@article{22262, abstract = {Mixed modes are observed in many low-mass evolved stars. They provide information about core rotation rates of these stars, which are lower than predicted by stellar evolution models. The mixed modes themselves have been invoked as an angular momentum (AM) transport mechanism, but estimating their transport efficiency requires knowledge of their amplitudes. We constrain, for the first time, the mixed-mode amplitudes in 2D hydrodynamical simulations of a 1.3M⊙ red giant using the code MUSIC. We perform two simulations with outer radial truncations at fractional radii ro/r⋆ = 0.90 and 0.98. We compare the modes in the simulation with those found using both GYRE and a Dedalus eigenvalue solver. Excellent frequency agreement is found for all p-dominated modes, with minor discrepancies for g-dominated modes, especially in the frequency range [60, 240] μHz. We find excellent eigenfunction agreement for all modes except those in this frequency range. According to empirical predictions, the largest kinetic energies are located around Vmax= 312.μHz, but in both simulations, the modes with frequencies of ν < 50 μHz have the largest kinetic energies. In the simulation with r/r⋆ = 0.98, the simulated modes have extrapolated surface velocities comparable to the empirical predictions, with the highest surface velocities in a bell-shaped curve peaking around ν = 700 μHz. The extrapolated surface velocities of the low-frequency modes are small and thus hard to observe, but their large kinetic energies deeper in the interior could significantly impact AM transport, which has not yet been investigated.}, author = {De Vries, Nils B. and Le Saux, Arthur and Baraffe, Isabelle and Guillet, Thomas and Townsend, Richard H.D. and Leclerc, Armand and Morison, Adrien}, issn = {1538-4357}, journal = {The Astrophysical Journal}, keywords = {Stellar physics, Stellar interiors, Asteroseismology, Stellar oscillations, Hydrodynamical simulations}, number = {2}, publisher = {IOP Publishing}, title = {{Revealing mixed modes in compressible hydrodynamical simulations of red giant stars}}, doi = {10.3847/1538-4357/ae7a3c}, volume = {1005}, year = {2026}, } @article{22261, abstract = {Climate change is significantly altering regional precipitation patterns across Europe and the Mediterranean. We analyze daily precipitation distribution changes in a 15-member Euro-CORDEX ensemble, through a diagnostic framework that separates occurrence changes, wet-days intensity shifts and distortions. At +4 ∘C global warming, Northern Europe shows a robust intensification of precipitation, driven by both higher occurrence and stronger events. Conversely, the Mediterranean exhibits a dominant drying signal, primarily due to fewer wet-days, which impacts daily precipitation distribution even for heavy rainfall. Transitional zones in the northern Mediterranean reveal “U-shape” regimes, with rising extremes but declining moderate rain. Comparing with ERA5 reanalysis over the past, low model agreement in the south highlights higher uncertainty in the Mediterranean region. The timing of robust signal emergence varies: Northern Europe shows robust patterns from +1 ∘C, while the Mediterranean exhibits delays until +3-4 ∘C. These findings are essential for informing risk-based adaptation strategies.}, author = {André, Julie and Chiabrando, Nicolas and Muller, Caroline J and Drobinski, Philippe and D’Andrea, Fabio}, issn = {2662-4435}, journal = {Communications Earth and Environment}, publisher = {Springer Nature}, title = {{Distinct regimes of precipitation changes across Europe and the Mediterranean under global warming}}, doi = {10.1038/s43247-026-03519-7}, volume = {7}, year = {2026}, } @article{22270, abstract = {The explosion of a white dwarf (WD) in a close binary can launch a surviving runaway star at velocities of ≳ 1000 km s−1 . Such runaways provide a direct probe of thermonuclear supernovae (SNe) in double-degenerate binaries. Several candidate runaways are known, but their evolutionary states and the demographics of the broader population are uncertain. To enable robust population inference, we carry out a systematic survey for hypervelocity