@article{19500,
  abstract     = {We consider the Brown measure of the free circular Brownian motion,  a+t√x , with an arbitrary initial condition  a , i.e.  a  is a general non-normal operator and  x  is a circular element  ∗ -free from  a . We prove that, under a mild assumption on  a , the density of the Brown measure has one of the following two types of behavior around each point on the boundary of its support -- either (i) sharp cut, i.e. a jump discontinuity along the boundary, or (ii) quadratic decay at certain critical points on the boundary. Our result is in direct analogy with the previously known phenomenon for the spectral density of free semicircular Brownian motion, whose singularities are either a square-root edge or a cubic cusp. We also provide several examples and counterexamples, one of which shows that our assumption on  a  is necessary.},
  author       = {Erdös, László and Ji, Hong Chang},
  issn         = {1431-0643},
  journal      = {Documenta Mathematica},
  number       = {2},
  pages        = {417--453},
  publisher    = {EMS Press},
  title        = {{Density of Brown measure of free circular Brownian motion}},
  doi          = {10.4171/DM/999},
  volume       = {30},
  year         = {2025},
}

@article{19502,
  abstract     = {Alkali dimers, Ak2, located on the surface of a helium nanodroplet, are set into rotation through the polarizability interaction with a nonresonant 1-ps-long laser pulse. The time-dependent degree of alignment is recorded using femtosecond-probe-pulse-induced Coulomb explosion into a pair of Ak+ fragment ions. The results, obtained for Na2, K2, and Rb2 in both the ground state 11Σ+g and the lowest-lying triplet state 13Σ+u, exhibit distinct, periodic revivals with a gradually decreasing amplitude. The dynamics differ from that expected for dimers had they behaved as free rotors. Numerically, we solve the time-dependent rotational Schrödinger equation, including an effective mean-field potential to describe the interaction between the dimer and the droplet. The experimental and simulated alignment dynamics agree well and their comparison enables us to determine the effective rotational constants of the alkali dimers with the exception of Rb2(13Σ+u) that only exhibits a prompt alignment peak but no subsequent revivals. For Na2(13Σ+u), K2(11Σ+g), K2(13Σ+u) and Rb2(11Σ+g), the alignment dynamics are well-described by a 2D rotor model. We ascribe this to a significant confinement of the internuclear axis of these dimers, induced by the orientation-dependent droplet-dimer interaction, to the tangential plane of their residence point on the droplet.},
  author       = {Kristensen, Henrik H. and Kranabetter, Lorenz and Ghazaryan, Areg and Schouder, Constant A. and Hansen, Emil and Jensen, Frank and Zillich, Robert E. and Lemeshko, Mikhail and Stapelfeldt, Henrik},
  issn         = {2469-9934},
  journal      = {Physical Review A},
  number       = {3},
  publisher    = {American Physical Society},
  title        = {{Nonadiabatic laser-induced alignment dynamics of alkali-metal dimers on the surface of a helium droplet}},
  doi          = {10.1103/PhysRevA.111.033114},
  volume       = {111},
  year         = {2025},
}

@article{19503,
  abstract     = {A tantalizing open problem, posed independently by Stiebitz in 1995 and by Alon in 1996 and again in 2006, asks whether for every pair of integers  s,t≥1 there exists a finite number  F(s,t)
such that the vertex set of every digraph of minimum out-degree at least  F(s,t) can be partitioned into non-empty parts  A  and  B  such that the subdigraphs induced on  A
  and  B  have minimum out-degree at least  s  and  t , respectively.
In this short note, we prove that if  F(2,2)  exists, then all the numbers  F(s,t)  with  s,t≥1
  exist and satisfy  F(s,t)=Θ(s+t) . In consequence, the problem of Alon and Stiebitz reduces to the case  s=t=2 . Moreover, the numbers  F(s,t)  with  s,t≥2  either all exist and grow linearly, or all of them do not exist.},
  author       = {Christoph, Micha and Petrova, Kalina H and Steiner, Raphael},
  issn         = {1469-2163},
  journal      = {Combinatorics Probability and Computing},
  number       = {4},
  pages        = {559--564},
  publisher    = {Cambridge University Press},
  title        = {{A note on digraph splitting}},
  doi          = {10.1017/S0963548325000045},
  volume       = {34},
  year         = {2025},
}

