@article{23050, abstract = {The resonant scattering nature of Lyα photons interacting with neutral hydrogen makes Lyα emitters (LAEs) robust tracers of the intergalactic neutral hydrogen fraction, and thus sensitive probes of cosmic reionization. We present an extensive study of the Lyα evolution from galaxies at 4.5 ≤ z ≤ 11 in the UDS field, observed as part of the CAPERS survey, and complemented with spectra from the DAWN JWST Archive. The combined sample includes 651 spectroscopically confirmed Lyα-break galaxies, among which we find 73 S/N > 3 LAEs in JWST-NIRSpec PRISM spectra. We trace the redshift evolution of the LAE fraction with EW0 > 25 Å (XLyα) between z = 5 and z = 9, extending such an analysis to the UDS field for the first time. At z = 5 and 6, the UDS results agree with the average JWST XLyα values from multiple fields. However, JWST measurements are consistently lower than ground-based results. To investigate this, we compare JWST observations to a population of star-forming galaxies at z ∼ 6 observed with VLT-FORS2. We find that a Lyα slit-loss of 35 ± 10% in JWST spectra accounts for the offset, as the resonant Lyα emission is more spatially extended than the stellar continuum. From z = 6 to 7, the UDS field shows a significant drop in Lyα visibility, from which we infer a neutral hydrogen fraction of XHI = 0.7–0.9. Finally, we identify two robust ionized bubbles at z = 7.29 and 7.77, with radii of Rion = 0.6 and 0.5 physical Mpc and photometric overdensities of N/⟨N⟩ = 3 and 4, based on candidate counts down to the photometric completeness limit. Compared to the large ionized region at z ∼ 7 in the EGS field, these results indicate significant field-to-field variation, supporting a patchy, inhomogeneous reionization process.}, author = {Napolitano, L. and Pentericci, L. and Dickinson, M. and Arrabal Haro, P. and Taylor, A. J. and Calabrò, A. and Bhagwat, A. and Santini, P. and Arevalo-Gonzalez, F. and Begley, R. and Castellano, M. and Ciardi, B. and Donnan, C. T. and Dottorini, D. and Dunlop, J. S. and Finkelstein, S. L. and Fontana, A. and Giavalisco, M. and Hirschmann, M. and Jung, I. and Koekemoer, A. M. and Kokorev, V. and Llerena, M. and Lucas, R. A. and Mascia, Sara and Merlin, E. and Pérez-González, P. G. and Stanton, T. M. and Tripodi, R. and Wang, X. and Weiner, B. J.}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7}}, doi = {10.1051/0004-6361/202556912}, volume = {708}, year = {2026}, } @article{23048, abstract = {The previously inaccessible star formation tracer Paschen-Alpha (Paα) can now be spatially resolved by JWST NIRCam slitless spectroscopy in distant galaxies up to cosmic noon. In the first study of its kind, we combine JWST NGDEEP NIRISS and FRESCO NIRCam slitless spectroscopy to provide the first direct comparison of spatially resolved dust-obscured (traced by Paα) versus unobscured (traced by Hα) star formation across the main sequence. We stacked Paα and Hα emission-line maps, along with stellar continuum images at both wavelengths of 31 galaxies at 1 < z < 1.8 in three bins of stellar mass spanning 7.7 ≤ log(M*/M⊙) < 11. Surface brightness profiles were measured and equivalent width (EW) profiles computed. Increasing Paα and Hα EW profiles with galactocentric radius across all stellar masses probed provides direct evidence for the inside-out growth of galaxies both via dust-obscured and unobscured star formation for the first time. For galaxies predominantly on the main sequence (log(M*/M⊙)≥8.8), a weakly positive (0.1 ± 0.1) Paα/Hα line profile gradient as a function of radius is found at 8.8 ≤ log(M*/M⊙) < 9.9, with a negative (−0.4 ± 0.1) Paα/Hα line profile gradient as a function of radius found at the highest stellar masses of 9.9 ≤ log(M*/M⊙) < 11.0. Low-mass galaxies (7.7 ≤ log(M*/M⊙) < 8.8) with predominantly high specific star formation rates relative to the main sequence are also found to have a negative (−0.5 ± 0.1) Paα/Hα line profile gradient as a function of radius. Our results demonstrate that while inside-out growth via star formation is ubiquitous across the main sequence just after cosmic noon, centrally concentrated dust attenuation is not. Along with other recent work in the literature, our findings now motivate future studies of resolved SFR and dust attenuation profiles in large samples of individual cosmic noon galaxies across the main sequence, aimed at understanding the intrinsic scatter in spatially resolved star formation.