressable self-assembly with efficient structure enumeration}},
  doi          = {10.1103/PhysRevLett.134.058204},
  volume       = {134},
  year         = {2025},
}

@article{19068,
  abstract     = {Whether or not the neuron emits a spike in response to stimulation by an excitatory current pulse is determined by a strength-duration curve (SDC) for the pulse parameters. The SDC is a dependence of the minimal pulse amplitude required to elicit the spiking response on either the pulse duration or its decay time. Excitatory neurons affect the others through pulses of excitatory postsynaptic current. A simple yet plausible approximation for the time course of such a pulse is the alpha function, with linear rise at the start and exponential decay at the end. However, an exact analytical SDC for this case is hitherto not known, even for the leaky integrate-and-fire (LIF) neuron, the simplest spiking neuron model used in practice. We have obtained general SDC equations for the LIF neuron. Using the Lambert W function — a widely-implemented special function, we have found the exact analytical SDC for the spiking response of the LIF neuron stimulated by an excitatory current pulse in the form of the alpha function. To compare results in a unified way, we have also derived the analytical SDCs for (i) rectangular pulse, (ii) ascending ramp pulse, and (iii) instantly rising and exponentially decaying pulse. In the limit of no leakage, we show that the SDC is reduced to the classical hyperbola for all considered cases.},
  author       = {Paraskevov, Alexander},
  issn         = {2590-0374},
  journal      = {Results in Applied Mathematics},
  publisher    = {Elsevier},
  title        = {{Analytical strength-duration curve for the spiking response of the LIF neuron to an alpha-function-shaped excitatory current pulse}},
  doi          = {10.1016/j.rinam.2025.100548},
  volume       = {25},
  year         = {2025},
}

@article{19069,
  abstract     = {Context. The hydrogen Lyman-alpha (Lyα) line, the brightest rest-frame ultraviolet line of high-redshift galaxies, exhibits a large variety of shapes, which is due to factors at different scales, from the interstellar medium to the intergalactic medium (IGM).
Aims. The aim of this work is to provide a systematic inventory and classification of the spectral shapes of Lyα emission lines to better understand the general population of high-redshift Lyα emitting galaxies (LAEs).
Methods. Using the unprecedentedly deep data from the MUSE eXtremely Deep Field (MXDF; up to 140 hour exposure time), we selected 477 galaxies observed in the ∼2.8−6.6 redshift range, 15 of which have a systemic redshift from nebular lines. We developed a method to classify Lyα emission lines in four spectral and three spatial categories by combining a pure spectral analysis with a narrow-band image analysis. We measured spectral properties, such as the peak separation and the blue-to-total flux ratio for the double-peaked galaxies.
Results. To ensure a robust sample for statistical analysis, we define two unbiased subsets, inclusive and restrictive, by applying thresholds for signal-to-noise ratio, peak separation, and Lyα luminosity, yielding a final unbiased sample of 206 galaxies. Our analysis reveals that between 32% and 51% of the galaxies exhibit double-peaked profiles, with peak separations ranging from 150 km s−1 to nearly 1600 km s−1. The fraction of double-peaked galaxies seems to evolve dependently with the Lyα luminosity, while we do not see a severe decrease in this fraction with redshift, which is expected given the IGM attenuation at high redshift. An artificial increase in the number of double-peaked galaxies at the highest redshifts may cause the observation of a plateau instead of a decrease. A notable number of these double-peaked profiles show blue-dominated spectra, suggesting unique gas dynamics and inflow characteristics in some high-redshift galaxies. The consequent fraction of blue-dominated spectra needs to be confirmed by obtaining new systemic redshift measurements. Among the double-peaked galaxies, 4% are spurious detections, that is, the blue and red peaks do not come from the same spatial location. Around 20% out of the 477 sources of the parent sample lie in a complex environment, meaning there are other clumps or galaxies at the same redshift within a distance of 30 kpc.
Conclusions. Our results suggest that the double-peaked LAE fraction may trace the evolution of IGM attenuation, but the faintest galaxies must be observed at high redshift. We also need more data to confirm the trend seen at low redshift. In addition, it is crucial to obtain secure systemic redshifts for LAEs to better constrain the nature of the Lyα double-peaked lines. Statistical samples of double-peaked and triple-peaked galaxies are a promising probe of the evolution of the physical properties of galaxies across cosmic time.},
  author       = {Vitte, Eloïse and Verhamme, Anne and Hibon, Pascale and Leclercq, Floriane and Alcalde Pampliega, Belén and Kerutt, Josephine and Kusakabe, Haruka and Matthee, Jorryt J and Guo, Yucheng and Bacon, Roland and Maseda, Michael and Richard, Johan and Pharo, John and Schaye, Joop and Boogaard, Leindert and Nanayakkara, Themiya and Contini, Thierry},
  issn         = {1432-0746},
  journal      = {Astronomy & Astrophysics},
  publisher    = {EDP Sciences},
  title        = {{The MUSE eXtremely Deep Field: Classifying the spectral shapes of Ly α -emitting galaxies}},
  doi          = {10.1051/0004-6361/202450426},
  volume       = {694},
  year         = {2025},
}