@article{19504,
  abstract     = {Observational studies have shown that galaxy disks were already in place in the first few billion years of the Universe. The early disks detected so far, with typical half-light radii of 3 kpc at stellar masses around 1011 M⊙ for redshift z ≈ 3, are significantly smaller than today’s disks with similar masses, which is in agreement with expectations from current galaxy models. Here we report observations of a giant disk at z = 3.25, when the Universe was only two billion years old, with a half-light radius of 9.6 kpc and stellar mass of (math formular). This galaxy is larger than any other kinematically confirmed disks at similar epochs and is surprisingly similar to today’s largest disks with regard to size and mass. James Webb Space Telescope imaging and spectroscopy reveal its spiral morphology and a rotational velocity consistent with a local Tully–Fisher relationship. Multiwavelength observations show that it lies in an exceptionally dense environment, where the galaxy number density is more than ten times higher than the cosmic average and mergers are frequent. The discovery of such a giant disk suggests the presence of favourable physical conditions for large-disk formation in dense environments in the early Universe, which may include efficient accretion of gas carrying coherent angular momentum and non-destructive mergers between exceptionally gas-rich progenitor galaxies.},
  author       = {Wang, Weichen and Cantalupo, Sebastiano and Pensabene, Antonio and Galbiati, Marta and Travascio, Andrea and Steidel, Charles C. and Maseda, Michael V. and Pezzulli, Gabriele and De Beer, Stephanie and Fossati, Matteo and Fumagalli, Michele and Gallego, Sofia G. and Lazeyras, Titouan and Mackenzie, Ruari and Matthee, Jorryt J and Nanayakkara, Themiya and Quadri, Giada},
  issn         = {2397-3366},
  journal      = {Nature Astronomy},
  pages        = {710--719},
  publisher    = {Springer Nature},
  title        = {{A giant disk galaxy two billion years after the Big Bang}},
  doi          = {10.1038/s41550-025-02500-2},
  volume       = {9},
  year         = {2025},
}

@article{19505,
  abstract     = {In this paper, we introduce and study the primitive equations with non-isothermal turbulent pressure and transport noise. They are derived from the Navier–Stokes equations by employing stochastic versions of the Boussinesq and the hydrostatic approximations. The temperature dependence of the turbulent pressure can be seen as a consequence of an additive noise acting on the small vertical dynamics. For such a model we prove global well-posedness in H^1 where the noise is considered in both the Itô and Stratonovich formulations. Compared to previous variants of the primitive equations, the one considered here presents a more intricate coupling between the velocity field and the temperature. The corresponding analysis is seriously more involved than in the deterministic setting. Finally, the continuous dependence on the initial data and the energy estimates proven here are new, even in the case of isothermal turbulent pressure.},
  author       = {Agresti, Antonio and Hieber, Matthias and Hussein, Amru and Saal, Martin},
  issn         = {1050-5164},
  journal      = {Annals of Applied Probability},
  number       = {1},
  pages        = {635--700},
  publisher    = {Institute of Mathematical Statistics},
  title        = {{The stochastic primitive equations with nonisothermal turbulent pressure}},
  doi          = {10.1214/24-AAP2124},
  volume       = {35},
  year         = {2025},
}

@article{19506,
  abstract     = {Hippocampal reactivation of waking neuronal assemblies in sleep is a key initial step of systems consolidation. Nevertheless, it is unclear whether reactivated assemblies are static or whether they reorganize gradually over prolonged sleep. We tracked reactivated CA1 assembly patterns over ∼20 h of sleep/rest periods and related them to assemblies seen before or after in a spatial learning paradigm using rats. We found that reactivated assembly patterns were gradually transformed and started to resemble those seen in the subsequent recall session. Periods of rapid eye movement (REM) sleep and non-REM (NREM) had antagonistic roles: whereas NREM accelerated the assembly drift, REM countered it. Moreover, only a subset of rate-changing pyramidal cells contributed to the drift, whereas stable-firing-rate cells maintained unaltered reactivation patterns. Our data suggest that prolonged sleep promotes the spontaneous reorganization of spatial assemblies, which can contribute to daily cognitive map changes or encoding new learning situations.},
  author       = {Bollmann, Lars and Baracskay, Peter and Stella, Federico and Csicsvari, Jozsef L},
  issn         = {1097-4199},
  journal      = {Neuron},
  number       = {9},
  pages        = {1446--1459.e6},
  publisher    = {Elsevier},
  title        = {{Sleep stages antagonistically modulate reactivation drift}},
  doi          = {10.1016/j.neuron.2025.02.025},
  volume       = {113},
  year         = {2025},
}