}, author = {Matharu, Jasleen and Shen, Lu and Shivaei, Irene and Oesch, Pascal A. and Papovich, Casey and Brammer, Gabriel and Reddy, Naveen A. and Cheng, Yingjie and Van Dokkum, Pieter and Finkelstein, Steven L. and Hathi, Nimish P. and Kartaltepe, Jeyhan S. and Koekemoer, Anton M. and Matthee, Jorryt J and Pirzkal, Nor and Wilkins, Stephen M. and Wozniak, Michael A. and Xiao, Mengyuan}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{A first look at a complete view of spatially resolved star formation at 1  <  z  <  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy}}, doi = {10.1051/0004-6361/202558205}, volume = {708}, year = {2026}, } @article{23045, abstract = {Context. In the convective envelopes of relatively cool (surface temperature ≲6700 K) stars, oscillations are excited by turbulent convection. In these so-called solar-like oscillators, radial oscillation modes appear at nearly equally spaced frequencies. This spacing is referred to as the ‘large-frequency separation’. Deviations from equally spaced frequencies are a result of the internal structure of a star being different from a sphere of ideal gas at constant temperature. Hence, these deviations provide information on the internal structure of the star. Aims. In this work, we investigate the second-order (quadratic) deviation from uniform spacing, referred to as curvature. We aim to provide homogeneous values for observed red-giant stars, understand differences between the results from observations and predictions from stellar models, and reveal the connection between curvature and stellar structure. Methods. We used Kepler data of red-giant stars and computed the curvature for several thousand stars. We compared these to the curvature derived from MESA models. We subsequently investigated the trends and differences between results from observations and models. Finally, we computed sensitivity kernels to identify the stellar region(s) to which the curvature is most sensitive and performed a glitch analysis. Results. We found that the curvature is sensitive to evolutionary phase and mass. Interestingly, the observed values and values from models show some discrepancies. Including the surface effect in the model frequencies reduces the discrepancies, though it introduces a frequency-dependent over- or under-estimation of the curvature from the models compared to the observations. From the kernels, we confirmed that the curvature is mostly sensitive to the near-surface layers of the star. The glitch analysis shows that in theory this provides information on the location and strength of the He I and H I ionisation layers. Conclusions. The curvature provides a probe into the near-surface structure of the star. The deviations between the curvature derived from observations and models call for improvements in the near-surface layers of stellar models.}, author = {Hekker, S. and Elsworth, Y. and Basu, S. and Ahlborn, F. and Ball, W. H. and Bellinger, E. P. and Buchele, Lynn and Espinoza-Rojas, F.}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars}}, doi = {10.1051/0004-6361/202557690}, volume = {709}, year = {2026}, } @article{23047, abstract = {Aims. We investigate signatures of pressure extrema on global oscillations in discs. Methods. We used the framework of wave topology to establish a generalised local dispersion relation that includes pressure gradients. We highlight the influence of a previously unrecognised epicyclic–acoustic frequency, and we derive an analytical criterion for the existence of a branch of modes transiting between the inertial and the pressure bands, known as topological modes. Results. We find that pressure extrema consist of wave guides in which such topological modes propagate. The fundamental mode trapped at a pressure bump can propagate at any frequency, allowing it to resonate with any temporal forcing. Conversely, the fundamental mode associated with a pressure dip propagates at any vertical phase velocity. These specific features make them attractive candidates for future discoseismology.