runaways with a simple selection function, selecting candidates based on large Gaia-inferred tangential velocities and blue colors. We classify 100% of the resulting 92 candidates using a combination of spectroscopic follow-up and archival data. The search yields ten suspected D6 stars and three LP 40-365 stars. Three D6 stars are new discoveries, including two hot (Teff ≳ 50,000 K) objects and one cool (Teff ≈ 7,000 K) object. We forward-model our survey under several proposed D6 star evolutionary models, coupling each to a Galactic model and the survey selection function. No single model reproduces the observed diversity of D6 stars, which likely reflects a range of remnant masses, ages, and heating mechanisms. Models in which runaway companions are heated by SN shocks alone are too faint and short-lived to explain most of the observed sample, while fully reheated models are too luminous and long-lived. Models with intermediate heating, as occurs in some simulations of violent mergers and partially disrupted remnants, best match the observed magnitude, distance, and kinematic-age distributions. The inferred D6 star birth rate is model dependent, but the models that best match the observed population require rates of only a few percent of the Galactic SN Ia rate, perhaps implying that most SNe Ia result from WD binaries in which both components explode. If most SNe Ia do produce surviving runaways, these must be fainter or shorter-lived than the currently known runaways.}, author = {El-Badry, Kareem and Werner, Klaus and Shen, Ken J. and Strader, Jay and Rodriguez, Antonio C. and Han, Jiwon Jesse and Chandra, Vedant and Chomiuk, Laura and Vanderbosch, Zachary P. and Blomberg, Lisa and Yamaguchi, Natsuko and Nagarajan, Pranav and Caiazzo, Ilaria and van Roestel, Joannes C and Glanz, Hila and Wong, Tin Long Sunny and Bhat, Aakash and Hollands, Mark A.}, issn = {2565-6120}, journal = {The Open Journal of Astrophysics}, keywords = {white dwarfs, binaries: close, stars: chemically peculiar}, publisher = {Maynooth Academic Publishing}, title = {{A systematic survey for hypervelocity runaways from thermonuclear supernovae}}, doi = {10.33232/001c.164326}, volume = {9}, year = {2026}, } @article{22269, abstract = {The divisome apparatus synthesizes septal peptidoglycan (PG) during bacterial division. In Escherichia coli, the class A penicillin-binding protein (aPBP) called PBP1b has been implicated in division, but its role in the process has remained unclear. Here we show using in situ cryo-electron tomography, genetics and other imaging methods that PBP1b is required to produce a wedge-like density of PG at the division site and that loss of this structure weakens the division site, making it hypersusceptible to osmotic lysis. Surprisingly, the activator LpoB needed for general PBP1b function was not required for its role in division. Of the two PBP1b isoforms produced in cells, we show that the one with an extended cytoplasmic N terminus localizes to and functions at the division site, probably via recruitment by the FtsA component of the divisome. The conservation of aPBPs with extended cytoplasmic N termini suggests that other Gram-negative bacteria may use similar mechanisms for division site reinforcement.}, author = {Navarro, Paula P. and Vettiger, Andrea and Hajdu, Roman and Ananda, Virly Y. and López-Tavares, Alejandro and Schmid, Ernst W. and Walter, Johannes C. and Loose, Martin and Chao, Luke H. and Bernhardt, Thomas G.}, issn = {2058-5276}, journal = {Nature Microbiology}, publisher = {Springer Nature}, title = {{The penicillin-binding protein PBP1b fortifies the Escherichia coli division site against osmotic rupture}}, doi = {10.1038/s41564-026-02403-6}, year = {2026}, } @article{22288, abstract = {Soft solids and their surface deformations control the response of many natural and artificial systems. Yet, their underlying properties are vigorously debated, particularly for polymer networks. While molecular-scale theories predict no interfacial changes with macroscopic deformation, multiple experiments suggest otherwise. To settle this issue, we measure displacement fields near the interface of a silicone gel, in the limit of small deformations. We discover an unexpected multiscale response. The shear modulus decreases smoothly by half with 20  μ⁢m of the interface. At the same time we observe a surface excess elasticity, that depends on history and outer medium composition. These results reveal the fundamentally multiscale nature of polymeric surfaces, and call for further experimental and theoretical investigations into the basic understanding of soft solid interfaces.