@article{19507,
  abstract     = {The epidermis provides a protective barrier against hostile environments. However, our knowledge of how this barrier forms during development and is subsequently maintained remains incomplete. The infundibulum is a cylindrical epidermal tissue compartment that serves as an outlet for hair follicles protruding from the skin and the excretion of the sebaceous glands that are essential for proper skin function. In this study, we applied quantitative fate mapping to address how infundibulum are maintained during adulthood. We demonstrate that progenitors build and maintain tissues through stochastic cell fate choices. Long-term analysis identified a preferential transient contribution from cells initially located at the bottom of the structure to the maintenance of the tissue, with bursts of local progenitor expansion associated with the phases of hair growth. Beyond providing compartment-wide insights into progenitor cell dynamics in infundibulum, these findings demonstrate how spatiotemporal regulation controls transient progenitor dominance.},
  author       = {Andersen, Marianne S. and Ulyanchenko, Svetlana and Schweiger, Pawel J. and Hannezo, Edouard B and Simons, Benjamin D. and Jensen, Kim B.},
  issn         = {1523-1747},
  journal      = {Journal of Investigative Dermatology},
  number       = {9},
  pages        = {2191--2202.e5},
  publisher    = {Elsevier},
  title        = {{Spatiotemporal switches in progenitor cell fate govern upper hair follicle growth and maintenance}},
  doi          = {10.1016/j.jid.2025.01.034},
  volume       = {145},
  year         = {2025},
}

@article{19529,
  abstract     = {NRF2 is a transcription factor responsible for coordinating the expression of over a thousand cytoprotective genes. Although NRF2 is constitutively expressed, its stability is modulated by the redox-sensitive protein KEAP1 and other conditional binding partner regulators. The new era of NRF2 research has highlighted the cooperation between NRF2 and PIN1 in modifying its cytoprotective effect. Despite numerous studies, the understanding of the PIN1-NRF2 interaction remains limited. Herein, we described the binding interaction of PIN1 and three different 14-mer long phospho-peptides mimicking NRF2 protein using computer-based, biophysical, and biochemical approaches. According to our computational analyses, the residues positioned in the WW domain of PIN1 (Ser16, Arg17, Ser18, Tyr23, Ser32, Gln33, and Trp34) were found to be crucial for PIN1-NRF2 interactions. Biophysical FP assays were used to verify the computational prediction. The data demonstrated that Pintide, a peptide predominantly interacting with the PIN1 WW-domain, led to a significant reduction in the binding affinity of the NRF2 mimicking peptides. Moreover, we evaluated the impact of known PIN1 inhibitors (juglone, KPT-6566, and EGCG) on the PIN1-NRF2 interaction. Among the inhibitors, KPT-6566 showed the most potent inhibitory effect on PIN1-NRF2 interaction within an IC<jats:sub>50</jats:sub> range of 0.3–1.4 µM. Furthermore, our mass spectrometry analyses showed that KPT-6566 appeared to covalently modify PIN1 via conjugate addition, rather than disulfide exchange of the sulfonyl-acetate moiety. Altogether, such inhibitors would also be highly valuable molecular probes for further investigation of PIN1 regulation of NRF2 in the cellular context and potentially pave the way for drug molecules that specifically inhibit the cytoprotective effects of NRF2 in cancer.},
  author       = {Ozleyen, Adem and Duran, Gizem Nur and Dönmez, Serhat and Ozbil, Mehmet and Doveston, Richard G. and Tumer, Tugba Boyunegmez},
  issn         = {2045-2322},
  journal      = {Scientific Reports},
  publisher    = {Springer Nature},
  title        = {{Identification and inhibition of PIN1-NRF2 protein–protein interactions through computational and biophysical approaches}},
  doi          = {10.1038/s41598-025-89342-0},
  volume       = {15},
  year         = {2025},
}

