@article{21899,
  abstract     = {Cell extrusion is an essential mechanism for controlling cell density in epithelial tissues. Another essential element of epithelia is curvature, which is required to achieve complex shapes, like in the lung or intestine. Here, we introduce a three-dimensional bubbly vertex model to study the interplay between extrusion and curvature. We find a generic cellular bulging instability at topological defects, which is much stronger than for standard vertex models. Analyzing cell shapes in three-dimensional imaging data of spherical mouse colon organoids, we infer that pentagonal cells have an increased basal interfacial tension, suggesting that cells at topological defects react to the different force conditions. Using the bubbly vertex model, we show that such basal tensions stabilize against the predicted instability and result in better cell shape control than tissue-scale mechanisms such as lumen pressure and spontaneous curvature. Our theory suggests that epithelial curvature naturally leads to bulged and extrusionlike cell shapes because the interfacial curvature of individual cells at the defects strongly amplifies buckling effected by tissue-scale topological defects in elastic sheets. Our results highlight the complex interplay of forces across scales in three-dimensional tissue organization.},
  author       = {Drozdowski, Oliver M and Kocameşe-Tamgac𝚤, Büşra and Boonekamp, Kim E. and Boutros, Michael and Schwarz, Ulrich S.},
  issn         = {2160-3308},
  journal      = {Physical Review X},
  number       = {2},
  publisher    = {American Physical Society},
  title        = {{Cell bulging and extrusion in a three-dimensional bubbly vertex model for curved epithelial sheets}},
  doi          = {10.1103/x82g-cq7n},
  volume       = {16},
  year         = {2026},
}

@article{21914,
  abstract     = {Cyclic adenosine monophosphate (cAMP) is a fundamental second messenger involved in diverse signaling pathways across both animals and plants. While the role of 3′,5′-cAMP has been extensively characterized, the biological significance of its structural isomer, 2′,3′-cAMP, remains largely unexplored, particularly in plants. Here, we show that 2′,3′-cAMP and 3′,5′-cAMP represent parallel signaling systems in Arabidopsis thaliana, with different enzymatic origins and largely distinct downstream effects. In vitro enzymatic assays show that plant adenylate cyclases (ACs), including AFB5 and HpAC1, produce specifically 3′,5′-cAMP from ATP, whereas the TIR domain of protein L7 also catalyzes the formation of 2′,3′-cAMP from RNA. Comprehensive multiomics analyses reveal that two isomers elicit distinct yet partially overlapping metabolic, proteomic, and transcriptional response: 2′,3′-cAMP activates broad, stress-adaptive gene expression reprogramming, while 3′,5′-cAMP fine-tunes responses related to nutrient status and cellular homeostasis. Our findings establish the existence of dual cAMP signaling systems in plants, each with specialized functions and provide insights into the complex regulatory networks governing plant physiology.},
  author       = {Li, Mingyue and Chodasiewicz, Monika and Muraleedharan, Malavika and Lopez, Israel M. and Gorka, Michal and Kerber, Olga and Alotaibi, Saqer S. and Nelson, Andrew D.L. and Lenobel, Rene and Friedecká, Jaroslava and Skirycz, Aleksandra and Friml, Jiří},
  issn         = {2375-2548},
  journal      = {Science Advances},
  number       = {19},
  publisher    = {AAAS},
  title        = {{Biogenesis and downstream effects of 3',5' and 2',3' cAMP isomers in plants}},
  doi          = {10.1126/sciadv.aea7828},
  volume       = {12},
  year         = {2026},
}