}, author = {Bain, Nicolas and Wilen, Lawrence A. and Gerber, Dominic and Zu, Mengjie and Goodrich, Carl Peter and Duraivel, Senthilkumar and Varma, Kaarthik and Koganti, Harsha and Style, Robert W. and Dufresne, Eric R.}, issn = {2160-3308}, journal = {Physical Review X}, number = {2}, publisher = {American Physical Society}, title = {{Multiscale interfacial mechanics of soft solids}}, doi = {10.1103/8msx-l8s7}, volume = {16}, year = {2026}, } @article{22286, abstract = {Plants are remarkable organisms. Unlike animals, they cannot flee and, rooted in one place, they must cope with whatever challenges arise — nutrient scarcity, drought, shade, wind or obstacles in the soil. Their extraordinary ability to survive in such unstable environmental conditions lies in their capacity to adapt. In response to environmental signals, plants can rapidly adjust the rate of organ growth, change the direction of growth, bend toward resources, or remodel their body architecture by promoting or suppressing the formation of new organs such as lateral roots, branches, leaves, or flowers. This unique developmental plasticity depends on chemical signals, plant hormones that serve as regulators and coordinators of endogenous molecular and cellular processes. Chief among these signals is auxin, a plant hormone central to nearly every aspect of plant life.}, author = {Leitner, Valentin and Benková, Eva}, issn = {0960-9822}, journal = {Current Biology}, number = {13}, pages = {R739--R744}, publisher = {Elsevier}, title = {{Auxin and the control of plant growth and development}}, doi = {10.1016/j.cub.2026.04.047}, volume = {36}, year = {2026}, } @article{22291, abstract = {Persistent homology is a fundamental tool in Topological Data Analysis. The associated algebraic structure is the persistence module, a sequence of vector spaces connected by linear maps. Persistence modules admit a complete and fast-to-compute invariant known as the persistence diagram. However, this is no longer the case for maps between persistence modules (i.e. persistence maps). We propose a new invariant for persistence maps, consisting of a partial matching between the persistence diagrams of the domain and codomain modules. We show that this invariant is additive with respect to the direct sum decomposition of persistence maps, is more discriminative than the image module, and is computable in cubic time. Furthermore, we provide an implementation and demonstrate its efficiency by integrating it with edge collapse techniques for flag complexes (e.g., Vietoris–Rips complexes). As a key technical contribution, we describe how to induce a persistence map between two flag complexes that have been independently simplified via edge collapses, even when a direct simplicial map between them is no longer available.}, author = {Gonzalez-Diaz, Rocio and Soriano Trigueros, Manuel and Torras-Casas, Alvaro}, issn = {1095-855X}, journal = {Journal of Symbolic Computation}, keywords = {Persistence module, Persistence map, Persistent homology}, publisher = {Elsevier}, title = {{Additive partial matchings induced by persistence maps}}, doi = {10.1016/j.jsc.2026.102598}, volume = {138}, year = {2026}, } @article{22289, abstract = {Single-stranded, helically folded aromatic oligoamides bearing anionic phosphonate side chains have been shown to bind to some DNA-binding proteins better than DNA itself. However, these DNA mimic foldamers have until now mainly consisted of a single repeat motif, like a poly(dA:dT) DNA duplex, and contained limited sequence information. Here, we introduce new monomers designed to display different chemical functionalities in the major groove of the DNA mimics. Four new Fmoc-protected amino acid monomers have been