}, author = {Leclerc, Armand and Laibe, Guillaume and Lynch, Elliot and Perez, Nicolas}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, keywords = {accretion, accretion disks, hydrodynamics, instabilities, waves, protoplanetary disks}, publisher = {EDP Sciences}, title = {{Radial modes of pressure bumps and dips in astrophysical discs}}, doi = {10.1051/0004-6361/202558428}, volume = {708}, year = {2026}, } @phdthesis{22744, author = {Javoor, Manjunath}, isbn = {978-3-99078-090-9 }, issn = {2663-337X}, keywords = {Actin cytoskeleton, Cell migration, cryo-electron tomography}, pages = {121}, publisher = {Institute of Science and Technology Austria }, title = {{Large-scale imaging of cellular actin networks at single filament resolution using montage cryo-electron tomography}}, doi = {10.15479/AT-ISTA-22744}, year = {2026}, } @article{21754, abstract = {The origin(s) of life (OoL), which has puzzled scientists for centuries, remains a major scientific challenge in the 21st century. Research on OoL spans many disciplines, including chemistry, physics, biology, planetary sciences, computer science, and mathematics. The sheer number of different scientific perspectives relevant to the problem has resulted in the coexistence of diverse tools, techniques, data, and software in OoL studies. This has made communication between the disciplines relevant to the OoL extremely difficult because the interpretation of data, analyses, or standards of evidence varies dramatically. Here, we hope to bridge this wide field of study by providing common ground via the consolidation of techniques rather than positing a unifying view on how life emerges. In part 1 of this review, we cover common experimental techniques that have been used significantly in OoL studies in recent years, while in part 2, we review theoretical, computational, and integrative methods. Here, we discuss the use of spectroscopy, spectrometry, chromatography, microscopy, and sequencing methods for characterizing diverse materials. We further discuss the role of data repositories in facilitating the analysis and dissemination of experimental data. This review provides a baseline expectation and understanding of the analytical aspects of origins’ research. Ultimately, we aim to provide an educational tool that can facilitate more post-disciplinary collaborations in OoL research by helping scientists understand what they can do about the problem of life’s origins, rather than telling them how to think about it.}, author = {Asche, Silke and Bautista, Carla and Blanco, Celia and Boulesteix, David and Champagne-Ruel, Alexandre and Mathis, Cole and Markovitch, Omer and Peng, Zhen and Dass, Avinash Vicholous and Adams, Alyssa and Camprubi, Eloi and Colizzi, Enrico Sandro and Colón-Santos, Stephanie and Dromiack, Hannah and Erastova, Valentina and Garcia, Amanda and Grimaud, Ghjuvan and Halpern, Aaron and Harrison, Stuart A. and Jordan, Seán F. and Jia, Tony Z. and Kahana, Amit and Kolchinsky, Artemy and Moron-Garcia, Odin and Mizuuchi, Ryo and Nan, Jingbo and Orlova, Yuliia and Pearce, Ben K.D. and Paschek, Klaus and Preiner, Martina and Pinna, Silvana and Rodríguez-Román, Eduardo and Schwander, Loraine and Sharma, Siddhant and Smith, Harrison B. and Vieira, Andrey and Xavier, Joana C.}, issn = {2666-3864}, journal = {Cell Reports Physical Science}, number = {4}, publisher = {Cell Press}, title = {{What it takes to solve the origin of life: An integrated review. Part 1–Experimental methods and data repositories}}, doi = {10.1016/j.xcrp.2026.103212}, volume = {7}, year = {2026}, } @article{21753, abstract = {The origin(s) of life (OoL), which has puzzled scientists for centuries, remains a major scientific challenge in the 21st century. Understanding the processes relevant to the OoL demands theoretical frameworks that can connect processes across scales, from microscopic dynamics to emergent levels of organization. While experimental studies generate a wealth of data, theoretical and computational approaches provide the structure necessary to interpret and generalize these findings. In Part 1, we examined the most widely used experimental techniques in the field. Here, we focus on the mathematical, physical, and computational techniques used to model phenomena relevant to life’s origin(s). We discuss methods