@article{21915,
  abstract     = {Hydrological models commonly use very simple snow accumulation and melt models based on air temperature information, namely, a temperature threshold for snow accumulation as well as for snowmelt, and a melt factor. This utility emerges due to the simplicity, efficiency, and generally good performance of such models if sufficient calibration information is available. At scales beyond single gauged catchments, the estimation and evaluation of the temperature thresholds and the melt factor has been difficult due to a lack of observations on snow accumulation and melt. Using a recently published Northern Hemisphere snow water equivalent dataset (NH-SWE) and co-located climate station observations of temperature and precipitation (4736 stations across the Northern Hemisphere), this work estimates melt factors and temperature thresholds for snow modelling based on station observations and provides the first large-scale and long-term (1950–2023) evaluation of a simple temperature-index snow model and its parameters across a diverse range of snow climates. Our study reveals that the 0 °C as precipitation-phase threshold captures most snowfall days (89 %) and the 0 °C as snowmelt initiation threshold captures most snowmelt days (76 %). Adjusting large-scale uniform threshold values does not consistently improve performance across all snow accumulation and melt metrics. Estimated melt factors based on observations converge towards 3–5 mm (°C d)−1 for deeper snowpack climates (peak snow water equivalent >300 mm), but their estimation may be more challenging for colder climates with shallower snowpacks (<300 mm), conditions where the derived melt factors cover a wider range (1 to 12 mm (°C d)−1) and a much higher interannual and spatial variability. The temperature-index snow model performs consistently well, on average, across the available Northern Hemisphere data set for estimating long-term mean values of seasonal snow cover onset, snowmelt season onset, mean snow accumulation and snowmelt rates, but challenges may arise due to biases in temperature records or solid precipitation undercatch. Peak snow water equivalent is likely underestimated for deep or alpine snowpacks, while it is likely overestimated for shallow snowpacks in the coldest and continental climates. The best median performance of the temperature-index approach lies on relatively shallow snowpacks in temperate climates. This study provides valuable insights into temperature-threshold snowfall modelling and temperature-index melt modelling for applications across diverse climates and environments, and the results should help refine regional modelling approaches to enhance our understanding of snowpack responses to global warming.},
  author       = {Fontrodona-Bach, Adrià and Schaefli, Bettina and Woods, Ross and Larsen, Joshua R.},
  issn         = {1607-7938},
  journal      = {Hydrology and Earth System Sciences},
  number       = {9},
  pages        = {2613--2636},
  publisher    = {Copernicus Publications},
  title        = {{Estimating robust melt factors and temperature thresholds for snow modelling across the Northern Hemisphere}},
  doi          = {10.5194/hess-30-2613-2026},
  volume       = {30},
  year         = {2026},
}

@article{21917,
  abstract     = {A defining feature of quantum many-body systems is the exponential scaling of the Hilbert space with the number of degrees of freedom. This exponential complexity naïvely renders a complete state characterization, for instance via the complete set of bipartite Renyi entropies for all disjoint regions, a challenging task. Recently, a compact way of storing subregions' purities by encoding them as amplitudes of a fictitious quantum wave function, known as entanglement feature, was proposed. Notably, the entanglement feature can be a simple object even for highly entangled quantum states. However the complexity and practical usage of the entanglement feature for general quantum states has not been explored. In this work, we demonstrate that the entanglement feature can be efficiently learned using only a polynomial amount of samples in the number of degrees of freedom through the so-called tensor cross interpolation (TCI) algorithm, assuming it is expressible as a finite bond dimension MPS. We benchmark this learning process on Haar and random MPS states, confirming analytic expectations. Applying the TCI algorithm to quantum eigenstates of various one dimensional quantum systems, we identify cases where eigenstates have entanglement feature learnable with TCI. We conclude with possible applications of the learned entanglement feature, such as quantifying the distance between different entanglement patterns and finding the optimal one-dimensional ordering of physical indices in a given state, highlighting the potential utility of the proposed purity interpolation method.},
  author       = {Kolisnyk, Dmytro and Medina Ramos, Raimel A and Vasseur, Romain and Serbyn, Maksym},
  issn         = {2521-327X},
  journal      = {Quantum},
  publisher    = {Verein zur Förderung des Open Access Publizierens in den Quantenwissenschaften},
  title        = {{Tensor cross interpolation of purities in quantum many-body systems}},
  doi          = {10.22331/q-2026-05-22-2114},
  volume       = {10},
  year         = {2026},
}

@phdthesis{21918,
  author       = {Khudiakova, Kseniia},
  issn         = {2663-337X},
  pages        = {89},
  publisher    = {Institute of Science and Technology Austria},
  title        = {{How epistasis and purifying selection shape genetic diversity}},
  doi          = {10.15479/AT-ISTA-21918},
  year         = {2026},
}

