@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{19364,
  abstract     = {Thermoelectric coolers (TECs) are pivotal in modern heat management but face limitations in efficiency and manufacturing scalability. We address these challenges by using an extrusion-based 3D printing technique to fabricate high-performance thermoelectric materials. Our ink formulations ensure the integrity of the 3D-printed structure and effective particle bonding during sintering, achieving record-high figure of merit (zT) values of 1.42 for p-type bismuth antimony telluride [(Bi,Sb)2Te3] and 1.3 for n-type silver selenide (Ag2Se) materials at room temperature. The resulting TEC demonstrates a cooling temperature gradient of 50°C in air. Moreover, this scalable and cost-effective method circumvents energy-intensive and time-consuming steps, such as ingot preparation and subsequently machining processes, offering a transformative solution for thermoelectric device production and heralding a new era of efficient and sustainable thermoelectric technologies.},
  author       = {Xu, Shengduo and Horta, Sharona and Lawal, Abayomi Q and Maji, Krishnendu and Lorion, Magali and Ibáñez, Maria},
  issn         = {1095-9203},
  journal      = {Science},
  number       = {6736},
  pages        = {845--850},
  publisher    = {AAAS},
  title        = {{Interfacial bonding enhances thermoelectric cooling in 3D-printed materials}},
  doi          = {10.1126/science.ads0426},
  volume       = {387},
  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},
}

@article{19369,
  abstract     = {Monitoring and estimating mountain snowpack mass over regional scales is still a challenge because of the inadequacy of observational networks in capturing spatiotemporal variability, and limitations in remotely sensed retrievals. Recent work using C-band synthetic aperture radar (SAR) backscatter data from the Sentinel-1 satellite mission has shown good promise for tracking mountain snow depth over specific northern hemisphere ranges, although the broader potential is still unknown. Here, we extend the new Sentinel-1 based modeling framework beyond the northern hemisphere by only utilizing globally available input data, and evaluate different model parametrization and model performance over the Chilean and Argentine Andes mountains, which contain the largest mountain snowpack in the southern hemisphere. The accuracy of Sentinel-1 snow depth estimates is evaluated against an extensive in situ network available for the region. Satellite-retrieved snow depth is found to have poorer performance across the Andes than observed for northern hemisphere mountain ranges because of greater sensitivity to evergreen forest cover and shallower snowpacks. The algorithm does offer some skill but performance is variable and site-dependent. Algorithm performance is best over regions with limited evergreen forest cover (<15%) and snow depths greater than 0.75 m, although the retrievals over-estimate snow depth across most sites. Systemic errors for specific snow classes and across different snow depths are shown, highlighting specific areas in need of further investigation and development.},
  author       = {Bulovic, N. and Johnson, F. and Lievens, H. and Shaw, Thomas and Mcphee, J. and Gascoin, S. and Demuzere, M. and Mcintyre, N.},
  issn         = {1944-7973},
  journal      = {Water Resources Research},
  number       = {2},
  publisher    = {Wiley},
  title        = {{Evaluating the performance of sentinel-1 SAR derived snow depth retrievals over the extratropical Andes cordillera}},
  doi          = {10.1029/2024WR037766},
  volume       = {61},
  year         = {2025},
}

@article{19370,
  abstract     = {Sex-linked and autosomal loci experience different selective pressures and evolutionary dynamics. X (or Z) chromosomes are often hemizygous in males (or females), as Y (or W) chromosomes often degenerate. Such hemizygous regions can be under greater efficacy of selection, as recessive mutations are immediately exposed to selection in the heterogametic sex leading to faster adaptation and faster divergence on the X chromosome (the so-called Faster-X or Faster-Z effect). However, in young nonrecombining regions, Y/W chromosomes often have many functional genes, and many X/Z-linked loci are therefore diploid. The sheltering of recessive mutations on the X/Z by the Y/W homolog is expected to drive slower adaptation for diploid X/Z loci, i.e. a reduction in the efficacy of selection. While the Faster-X effect has been studied extensively, much less is known empirically about the evolutionary dynamics of diploid X or Z chromosomes. Here, we took advantage of published population genomic data in the female-heterogametic human parasite Schistosoma japonicum to characterize the gene content and diversity levels of the diploid and hemizygous regions of the Z chromosome. We used different metrics of selective pressures acting on genes to test for differences in the efficacy of selection in hemizygous and diploid Z regions, relative to autosomes. We found consistent patterns suggesting reduced Ne, and reduced efficacy of purifying selection, on both hemizygous and diploid Z regions. Moreover, relaxed selection was particularly pronounced for female-biased genes on the diploid Z, as predicted by recent theoretical work.},
  author       = {Mrnjavac, Andrea and Vicoso, Beatriz},
  issn         = {1759-6653},
  journal      = {Genome Biology and Evolution},
  number       = {2},
  publisher    = {Oxford University Press},
  title        = {{Reduced efficacy of selection on a young Z chromosome region of schistosoma japonicum}},
  doi          = {10.1093/gbe/evaf021},
  volume       = {17},
  year         = {2025},
}

