TY - JOUR AB - For some k∈Z≥0∪{∞}, we call a linear forest k-bounded if each of its components has at most k edges. We will say a (k,ℓ)-bounded linear forest decomposition of a graph G is a partition of E(G) into the edge sets of two linear forests Fk,Fℓ where Fk is k-bounded and Fℓ is ℓ-bounded. We show that the problem of deciding whether a given graph has such a decomposition is NP-complete if both k and ℓ are at least 2, NP-complete if k≥9 and ℓ=1, and is in P for (k,ℓ)=(2,1). Before this, the only known NP-complete cases were the (2,2) and (3,3) cases. Our hardness result answers a question of Bermond et al. from 1984. We also show that planar graphs of girth at least nine decompose into a linear forest and a matching, which in particular is stronger than 3-edge-colouring such graphs. AU - Campbell, Rutger AU - Hörsch, Florian AU - Moore, Benjamin ID - 15163 IS - 6 JF - Discrete Mathematics SN - 0012-365X TI - Decompositions into two linear forests of bounded lengths VL - 347 ER - TY - JOUR AB - Characterizing the prevalence and properties of faint active galactic nuclei (AGNs) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs) and determining their role in cosmic reionization. We perform a spectroscopic search for broad Hα emitters at z ≈ 4–6 using deep JWST/NIRCam imaging and wide field slitless spectroscopy from the EIGER and FRESCO surveys. We identify 20 Hα lines at z = 4.2–5.5 that have broad components with line widths from ∼1200–3700 km s−1, contributing ∼30%–90% of the total line flux. We interpret these broad components as being powered by accretion onto SMBHs with implied masses ∼107–8M⊙. In the UV luminosity range MUV,AGN+host = −21 to −18, we measure number densities of ≈10−5 cMpc−3. This is an order of magnitude higher than expected from extrapolating quasar UV luminosity functions (LFs). Yet, such AGN are found in only <1% of star-forming galaxies at z ∼ 5. The number density discrepancy is much lower when compared to the broad Hα LF. The SMBH mass function agrees with large cosmological simulations. In two objects, we detect complex Hα profiles that we tentatively interpret as caused by absorption signatures from dense gas fueling SMBH growth and outflows. We may be witnessing early AGN feedback that will clear dust-free pathways through which more massive blue quasars are seen. We uncover a strong correlation between reddening and the fraction of total galaxy luminosity arising from faint AGN. This implies that early SMBH growth is highly obscured and that faint AGN are only minor contributors to cosmic reionization. AU - Matthee, Jorryt J AU - Naidu, Rohan P. AU - Brammer, Gabriel AU - Chisholm, John AU - Eilers, Anna-Christina AU - Goulding, Andy AU - Greene, Jenny AU - Kashino, Daichi AU - Labbe, Ivo AU - Lilly, Simon J. AU - Mackenzie, Ruari AU - Oesch, Pascal A. AU - Weibel, Andrea AU - Wuyts, Stijn AU - Xiao, Mengyuan AU - Bordoloi, Rongmon AU - Bouwens, Rychard AU - van Dokkum, Pieter AU - Illingworth, Garth AU - Kramarenko, Ivan AU - Maseda, Michael V. AU - Mason, Charlotte AU - Meyer, Romain A. AU - Nelson, Erica J. AU - Reddy, Naveen A. AU - Shivaei, Irene AU - Simcoe, Robert A. AU - Yue, Minghao ID - 15180 IS - 2 JF - The Astrophysical Journal KW - Space and Planetary Science KW - Astronomy and Astrophysics SN - 0004-637X TI - Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys VL - 963 ER - TY - JOUR AB - The fungal bioluminescence pathway can be reconstituted in other organisms allowing luminescence imaging without exogenously supplied substrate. The pathway starts from hispidin biosynthesis—a step catalyzed by a large fungal polyketide synthase that requires a posttranslational modification for activity. Here, we report identification of alternative compact hispidin synthases encoded by a phylogenetically diverse group of plants. A hybrid bioluminescence pathway that combines plant and fungal genes is more compact, not dependent on availability of machinery for posttranslational modifications, and confers autonomous bioluminescence in yeast, mammalian, and plant hosts. The compact size of plant hispidin synthases enables additional