@inproceedings{21921,
  abstract     = {A variety of problems in geometry processing boil down to finding the most
parallel field relative to a connection. Instances of this prototypical problem
show up in computing direction fields and stripe patterns, quadrilateral
meshing, and visualization of fluid flows. When the class of allowed fields
includes those with topological defects, a relaxation is required to make
the problem well-posed. We observe that these problems can be viewed
as synchronization problems, which admit a natural semidefinite relaxation.
We propose a unified method of solving all these problems via the efficient
Burer-Monteiro factorization method. Geometrically, this amounts to lifting the field values to a higher-dimensional manifold, naturally resolving
the singular nature of defects. Practically, we show that our convex relaxation method achieves better and more reliable optima than previous work
employing alternative relaxations},
  author       = {Pacheco-Tallaj, Natalia and Couplet, Matteo and Chien, Edward and Palmer, David},
  booktitle    = {SIGGRAPH Conference Papers},
  location     = {Los Angeles, CA, United States},
  publisher    = {ACM},
  title        = {{Synchronizing fields with singularities}},
  doi          = {10.1145/3799902.3811225},
  year         = {2026},
}

@article{21928,
  abstract     = {Antibiotic combination in time and space is a key strategy to combat antimicrobial resistance. The success of such treatment designs requires their robust efficacy across treatment conditions and a pathogen’s genomic diversity. This study found that an initial treatment with a β-lactam antibiotic causes robust cellular sensitization towards an aminoglycoside antibiotic across the high-risk human pathogen Pseudomonas aeruginosa, including resistant strains. This phenomenon of cellular sensitization, termed negative hysteresis, is modulated by the Cpx envelope stress response system and linked to membrane stress during growth. The increase in efficacy is achieved through a β-lactam induced elevated cellular uptake of the subsequently administered aminoglycoside. Negative hysteresis and the Cpx system are linked in several cases to the expression of synergistic drug interactions, thus enhancing efficacy of antibiotic combinations. Overall, our study identifies the phenomenon of negative hysteresis as a robustly inducible phenotype and thus a unique focus for optimizing antimicrobial therapy.},
  author       = {Buchholz, Florian and Upterworth, Lina M. and Tueffers, Leif and Groth, Espen E. and Haas, Kira and Schütz, Daniel and Savietto Scholz, Abigail and Batra, Aditi and Pal, Surajit and Banerjee, Samarpita and Dubey, Badri N. and Franzenburg, Sören and Kalsdorf, Barbara and Rabe, Klaus F. and Nurjadi, Dennis and Rupp, Jan and Andersson, Dan I. and Sondermann, Holger and Bramkamp, Marc and Römhild, Roderich and Schulenburg, Hinrich},
  issn         = {2041-1723},
  journal      = {Nature Communications},
  publisher    = {Springer Nature},
  title        = {{Robust antibiotic sensitization of pathogenic Pseudomonas aeruginosa via negative hysteresis in the cell envelope}},
  doi          = {10.1038/s41467-026-71178-5},
  volume       = {17},
  year         = {2026},
}

@article{21929,
  abstract     = {The import of proteins into mitochondria poses fundamental mechanistic challenges: aggregation-prone precursor proteins must be maintained in aqueous compartments and threaded through narrow pores without becoming stuck or mislocalized. Recent evidence from mitochondrial protein import studies and other chaperone systems underscores the critical role of dynamics in balancing sufficiently tight binding, promiscuity, specificity, and release. Dynamic binding of client precursor proteins to import machinery components arises naturally from the avidity of their interactions. Conformational entropy enhances their stability, while the multivalent nature of these interactions ensures that client transfer to downstream insertases occurs without a substantial energy barrier. Here, we discuss this emerging paradigm of dynamic protein handling, using examples where dynamic structures have been resolved and highlight outstanding questions.},
  author       = {Schneider, Jakob and Guillerm, Undina and Simoes Pereira, Caroline and Schanda, Paul},
  issn         = {1469-896X},
  journal      = {Protein Science},
  number       = {6},
  publisher    = {Wiley},
  title        = {{Dynamic disorder is crucial for mitochondrial protein import}},
  doi          = {10.1002/pro.70630},
  volume       = {35},
  year         = {2026},
}