ranging from quantum chemistry and molecular dynamics to chemical reaction networks, autocatalysis, and evolutionary modeling, as well as information-theoretic and phylogenetic approaches that link chemical and biological organization. We further highlight emerging trends such as synthetic biology, omics-based methods, and laboratory automation as novel points of contact for theory-experiment integration. Ultimately, we aim to provide an educational tool that can facilitate more post-disciplinary collaborations in OoL research by helping scientists understand what they can do about the problem of life’s origins, rather than telling them how to think about it.}, author = {Asche, Silke and Bautista, Carla and Blanco, Celia and Boulesteix, David and Champagne-Ruel, Alexandre and Mathis, Cole and Markovitch, Omer and Peng, Zhen and Dass, Avinash Vicholous and Adams, Alyssa and Camprubi, Eloi and Colizzi, Enrico Sandro and Colón-Santos, Stephanie and Dromiack, Hannah and Erastova, Valentina and Garcia, Amanda and Grimaud, Ghjuvan and Halpern, Aaron and Harrison, Stuart A. and Jordan, Seán F. and Jia, Tony Z. and Kahana, Amit and Kolchinsky, Artemy and Moron-Garcia, Odin and Mizuuchi, Ryo and Nan, Jingbo and Orlova, Yuliia and Pearce, Ben K.D. and Paschek, Klaus and Preiner, Martina and Pinna, Silvana and Rodríguez-Román, Eduardo and Schwander, Loraine and Sharma, Siddhant and Smith, Harrison B. and Vieira, Andrey and Xavier, Joana C.}, issn = {2666-3864}, journal = {Cell Reports Physical Science}, number = {4}, publisher = {Cell Press}, title = {{What it takes to solve the origins of life: An integrated review. Part 2: Theoretical methods and emerging trends}}, doi = {10.1016/j.xcrp.2026.103211}, volume = {7}, year = {2026}, } @article{21744, abstract = {The paraventricular hypothalamus (PVH) controls behavioral and physiologic processes, including appetite, social behavior, autonomic outflow, and pituitary hormone secretion. However, molecular markers for centrally projecting PVH neuron populations remain largely undefined, and a complete census of PVH cell types has not been established. Therefore, we performed extensive single-cell/nucleus RNA sequencing to catalog PVH neuron subtypes and multiplexed error-robust fluorescence in situ hybridization (MERFISH) to map them spatially. Our spatial transcriptomic atlas resolves 26 Sim1+ and 29 GABAergic neuron populations from the PVH and surrounding areas. Additionally, projection-based profiling identified neurons that project to the parabrachial region (PB) and spinal cord, helping to determine PVH populations that regulate satiety and sympathetic nervous system activity, respectively. Notably, activation of PB-projecting PVH neurons expressing Brs3 reduces food intake, and silencing them causes obesity. Together, this atlas contributes high-resolution PVH spatial and circuit-based gene expression profiles, representing a valuable resource for the field of homeostasis.}, author = {Li, Yuxi and Butler, Trevor C. and Nardone, Stefano and Jacobs, Christopher L. and Douglass, Amelia May Barnett and Madara, Joseph C. and McDonough, Miriam C. and Tao, Jenkang and Lowenstein, Elijah D. and Wang, Luhong and Pant, Deepti and Walker, Samuel J. and Wang, Annette and Srinivasan, Harini and Yang, Zongfang and Campbell, John N. and Tsai, Linus T. and Lowell, Bradford B. and Resch, Jon M.}, issn = {2211-1247}, journal = {Cell Reports}, number = {2}, publisher = {Cell Press}, title = {{A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types}}, doi = {10.1016/j.celrep.2025.116904}, volume = {45}, year = {2026}, } @article{21490, abstract = {Auxin canalization is a self-organizing process that governs the flexible formation of vasculature by reinforcing the formation of auxin transport channels. A key prerequisite is the feedback between auxin signaling and directional auxin transport, mediated by PIN transporters. Despite the developmental importance of canalization, the molecular components linking auxin perception to the regulation of PIN auxin transporters remain poorly understood. Here, we identify TOW, a novel and essential component of auxin canalization that links intracellular auxin signaling with cell surface auxin perception. TOW is regulated downstream of TIR1/AFB-Aux/IAA-WRKY23 