modes of delivery of autoluminescence, such as delivery with viral vectors. AU - Palkina, Kseniia A. AU - Karataeva, Tatiana A. AU - Perfilov, Maxim M. AU - Fakhranurova, Liliia I. AU - Markina, Nadezhda M. AU - Gonzalez Somermeyer, Louisa AU - Garcia-Perez, Elena AU - Vazquez-Vilar, Marta AU - Rodriguez-Rodriguez, Marta AU - Vazquez-Vilriales, Victor AU - Shakhova, Ekaterina S. AU - Mitiouchkina, Tatiana AU - Belozerova, Olga A. AU - Kovalchuk, Sergey I. AU - Alekberova, Anna AU - Malyshevskaia, Alena K. AU - Bugaeva, Evgenia N. AU - Guglya, Elena B. AU - Balakireva, Anastasia AU - Sytov, Nikita AU - Bezlikhotnova, Anastasia AU - Boldyreva, Daria I. AU - Babenko, Vladislav V. AU - Kondrashov, Fyodor AU - Choob, Vladimir V. AU - Orzaez, Diego AU - Yampolsky, Ilia V. AU - Mishin, Alexander S. AU - Sarkisyan, Karen S. ID - 15179 IS - 10 JF - Science Advances SN - 2375-2548 TI - A hybrid pathway for self-sustained luminescence VL - 10 ER - TY - JOUR AB - The elimination of rain evaporation in the planetary boundary layer (PBL) has been found to lead to convective self‐aggregation (CSA) even without radiative feedback, but the precise mechanisms underlying this phenomenon remain unclear. We conducted cloud‐resolving simulations with two domain sizes and progressively reduced rain evaporation in the PBL. Surprisingly, CSA only occurred when rain evaporation was almost completely removed. The additional convective heating resulting from the reduction of evaporative cooling in the moist patch was found to be the trigger, thereafter a dry subsidence intrusion into the PBL in the dry patch takes over and sets CSA in motion. Temperature and moisture anomalies oppose each other in their buoyancy effects, hence explaining the need for almost total rain evaporation removal. We also found radiative cooling and not cold pools to be the leading cause for the comparative ease of CSA to take place in the larger domain. AU - Hwong, Yi-Ling AU - Muller, Caroline J ID - 15186 IS - 6 JF - Geophysical Research Letters KW - General Earth and Planetary Sciences KW - Geophysics SN - 0094-8276 TI - The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation VL - 51 ER - TY - JOUR AB - We demonstrate the failure of the adiabatic Born-Oppenheimer approximation to describe the ground state of a quantum impurity within an ultracold Fermi gas despite substantial mass differences between the bath and impurity species. Increasing repulsion leads to the appearance of nonadiabatic couplings between the fast bath and slow impurity degrees of freedom, which reduce the parity symmetry of the latter according to the pseudo Jahn-Teller effect. The presence of this mechanism is associated to a conical intersection involving the impurity position and the inverse of the interaction strength, which acts as a synthetic dimension. We elucidate the presence of these effects via a detailed ground-state analysis involving the comparison of ab initio fully correlated simulations with effective models. Our study suggests ultracold atomic ensembles as potent emulators of complex molecular phenomena. AU - Becker, A. AU - Koutentakis, Georgios AU - Schmelcher, P. ID - 15181 IS - 1 JF - Physical Review Research SN - 2643-1564 TI - Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions VL - 6 ER - TY - JOUR AB - Thermoelectric materials convert heat into electricity, with a broad range of applications near room temperature (RT). However, the library of RT high-performance materials is limited. Traditional high-temperature synthetic methods constrain the range of materials achievable, hindering the ability to surpass crystal structure limitations and engineer defects. Here, a solution-based synthetic approach is introduced, enabling RT synthesis of powders and exploration of densification at lower temperatures to influence the material's microstructure. The approach is exemplified by Ag2Se, an n-type alternative to bismuth telluride. It is demonstrated that the concentration of Ag interstitials, grain boundaries, and dislocations are directly correlated to the sintering temperature, and achieve a figure of merit of 1.1 from RT