@article{19371,
  abstract     = {We investigate a molecular quantum rotor in a two-dimensional Bose-Einstein condensate. The focus is on studying the angulon quasiparticle concept in the crossover from few- to many-body physics. To this end, we formulate the problem in real space and solve it with a mean-field approach in the frame co-rotating with the impurity. We show that the system starts to feature angulon characteristics when the size of the bosonic cloud is large enough to screen the rotor. More importantly, we demonstrate the departure from the angulon picture for large system sizes or large angular momenta where the properties of the system are determined by collective excitations of the Bose gas.},
  author       = {Suchorowski, Michał and Badamshina, Alina and Lemeshko, Mikhail and Tomza, Michał and Volosniev, Artem},
  issn         = {2542-4653},
  journal      = {SciPost Physics},
  number       = {2},
  publisher    = {SciPost Foundation},
  title        = {{Quantum rotor in a two-dimensional mesoscopic Bose gas}},
  doi          = {10.21468/SciPostPhys.18.2.059},
  volume       = {18},
  year         = {2025},
}

@article{19372,
  abstract     = {We consider the confined Fröhlich polaron and establish an asymptotic series for the low-energy eigenvalues in negative powers of the coupling constant. The coefficients of the series are derived through a two-fold perturbation approach, involving expansions around the electron Pekar minimizer and the excitations of the quantum field.},
  author       = {Brooks, Morris and Mitrouskas, David Johannes},
  issn         = {2690-1005},
  journal      = {Probability and Mathematical Physics},
  number       = {1},
  pages        = {281--325},
  publisher    = {Mathematical Sciences Publishers},
  title        = {{ Asymptotic series for low-energy excitations of the Fröhlich polaron at strong coupling}},
  doi          = {10.2140/pmp.2025.6.281},
  volume       = {6},
  year         = {2025},
}

@article{19373,
  abstract     = {Reproducible pattern and form generation during embryogenesis is poorly understood. Intestinal organoid morphogenesis involves a number of mechanochemical regulators such as cell-type-specific cytoskeletal forces and osmotically driven lumen volume changes. It is unclear how these forces are coordinated in time and space to ensure robust morphogenesis. Here we show how mechanosensitive feedback on cytoskeletal tension gives rise to morphological bistability in a minimal model of organoid morphogenesis. In the model, lumen volume changes can impact the epithelial shape via both direct mechanical and indirect mechanosensitive mechanisms. We find that both bulged and budded crypt states are possible and dependent on the history of volume changes. We test key modelling assumptions via biophysical and pharmacological experiments to demonstrate how bistability can explain experimental observations, such as the importance of the timing of lumen shrinkage and robustness of the final morphogenetic state to mechanical perturbations. This suggests that bistability arising from feedback between cellular tensions and fluid pressure could be a general mechanism that coordinates multicellular shape changes in developing systems.},
  author       = {Xue, Shi-lei and Yang, Qiutan and Liberali, Prisca and Hannezo, Edouard B},
  issn         = {1745-2481},
  journal      = {Nature Physics},
  publisher    = {Springer Nature},
  title        = {{Mechanochemical bistability of intestinal organoids enables robust morphogenesis}},
  doi          = {10.1038/s41567-025-02792-1},
  volume       = {21},
  year         = {2025},
}