synthesized and incorporated into oligomers. Sixteen foldamer sequences were prepared on solid phase. Their conformations in solution and in the solid state and their conformational dynamics were investigated using nuclear magnetic resonance, circular dichroism, molecular modeling, and X-ray crystallography. The results show that three of the four new monomers behaved as designed and that their introduction enhances the conformational dynamics of the DNA mimic foldamers. In a fourth case, conformational behavior proved to be more complex than expected. The modified sequences retained the ability to bind to the bacterial histone-like protein HU. These results showcase design strategies to manipulate large molecular biomimetics in which not only side chains but also main chain components are varied. The new monomers pave the way to complex DNA mimic foldamer sequences targeting proteins that recognize sequence-selective DNA-binding proteins such as transcription factors or restriction enzymes.}, author = {Wu, Jiaojiao and Corvaglia, Valentina and Chakrabortty, Tulika and Mandal, Pradeep K and Huc, Ivan}, issn = {2041-6539}, journal = {Chemical Science}, publisher = {Royal Society of Chemistry}, title = {{Tailoring the major groove of DNA mimic foldamers}}, doi = {10.1039/d6sc00798h}, year = {2026}, } @article{22290, abstract = {We introduce a multi-band BCS free energy functional and prove that for a multi-band superconductor the effect of inter-band coupling can only increase the critical temperature, irrespective of its attractive or repulsive nature and its strength. Further, for weak coupling and weaker inter-band coupling, we prove that the dependence of the increase in critical temperature on the inter-band coupling is (1) linear, if there are two or more equally strongly superconducting bands, or (2) quadratic, if there is only one dominating band.}, author = {Henheik, Sven Joscha and Langmann, Edwin and Lauritsen, Asbjørn Bækgaard}, issn = {1424-0661}, journal = {Annales Henri Poincaré}, publisher = {Springer Nature}, title = {{Multi-band superconductors have enhanced critical temperatures}}, doi = {10.1007/s00023-026-01706-y}, year = {2026}, } @article{22292, abstract = {We show that a suitable choice of boundary conditions for the Laplacian allows for the appearance of an arbitrary number of condensates, described by arbitrary harmonic functions, in the thermodynamic limit of an ideal Bose gas.}, author = {De Wilde, Michiel and Seiringer, Robert}, issn = {1089-7658}, journal = {Journal of Mathematical Physics}, number = {6}, publisher = {AIP Publishing}, title = {{Arbitrary harmonic functions as Bose–Einstein condensates}}, doi = {10.1063/5.0325354}, volume = {67}, year = {2026}, } @inbook{22293, abstract = {In order to cope with arid terrestrial environments, angiosperms have evolved a unique fertilization way—siphonogamy. The success of siphonogamy requires several prerequisites, including the normal development of the female gametophyte and male gametophyte (pollen). Appropriate pollination methods ensure the successful encounter between pollen and the stigma. After pollen lands on the stigma, pollen/pollen tube interacts with different tissues and cells of the pistil, completing a series of male-female communications. The smooth progress of these interactions ensures that the pollen tube can enter the female gametophyte, burst, and release sperm cells to complete the double fertilization. In this chapter, we provide an overview of pollination and the interactions between male and female, comprehensively summarizing the factors involved in these processes.