transcriptional auxin signaling. tow mutants exhibit defects in regeneration and de novo vasculature formation, along with impaired formation of polarized, PIN-expressing auxin channels. At the subcellular level, these mutants display disrupted auxin-induced PIN polarization and altered PIN endocytic trafficking dynamics. TOW localizes predominantly to the plasma membrane, where it interacts with receptor-like kinases involved in auxin canalization, including the TMK1 auxin co-receptor and the CAMEL-CANAR complex. TOW promotes PIN interaction with these kinases and stabilizes PINs at the cell surface. Together, our findings identify TOW as a molecular link between intracellular and cell surface auxin signaling mechanisms that converge on PIN trafficking and polarity, providing new insights into how auxin signaling regulates directional auxin transport for the self-organizing formation of vasculature during flexible plant development.}, author = {Li, Mingyue and Rydza, Nikola and Mazur, Ewa and Molnar, Gergely and Nodzyński, Tomasz and Friml, Jiří}, issn = {0960-9822}, journal = {Current Biology}, number = {6}, pages = {1468--1480.e6}, publisher = {Cell Press}, title = {{Receptor-like-kinase-interacting protein TOW stabilizes PIN transporters for auxin canalization}}, doi = {10.1016/j.cub.2026.02.023}, volume = {36}, year = {2026}, } @article{21509, abstract = {Chromatin remodeling complexes mobilize nucleosomes and promote transcription factor (TF) binding. Using ensemble and single-molecule assays combined with cryo-electron microscopy (cryo-EM), we studied the interaction between pioneer TFs OCT4–SOX2 and the human BRG1/BRM-associated factor (BAF) complex on nucleosomes. BAF engages TF-bound substrates in two orientations, placing OCT4–SOX2 at either the remodeler ENTRY or EXIT site. At the ENTRY site, OCT4–SOX2 initially coexists with BAF without structural interference. However, continued DNA translocation is expected to cause collisions with bound TFs, which can trigger remodeling direction reversals or may induce TF dissociation. To accommodate TFs at the EXIT site, BAF undergoes structural rearrangements, and ensemble assays reveal a nucleosome subpopulation translocating away from TF-binding sites. Moreover, single-molecule experiments show that nucleosome-bound BAF frequently changes remodeling direction, and we identify an ADP-bound remodeler conformation as a potential intermediate. Together, these findings reveal key aspects of the conformational dynamics and remodeling outcomes underlying BAF processing of TF-bound nucleosomes.}, author = {Weiss, Joscha and Vecchia, Luca and Domjan, David and Cavadini, Simone and Sabantsev, Anton and Kempf, Georg and Pathare, Ganesh R. and Brackmann, Klaus and Michael, Alicia and Kater, Lukas and Hietter-Pfeiffer, Eric and Haddawi, Mina and Kuber, Urja P. and Mühlhäusser, Sandra and Grand, Ralph S. and Stadler, Michael B. and Deindl, Sebastian and Thomä, Nicolas H.}, issn = {1097-2765}, journal = {Molecular Cell}, number = {4}, pages = {625--639.e8}, publisher = {Cell Press}, title = {{The human BAF chromatin remodeler processes nucleosomes bound by pioneer transcription factors OCT4–SOX2}}, doi = {10.1016/j.molcel.2026.01.021}, volume = {86}, year = {2026}, } @article{21761, abstract = {Neural tube closure is a critical morphogenetic process in vertebrate development, and failure to close cranial regions such as the hindbrain neuropore (HNP) leads to severe congenital malformations. While mechanical forces such as actomyosin purse-string contraction and directional cell crawling have been implicated in driving HNP closure, how these forces organize local cell shape and motion to produce large-scale tissue remodeling remains poorly understood. Using live and fixed imaging of mouse embryos combined with cell-based biophysical modeling, we show that these force-generating mechanisms are insufficient to explain the reproducible patterns of cell elongation and nematic alignment observed at the HNP border. Instead, we show that local anisotropic stress and cytoskeletal organization are required to generate these patterns and promote midline cell motion. Our model captures key features of cell shape dynamics and emergent nematic order, which we confirm experimentally, including the alignment of actin fibers with cell shape and enhanced midline cell speed. Comparative analysis with chick embryos, which lack supracellular purse strings, supports a conserved link between tension generation and cellular patterning. These findings establish a physical framework connecting force generation, cell shape anisotropy, and tissue morphodynamics during epithelial gap closure.