@article{19070,
  abstract     = {Context. Recent observations suggest a significant and rapid buildup of dust in galaxies at high redshift (z > 4); this presents new challenges to our understanding of galaxy formation in the early Universe. Although our understanding of the physics of dust production and destruction in a galaxy’s interstellar medium (ISM) is improving, investigating the baryonic processes in the early universe remains a complex task owing to the inherent degeneracies in cosmological simulations and chemical evolution models.
Aims. In this work we characterized the evolution of 98 z ∼ 5 star-forming galaxies observed as part of the ALMA Large Program ALPINE by constraining the physical processes underpinning the gas and dust production, consumption, and destruction in their ISM.
Methods. We made use of chemical evolution models to simultaneously reproduce the observed dust and gas content of our galaxies, obtained respectively from spectral energy distribution (SED) fitting and ionized carbon measurements. For each galaxy we constrained the initial gas mass, gas inflows and outflows, and efficiencies of dust growth and destruction. We tested these models with both the canonical Chabrier and a top-heavy initial mass function (IMF); the latter allowed rapid dust production on shorter timescales.
Results. We successfully reproduced the gas and dust content in most of the older galaxies (≳600 Myr) regardless of the assumed IMF, predicting dust production primarily through Type II supernovae (SNe) and no dust growth in the ISM, as well as moderate inflow of primordial gas. In the case of intermediate-age galaxies (300−600 Myr), we reproduced the gas and dust content through Type II SNe and dust growth in ISM, though we observed an overprediction of dust mass in older galaxies, potentially indicating an unaccounted dust destruction mechanism and/or an overestimation of the observed dust masses. The number of young galaxies (≲300 Myr) reproduced, increases for models assuming top-heavy IMF but with maximal prescriptions of dust production. Galactic outflows are required (up to a mass-loading factor of 2) to reproduce the observed gas and dust mass, and to recover the decreasing trend of gas and dust over stellar mass with age. Assuming the Chabrier IMF, models are able to reproduce ∼65% of the total sample, while with top-heavy IMF the fraction increases to ∼93%, alleviating the tension between the observations and the models. Observations from the James Webb Space Telescope (JWST) will allow us to remove degeneracies in the diverse intrinsic properties of these galaxies (e.g., star formation histories and metallicity), thereby refining our models.},
  author       = {Sawant, P. and Nanni, A. and Romano, M. and Donevski, D. and Bruzual, G. and Ysard, N. and Lemaux, B. C. and Inami, H. and Calura, F. and Pozzi, F. and Małek, K. and Junais, J. and Boquien, M. and Faisst, A. L. and Hamed, M. and Ginolfi, M. and Zamorani, G. and Lorenzon, G. and Molina, J. and Bardelli, S. and Ibar, E. and Vergani, D. and Di Cesare, Claudia and Béthermin, M. and Burgarella, D. and Cassata, P. and Dessauges-Zavadsky, M. and D'Onghia, E. and Dubois, Y. and Magdis, G. E. and Mendez-Hernandez, H.},
  issn         = {1432-0746},
  journal      = {Astronomy & Astrophysics},
  publisher    = {EDP Sciences},
  title        = {{The ALPINE-ALMA [CII] survey: Unveiling the baryon evolution in the interstellar medium of z ∼ 5 star-forming galaxies}},
  doi          = {10.1051/0004-6361/202451542},
  volume       = {694},
  year         = {2025},
}