}, author = {Zhong, Sheng and Lan, Zijun and Ge, Zengxiang and Qu, Li-Jia}, booktitle = {Regulation of Plant Development}, editor = {Chang, Fang and Wang, Yingxiang and Ma, Hong}, isbn = {9789819570324}, pages = {537--615}, publisher = {Springer Nature}, title = {{Pollination and Fertilization}}, doi = {10.1007/978-981-95-7033-1_14}, year = {2026}, } @article{21378, abstract = {From insects to mammals, essential brain functions, such as forming long-term memories (LTMs), increase metabolic activity in stimulated neurons to meet the energetic demand associated with brain activation. However, while impairing neuronal metabolism limits brain performance, whether expanding the metabolic capacity of neurons boosts brain function remains poorly understood. Here, we show that LTM formation of flies and mice can be enhanced by increasing mitochondrial metabolism in central memory circuits. By knocking down the mitochondrial Ca2+ exporter Letm1, we favour Ca2+ retention in the mitochondrial matrix of neurons due to reduction of mitochondrial H+/Ca2+ exchange. The resulting increase in mitochondrial Ca2+ over-activates mitochondrial metabolism in neurons of central memory circuits, leading to improved LTM storage in training paradigms in which wild-type counterparts of both species fail to remember. Our findings unveil an evolutionarily conserved mechanism that controls mitochondrial metabolism in neurons and indicate its involvement in shaping higher brain functions, such as LTM.}, author = {Amrapali Vishwanath, Anjali and Comyn, Typhaine and Mira, Rodrigo G. and Brossier, Claire and Pascual-Caro, Carlos and Faour, Maya and Boumendil, Kahina and Chintaluri, Chaitanya and Ramon-Duaso, Carla and Fan, Ruolin and Ghosh, Kishalay and Farrants, Helen and Berwick, Jean-Paul and Sivakumar, Riya and Lopez-Manzaneda, Mario and Schreiter, Eric R. and Preat, Thomas and Vogels, Tim P and Rangaraju, Vidhya and Busquets-Garcia, Arnau and Plaçais, Pierre-Yves and Pavlowsky, Alice and de Juan-Sanz, Jaime}, issn = {2522-5812}, journal = {Nature Metabolism}, number = {2}, pages = {467--488}, publisher = {Springer Nature}, title = {{Mitochondrial Ca2+ efflux controls neuronal metabolism and long-term memory across species}}, doi = {10.1038/s42255-026-01451-w}, volume = {8}, year = {2026}, } @article{22296, abstract = {The detection of strong Balmer breaks and absorption features in Little Red Dots (LRDs) suggests they host active galactic nuclei embedded within dense gas envelopes, potentially powered by super-Eddington accretion. We present GLIMPSE-17775, a luminous (Lbol ∼ 1045 erg s−1) LRD at z = 3.501 behind Abell S1063 (μ ∼ 2), observed with deep JWST/NIRCam and a ∼20 hr (80 hr delensed) NIRSpec G395M spectrum. The data reveal over 40 emission and absorption features, including a rich forest of low-ionization Fe ii lines and numerous broad hydrogen recombination transitions. We use this depth to test the dense-gas interpretation through five independent diagnostics. Nearly all permitted lines show exponential wings with consistent FWHM, a signature of Thomson scattering requiring ne ≳ 108 cm−3. Adopting this width yields MBH ∼ 106.7M⊙, a factor of 10 lower than Gaussian fits, and λEdd ∼ 1.8. Additional diagnostics support the same picture: a pronounced Balmer break (fν,4050/fν,3670 = 2.0 ± 0.1), enhanced He i λ7065 and λ10830 with P-Cygni absorption, Bowen-fluorescent O i λ8446–λ11290 emission requiring Lyβ pumping, and 16 Fe ii lines matching fluorescence models. These features indicate a dense (n ∼ 108 cm−3), partially ionized cocoon where scattering and fluorescence dominate line formation, providing strong evidence that at least some LRDs are powered by super-Eddington black hole growth in the early Universe.}, author = {Kokorev, Vasily and Chisholm, John and Naidu, Rohan P. and Fujimoto, Seiji and Atek, Hakim and Brammer, Gabriel and Finkelstein, Steven L. and Akins, Hollis B. and Berg, Danielle A. and Furtak, Lukas J. and Fei, Qinyue and Hsiao, Tiger Yu-Yang and Labbé, Ivo and Matthee, Jorryt J and Muñoz, Julian B. and Oesch, Pascal A. and Pan, Richard and Rinaldi, Pierluigi and Saldana-Lopez, Alberto and Schaerer, Daniel and Volonteri, Marta and Zitrin, Adi}, issn = {1538-4357}, journal = {The Astrophysical Journal}, number = {2}, publisher = {IOP Publishing}, title = {{The Deepest GLIMPSE of a dense gas cocoon enshrouding a Little Red Dot}}, doi = {10.3847/1538-4357/ae4ed7}, volume = {1004}, year = {2026}, } @article{22297, abstract = {Determination of the rheological properties of cells is known to require active measurements, which largely depend on the internalization of mechanical probes. Here, we circumvent this problem via the introduction of Rheological focused light-induced cytoplasmic