@article{21930,
  abstract     = {We present the discovery of extreme nitrogen enrichment by Wolf Rayet nitrogen (WN) stars in the metal-poor (∼10%Z⊙), lensed, compact (Reff ∼ 20 pc) galaxy RXCJ2248 at z = 6.1, revealed by unprecedentedly deep
JWST/NIRSpec medium-resolution spectroscopy from the GLIMPSE-D Survey. The exquisite signal-to-noise
ratio reveals multiple high-ionization nebular lines and broad Balmer and [O III] components (FWHM
∼700–3000 km s
−1
). We detect broadened He II λ1640 and λ4687 (FWHM ∼ 530 km s
−1
) and strong N III λ4642
emission consistent with a population of WN stars, making RXCJ2248 the most distant galaxy with confirmed
Wolf Rayet (WR) features to date. We measure the multiphase nebular density across five ions, the direct-method
metallicity (
12 + log(O/H) = 7.753 ± 0.025
), and a nonuniform elemental enrichment pattern of extreme N/O
enhancement (
log(N/O) = 0.391 ± 0.037
from N+, N+2
, and N+3
) but suppressed C/O relative to empirical
C/N trends. We show that this abundance pattern can be explained by enrichment from a dual-burst with a low
WR carbon/WN ratio, as expected at low metallicities. Crucially, these signatures can only arise during a brief,
rare evolutionary window shortly after a burst (∼3–6 Myr), when WN stars dominate chemical feedback but
before dilution by later yields (e.g., supernovae). The observed frequency of strong N emitters at high−z implies a
∼50 Myr burst duty cycle, suggesting that N/O outliers may represent a brief but ubiquitous phase in the
evolution of highly star-forming early galaxies. The WN detection in RXCJ2248, therefore, provides the first
direct evidence of WR-driven nitrogen enrichment in the first billion years of the Universe and a novel timing
argument for the bursty star formation cycles that shaped galaxies at cosmic dawn.},
  author       = {Berg, Danielle A. and Naidu, Rohan P. and Chisholm, John and Atek, Hakim and Fujimoto, Seiji and Kokorev, Vasily and Furtak, Lukas J. and Kobayashi, Chiaki and Schaerer, Daniel and Adamo, Angela and Fei, Qinyue and Korber, Damien and Matthee, Jorryt J and Marques-Chaves, Rui and Martinez, Zorayda and Mcquinn, Kristen B.W. and Muñoz, Julian B. and Oesch, Pascal A. and Saldana-Lopez, Alberto and Stark, Daniel P. and Stephenson, Mabel G. and Hsiao, Tiger Yu Yang},
  issn         = {1538-4357},
  journal      = {The Astrophysical Journal},
  number       = {2},
  publisher    = {IOP Publishing},
  title        = {{A fleeting GLIMPSE of N/O enrichment at cosmic dawn: Evidence for Wolf Rayet N stars in a z = 6.1 galaxy}},
  doi          = {10.3847/1538-4357/ae5e4c},
  volume       = {1003},
  year         = {2026},
}

@inproceedings{21932,
  abstract     = {We present LLMQ, an end-to-end CUDA/C++ implementation for medium-sized language-model training, e.g. 3B to 32B parameters, on affordable, commodity GPUs. These devices are characterized by low memory availability and slow communication compared to datacentre-grade GPUs. Consequently, we showcase a range of optimizations that target these bottlenecks, including activation checkpointing, offloading, and copy-engine based collectives. LLMQ is able to train or fine-tune a 7B model on a single 16GB mid-range gaming card, or a 32B model on a workstation equipped with 4 RTX 4090s. This is achieved while executing a standard 8-bit training pipeline, without additional algorithmic approximations, and maintaining FLOP utilization of around 50%. The efficiency of LLMQ rivals that of production-scale systems on much more expensive cloud-grade GPUs.},
  author       = {Schultheis, Erik and Alistarh, Dan-Adrian},
  booktitle    = {2nd Conference on Parsimony and Learning},
  issn         = {2640-3498},
  location     = {Stanford, CA, United States},
  pages        = {265--284},
  publisher    = {ML Research Press},
  title        = {{LLMQ: Efficient lower-precision LLM training for consumer GPUs}},
  volume       = {328},
  year         = {2026},
}