to 100 °C after optimization. Moreover, insights into and resolve Ag2Se's challenges are provided, including stoichiometry issues leading to irreproducible performances. This work highlights the potential of RT solution synthesis in expanding the repertoire of high-performance thermoelectric materials for practical applications. AU - Kleinhanns, Tobias AU - Milillo, Francesco AU - Calcabrini, Mariano AU - Fiedler, Christine AU - Horta, Sharona AU - Balazs, Daniel AU - Strumolo, Marissa J. AU - Hasler, Roger AU - Llorca, Jordi AU - Tkadletz, Michael AU - Brutchey, Richard L. AU - Ibáñez, Maria ID - 15182 JF - Advanced Energy Materials SN - 1614-6832 TI - A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se ER - TY - JOUR AB - Current knowledge suggests a drought Indian monsoon (perhaps a severe one) when the El Nino Southern Oscillation and Pacific Decadal Oscillation each exhibit positive phases (a joint positive phase). For the monsoons, which are exceptions in this regard, we found northeast India often gets excess pre-monsoon rainfall. Further investigation reveals that this excess pre-monsoon rainfall is produced by the interaction of the large-scale circulation associated with the joint phase with the mountains in northeast India. We posit that a warmer troposphere, a consequence of excess rainfall over northeast India, drives a stronger monsoon circulation and enhances monsoon rainfall over central India. Hence, we argue that pre-monsoon rainfall over northeast India can be used for seasonal monsoon rainfall prediction over central India. Most importantly, its predictive value is at its peak when the Pacific Ocean exhibits a joint positive phase and the threat of extreme drought monsoon looms over India. AU - Goswami, Bidyut B ID - 15165 IS - 5 JF - Geophysical Research Letters SN - 0094-8276 TI - A pre-monsoon signal of false alarms of Indian monsoon droughts VL - 51 ER - TY - JOUR AB - Reducing defects boosts room-temperature performance of a thermoelectric device AU - Navita, Navita AU - Ibáñez, Maria ID - 15166 IS - 6688 JF - Science SN - 0036-8075 TI - Electron highways are cooler VL - 383 ER - TY - JOUR AB - The extracellular matrix (ECM) serves as a scaffold for cells and plays an essential role in regulating numerous cellular processes, including cell migration and proliferation. Due to limitations in specimen preparation for conventional room-temperature electron microscopy, we lack structural knowledge on how ECM components are secreted, remodeled, and interact with surrounding cells. We have developed a 3D-ECM platform compatible with sample thinning by cryo-focused ion beam milling, the lift-out extraction procedure, and cryo-electron tomography. Our workflow implements cell-derived matrices (CDMs) grown on EM grids, resulting in a versatile tool closely mimicking ECM environments. This allows us to visualize ECM for the first time in its hydrated, native context. Our data reveal an intricate network of extracellular fibers, their positioning relative to matrix-secreting cells, and previously unresolved structural entities. Our workflow and results add to the structural atlas of the ECM, providing novel insights into its secretion and assembly. AU - Zens, Bettina AU - Fäßler, Florian AU - Hansen, Jesse AU - Hauschild, Robert AU - Datler, Julia AU - Hodirnau, Victor-Valentin AU - Zheden, Vanessa AU - Alanko, Jonna H AU - Sixt, Michael K AU - Schur, Florian KM ID - 15146 IS - 6 JF - Journal of Cell Biology SN - 0021-9525 TI - Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix VL - 223 ER - TY - JOUR AB - We prove an upper bound on the ground state energy of the dilute spin-polarized Fermi gas capturing the leading correction to the kinetic energy resulting from repulsive interactions. One of the main ingredients in the proof is a rigorous implementation of the fermionic cluster expansion of Gaudin et al. (1971) [15]. AU - Lauritsen, Asbjørn Bækgaard AU - Seiringer, Robert ID - 14931 IS - 7 JF - Journal of Functional Analysis SN - 0022-1236 TI - Ground state energy of the dilute spin-polarized Fermi gas: Upper bound via cluster expansion VL - 286 ER -