@article{19071,
  abstract     = {An action of a complex reductive group G on a smooth projective variety X is regular when all regular unipotent elements in G act with finitely many fixed points. Then the complex G
-equivariant cohomology ring of X is isomorphic to the coordinate ring of a certain regular fixed point scheme. Examples include partial flag varieties, smooth Schubert varieties and Bott-Samelson varieties. We also show that a more general version of the fixed point scheme allows a generalisation to GKM spaces, such as toric varieties.},
  author       = {Hausel, Tamás and Rychlewicz, Kamil P},
  issn         = {2491-6765},
  journal      = {Epijournal de Geometrie Algebrique},
  publisher    = {EPI Sciences},
  title        = {{Spectrum of equivariant cohomology as a fixed point scheme}},
  doi          = {10.46298/epiga.2025.12591},
  volume       = {9},
  year         = {2025},
}

@article{19072,
  abstract     = {Pathogenic fungal and bacterial cells are enveloped within a cell wall, a molecular barrier at their cell surface, and a critical architecture that constantly evolves during pathogenesis. Understanding the molecular composition, structural organization, and mobility of polysaccharides constituting this cell envelope is crucial to correlate cell wall organization with its role in pathogenicity and to identify potential antifungal targets. For the fungal pathogen Cryptococcus neoformans, the characterization of the cell envelope has been complexified by the presence of an additional external polysaccharide capsular shell. Here, we investigate how magic-angle spinning (MAS) solid-state NMR techniques increase the analytical capabilities to characterize the structure and dynamics of this encapsulated pathogen. The versatility of proton detection experiments, dynamic-based filters, and relaxation measurements facilitate the discrimination of the highly mobile external capsular structure from the internal rigid cell wall of C. neoformans. In addition, we report the in situ detection of triglyceride molecules from lipid droplets based on NMR dynamic filters. Together, we demonstrate a nondestructive technique to study the cell wall architecture of encapsulated microbes using C. neoformans as a model, an airborne opportunistic fungal pathogen that infects mainly immunocompromised but also competent hosts.},
  author       = {Lends, Alons and Lamon, Gaelle and Delcourte, Loic and Sturny-Leclere, Aude and Grélard, Axelle and Morvan, Estelle and Abdul-Shukkoor, Muhammed Bilal and Berbon, Mélanie and Vallet, Alicia and Habenstein, Birgit and Dufourc, Erick J. and Schanda, Paul and Aimanianda, Vishukumar and Loquet, Antoine},
  issn         = {1520-5126},
  journal      = {Journal of the American Chemical Society},
  number       = {8},
  pages        = {6813--6824},
  publisher    = {American Chemical Society},
  title        = {{Molecular distinction of cell wall and capsular polysaccharides in encapsulated pathogens by in situ magic-angle spinning NMR techniques}},
  doi          = {10.1021/jacs.4c16975},
  volume       = {147},
  year         = {2025},
}

@article{19075,
  abstract     = {Thermoelectric (TE) materials can convert the heat produced during biochemical reactions into electrical signals, enabling the self-powered detection of biomarkers. In this work, we design and fabricate a simple Ag2Se nanofilm-based TE biosensor to precisely quantify hydrogen peroxide (H2O2) levels in liquid samples. A chemical reaction involving horseradish peroxidase, ABTS and H2O2 in the specimens produces a photothermal agent—ABTS (2,2′-azino-bis(3-ethylbenzothiazoline-6-sulfonic acid)) free radical, which triggers the heat fluctuations at the TE sensor through the photo-thermal effect, eventually enabling the sensing of H2O2. Consequently, the constructed sensor can achieve a detection limit of 0.26 μM by a three-leg TE device design. Further investigations suggest that the application of our TE sensor can be extended in testing H2O2 in beverages (including milk, soda water, and lemonade) and evaluating the load of bacterial pathogens relevant to dental diseases and infections including Streptococcus sanguinis and Methicillin-resistant Staphylococcus aureus with high analytical accuracy. This strategy utilizes the combination of high thermoelectric performance with chemical reactions to realize a straightforward and accurate biomarker detection method, making it suitable for applications in medical diagnostics, personalized health monitoring, and the food industry.},
  author       = {Ma, Huangshui and Pu, Shiyu and Jia, Shiyu and Xu, Shengduo and Yu, Qiwei and Yang, Lei and Wu, Hao and Sun, Qiang},
  issn         = {2040-3372},
  journal      = {Nanoscale},
  number       = {10},
  pages        = {5858--5868},
  publisher    = {Royal Society of Chemistry},
  title        = {{Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens}},
  doi          = {10.1039/d4nr04860a},
  volume       = {17},
  year         = {2025},
}