@article{21933,
  abstract     = {We consider the liquid drop model with a positive background density in the thermodynamic limit. We prove a two-term asymptotics for the ground state energy per unit volume in the dilute limit. Our proof justifies the expectation that optimal configurations consist of droplets of unit size that arrange themselves according to minimizers for the Jellium problem for point particles. In particular, we provide the first rigorous derivation of what is known as the gnocchi phase in astrophysics.},
  author       = {Frank, Rupert L. and Lewin, Mathieu and Seiringer, Robert},
  issn         = {1097-0312},
  journal      = {Communications on Pure and Applied Mathematics},
  publisher    = {Wiley},
  title        = {{Liquid drop model for nuclear matter in the low density limit}},
  doi          = {10.1002/cpa.70039},
  year         = {2026},
}

@article{21934,
  abstract     = {An accurate characterisation of the physical properties of galaxies at cosmic dawn is key to understanding
the origin of the high abundance of UV-bright galaxies at z≳10. We exploit deep (9.1-hour exposure time)
NIRSpec PRISM observations of GHZ2 to constrain the sources of ionising radiation and the properties of the
interstellar medium (ISM) in this bright, compact, and highly ionising galaxy at z=12.3. We measure with
high significance the prominent N IV, C IV, He II, O III, C III, O II, and Ne III emission features previously
detected in shallower observations, and confirm the detection of the N III] λ1750 multiplet, yielding tight
constraints on the N/O ratio, which is found to be ≃2 times the solar value. We also detect the Mg II λ2800,
[Fe IV] λ2833 and Si II λ1812 doublets, the H8+HeI λλ3889 blend, and the Si IV+O IV] λλ1400 absorption
complex. The O III λ3133 fluorescence line is only detected in the first observing epoch, implying variability
on a rest-frame time span of 19 days, strongly suggesting the presence of an active nucleus. Combining the
NIRSpec dataset with available optical and far-infrared constraints from MIRI and ALMA, we show that the
emission spectrum of GHZ2 cannot be reproduced by single-density spectro-photometric models, even under
extreme assumptions on the ionisation parameter and electron density. Multi-zone photoionisation modelling
performed with the HOMERUN code demonstrates that star formation must be occurring in a strongly stratified
ISM, where both low-/intermediate-density gas and high-density regions (log(ne/cm−3
) ≳ 4) coexist. The
GHZ2 emission landscape is consistent with either a composite star-formation plus AGN scenario, or with
star formation occurring in a combination of radiation- and matter-bounded regions. Purely radiation-bounded
stellar models fail to reproduce the observed He II emission, making an additional hard ionising component
unavoidable.},
  author       = {Castellano, M. and Napolitano, L. and Moreschini, B. and Calabrò, A. and Christensen, L. and Llerena, M. and Bakx, T. J.L.C. and Belfiore, F. and Bevacqua, D. and Dickinson, M. and Fontana, A. and Gandolfi, G. and Gasparetto, T. and Marconi, A. and Mascia, Sara and Merlin, E. and Morishita, T. and Nanayakkara, T. and Paris, D. and Pentericci, L. and Pérez-Díaz, B. and Roberts-Borsani, G. and Rojas-Ruiz, S. and Santini, P. and Treu, T. and Vanzella, E. and Vulcani, B. and Wang, X. and Yoon, I. and Zavala, J.},
  issn         = {2565-6120},
  journal      = {The Open Journal of Astrophysics},
  publisher    = {Maynooth Academic Publishing},
  title        = {{Investigating ionising sources and the complex interstellar medium of GHZ2 at z=12.3}},
  doi          = {10.33232/001c.160281},
  volume       = {9},
  year         = {2026},
}