@article{19374,
  abstract     = {In the present study, the new ternary rare earth intermetallic compound PrNi6Si6 has been investigated. This work completes the study of the RNi6Si6 series (R = rare earth). While the RNi6Si6 compounds for R = La and Ce adopt the CeNi6Si6-type (tP52, P4/nbm, No. 125), surprisingly PrNi6Si6 crystallizes in the YNi6Si6 prototype (tP52, P − 4b2, No. 117) as do all the heavier lanthanides (but Lu). The YNi6Si6-type and its homolog CeNi6Si6 are two tetragonal ordered derivative of the cubic NaZn13-type structure. Lattice parameters for PrNi6Si6 are a = 7.7846(1) Å, c = 11.2144(1) Å, with a unit cell volume, Vobs = 679.585(5) Å3. The temperature dependence of the inverse magnetic susceptibility χ−1(T) follows the Curie–Weiss law, with calculated values of the effective magnetic moment (µeff) and Weiss temperature (Θpm) of 3.55 μB and − 4.5 K, respectively. While the observed µeff is very close to the theoretical value of 3.58 µB for the free Pr3+ ions, a negative value of the Weiss temperature suggests antiferromagnetic interactions in PrNi6Si6. Magnetization measurements confirm that PrNi₆Si₆ orders antiferromagnetically (AFM) below a Néel temperature (TN) of 9 K. The Ni atoms contribute negligibly to the magnetic properties of this phase. The specific heat of PrNi₆Si₆ is approximately 0.42 J K  − 1  g − 1. Measurements of electric and thermal transport reveal that PrNi₆Si₆ exhibits metallic behavior across a wide temperature range of 2–900 K, accompanied by a relatively low thermal conductivity of around 6 W K − 1 m − 1 at room temperature. Such properties, together with its high-temperature refractory behavior, make PrNi₆Si₆ worthy of consideration in technological applications where fairly good electrical conductivity should be accompanied by a limited thermal conductivity.},
  author       = {Singh, Saurabh and Provino, A. and Pallecchi, I. and Caglieris, F. and Mödlinger, M. and Mele, P. and Latronico, G. and Takeuchi, T. and Manfrinetti, P.},
  issn         = {1573-4803},
  journal      = {Journal of Materials Science},
  publisher    = {Springer Nature},
  title        = {{The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K)}},
  doi          = {10.1007/s10853-024-10582-y},
  volume       = {60},
  year         = {2025},
}

@inproceedings{19375,
  abstract     = {Despite the advances in probabilistic model checking, the scalability of the verification methods remains limited. In particular, the state space often becomes extremely large when instantiating parameterized Markov decision processes (MDPs) even with moderate values. Synthesizing policies for such huge MDPs is beyond the reach of available tools. We propose a learning-based approach to obtain a reasonable policy for such huge MDPs.

The idea is to generalize optimal policies obtained by model-checking small instances to larger ones using decision-tree learning. Consequently, our method bypasses the need for explicit state-space exploration of large models, providing a practical solution to the state-space explosion problem. We demonstrate the efficacy of our approach by performing extensive experimentation on the relevant models from the quantitative verification benchmark set. The experimental results indicate that our policies perform well, even when the size of the model is orders of magnitude beyond the reach of state-of-the-art analysis tools.},
  author       = {Azeem, Muqsit and Chakraborty, Debraj and Kanav, Sudeep and Kretinsky, Jan and Mohagheghi, Mohammadsadegh and Mohr, Stefanie and Weininger, Maximilian},
  booktitle    = {26th International Conference on Verification, Model Checking, and Abstract Interpretation},
  isbn         = {9783031827020},
  issn         = {1611-3349},
  location     = {Denver, CO, United States},
  pages        = {97--120},
  publisher    = {Springer Nature},
  title        = {{1–2–3–Go! Policy synthesis for parameterized Markov decision processes via decision-tree learning and generalization}},
  doi          = {10.1007/978-3-031-82703-7_5},
  volume       = {15530},
  year         = {2025},
}

@article{19401,
  abstract     = {High kinetic inductance superconductors are gaining increasing interest for the realisation of qubits, amplifiers and detectors. Moreover, thanks to their high impedance, quantum buses made of such materials enable large zero-point fluctuations of the voltage, boosting the coupling rates to spin and charge qubits. However, fully exploiting the potential of disordered or granular superconductors is challenging, as their inductance and, therefore, impedance at high values are difficult to control. Here, we report a reproducible fabrication of granular aluminium resonators by developing a wireless ohmmeter, which allows in situ measurements during film deposition and, therefore, control of the kinetic inductance of granular aluminium films. Reproducible fabrication of circuits with impedances (inductances) exceeding 13 kΩ (1 nH per square) is now possible. By integrating a 7.9 kΩ resonator with a germanium double quantum dot, we demonstrate strong charge-photon coupling with a rate of gc/2π = 566 ± 2 MHz. This broadly applicable method opens the path for novel qubits and high-fidelity, long-distance two-qubit gates.},
  author       = {Janik, Marian and Roux, Kevin Etienne Robert and Borja Espinosa, Carla N and Sagi, Oliver and Baghdadi, Abdulhamid and Adletzberger, Thomas and Calcaterra, Stefano and Botifoll, Marc and Garzón Manjón, Alba and Arbiol, Jordi and Chrastina, Daniel and Isella, Giovanni and Pop, Ioan M. and Katsaros, Georgios},
  issn         = {2041-1723},
  journal      = {Nature Communications},
  publisher    = {Springer Nature},
  title        = {{Strong charge-photon coupling in planar germanium enabled by granular aluminium superinductors}},
  doi          = {10.1038/s41467-025-57252-4},
  volume       = {16},
  year         = {2025},
}