}, author = {Perez Verdugo, Fernanda L and Maniou, Eirini and Galea, Gabriel L. and Banerjee, Shiladitya}, issn = {1879-0445}, journal = {Current Biology}, number = {8}, pages = {1903--1917.e5}, publisher = {Cell Press}, title = {{Mechanosensitive feedback organizes cell shape and motion during hindbrain neuropore morphogenesis}}, doi = {10.1016/j.cub.2026.02.068}, volume = {36}, year = {2026}, } @article{21955, abstract = {AgRP neurons cause hunger, the drive to seek and consume food. Their activation by fasting is key for survival and is thought to be triggered by feedback when energy stores are low. However, we know that environmental cues can also regulate AgRP neurons since cues that predict future food intake rapidly inhibit AgRP neurons, but is the converse true: can the prediction of future fasting rapidly activate AgRP neurons? Here, we show in mice that such rapid fasting activation of AgRP neurons does occur. This rapid activation is driven by excitatory input from paraventricular hypothalamic (PVH) neurons expressing Sim2, which are bidirectionally sensitive to predictions of future energy state. Thus, cognitively processed contextual information conveyed by PVHSim2 neurons strongly activates AgRP neurons. Lastly, chronic silencing of PVHSim2 neurons causes persistent hypophagia. This PVHSim2-to-AgRP-neuron circuit, by anticipating and preventing negative energy balance, provides an important new dimension of hunger regulation.}, author = {Walker, Samuel J. and Lowenstein, Elijah D. and Douglass, Amelia May Barnett and Thomas, Callum M.P. and Madara, Joseph C. and Kucukdereli, Hakan and Barbosa-Meillon, Eunice A. and Tao, Jenkang and Resch, Jon M. and Lowell, Bradford B.}, issn = { 1097-4199}, journal = {Neuron}, keywords = {hunger, hypothalamus, AGRP neurons, neuroscience, metabolism, homeostasis, feeding, food intake, energy balance, appetite}, publisher = {Cell Press}, title = {{A hypothalamic circuit for anticipating future changes in energy balance}}, doi = {10.1016/j.neuron.2026.05.010}, year = {2026}, } @article{22144, abstract = {Most cells polarize and migrate in response to electrical fields. In this issue of Cell, Belliveau et al. identify TMEM154/Galvanin, a receptor that serves as a cellular antenna to sense electrical gradients and guide migration toward the cathode.}, author = {Riedl, Michael and Sixt, Michael K}, issn = {1097-4172}, journal = {Cell}, number = {13}, pages = {3845--3846}, publisher = {Cell Press}, title = {{A new sense for electrical fields}}, doi = {10.1016/j.cell.2026.05.038}, volume = {189}, year = {2026}, } @article{20972, abstract = {Small amounts of stress are thought to have beneficial effects. A new study reports a mechanism by which the psychedelic drug, psilocybin, causes acute release of stress hormones, despite its known long-term anti-anxiety effects.}, author = {Kücükdereli, Hakan and Douglass, Amelia May Barnett}, issn = {1879-0445}, journal = {Current Biology}, number = {1}, pages = {R27--R29}, publisher = {Cell Press}, title = {{Neuroscience: What doesn’t kill you makes you stronger}}, doi = {10.1016/j.cub.2025.11.056}, volume = {36}, year = {2026}, } @article{20859, abstract = {Effective immune responses rely on the efficient migration of leukocytes. Yet, how temperature regulates migration dynamics at the single-cell level has remained poorly understood. Using zebrafish embryos and mouse tissue explants, we found that temperature positively regulates leukocyte migration speed, exploration, and arrival frequencies to wounds and lymph vessels. Complementary 2D and 3D cultures revealed that this thermokinetic control of cell migration is conserved across immune cell types, independently of the 3D tissue environment. By applying precise (sub-)cellular temperature modulation, we identified a rapid and reversible thermo-response that depends on myosin II activity. Small physiological increases in temperature (1°C –2°C), as present during fever-like conditions, profoundly increased immune responses by accelerating arrival times at lymphatic vessels and tissue wounds. These findings identify myosin-II-dependent actomyosin contractility as a critical mechanical structure regulating single-cell thermo-adaptability, with physiological implications for tuning the speed of immune responses in vivo.