@article{19076,
  abstract     = {For accurate perception and motor control, an animal must distinguish between sensory experiences elicited by external stimuli and those elicited by its own actions. The diversity of behaviors and their complex influences on the senses make this distinction challenging. Here, we uncover an action–cue hub that coordinates motor commands with visual processing in the brain’s first visual relay. We show that the ventral lateral geniculate nucleus (vLGN) acts as a corollary discharge center, integrating visual translational optic flow signals with motor copies from saccades, locomotion and pupil dynamics. The vLGN relays these signals to correct action-specific visual distortions and to refine perception, as shown for the superior colliculus and in a depth-estimation task. Simultaneously, brain-wide vLGN projections drive corrective actions necessary for accurate visuomotor control. Our results reveal an extended corollary discharge architecture that refines early visual transformations and coordinates actions via a distributed hub-and-spoke network to enable visual perception during action.},
  author       = {Vega Zuniga, Tomas A and Sumser, Anton L and Symonova, Olga and Koppensteiner, Peter and Schmidt, Florian and Jösch, Maximilian A},
  issn         = {1546-1726},
  journal      = {Nature Neuroscience},
  publisher    = {Springer Nature},
  title        = {{A thalamic hub-and-spoke network enables visual perception during action by coordinating visuomotor dynamics}},
  doi          = {10.1038/s41593-025-01874-w},
  volume       = {28},
  year         = {2025},
}

@article{19080,
  abstract     = {We examine mesoscale convective organisation in the tropical western Pacific using a multivariate analysis of column humidity, precipitation and sea surface temperature (SST) observations. We demonstrate that in boreal summer and autumn, convection remains spatially random despite radiative-feedbacks acting to aggregate convection, which we attribute to the high density of convective moisture sources and the role of wind shear. Instead, in winter and spring, a weak meridional SST gradient exists and convection is usually clustered over the regions of warmer SSTs, with significant meridional humidity gradients. However, this is sporadically interrupted by episodes of convection migration to the coldest SSTs and limited spatial humidity variance. These episodes are the result of westward propagating equatorial waves, which remove meridional humidity gradients. It appears that the drivers of mesoscale convective clustering and humidity variability in the Pacific warm pool are the SST gradients, shear, and equatorial wave dynamics.},
  author       = {Tompkins, Adrian Mike and Casallas Garcia, Alejandro and De Vera, Michie Vianca},
  issn         = {2397-3722},
  journal      = {npj Climate and Atmospheric Science},
  publisher    = {Springer Nature},
  title        = {{Drivers of mesoscale convective aggregation and spatial humidity variability in the tropical western Pacific}},
  doi          = {10.1038/s41612-024-00848-2},
  volume       = {8},
  year         = {2025},
}

@article{19276,
  abstract     = {Impurity motion in a many-body environment has been a central issue in the field of low-temperature physics for decades. In bosonic quantum fluids, the onset of a drag force experienced by point-like objects is due to collective environment excitations, driven by the exchange of linear momentum between the impurity and the many-body bath. In this work we consider a rotating impurity, with the aim of exploring how angular momentum is exchanged with the surrounding bosonic environment. In order to elucidate these issues, we employ a quasiparticle approach based on the angulon theory, which allows us to effectively deal with the non-trivial algebra of quantized angular momentum in the presence of a many-body environment. We uncover how impurity dressing by environmental excitations can establish an exchange channel, whose effectiveness crucially depends on the initial state of the impurity. Remarkably, we find that there is a critical value of initial angular momentum, above which this channel effectively freezes.},
  author       = {Cappellaro, Alberto and Bighin, Giacomo and Cherepanov, Igor and Lemeshko, Mikhail},
  issn         = {1089-7690},
  journal      = {Journal of Chemical Physics},
  number       = {7},
  publisher    = {AIP Publishing},
  title        = {{Environment-limited transfer of angular momentum in Bose liquids}},
  doi          = {10.1063/5.0253451},
  volume       = {162},
  year         = {2025},
}