@article{19402,
  abstract     = {Recent advances in the field of bottom-up synthetic biology have led to the development of synthetic cells that mimic some features of real cells, such as division, protein synthesis, or DNA replication. Larger assemblies of synthetic cells may be used to form prototissues. However, existing prototissues are limited by their relatively small lateral dimensions or their lack of remodeling ability. Here, we introduce a lipid-based tissue mimetic that can be easily prepared and functionalized, consisting of a millimeter-sized “lipid-foam” with individual micrometer-sized compartments bound by lipid bilayers. We characterize the structural and mechanical properties of the lipid-foam tissue mimetic, and we demonstrate self-healing capabilities enabled by the fluidity of the lipid bilayers. Upon inclusion of bacteria in the tissue compartments, we observe that the tissue mimetic exhibits network-wide tension fluctuations driven by membrane tension generation by the swimming bacteria. Active tension fluctuations facilitate the fluidization and reorganization of the prototissue, providing a versatile platform for understanding and mimicking biological tissues.},
  author       = {Gu, Andre A. and Ucar, Mehmet C and Tran, Peter and Prindle, Arthur and Kamat, Neha P. and Steinkühler, Jan},
  issn         = {2041-1723},
  journal      = {Nature Communications},
  publisher    = {Springer Nature},
  title        = {{Remodeling of lipid-foam prototissues by network-wide tension fluctuations induced by active particles}},
  doi          = {10.1038/s41467-025-57178-x},
  volume       = {16},
  year         = {2025},
}

@article{19403,
  abstract     = {We study the BCS critical temperature on half-spaces in dimensions d =1, 2, 3 with Dirichlet or Neumann boundary conditions. We prove that the critical temperature on a half-space is strictly higher than on Rd, at least at weak coupling in d = 1, 2 and weak coupling and small chemical potential in d = 3. Furthermore, we show that the relative shift in critical temperature vanishes in the weak coupling limit.},
  author       = {Roos, Barbara and Seiringer, Robert},
  issn         = {1432-0673},
  journal      = {Archive for Rational Mechanics and Analysis},
  publisher    = {Springer Nature},
  title        = {{BCS critical temperature on half-spaces}},
  doi          = {10.1007/s00205-025-02088-x},
  volume       = {249},
  year         = {2025},
}

@article{19404,
  abstract     = {Cell migration is a fundamental process during embryonic development. Most studies in vivo have focused on the migration of cells using the extracellular matrix (ECM) as their substrate for migration. In contrast, much less is known about how cells migrate on other cells, as found in early embryos when the ECM has not yet formed. Here, we show that lateral mesendoderm (LME) cells in the early zebrafish gastrula use the ectoderm as their substrate for migration. We show that the lateral ectoderm is permissive for the animal-pole-directed migration of LME cells, while the ectoderm at the animal pole halts it. These differences in permissiveness depend on the lateral ectoderm being more cohesive than the animal ectoderm, a property controlled by bone morphogenetic protein (BMP) signaling within the ectoderm. Collectively, these findings identify ectoderm tissue cohesion as one critical factor in regulating LME migration during zebrafish gastrulation.},
  author       = {Tavano, Ste and Brückner, David and Tasciyan, Saren and Tong, Xin and Kardos, Roland and Schauer, Alexandra and Hauschild, Robert and Heisenberg, Carl-Philipp J},
  issn         = {2211-1247},
  journal      = {Cell Reports},
  number       = {3},
  publisher    = {Elsevier},
  title        = {{BMP-dependent patterning of ectoderm tissue material properties modulates lateral mesendoderm cell migration during early zebrafish gastrulation}},
  doi          = {10.1016/j.celrep.2025.115387},
  volume       = {44},
  year         = {2025},
}