}, author = {Company-Garrido, Iván and Zurita Carpio, Alberto and Colomer-Rosell, Mariona and Ciraulo, Bernard and Molkenbur, Ronja and Lanzerstorfer, Peter and Pezzano, Fabio and Agazzi, Costanza and Hauschild, Robert and Jain, Saumey and Jacques, Jeroen M. and Venturini, Valeria and Knapp, Christian and Xie, Yufei and Merrin, Jack and Weghuber, Julian and Schaaf, Marcel and Quidant, Romain and Kiermaier, Eva and Ortega Arroyo, Jaime and Ruprecht, Verena and Wieser, Stefan}, issn = {1878-1551}, journal = {Developmental Cell}, keywords = {thermobiology, cell migration, thermo-adaptability of immune cells}, number = {2}, pages = {356--371.e12}, publisher = {Cell Press}, title = {{Myosin II regulates cellular thermo-adaptability and the efficiency of immune responses}}, doi = {10.1016/j.devcel.2025.10.006}, volume = {61}, year = {2026}, } @article{20935, abstract = {In situ cryo-electron tomography (cryo-ET) has emerged as the method of choice to investigate the structures of biomolecules in their native context. However, challenges remain for the efficient production and sharing of large-scale cryo-ET datasets. Here, we combined cryogenic plasma-based focused ion beam (cryo-PFIB) milling with recent advances in cryo-ET acquisition and processing to generate a dataset of 1,829 annotated tomograms of the green alga Chlamydomonas reinhardtii, which we provide as a community resource to drive method development and inspire biological discovery. To assay data quality, we performed subtomogram averaging of both soluble and membrane-bound complexes ranging in size from >3 MDa to ∼200 kDa, including 80S ribosomes, Rubisco, nucleosomes, microtubules, clathrin, photosystem II, and mitochondrial ATP synthase. The majority of these density maps reached sub-nanometer resolution, demonstrating the potential of this C. reinhardtii dataset as well as the promise of modern cryo-ET workflows and open data sharing to empower visual proteomics.}, author = {Kelley, Ron and Khavnekar, Sagar and Righetto, Ricardo D. and Heebner, Jessica and Obr, Martin and Zhang, Xianjun and Chakraborty, Saikat and Tagiltsev, Grigory and Michael, Alicia and Van Dorst, Sofie and Waltz, Florent and Mccafferty, Caitlyn L. and Lamm, Lorenz and Zufferey, Simon and Van Der Stappen, Philippe and Van Den Hoek, Hugo and Wietrzynski, Wojciech and Harar, Pavol and Wan, William and Briggs, John A.G. and Plitzko, Jürgen M. and Engel, Benjamin D. and Kotecha, Abhay}, issn = {1097-4164}, journal = {Molecular Cell}, number = {1}, pages = {213--230.e7}, publisher = {Cell Press}, title = {{Toward community-driven visual proteomics with large-scale cryo-electron tomography of Chlamydomonas reinhardtii}}, doi = {10.1016/j.molcel.2025.11.029}, volume = {86}, year = {2026}, } @article{20986, abstract = {During complex vocal interactions, different features of acoustic stimuli are integrated to produce appropriate vocal responses,1 such as copying sounds during vocal matching behavior in some animals.2,3,4,5,6,7,8,9,10,11,12 However, little is known about the interplay and possible trade-offs between the different temporal and spectral acoustic features during these vocal exchanges.2,13,14 Nightingales can flexibly match the pitch of their tonal “whistle songs” in real time during counter-singing duels.15,16 Here, we show that the syllable duration of whistle playbacks could alter the song responses of wild nightingales, causing their whistle duration distribution to shift toward the presented stimulus duration. When exposed to whistle playbacks featuring unnatural combinations of pitch and duration, nightingales demonstrate a flexible trade-off between pitch matching and temporal imitation, yet they are constrained by their vocal repertoire. They selectively adapted their vocal responses to approximate these novel stimuli, aligning them with their natural whistle repertoire. We developed a computational model of nightingale whistle-matching behavior that revealed a hierarchical organization of acoustic feature production. During whistle matching, the feature integration process is constrained by the duration of syllables, and pitch matching follows within this temporal framework, forcing a trade-off between the two features. Our findings reveal a complex interplay between the spectral and temporal domains that shapes song-matching behavior.