@article{19277,
  abstract     = {Light-driven molecular rotary motors perform chirality-controlled unidirectional rotations fueled by light and heat. This unique function renders them appealing for the construction of dynamic molecular systems, actuating materials, and molecular machines. Achieving a combination of high photoefficiency, visible-light responsiveness, synthetic accessibility, and easy tuning of dynamic properties within a single scaffold is critical for these applications but remains a longstanding challenge. Herein, a series of highly photoefficient visible-light–responsive molecular motors (MMs), featuring various rotary speeds, was obtained by a convenient one-step formylation of their parent motors. This strategy greatly improves all aspects of the performance of MMs—red-shifted wavelengths of excitation, high photoisomerization quantum yields, and high photostationary state distributions of isomers—beyond the state-of-the-art light-responsive MM systems. The development of this late-stage functionalization strategy of MMs opens avenues for the construction of high-performance molecular machines and devices for applications in materials science and biological systems, representing a major advance in the synthetic toolbox of molecular machines.},
  author       = {Sheng, Jinyu and Van Beek, Carlijn L.F. and Stindt, Charlotte N. and Danowski, Wojciech and Jankowska, Joanna and Crespi, Stefano and Pooler, Daisy R.S. and Hilbers, Michiel F. and Buma, Wybren Jan and Feringa, Ben L.},
  issn         = {2375-2548},
  journal      = {Science Advances},
  number       = {8},
  publisher    = {AAAS},
  title        = {{General strategy for boosting the performance of speed-tunable rotary molecular motors with visible light}},
  doi          = {10.1126/sciadv.adr9326},
  volume       = {11},
  year         = {2025},
}

@article{19279,
  abstract     = {Recent experimental advances in nanofluidics have allowed to explore ion transport across molecular-scale pores, in particular, for iontronic applications. Two-dimensional nanochannels—in which a single molecular layer of electrolyte is confined between solid walls—constitute a unique platform to investigate fluid and ion transport in extreme confinement, highlighting unconventional transport properties. In this work, we study ionic association in 2D nanochannels, and its consequences on non-linear ionic transport, using both molecular dynamics simulations and analytical theory. We show that under sufficient confinement, ions assemble into pairs or larger clusters in a process analogous to a Kosterlitz–Thouless transition, here modified by the dielectric confinement. We further show that the breaking of pairs results in an electric-field dependent conduction, a mechanism usually known as the second Wien effect. However the 2D nature of the system results in non-universal, temperature-dependent, scaling of the conductivity with electric field, leading to ionic coulomb blockade in some regimes. A 2D generalization of the Onsager theory fully accounts for the non-linear transport. These results suggest ways to exploit electrostatic interactions between ions to build new nanofluidic devices.},
  author       = {Toquer, Damien and Bocquet, Lydéric and Robin, Paul},
  issn         = {1089-7690},
  journal      = {Journal of Chemical Physics},
  number       = {6},
  publisher    = {AIP Publishing},
  title        = {{Ionic association and Wien effect in 2D confined electrolytes}},
  doi          = {10.1063/5.0241949},
  volume       = {162},
  year         = {2025},
}