streaming (Rheo-FLUCS): an active, yet probe-free approach that leverages light-induced flows to access mechanical changes in complex systems. While Rheo-FLUCS is facilitated by thermoviscous expansion phenomena rather than external forces, here we show equivalence in its ability to measure relative viscoelastic properties. Specifically, we demonstrate a phase-lag equivalence with probe-dependent active microrheology in a wide range of physically different, yet chemically identical materials. We exemplify the utility of Rheo-FLUCS in three distinctly different biological systems: compound-treated mouse fibroblasts (NIH-3T3), genetically modified human osteoblasts (U2OS) to elucidate the role of myosins in cytoplasmic mechanics, and early ascidian oocytes of Phallusia mammillata at fertilization stage. Our biological use-cases exemplify the application versatility of Rheo-FLUCS, which in the future may use phase information as a marker for developmental success.}, author = {Stoev, Iliya D and Bolger-Munro, Madison and Minopoli, Antonio and Wagner, Susan and Krishnaswamy, Venkat Raghavan and Erben, Elena and Weißenbruch, Kai and Maghelli, Nicola and Bastmeyer, Martin and Heisenberg, Carl-Philipp J and Kreysing, Moritz}, issn = {2752-6542}, journal = {PNAS Nexus}, keywords = {cell mechanics, active microrheology, noninvasiveness, thermoviscous flows, FLUCS}, number = {6}, publisher = {Oxford University Press}, title = {{Active and probe-free intracellular rheology via phase-sensitive thermoviscous flows}}, doi = {10.1093/pnasnexus/pgag190}, volume = {5}, year = {2026}, } @inbook{22300, abstract = {As seen in previous chapters, a graph game proceeds by placing a token on one of the vertices and allowing the players to move it throughout the graph to produce an infinite trace, which determines the winner or payoff of the game.}, author = {Avni, Guy and Henzinger, Thomas A}, booktitle = {Games on Graphs. From Logic and Automata to Algorithms}, editor = {Fijalkow, ‪Nathanaël}, isbn = {9781009500685}, pages = {529--569}, publisher = {Cambridge University Press}, title = {{Bidding Games}}, doi = {10.1017/9781009500678.022}, year = {2026}, } @article{22303, abstract = {We present the discovery of AT 2024wpp (‘Whippet’), a fast and luminous 18cow-like transient. At a redshift of z = 0 . 0868 , revealed by Keck Cosmic Web Imager spectroscopy of its faint star-forming host, it is the fourth-nearest example of its class to date. Rapid identification of the source in the Zwicky Transient Facility data stream permitted ultraviolet-through- optical observations to be obtained prior to peak, allowing the first determination of the peak bolometric luminosity ( 2 ×1045 erg s−1 ), maximum photospheric radius ( 1015 cm), and total radiated energy ( 1051 erg) of an 18cow-like object. We present results from a comprehensive multiwavelength observing campaign, including a far-ultraviolet spectrum from the Cosmic Origins Spectrograph on the Hubble Space Telescope and deep imaging extending > 100 d post-explosion from the Very Large Telescope, Hubble Space Telescope , Very Large Array, and Atacama Large Millimetre Array. We interpret the observations under a model in which a rapidly accreting central engine blows a fast ( ∼0.2 c ) wind into the surrounding medium and irradiates it with X-rays. The high Doppler velocities and intense ionization within this wind prevent identifiable spectroscopic features from appearing in the ejecta or in the surrounding circumstellar material. Weak H and He signatures do emerge in the spectra after 35 d in the form of double-peaked narrow lines. Each peak is individually narrow (full width δv ∼3000 km s−1 ) but the two components are separated by v ∼6600 km s−1 , indicating stable structures of denser material, possibly representing streams of tidal ejecta or an ablated companion star.