}, author = {Calderon Garcia, Juan Sebastian and Costalunga, Giacomo and Vogels, Tim P and Vallentin, Daniela}, issn = {1879-0445}, journal = {Current Biology}, number = {3}, pages = {791--798.e6}, publisher = {Cell Press}, title = {{Interplay between syllable duration and pitch during whistle matching in wild nightingales}}, doi = {10.1016/j.cub.2025.12.025}, volume = {36}, year = {2026}, } @article{21502, abstract = {The mammalian brain stores glucose, the main circulating energy substrate, as glycogen. In rodents, the cerebellum contains relatively high glycogen levels, yet its cellular and subcellular distribution remains poorly defined. Using monoclonal antibodies against glycogen, we examined its distribution in the mouse cerebellar cortex. Glycogen was predominantly localized to Bergmann glia (BG) processes in the molecular layer and was also detected in Purkinje cells (PCs), the principal cerebellar neurons. To assess the functional significance of cerebellar glycogen, we analyzed behavior in mice lacking glycogen synthase 1 (Gys1) in BG or PCs using a floxed Gys1 line. Gys1 deficiency in either PCs or GFAP-positive cells reduced anxiety-like behavior, whereas combined deletion caused PC degeneration and ataxia. These findings reveal a critical role for glycogen metabolism in both astrocytes and neurons in cerebellar function.}, author = {Akther, Sonam and Lee, Ashley Bomin and Konno, Ayumu and Asiminas, Antonis and Vittani, Marta and Mishima, Tsuneko and Hirai, Hirokazu and Meehan, Claire Francesca and Duran, Jordi and Guinovart, Joan and Ashida, Hitoshi and Morita, Tsuyoshi and Baba, Otto and Shigemoto, Ryuichi and Nedergaard, Maiken and Hirase, Hajime}, issn = {2589-0042}, journal = {iScience}, number = {4}, publisher = {Cell Press}, title = {{Distribution and functional significance of rodent cerebellar glycogen}}, doi = {10.1016/j.isci.2026.115192}, volume = {29}, year = {2026}, } @article{20924, abstract = {Pioneer transcription factors (TFs) possess the ability to read out DNA motifs embedded within nucleosomes, driving changes in gene expression during cellular differentiation and reprogramming. Here, we present selected engagement on nucleosome sequencing (SeEN-seq), a protocol designed to systematically identify potential TF-binding sites on the nucleosome. We describe steps for nucleosome library assembly, SeEN-seq assay, and cryoelectron microscopy (cryo-EM) sample preparation. This protocol facilitates the preparation of homogeneous pioneer TF-nucleosome complexes for cryo-EM structure determination using single-particle analysis. For complete details on the use and execution of this protocol, please refer to Michael et al.1}, author = {Kobayashi, Wataru and Michael, Alicia and Ruangroengkulrith, Siwat and Kümmecke, Maximilian and Tachibana, Kikuë}, issn = {2666-1667}, journal = {STAR Protocols}, number = {1}, publisher = {Cell Press}, title = {{Protocol for integrative analysis of transcription factor-nucleosome interactions using SeEN-seq and cryo-EM structure determination}}, doi = {10.1016/j.xpro.2025.104295}, volume = {7}, year = {2026}, } @article{20725, abstract = {The canonical mechanism by which the phytohormone auxin regulates transcription has been one of the cornerstones of plant signaling. The recent unexpected discovery of cyclic AMP (cAMP) as a second messenger in this pathway has revised its foundations while leaving many open questions and gaps in our understanding; these will be discussed in this forum article.}, author = {Friml, Jiří}, issn = {1878-4372}, journal = {Trends in Plant Science}, number = {2}, pages = {136--138}, publisher = {Cell Press}, title = {{Role of cAMP in TIR1/AFB auxin signaling: Open issues}}, doi = {10.1016/j.tplants.2025.10.018}, volume = {31}, year = {2026}, }