@article{21948,
  abstract     = {The cerebral cortex comprises diverse neuron and glial cell types generated by radial glial progenitors (RGPs) during development. Although RGPs broadly differentiate according to temporally and spatially regulated molecular logics, the lineage hierarchies linking individual progenitors to defined cell (sub)types are not well understood. Clone-resolved transcriptomics, combining molecular barcoding and single-cell RNA sequencing, allow high-resolution lineage tracing at the single-clone/cell level across different species and models. In this mini-review, we synthesize recent advances in this field, uncovering unexpected lineage relationships in the developing brain, with a particular focus on the cerebral cortex. We further highlight new insights into species-specific differences in the developmental programs generating cell-type diversity, linking changes in clonal architecture to lineage diversification during cortical evolution.},
  author       = {Varela Martínez, Irene and Pipicelli, Fabrizia and Hippenmeyer, Simon},
  issn         = {1879-0380},
  journal      = {Current Opinion in Genetics and Development},
  publisher    = {Elsevier},
  title        = {{Tracing cell lineages in the developing brain: Insights from mosaic analysis and clone-resolved transcriptomics}},
  doi          = {10.1016/j.gde.2026.102487},
  volume       = {99},
  year         = {2026},
}

@inproceedings{21949,
  abstract     = {Cardiac T1 mapping provides critical quantitative insights into myocardial tissue composition, enabling the assessment of pathologies such as fibrosis, inflammation, and edema.
However, the inherently dynamic nature of the heart imposes strict limits on acquisition
times, making high-resolution T1 mapping a persistent challenge. Compressed sensing (CS)
approaches have reduced scan durations by undersampling k-space and reconstructing images from partial data, and recent studies show that jointly optimizing the undersampling
patterns with the reconstruction network can substantially improve performance. Still,
most current T1 mapping pipelines rely on static, hand-crafted masks that do not exploit
the full acceleration and accuracy potential. Furthermore, most existing methods do not
levarage the physical T1 decay model in optimization. In this work, we introduce T1-
PILOT: an end-to-end method that explicitly incorporates the T1 signal relaxation model
into the sampling–reconstruction framework to guide the learning of non-Cartesian trajectories, cross-frame alignment, and T1 decay estimation. Through extensive experiments
on the CMRxRecon dataset, T1-PILOT significantly outperforms several baseline strategies (including learned single-mask and fixed radial or golden-angle sampling schemes),
achieving higher T1 map fidelity at greater acceleration factors. In particular, we observe consistent gains in PSNR and VIF relative to existing methods, along with marked
improvements in delineating finer myocardial structures. Our results highlight that optimizing sampling trajectories in tandem with the physical relaxation model leads to both
enhanced quantitative accuracy and reduced acquisition times. Code for reproducing all
experiments and results is available at https://github.com/tamirshor7/T1-PILOT},
  author       = {Shor, Tamir and Freiman, Moti and Baskin, Chaim and Bronstein, Alexander},
  booktitle    = {Medical Imaging with Deep Learning},
  issn         = {2640-3498},
  keywords     = {Cardiac T1 Mapping, Trajectory Optimization and Reconstruction, PhysicsInformed Deep-Learning},
  location     = {Taipei, Taiwan},
  pages        = {1969--1982},
  publisher    = {ML Research Press},
  title        = {{T1-PILOT: Physics-informed learned optimized trajectories for T1 mapping acceleration}},
  volume       = {315},
  year         = {2026},
}