@article{19405,
  abstract     = {In the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology. We used 10 independent asteroseismic analysis techniques and anchor our system on fundamental radii derived from Gaia L and spectroscopic Teff. We provide evolutionary state, asteroseismic surface gravity, mass, radius, age, and the data used to derive them for 12,418 stars. This includes 10,036 exceptionally precise measurements, with median fractional uncertainties in 
vmax, Δν, mass, radius, and age of 0.6%, 0.6%, 3.8%, 1.8%, and 11.1%, respectively. We provide more limited data for 1624 additional stars that either have lower-quality data or are outside of our primary calibration domain. Using lower red giant branch (RGB) stars, we find a median age for the chemical thick disk of 9.14 ± 0.05(ran) ± 0.9(sys) Gyr with an age dispersion of 1.1 Gyr, consistent with our error model. We calibrate our red clump (RC) mass loss to derive an age consistent with the lower RGB and provide asymptotic GB and RGB ages for luminous stars. We also find a sharp upper-age boundary in the chemical thin disk. We find that scaling relations are precise and accurate on the lower RGB and RC, but they become more model dependent for more luminous giants and break down at the tip of the RGB. We recommend the use of multiple methods, calibration to a fundamental scale, and the use of stellar models to interpret frequency spacings.},
  author       = {Pinsonneault, Marc H. and Zinn, Joel C. and Tayar, Jamie and Serenelli, Aldo and García, Rafael A. and Mathur, Savita and Vrard, Mathieu and Elsworth, Yvonne P. and Mosser, Benoit and Stello, Dennis and Bell, Keaton J. and Bugnet, Lisa Annabelle and Corsaro, Enrico and Gaulme, Patrick and Hekker, Saskia and Hon, Marc and Huber, Daniel and Kallinger, Thomas and Cao, Kaili and Johnson, Jennifer A. and Liagre, Bastien and Patton, Rachel A. and Santos, Ângela R.G. and Basu, Sarbani and Beck, Paul G. and Beers, Timothy C. and Chaplin, William J. and Cunha, Katia and Frinchaboy, Peter M. and Girardi, Léo and Godoy-Rivera, Diego and Holtzman, Jon A. and Jönsson, Henrik and Mészáros, Szabolcs and Reyes, Claudia and Rix, Hans Walter and Shetrone, Matthew and Smith, Verne V. and Spoo, Taylor and Stassun, Keivan G. and Wang, Ji},
  issn         = {0067-0049},
  journal      = {Astrophysical Journal, Supplement Series},
  number       = {2},
  publisher    = {IOP Publishing},
  title        = {{APOKASC-3: The third joint spectroscopic and asteroseismic catalog for evolved stars in the Kepler fields}},
  doi          = {10.3847/1538-4365/ad9fef},
  volume       = {276},
  year         = {2025},
}

@article{19406,
  abstract     = {Polyploidization is a common occurrence in the evolutionary history of flowering plants, significantly contributing to their adaptability and diversity. However, the molecular mechanisms behind these adaptive advantages are not well understood.
Through comprehensive phenotyping of diploid and tetraploid clones from Citrus and Poncirus genera, we discovered that genome doubling significantly enhances salt stress resilience. Epigenetic and transcriptomic analyses revealed that increased ethylene production in the roots of tetraploid plants was associated with hypomethylation and enhanced chromatin accessibility of the ACO1 gene. This increased ethylene production activates the transcription of reactive oxygen species scavenging genes and stress-related hormone biosynthesis genes. Consequently, tetraploid plants exhibited superior root functionality under salt stress, maintaining improved cytosolic K+/Na+ homeostasis.
To genetically validate the link between salt stress resilience and ACO1 expression, we generated overexpression and knockout lines, confirming the central role of ACO1 expression regulation following genome doubling in salt stress resilience.
Our work elucidates the molecular mechanisms underlying the role of genome doubling in stress resilience. We also highlight the importance of chromatin dynamics in fine-tuning ethylene gene expression and activating salt stress resilience pathways, offering valuable insights into plant adaptation and crop genome evolution.},
  author       = {Song, Xin and Zhang, Miao and Wang, Ting Ting and Duan, Yao Yuan and Ren, Jie and Gao, Hu and Fan, Yan Jie and Xia, Qiang Ming and Cao, Hui Xiang and Xie, Kai Dong and Wu, Xiao Meng and Zhang, Fei and Zhang, Si Qi and Huang, Ying and Boualem, Adnane and Bendahmane, Abdelhafid and Tan, Feng Quan and Guo, Wen Wu},
  issn         = {1469-8137},
  journal      = {New Phytologist},
  number       = {1},
  pages        = {176--191},
  publisher    = {Wiley},
  title        = {{Polyploidization leads to salt stress resilience via ethylene signaling in citrus plants}},
  doi          = {10.1111/nph.20428},
  volume       = {246},
  year         = {2025},
}