@article{19531,
  abstract     = {In standard quantum electrodynamics (QED), the so-called non-minimal (Pauli) coupling is suppressed for elementary particles and has no physical implications. Here, we show that the Pauli term naturally appears in a known family of Dirac materials—the lead-halide perovskites, suggesting a novel playground for the study of analog QED effects. We outline measurable manifestations of the Pauli term in the phenomena pertaining to (i) relativistic corrections to bound states (ii) the Klein paradox, and (iii) spin effects in scattering. In particular, we demonstrate that (a) the binding energy of an electron in the vicinity of a positively charged defect is noticeably decreased due to the polarizability of lead ions and the appearance of a Darwin-like term, (b) strong spin-orbit coupling due to the Pauli term affects the exciton states, and (c) scattering of an electron off an energy barrier with broken mirror symmetry produces spin polarization in the outgoing current. Our study adds to the understanding of quantum phenomena in lead-halide perovskites and paves the way for tabletop simulations of analog Dirac-Pauli equations.},
  author       = {Shiva Kumar, Abhishek and Maslov, Mikhail and Lemeshko, Mikhail and Volosniev, Artem and Alpichshev, Zhanybek},
  issn         = {2397-4648},
  journal      = {npj Quantum Materials},
  publisher    = {Springer Nature},
  title        = {{Massive Dirac-Pauli physics in lead-halide perovskites}},
  doi          = {10.1038/s41535-025-00754-7},
  volume       = {10},
  year         = {2025},
}

@article{19554,
  abstract     = {In 1981, Karp and Sipser proved a law of large numbers for the matching number of a sparse Erdős–Rényi random graph, in an influential paper pioneering the so-called differential equation method for analysis of random graph processes. Strengthening this classical result, and answering a question of Aronson, Frieze and Pittel, we prove a central limit theorem in the same setting: the fluctuations in the matching number of a sparse random graph are asymptotically Gaussian. Our new contribution is to prove this central limit theorem in the subcritical and critical regimes, according to a celebrated algorithmic phase transition first observed by Karp and Sipser. Indeed, in the supercritical regime, a central limit theorem has recently been proved in the PhD thesis of Kreačić, using a stochastic generalisation of the differential equation method (comparing the so-called Karp–Sipser process to a system of stochastic differential equations). Our proof builds on these methods, and introduces new techniques to handle certain degeneracies present in the subcritical and critical cases. Curiously, our new techniques lead to a non-constructive result: we are able to characterise the fluctuations of the matching number around its mean, despite these fluctuations being much smaller than the error terms in our best estimates of the mean. We also prove a central limit theorem for the rank of the adjacency matrix of a sparse random graph.},
  author       = {Glasgow, Margalit and Kwan, Matthew Alan and Sah, Ashwin and Sawhney, Mehtaab},
  issn         = {1469-7750},
  journal      = {Journal of the London Mathematical Society},
  number       = {4},
  publisher    = {Wiley},
  title        = {{A central limit theorem for the matching number of a sparse random graph}},
  doi          = {10.1112/jlms.70101},
  volume       = {111},
  year         = {2025},
}

@article{19555,
  abstract     = {The charged arginine side chain is unique in determining many innate properties of proteins, contributing to stability and interaction surfaces, and directing allosteric regulation and enzymatic catalysis. NMR experiments can be used to reveal these processes at the molecular level, but it often requires selective insertion of carbon-13, nitrogen-15, and deuterium at defined atomic positions. We introduce a method to endow arginine residues with defined isotope patterns, combining synthetic organic chemistry and cell-based protein overexpression. The resulting proteins feature NMR active spin systems with optimized relaxation pathways leading to simplified NMR spectra with a sensitive response to changes in the chemical environment of the nuclei observed.},
  author       = {Rohden, Darja and Toscano, Giorgia and Schanda, Paul and Lichtenecker, Roman J.},
  issn         = {1521-3765},
  journal      = {Chemistry - A European Journal},
  number       = {24},
  publisher    = {Wiley},
  title        = {{Synthesis of selectively 13C/2H/15N- labeled arginine to probe protein conformation and interaction by NMR spectroscopy}},
  doi          = {10.1002/chem.202500408},
  volume       = {31},
  year         = {2025},
}

@phdthesis{19557,
  author       = {Schwarz, Lena A},
  issn         = {2663-337X},
  pages        = {124},
  publisher    = {Institute of Science and Technology Austria},
  title        = {{Mapping developmental dynamics of autism spectrum disorder mouse models at single-cell resolution}},
  doi          = {10.15479/AT-ISTA-19557},
  year         = {2025},
}