@inproceedings{19281,
  abstract     = {In this work, we consider the list-decodability and list-recoverability of codes in the zero-rate regime. Briefly, a code 𝒞 ⊆ [q]ⁿ is (p,𝓁,L)-list-recoverable if for all tuples of input lists (Y₁,… ,Y_n) with each Y_i ⊆ [q] and |Y_i| = 𝓁, the number of codewords c ∈ 𝒞 such that c_i ∉ Y_i for at most pn choices of i ∈ [n] is less than L; list-decoding is the special case of 𝓁 = 1. In recent work by Resch, Yuan and Zhang (ICALP 2023) the zero-rate threshold for list-recovery was determined for all parameters: that is, the work explicitly computes p_*: = p_*(q,𝓁,L) with the property that for all ε > 0 (a) there exist positive-rate (p_*-ε,𝓁,L)-list-recoverable codes, and (b) any (p_*+ε,𝓁,L)-list-recoverable code has rate 0. In fact, in the latter case the code has constant size, independent on n. However, the constant size in their work is quite large in 1/ε, at least |𝒞| ≥ (1/(ε))^O(q^L).
Our contribution in this work is to show that for all choices of q,𝓁 and L with q ≥ 3, any (p_*+ε,𝓁,L)-list-recoverable code must have size O_{q,𝓁,L}(1/ε), and furthermore this upper bound is complemented by a matching lower bound Ω_{q,𝓁,L}(1/ε). This greatly generalizes work by Alon, Bukh and Polyanskiy (IEEE Trans. Inf. Theory 2018) which focused only on the case of binary alphabet (and thus necessarily only list-decoding). We remark that we can in fact recover the same result for q = 2 and even L, as obtained by Alon, Bukh and Polyanskiy: we thus strictly generalize their work. 
Our main technical contribution is to (a) properly define a linear programming relaxation of the list-recovery condition over large alphabets; and (b) to demonstrate that a certain function defined on a q-ary probability simplex is maximized by the uniform distribution. This represents the core challenge in generalizing to larger q (as a binary simplex can be naturally identified with a one-dimensional interval). We can subsequently re-utilize certain Schur convexity and convexity properties established for a related function by Resch, Yuan and Zhang along with ideas of Alon, Bukh and Polyanskiy.},
  author       = {Resch, Nicolas and Yuan, Chen and Zhang, Yihan},
  booktitle    = {16th Innovations in Theoretical Computer Science Conference},
  isbn         = {9783959773614},
  issn         = {1868-8969},
  location     = {New York, NY, United States},
  publisher    = {Schloss Dagstuhl - Leibniz-Zentrum für Informatik},
  title        = {{Tight bounds on list-decodable and list-recoverable zero-rate codes}},
  doi          = {10.4230/LIPIcs.ITCS.2025.82},
  volume       = {325},
  year         = {2025},
}

@article{19282,
  abstract     = {Osmium complexes with osmium in different oxidation states (II, III, IV, and VI) have been reported to exhibit antiproliferative activity in cancer cell lines. Herein, we demonstrate unexplored opportunities offered by 187Os nuclear forward scattering (NFS) and nuclear inelastic scattering (NIS) of synchrotron radiation for characterization of hyperfine interactions and lattice dynamics in a benchmark Os(VI) complex, K2[OsO2(OH)4]. We determined the isomer shift [δ = 3.3(1) millimeters per second] relative to [OsIVCl6]2− and quadrupole splitting [ΔEQ = 12.0(2) millimeters per second] with NFS. We estimated the Lamb-Mössbauer factor [0.80(4)], extracted the density of phonon states, and carried out a thermodynamics characterization using the NIS data combined with first-principles calculations. Overall, we provide evidence that 187Os nuclear resonance scattering is a reliable technique for the investigation of hyperfine interactions and Os-specific vibrations in osmium(VI) species and is thus applicable for such measurements in osmium complexes of other oxidation states, including those with anticancer activity such as Os(III) and Os(IV).},
  author       = {Stepanenko, Iryna and Huang, Zhishuo and Ungur, Liviu and Bessas, Dimitrios and Chumakov, Aleksandr and Sergueev, Ilya and Büchel, Gabriel E. and Al-Kahtani, Abdullah A. and Chibotaru, Liviu F. and Telser, Joshua and Arion, Vladimir B.},
  issn         = {2375-2548},
  journal      = {Science Advances},
  number       = {6},
  publisher    = {AAAS},
  title        = {{187Os nuclear resonance scattering to explore hyperfine interactions and lattice dynamics for biological applications}},
  doi          = {10.1126/sciadv.ads3406},
  volume       = {11},
  year         = {2025},
}

@article{19283,
  abstract     = {Context. The presence of dips in the gravity mode period spacing versus period diagram of γ Doradus stars is now well established thanks to recent asteroseismic studies. Such Lorentzian-shaped inertial dips arise from the interaction of gravito-inertial modes in the radiative envelope of intermediate-mass main sequence stars with pure inertial modes in their convective core, and allow us to study stellar internal properties. This window onto stellar internal dynamics is extremely valuable in the context of the understanding of angular-momentum transport inside stars, as it allows us to probe rotation in their core.

Aims. We investigate the signature and the detectability of a differential rotation between the convective core and the near-core region inside γ Doradus stars from the properties of inertial dips.

Methods. We studied the coupling between gravito-inertial modes in the radiative zone and pure inertial modes in the convective core in the sub-inertial regime, allowing for a two-zone differential rotation from the two sides of the core-to-envelope boundary. We solved the coupling equation numerically and matched the result to an analytical derivation of the Lorentzian dip properties. We then used typical values of measured near-core rotation and buoyancy travel time to infer ranges of parameters for which differential core to near-core rotation would be detectable in current Kepler data.