@article{21951,
  abstract     = {The central engines of Little Red Dots (LRDs) may be “black hole stars” (BH*s), early stages of
black hole growth characterized by dense gas envelopes. So far, the most direct evidence for BH*s
comes from a handful of sources where the host galaxy is completely outshone as suggested by their
remarkably steep Balmer breaks. Here we present a novel scheme to disentangle BH*s from their
host galaxies assuming that the [O III]5008˚A line arises exclusively from the host. Using a sample
of 98 LRDs (z ≈ 2 − 9) with high quality NIRSpec/PRISM spectra, we demonstrate that the hostsubtracted median stack displays a Balmer break > 2× stronger than massive quiescent galaxies,
with the rest-optical continuum resembling a blackbody-like SED (Teff ≈ 4050 K, log(Lbol) ≈ 43.9
erg s−1
, Reff ≈ 1300 au). We measure a steep Balmer decrement (Hα/Hβ > 10) and numerous
density-sensitive features (e.g., Fe II, He I, O I). These are hallmark signatures of dense gas envelopes,
providing population-level evidence that BH*s indeed power LRDs. In the median LRD, BH*s account
for ∼ 20% of the UV emission, ∼ 50% at the Balmer break, and ∼ 90% at wavelengths longer
than Hα with the remainder arising from the host. BH*s preferentially reside in low-mass galaxies
(M⋆ ≈ 108 M⊙) undergoing recent starbursts, as evidenced by extreme emission line EWs (e.g.,
[O III]5008˚A≈ 1100˚A, C III]≈ 12˚A), thereby favoring BH* origins linked to star-formation. We show
V-shaped LRD selections are biased to high BH*/host fractions (≳ 60% at 5500˚A) – less dominant
BH*s may be powering JWST’s blue broad-line AGN. We find BH*s are so commonplace and transient
(duty cycle ∼ 1%, lifetime ∼ 10 Myrs) that every massive black hole may have once shone as a BH*.
},
  author       = {Sun, Wendy Q. and Naidu, Rohan P. and Matthee, Jorryt J and De Graaff, Anna and Chisholm, John and Greene, Jenny E. and Oesch, Pascal A. and Torralba Torregrosa, Alberto and Hviding, Raphael E. and Brammer, Gabriel and Simcoe, Robert A. and Bose, Sownak and Bouwens, Rychard and Dayal, Pratika and Eilers, Anna Christina and Fei, Qinyue and Furtak, Lukas J. and Gottumukkala, Rashmi and Goulding, Andy and Heintz, Kasper E. and Hirschmann, Michaela and Kokorev, Vasily and Leja, Joel and Liu, Zhaoran and Natarajan, Priyamvada and Santarelli, Andrew D. and Setton, David J. and Smith, Aaron and Tacchella, Sandro and Volonteri, Marta and Walter, Fabian and Weibel, Andrea and Williams, Christina C.},
  issn         = {2565-6120},
  journal      = {The Open Journal of Astrophysics},
  publisher    = {Maynooth Academic Publishing},
  title        = {{Little Red Dot - Host Galaxy = Black Hole Star: A gas-enshrouded heart at the center of every Little Red Dot}},
  doi          = {10.33232/001c.162505},
  volume       = {9},
  year         = {2026},
}

@article{21953,
  abstract     = {Several Streptomyces strains were isolated from freshwater sediments collected in the Laxenburg ponds (Lower Austria). Genome sequencing and bioinformatics analyses revealed biosynthetic gene clusters (BGCs) that may specify production of chemically diverse secondary metabolites. Various culture conditions were employed to induce metabolite production, and subsequent LC-MS analyses facilitated the identification of the produced compounds and their correlation with the corresponding BGCs. These analyses of sediment-derived Streptomyces spp. highlight their extensive biosynthetic potential, revealing a diverse range of bioactive secondary metabolites, including siderophores, antibiotics, and other compounds with potential therapeutic applications. Genomes of two Streptomyces isolates, one of them representing a potentially new species, harbored several uncharacterized BGCs that may specify biosynthesis of novel secondary metabolites. Although targeted overexpression of pathway-specific regulators from these BGCs did not yield additional metabolites, whereas knockout experiments led to metabolic changes, presumably reflecting regulatory or compensatory interactions between multiple biosynthetic pathways. Continued exploration of these strains and their BGCs may lead to the discovery of new bioactive molecules with pharmaceutical and biotechnological applications.},
  author       = {Tocino-Márquez, Inmaculada and Zehl, Martin and Batajic, Jovana and Séneca, Joana and Pjevac, Petra and Murillo-Alba, José and Martín, Jesús and Sekurova, Olga N. and Zotchev, Sergey B.},
  issn         = {1664-302X},
  journal      = {Frontiers in Microbiology},
  publisher    = {Frontiers Media},
  title        = {{Unveiling the genomes and secondary metabolomes of Streptomyces spp. from freshwater sediments}},
  doi          = {10.3389/fmicb.2026.1793713},
  volume       = {17},
  year         = {2026},
}