@article{19565,
  abstract     = {Measuring distances in a multidimensional setting is a challenging problem, which appears in many fields of science and engineering. In this paper, to measure the distance between two multivariate distributions, we introduce a new measure of discrepancy which is scale invariant and which, in the case of two independent copies of the same distribution, and after normalization, coincides with the scaling invariant multidimensional version of the Gini index recently proposed in [P. Giudici, E. Raffinetti and G. Toscani, Measuring multidimensional inequality: A new proposal based on the Fourier transform, preprint (2024), arXiv:2401.14012 ]. A byproduct of the analysis is an easy-to-handle discrepancy metric, obtained by application of the theory to a pair of Gaussian multidimensional densities. The obtained metric does improve the standard metrics, based on the mean squared error, as it is scale invariant. The importance of this theoretical finding is illustrated by means of a real problem that concerns measuring the importance of Environmental, Social and Governance factors for the growth of small and medium enterprises. },
  author       = {Auricchio, Gennaro and Brigati, Giovanni and Giudici, Paolo and Toscani, Giuseppe},
  issn         = {1793-6314},
  journal      = {Mathematical Models and Methods in Applied Sciences},
  number       = {5},
  pages        = {1267--1296},
  publisher    = {World Scientific Publishing},
  title        = {{Multivariate Gini-type discrepancies}},
  doi          = {10.1142/s0218202525500174},
  volume       = {35},
  year         = {2025},
}

@article{19566,
  abstract     = {Purpose: Optic nerve crush (ONC) is a model for studying optic nerve trauma. Unilateral ONC induces massive retinal ganglion cell (RGC) degeneration in the affected eye, leading to vision loss within a month. A common assumption has been that the non-injured contralateral eye is unaffected due to the minimal retino-retinal projections of the RGCs at the chiasm. Yet, recently, microglia, the brain-resident macrophages, have shown a responsive phenotype in the contralateral eye after ONC. Whether RGC loss accompanies this phenotype is still controversial.

Methods: Using the available RGCode algorithm and developing our own RGC-Quant deep-learning-based tool, we quantify RGC's total number and density across the entire retina after ONC.

Results: We confirm a short-term microglia response in the contralateral eye after ONC, but this did not affect the microglia number. Furthermore, we cannot confirm the previously reported RGC loss between naïve and contralateral retinas 5 weeks after ONC induction across the commonly used Cx3cr1creERT2 and C57BL6/J mouse models. Neither sex nor the direct comparison of the RGC markers Brn3a and RBPMS, with Brn3a co-labeling, on average, 89% of the RBPMS+-cells, explained this discrepancy, suggesting that the early microglia-responsive phenotype does not have immediate consequences on the RGC number.

Conclusions: Our results corroborate that unilateral optic nerve injury elicits a microglial response in the uninjured contralateral eye but without RGC loss. Therefore, the contralateral eye should be treated separately and not as an ONC control.},
  author       = {Schoot Uiterkamp, Florianne E and Maes, Margaret E and Alamalhoda, Mohammad and Firoozi, Arsalan and Colombo, Gloria and Siegert, Sandra},
  issn         = {1552-5783},
  journal      = {Investigative Ophthalmology & Visual Science},
  number       = {3},
  publisher    = {Association for Research in Vision and Ophthalmology},
  title        = {{Optic nerve crush does not induce retinal ganglion cell loss in the contralateral eye}},
  doi          = {10.1167/iovs.66.3.49},
  volume       = {66},
  year         = {2025},
}