}, author = {Perley, Daniel A and Ho, Anna Y Q and McGrath, Zoë and Camilo, Michael and Sevilla, Cassie and Chen, Ping and Schroeder, Genevieve and Govreen-Segal, Taya and Bochenek, Aleksandra and Qin, Yu-Jing and Gillanders, James H and Amend, Benjamin and Anderson, Joseph P and Andreoni, Igor and Aryan, Amar and Bellm, Eric C and Bloom, Joshua S and de Boer, Thomas and Carney, Jonathan and Caiazzo, Ilaria and Chambers, Ken C and Charalampopoulos, Panos and Chen, Ting-Wan and Chen, Tracy X and Coughlin, Eric R and Coughlin, Michael and Dennefeld, Michel and Dimitriadis, Georgios and Fremling, Christoffer and Frostig, Danielle and Gal-Yam, Avishay and Galbany, Lluís and Gangopadhyay, Anjashay and Ghendrih, Melzie and Graham, Matthew J and Gromadzki, Mariusz and Groom, Steven L and Gutiérrez, Claudia P and Hinds, K -Ryan and Huber, Mark E and Inserra, Cosimo and Kaiser, Benjamin C and Kasliwal, Mansi M and Koivisto, Niilo E and Lin, Chien-Cheng and Liu, Chang and Lowe, Thomas B and Magnier, Eugene and Mahabal, Ashish A and Milligan, Andrew and Minguez, Paloma and Mo, Geoffrey and Müller-Bravo, Tomás E and Nicholl, Matt and Pessi, Priscila J and Pignata, Giuliano and Purdum, Josiah and Rehemtulla, Nabeel and Rich, R Michael and Sahu, Anwesha and Singh, Avinash and Smartt, Stephen J and Smith, Ian A and Sollerman, Jesper and Srinivasaragavan, Gokul and Srivastav, Shubham and Stein, Robert D and Schulze, Steve and Tweddle, Jack W and Wainscoat, Richard and Wise, Jacob L and Yan, Lin and Young, David R}, issn = {1365-2966}, journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {stars: black holes, supernovae: individual: AT2024wpp, radio continuum: transients}, number = {1}, publisher = {Oxford University Press}, title = {{AT 2024wpp: An extremely luminous fast ultraviolet transient powered by accretion onto a black hole}}, doi = {10.1093/mnras/stag678}, volume = {549}, year = {2026}, } @article{22301, abstract = {Auxin, primarily indole-3-acetic acid (IAA), is a central regulator of growth and development in land plants, but its physiological role in chlorophyte algae remains unclear. Here, we show that exogenous IAA modulates growth in Chlorella sorokiniana, Chlorella variabilis, and Chlamydomonas reinhardtii in a concentration-dependent manner. Low IAA concentrations promoted growth by accelerating the onset of cell division without affecting cell size, whereas higher concentrations inhibited proliferation. Radiotracer assays showed that all three species take up and release IAA across the plasma membrane through a combination of passive diffusion and energy-dependent, saturable processes. Competition by excess unlabeled natural and synthetic auxins further supported the presence of carrier-mediated transport with broad substrate recognition. Phylogenetic analyses identified potential PIN-like auxin exporters in chlorophytes and other non-plant eukaryotes, and structural modeling supported conservation of the overall PIN fold and predicted auxin-binding residues. However, functional assays in Xenopus laevis oocytes, tobacco BY-2 cultured cells, and Arabidopsis thaliana did not support a role for these proteins in directional auxin export. Instead, non-plant PIN homologs localized predominantly to the endoplasmic reticulum and showed limited or no transport activity in heterologous systems. Together, these findings indicate that auxin responsiveness and basic cellular auxin transport predate canonical PIN-mediated directional auxin export, which appears to be a later innovation of the streptophyte lineage.}, author = {Smoljan, Adrijana and Koutnik‐Abele, Sarah and Vladimirtsev, Dmitrii and Klíma, Petr and Bírošíková, Anita and Zhang, Yuzhou and Merrin, Jack and Schuster, Maximilian and Kurtović, Katarina and Hammes, Ulrich Z. and Petrášek, Jan and Friml, Jiří}, issn = {1744-7909}, journal = {Journal of Integrative Plant Biology}, publisher = {Wiley}, title = {{Auxin response and PIN‐mediated transport in chlorophyte algae}}, doi = {10.1111/jipb.70309}, year = {2026}, } @inproceedings{22129, abstract = {Inside–outside classification is widely used for geometry processing tasks such as surface reconstruction, geometry completion, and calculating signed distance fields. We introduce a new integral formulation of this problem, which assigns confidence scores that points are inside or outside, given incomplete boundary geometry. Even though our geometric construction does not appear in previous work, we show that it is unexpectedly linked to both the