Results. We show that increasing the convective core rotation with respect to the near-core rotation leads to a shift of the period of the observed dip to lower periods. In addition, the dip gets deeper and thinner as the convective core rotation increases. We demonstrate that such a signature is detectable in Kepler data, given appropriate dip-parameter ranges and near-core structural properties.

Conclusions. Studying the dip properties in asteroseismic data thus allows us to access core to near-core radial differential rotation and to better understand the transport of angular momentum at convective–radiative interfaces in intermediate-mass main sequence stars.},
  author       = {Barrault, Lucas and Mathis, S. and Bugnet, Lisa Annabelle},
  issn         = {1432-0746},
  journal      = {Astronomy & Astrophysics},
  publisher    = {EDP Sciences},
  title        = {{Constraining differential rotation in γ Doradus stars from the properties of inertial dips}},
  doi          = {10.1051/0004-6361/202451541},
  volume       = {694},
  year         = {2025},
}

@article{19284,
  abstract     = {The Hα nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z > 3 for the first time. We present a catalog of 1050 Hα emitters at 3.7 < z < 6.7 in the GOODS fields obtained from a blind search in JWST NIRCam/grism data. We made use of the FRESCO survey’s 124 arcmin2 of observations in GOODS-North and GOODS-South with the F444W filter, probing Hα at 4.9 < z < 6.7, and the CONGRESS survey’s 62 arcmin2 of observations in GOODS-North with F356W, probing Hα at 3.8 < z < 5.1. We found an overdensity with 98 sources at z ∼ 4.4 in GOODS-N, and confirmed previously reported overdensities at z ∼ 5.2 in GOODS-N and at z ∼ 5.4 and z ∼ 5.9 in GOODS-S. We computed the observed Hα luminosity functions (LFs) in three bins centered at z ∼ 4.45, 5.30, and 6.15, which are the first such measurements at z > 3 obtained based purely on spectroscopic data, robustly tracing galaxy star formation rates (SFRs) beyond the peak of the cosmic star formation history. We compared our results with theoretical predictions from three different simulations and found good agreement at z ∼ 4 − 6. The UV LFs of this spectroscopically confirmed sample are in good agreement with pre-JWST measurements obtained with photometrically selected objects. Finally, we derived SFR functions and integrated them to compute the evolution of the cosmic SFR densities across z ∼ 4 − 6, finding values in good agreement with recent UV estimates from Lyman-break galaxies, which imply a continuous decrease in SFR density by a factor of three over z ∼ 4 to z ∼ 6. Our work shows the power of NIRCam grism observations to efficiently provide new tests for early galaxy formation models based on emission line statistics.},
  author       = {Covelo-Paz, Alba and Giovinazzo, Emma and Oesch, Pascal A. and Meyer, Romain A. and Weibel, Andrea and Brammer, Gabriel and Fudamoto, Yoshinobu and Kerutt, Josephine and Lin, Jamie and Matharu, Jasleen and Naidu, Rohan P. and Velichko, Anna and Bollo, Victoria and Bouwens, Rychard and Chisholm, John and Illingworth, Garth D. and Kramarenko, Ivan and Magee, Daniel and Maseda, Michael and Matthee, Jorryt J and Nelson, Erica and Reddy, Naveen and Schaerer, Daniel and Stefanon, Mauro and Xiao, Mengyuan},
  issn         = {1432-0746},
  journal      = {Astronomy & Astrophysics},
  publisher    = {EDP Sciences},
  title        = {{An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy}},
  doi          = {10.1051/0004-6361/202452363},
  volume       = {694},
  year         = {2025},
}

@article{19363,
  abstract     = {For a general family of non-negative functions matching upper and lower bounds are established for their average over the values of any equidistributed sequence.},
  author       = {Chan, Yik Tung and Koymans, Peter and Pagano, Carlo and Sofos, Efthymios},
  issn         = {0022-314X},
  journal      = {Journal of Number Theory},
  pages        = {1--36},
  publisher    = {Elsevier},
  title        = {{Averages of multiplicative functions along equidistributed sequences}},
  doi          = {10.1016/j.jnt.2025.01.005},
  volume       = {273},
  year         = {2025},
}