@article{19585,
  abstract     = {Air quality in northern South America faces significant challenges due to insufficient high-resolution emission inventories and sparse atmospheric studies. This study addresses these gaps by developing a novel framework that integrates high-resolution nighttime light data from SDGSAT-1 and multisource remote sensing datasets with deep learning techniques to downscale emission inventories. The refined inventories are coupled with meteorological inputs into the Weather Research and Forecasting (WRF-Chem) model, enabling precise simulation of pollutant dynamics. Validated against ground measurements from Colombia's SISAIRE monitoring network, demonstrates significant improvements in spatiotemporal accuracy, particularly for particulate matter (PM) and nitrogen dioxide (NO₂) with error reductions of 22–30 % and correlation coefficients increasing from 0.68 to 0.85. These findings underscore the critical role of satellite-enhanced inventories in resolving localized emission patterns and seasonal variability, such as dry-season PM₁₀ spikes (150 % increase from wildfires). The framework provides policymakers with actionable insights to prioritize mitigation in rapidly urbanizing regions and manage transboundary pollution. By bridging data scarcity gaps, this replicable methodology offers transformative potential for global air quality management and public health protection, advocating for expanded ground monitoring networks and real-time satellite data integration in future applications.},
  author       = {Antezana-Lopez, Franz and Casallas Garcia, Alejandro and Zhou, Guanhua and Zhang, Kai and Jing, Guifei and Ali, Aamir and Lopez-Barrera, Ellie and Belalcazar, Luis Carlos and Rojas, Nestor and Jiang, Hongzhi},
  issn         = {1879-0704},
  journal      = {Remote Sensing of Environment},
  publisher    = {Elsevier},
  title        = {{High-resolution anthropogenic emission inventories with deep learning in northern South America}},
  doi          = {10.1016/j.rse.2025.114761},
  volume       = {324},
  year         = {2025},
}

@article{19594,
  abstract     = {In this issue of Developmental Cell, Lee et al. identify a pivotal role for glutathione (GSH) in plant regeneration, a vital biological process enabling plants to regrow tissues and organs after injury. Applying single-cell RNA sequencing (scRNA-seq) and live imaging, the authors demonstrate that GSH, released upon tissue damage, accelerates cell-cycle transitions, particularly shortening the G1 phase, thereby facilitating efficient organ regeneration.},
  author       = {Benková, Eva},
  issn         = {1878-1551},
  journal      = {Developmental Cell},
  number       = {8},
  pages        = {1137--1139},
  publisher    = {Elsevier},
  title        = {{Unlocking plant regeneration: The role for glutathione}},
  doi          = {10.1016/j.devcel.2025.03.012},
  volume       = {60},
  year         = {2025},
}

@article{19595,
  abstract     = {We investigate the locality of magnetic response in polycyclic aromatic molecules using a novel deep-learning approach. Our method employs graph neural networks (GNNs) with a graph-of-rings representation to predict nucleus independent chemical shifts (NICS) in the space around the molecule. We train a series of models, each time reducing the size of the largest molecules used in training. The accuracy of prediction remains high (MAE < 0.5 ppm), even when training the model only on molecules with up to four rings, thus providing strong evidence for the locality of magnetic response. To overcome the known problem of generalization of GNNs, we implement a k-hop expansion strategy and succeed in achieving accurate predictions for molecules with up to 15 rings (almost 4 times the size of the largest training example). Our findings have implications for understanding the magnetic response in complex molecules and demonstrate a promising approach to overcoming GNN scalability limitations. Furthermore, the trained models enable rapid characterization, without the need for more expensive DFT calculations.},
  author       = {Davidson, Yair and Philipp, Aviad and Chakraborty, Sabyasachi and Bronstein, Alexander and Gershoni-Poranne, Renana},
  issn         = {1089-7690},
  journal      = {Journal of Chemical Physics},
  number       = {14},
  publisher    = {AIP Publishing},
  title        = {{How local is “local”? Deep learning reveals locality of the induced magnetic field of polycyclic aromatic hydrocarbons}},
  doi          = {10.1063/5.0257558},
  volume       = {162},
  year         = {2025},
}