well-established generalized winding number (GWN) and pseudonormal methods for geometry completion, and it provably reduces to either one of them for specific values of a control parameter. The results obtained with our method frequently outperform screened Poisson surface reconstruction (PSR), GWN, and the pseudonormal method in terms of quality, and are at least on par with them on all of our examples. Unlike these methods, our algorithm naturally extends to the multi-label setting, in which regions with an arbitrary number of colors or physical materials can be reconstructed, and non-manifold features such as T-junctions may appear in the interface and boundary geometry}, author = {Wei, Ziyu and Hafner, Christian and Kalinov, Aleksei and Synak, Peter and Wojtan, Christopher J}, booktitle = {Computer Graphics Forum}, location = {Bern, Switzerland}, number = {5}, publisher = {Wiley}, title = {{Circles of confidence for multi-label geometry completion}}, doi = {10.1111/cgf.70516}, volume = {45}, year = {2026}, } @inproceedings{22299, abstract = {The depth poset of a filtered Lefschetz complex reflects the dependencies between the cancellations of different shallow birth-death pairs. Using the fast algorithms for computing the depth poset in [Edelsbrunner et al., 2026] and for updating the persistence diagram under transpositions in [Cohen-Steiner et al., 2006], we give a complete case analysis of how transpositions of cells in the filter affect the depth poset. In addition, we present statistics on the depth poset for random point data and its sensitivity to the transpositions that occur in random straight-line homotopies.}, author = {Edelsbrunner, Herbert and Lipiński, Michał and Mrozek, Marian and Soriano Trigueros, Manuel and Zimin, Fedor}, booktitle = {42nd International Symposium on Computational Geometry}, isbn = {9783959774185}, issn = {1868-8969}, keywords = {Algebraic topology, Lefschetz complexes, persistent homology, vines and vineyards, birth-death pairs, shallow pairs, relations, partial orders, transpositions, Theory of computation → Computational geometry}, location = {New Brunswick, NJ, United States}, publisher = {Schloss Dagstuhl – Leibniz-Zentrum für Informatik}, title = {{The depth poset under transpositions in the filter}}, doi = {10.4230/LIPICS.SOCG.2026.41}, volume = {367}, year = {2026}, } @inproceedings{22298, abstract = {Air traffic management is a critical component of aviation, aiming to balance safety, capacity and demand within controlled airspace. This research analyses Iran's domestic air transport network (2018-2021) by developing annual Origin-Destination (OD) impedance matrices based on flight frequency. The methodology quantifies network connectivity, revealing a highly centralized structure dominated by core corridors like Tehran-Mashhad, which carried over 10,500 flights in 2019. The COVID-19 pandemic caused a severe disruption in 2020, with traffic on major routes falling by nearly half, followed by a partial recovery in 2021. Analysis shows core hubs rebounded faster than peripheral airports, widening accessibility gaps. Through origin-destination matrix processing, the system identifies high density air routes and analyses historical trends in airspace utilization. The impedance matrix, validated against data (R²=0.87), successfully maps the intense service on hub links and the high impedance of sparse peripheral routes. Then an interactive Web GIS platform was implemented for spatiotemporal analysis of air traffic density.}, author = {Eghbali Mardekheh, Masoumeh and Argany, Meysam and Karimipour, Farid and Sedghitabar, Seyed Mohammad}, booktitle = {8th ISPRS Geospatial Conference}, issn = {2194-9050}, keywords = {Air Traffic simulation, Dynamic Air Traffic Corridors, Origin Destination matrix, Interactive Web GIS, Iran Aviation Network, Spatiotemporal Modelling}, location = {Tehran, Iran}, number = {-4/W8-2025}, pages = {493--500}, publisher = {Copernicus Publications}, title = {{Real time interactive web GIS based modelling of high traffic air corridors in Iran using origin destination matrix analysis}}, doi = {10.5194/isprs-annals-x-4-w8-2025-493-2026}, volume = {X}, year = {2026}, }