@article{21954,
  abstract     = {We investigate a framework for train-free MRI segmentation based on Topological Data Analysis. The pipeline proceeds in three steps, first identifying the whole object to segment via automatic thresholding, then detecting a distinctive subset whose topology is known in advance, and finally deducing the various components of the segmentation. A key ingredient is the extraction of approximate representative cycles from persistence diagrams, which provides an interpretable link between persistent features and anatomical components. To clarify the method’s scope, we make the underlying topological and intensity assumptions explicit, quantify when they hold on real data, and analyze typical failure modes. We evaluate the approach on glioblastoma and on fetal cortical plate segmentation, with comparisons to unsupervised and deep-learning references. By operating without large annotated datasets, the method is well suited to scarce-data settings and provides an interpretable baseline and practical initialization for expert refinement or learning-based pipelines.},
  author       = {François, Anton and Tinarrage, Raphaël},
  issn         = {1573-7683},
  journal      = {Journal of Mathematical Imaging and Vision},
  number       = {3},
  publisher    = {Springer Nature},
  title        = {{Train-free segmentation in MRI with cubical persistent homology}},
  doi          = {10.1007/s10851-026-01300-1},
  volume       = {68},
  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    = {Elsevier},
  title        = {{A hypothalamic circuit for anticipating future changes in energy balance}},
  doi          = {10.1016/j.neuron.2026.05.010},
  year         = {2026},
}

@misc{21960,
  abstract     = {Solitons - localized wave packets that travel without spreading - play a central role in understanding transport and properties of nonlinear systems. In quantum many-body systems, however, such robust excitations are typically destroyed by thermalization. Here, we theoretically demonstrate the existence of solitonic excitations in high-energy states of Rydberg atom chains in the regime of strong nearest-neighbor Rydberg blockade. 
These localized wave packets propagate directionally atop a special class of reviving initial states related to quantum many-body scars and are capable of carrying energy. Exhibiting long coherence times, these states constitute a form of non-ergodic quantum dynamics and can be efficiently implemented on Rydberg atom simulators. In this work, in addition to a phenomenological description of solitons, we identify their counterpart in a classical nonlinear dynamical system, demonstrate their potential use in quantum information transfer, and conjecture their relevance for anomalous energy transport reported in numerical studies of Rydberg atom arrays.},
  author       = {Kerschbaumer, Aron},
  publisher    = {Institute of Science and Technology Austria},
  title        = {{Research Data: "Quasi-solitons in Rydberg atom chains"}},
  doi          = {10.15479/AT-ISTA-21960},
  year         = {2026},
}

@unpublished{21962,
  abstract     = {The generation of faithful cell-type diversity and correct projection neuron numbers is essential for cerebral cortex development. Corticogenesis is however susceptible to genetic interference of critical signaling pathways, including mutations in Mtor/Rptor that lead to microcephaly. How the loss of Rptor/mTORC1 function affects cortical developmental programs, at single cell level, is still unknown. Here, we utilized Mosaic Analysis with Double Markers (MADM) technology to probe Rptor gene function upon sparse single cell- or global tissue-wide ablation. We found that tissue-wide effects drive the etiology of cortical microcephaly upon loss of Rptor, rather than deficits in projection neuron genesis. Conversely, Rptor function is cell-autonomously required for postnatal projection neuron survival in a highly cell-type-specific manner. Collectively, our results suggest that the fine balance of precise cell-type-specific cell-autonomous Rptor/mTORC1 function in concert with non-cell-autonomous tissue-wide effects is essential for the development of a properly-sized cerebral cortex with accurate projection neuron diversity.},
  author       = {Villalba Requena, Ana and Beattie, Robert J and Pauler, Florian and Streicher, Carmen and Miranda, Osvaldo and Krausgruber, Thomas and Senekowitsch, Martin and Farlik, Matthias and Bock, Christoph and Rülicke, Thomas and Hippenmeyer, Simon},
  booktitle    = {bioRxiv},
  title        = {{Mtor/Rptor function globally prevents cortical microcephaly and cell-autonomously promotes postnatal neuron survival in cell type specific manner}},
  doi          = {10.64898/2026.05.01.722172},
  year         = {2026},
}