@article{19596,
  abstract     = {We report the spectroscopic discovery of a massive quiescent galaxy at zspec = 7.29 ± 0.01, just ∼700 Myr after the big bang. RUBIES-UDS-QG-z7 was selected from public JWST/NIRCam and MIRI imaging from the PRIMER survey and observed with JWST/NIRSpec as part of RUBIES. The NIRSpec/PRISM spectrum reveals one of the strongest Balmer breaks observed thus far at z > 6, with no emission lines but tentative Balmer and Ca absorption features, as well as a Lyman break. Simultaneous modeling of the NIRSpec/PRISM spectrum and NIRCam and MIRI photometry (spanning 0.9–18 μm) shows that the galaxy formed a stellar mass of
(math. formular) before z ∼ 8 and ceased forming stars 50–100 Myr prior to the time of observation, resulting in log (sSFR/Gyr- 1) < -1 . We measure a small physical size of (math formular) , which implies a high stellarmass surface density within the effective radius of (math formular) comparable to the highest densities measured in quiescent galaxies at z ∼ 2–5. The 3D stellar-mass density profile of RUBIES-UDS-QG-z7 is remarkably similar to the central densities of local massive ellipticals, suggesting that at least some of their cores may have already been in place at z > 7. The discovery of RUBIES-UDS-QG-z7 has strong implications for galaxy formation models: the estimated number density of quiescent galaxies at z ∼ 7 is >100 × larger than predicted from any model to date, indicating that quiescent galaxies have formed earlier than previously expected. },
  author       = {Weibel, Andrea and De Graaff, Anna and Setton, David J. and Miller, Tim B. and Oesch, Pascal A. and Brammer, Gabriel and Lagos, Claudia D.P. and Whitaker, Katherine E. and Williams, Christina C. and Baggen, Josephine F.W. and Bezanson, Rachel and Boogaard, Leindert A. and Cleri, Nikko J. and Greene, Jenny E. and Hirschmann, Michaela and Hviding, Raphael E. and Kuruvanthodi, Adarsh and Labbé, Ivo and Leja, Joel and Maseda, Michael V. and Matthee, Jorryt J and Mcconachie, Ian and Naidu, Rohan P. and Roberts-Borsani, Guido and Schaerer, Daniel and Suess, Katherine A. and Valentino, Francesco and Van Dokkum, Pieter and Wang, Bingjie},
  issn         = {1538-4357},
  journal      = {The Astrophysical Journal},
  number       = {1},
  publisher    = {IOP Publishing},
  title        = {{RUBIES reveals a massive quiescent galaxy at z = 7.3}},
  doi          = {10.3847/1538-4357/adab7a},
  volume       = {983},
  year         = {2025},
}

@article{19597,
  abstract     = {Superconductor–semiconductor hybrid systems play a crucial role in realizing nanoscale quantum devices, including hybrid qubits, Majorana bound states, and Kitaev chains. For such hybrid devices, subgap states play a prominent role in their operation. In this paper, we study these subgap states via Coulomb and tunneling spectroscopy through a superconducting island defined in a semiconductor nanowire fully coated by a superconductor. We systematically explore regimes ranging from an almost decoupled island to the open configuration. In the weak-coupling regime, the experimental observations are very similar in the absence of a magnetic field and when one flux quantum pierces the superconducting shell. Conversely, in the strong-coupling regime, significant distinctions emerge between the two cases. We attribute this distinct behavior to the existence of subgap states at one flux quantum, which become observable only for sufficiently strong coupling to the leads. We support our interpretation using a simple model to describe transport through the island. Our study highlights the importance of studying a broad range of tunnel couplings for understanding the rich physics of hybrid devices.},
  author       = {Valentini, Marco and Souto, Rubén Seoane and Borovkov, Maksim and Krogstrup, Peter and Meir, Yigal and Leijnse, Martin and Danon, Jeroen and Katsaros, Georgios},
  issn         = {2643-1564},
  journal      = {Physical Review Research},
  number       = {2},
  publisher    = {American Physical Society},
  title        = {{Subgap transport in superconductor-semiconductor hybrid islands: Weak and strong coupling regimes}},
  doi          = {10.1103/PhysRevResearch.7.023022},
  volume       = {7},
  year         = {2025},
}

@article{19598,
  abstract     = {We establish universal Gaussian fluctuations for the mesoscopic linear eigenvalue statistics in the vicinity of the cusp-like singularities of the limiting spectral density for Wigner-type random matrices. Prior to this work, the linear eigenvalue statistics at the cusp-like singularities were not studied in any ensemble. Our analysis covers not only the exact cusps but the entire transitionary regime from the square-root singularity at a regular edge through the sharp cusp to the bulk. We identify a new one-parameter family of functionals that govern the limiting bias and variance, continuously interpolating between the previously known formulas in the bulk and at a regular edge. Since cusps are the only possible singularities besides the regular edges, our result gives a complete description of the linear eigenvalue statistics in all regimes.},
  author       = {Riabov, Volodymyr},
  issn         = {1432-2064},
  journal      = {Probability Theory and Related Fields},
  pages        = {1183--1237},
  publisher    = {Springer Nature},
  title        = {{Linear Eigenvalue statistics at the cusp}},
  doi          = {10.1007/s00440-025-01373-w},
  volume       = {193},
  year         = {2025},
}