@article{19365,
  abstract     = {We present a comprehensive analysis of H i absorption around 96 Lyα emitters (LAEs) at z ≈ 3.3 (median Lyα luminosity ≈1042 erg s−1). These LAEs were identified within eight MUSE fields, each (math. formular) on the sky and centered on a bright background quasar, as part of the MUSEQuBES survey. Using Voigt profile fitting for all H i absorbers detected within ±​​​​​​500 km s−1 of these LAEs, we compiled a catalog of 800 H i absorption components. Our analysis shows that H i absorption is enhanced near the LAEs compared to the intergalactic medium. However, no trend is found between the column densities of H i absorbers and their impact parameters from the LAEs (spanning ​​​​​​≈54–260 pkpc). Additionally, all galaxies associated with Lyman-limit systems have impact parameters >50 pkpc from the quasar sightlines, suggesting that true absorber hosts may be too faint to detect. The LAEs show an overall H i covering fraction (fc(H i)) of ≈88% for a threshold (math. formular) (H i) = 15. Notably, at the same threshold, the LAEs in pairs/groups exhibit a 100% H i covering fraction out to ≈250 pkpc. In contrast, isolated LAEs consistently show a lower fc(H i) of ≈80%. This environmental influence on fc(H i) is also evident up to ≈300 km s−1 in differential bins of line-of-sight velocity. We find an anticorrelation between fc(H i) and the equivalent width of rest-frame Lyα emission (EW0). Based on the Lyα shell model, this could imply that gas-rich galaxies tend to reside in gas-rich environments or that the LAEs with higher EW0 are more efficient at ionizing their surrounding medium.},
  author       = {Banerjee, Eshita and Muzahid, Sowgat and Schaye, Joop and Blaizot, Jérémy and Bouché, Nicolas and Cantalupo, Sebastiano and Johnson, Sean D. and Matthee, Jorryt J and Verhamme, Anne},
  issn         = {1538-4357},
  journal      = {The Astrophysical Journal},
  number       = {2},
  publisher    = {IOP Publishing},
  title        = {{MUSEQuBES: Connecting H i Absorption with Lyα emitters at z ≈ 3.3}},
  doi          = {10.3847/1538-4357/ada7e9},
  volume       = {980},
  year         = {2025},
}

@article{19366,
  abstract     = {Staphylococcus aureus (S. aureus) is one of the most common causative agents of mammary gland infection and mastitis, but the specific role of S. aureus-derived extracellular vesicles (SaEVs) in mastitis has been poorly studied to date. Here, we aimed to investigate the response of bovine monocyte-derived macrophages (boMdM) to SaEVs of the genotype B (GTB) mastitis-related strain M5512B. Specifically, we evaluated the effects on the actin cytoskeleton, gene expression, and the SaEV proteomic cargo. Furthermore, we assessed to what extent the cellular and molecular response of boMdM to SaEVs differed from peripheral mononuclear blood cells (PBMCs) used for in vitro derivation of the former. We observed that SaEVs induced morphological changes in boMdM, leading to a pro-inflammatory and pyroptosis-related increased gene expression. Additionally, our study revealed that boMdM and PBMCs exhibited stimulus-specific differing responses. The proteomic analysis of SaEVs identified clusters of proteins related to virulence and antibiotic resistance, supporting the theory that S. aureus might use EVs to evade host defences and colonize the mammary gland. Our results bring new insights into how SaEVs might impact the host during an S. aureus infection, which can be useful for future S. aureus vaccine development.},
  author       = {Saenz-De-Juano, Mara D. and Silvestrelli, Giulia and Buri, Samuel and Zinsli, Léa V. and Schmelcher, Mathias and Ulbrich, Susanne E.},
  issn         = {2045-2322},
  journal      = {Scientific Reports},
  pages        = {6059},
  publisher    = {Springer Nature},
  title        = {{Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages}},
  doi          = {10.1038/s41598-025-90466-6},
  volume       = {15},
  year         = {2025},
}

@article{19367,
  author       = {De Jaeger-Braet, Joke G},
  issn         = {1532-2548},
  journal      = {Plant Physiology},
  number       = {2},
  publisher    = {Oxford University Press},
  title        = {{Arabidopsis accessions and their difference in heat tolerance during meiosis}},
  doi          = {10.1093/plphys/kiaf055},
  volume       = {197},
  year         = {2025},
}