TY - JOUR A1 - Miller, Amy E. A1 - Cioni, Maria-Rosa L. A1 - de Grijs, Richard A1 - Sun, Ning-Chen A1 - Bell, Cameron P. M. A1 - Choudhury, Samyaday A1 - Ivanov, Valentin D. A1 - Marconi, Marcella A1 - Oliveira, Joana M. A1 - Petr-Gotzens, Monika A1 - Ripepi, Vincenzo A1 - van Loon, Jacco Th. T1 - The VMC survey - XLVII. Turbulence-controlled hierarchical star formation in the large magellanic cloud JF - Monthly notices of the Royal Astronomical Society N2 - We perform a statistical clustering analysis of upper main-sequence stars in the Large Magellanic Cloud (LMC) using data from the Visible and Infrared Survey Telescope for Astronomy survey of the Magellanic Clouds. We map over 2500 young stellar structures at 15 significance levels across similar to 120 square degrees centred on the LMC. The structures have sizes ranging from a few parsecs to over 1 kpc. We find that the young structures follow power-law size and mass distributions. From the perimeter-area relation, we derive a perimeter-area dimension of 1.44 +/- 0.20. From the mass-size relation and the size distribution, we derive two-dimensional fractal dimensions of 1.50 +/- 0.10 and 1.61 +/- 0.20, respectively. We find that the surface density distribution is well represented by a lognormal distribution. We apply the Larson relation to estimate the velocity dispersions and crossing times of these structures. Our results indicate that the fractal nature of the young stellar structures has been inherited from the gas clouds from which they form and that this architecture is generated by supersonic turbulence. Our results also suggest that star formation in the LMC is scale-free from 10 to 700 pc. KW - methods: statistical KW - stars: early-type KW - stars: formation KW - galaxies: individual: Magellanic Clouds KW - galaxies: stellar content KW - galaxies: structure Y1 - 2022 U6 - https://doi.org/10.1093/mnras/stac508 SN - 0035-8711 SN - 1365-2966 VL - 512 IS - 1 SP - 1196 EP - 1213 PB - Oxford Univ. Press CY - Oxford ER - TY - JOUR A1 - Griggio, Massimo A1 - Bedin, Luigi R. A1 - Raddi, Roberto A1 - Reindl, Nicole A1 - Tomasella, Lina A1 - Scalco, M. A1 - Salaris, M. A1 - Cassisi, S. A1 - Ochner, P. A1 - Ciroi, S. A1 - Rosati, P. A1 - Nardiello, Domenico A1 - Anderson, J. A1 - Libralato, Mattia A1 - Bellini, A. A1 - Vallenari, A. A1 - Spina, L. A1 - Pedani, M. T1 - Astro-photometric study of M37 with Gaia and wide-field ugi-imaging JF - Monthly notices of the Royal Astronomical Society N2 - We present an astrometric and photometric wide-field study of the Galactic open star cluster M37 (NGC 2099). The studied field was observed with ground-based images covering a region of about four square degrees in the Sloan-like filters ugi. We exploited the Gaia catalogue to calibrate the geometric distortion of the large field mosaics, developing software routines that can be also applied to other wide-field instruments. The data are used to identify the hottest white dwarf (WD) member candidates of M37. Thanks to the Gaia EDR3 exquisite astrometry we identified seven such WD candidates, one of which, besides being a high-probability astrometric member, is the putative central star of a planetary nebula. To our knowledge, this is a unique object in an open cluster, and we have obtained follow-up low-resolution spectra that are used for a qualitative characterization of this young WD. Finally, we publicly release a three-colour atlas and a catalogue of the sources in the field of view, which represents a complement of existing material. KW - catalogues KW - white dwarfs KW - open clusters and associations: individual: KW - M37 (NGC2099) Y1 - 2022 U6 - https://doi.org/10.1093/mnras/stac1920 SN - 0035-8711 SN - 1365-2966 VL - 515 IS - 2 SP - 1841 EP - 1853 PB - Oxford University Press CY - Oxford ER - TY - JOUR A1 - Kamali, Bahareh A1 - Jahanbakhshi, Farshid A1 - Dogaru, Diana A1 - Dietrich, Jörg A1 - Nendel, Claas A1 - AghaKouchak, Amir T1 - Probabilistic modeling of crop-yield loss risk under drought: a spatial showcase for sub-Saharan Africa JF - Environmental research letters N2 - Assessing the risk of yield loss in African drought-affected regions is key to identify feasible solutions for stable crop production. Recent studies have demonstrated that Copula-based probabilistic methods are well suited for such assessment owing to reasonably inferring important properties in terms of exceedance probability and joint dependence of different characterization. However, insufficient attention has been given to quantifying the probability of yield loss and determining the contribution of climatic factors. This study applies the Copula theory to describe the dependence between drought and crop yield anomalies for rainfed maize, millet, and sorghum crops in sub-Saharan Africa (SSA). The environmental policy integrated climate model, calibrated with Food and Agriculture Organization country-level yield data, was used to simulate yields across SSA (1980-2012). The results showed that the severity of yield loss due to drought had a higher magnitude than the severity of drought itself. Sensitivity analysis to identify factors contributing to drought and high-temperature stresses for all crops showed that the amount of precipitation during vegetation and grain filling was the main driver of crop yield loss, and the effect of temperature was stronger for sorghum than for maize and millet. The results demonstrate the added value of probabilistic methods for drought-impact assessment. For future studies, we recommend looking into factors influencing drought and high-temperature stresses as individual/concurrent climatic extremes. KW - Copula theory KW - crop model KW - drought stress KW - joint probability KW - risk Y1 - 2022 U6 - https://doi.org/10.1088/1748-9326/ac4ec1 SN - 1748-9326 VL - 17 IS - 2 PB - IOP Publishing CY - Bristol ER - TY - JOUR A1 - Pelisoli, Ingrid A1 - Dorsch, Matti A1 - Heber, Ulrich A1 - Gänsicke, Boris A1 - Geier, Stephan A1 - Kupfer, Thomas A1 - Nemeth, Peter A1 - Scaringi, Simone A1 - Schaffenroth, Veronika T1 - Discovery and analysis of three magnetic hot subdwarf stars BT - evidence for merger-induced magnetic fields JF - Monthly notices of the Royal Astronomical Society N2 - Magnetic fields can play an important role in stellar evolution. Among white dwarfs, the most common stellar remnant, the fraction of magnetic systems is more than 20 per cent. The origin of magnetic fields in white dwarfs, which show strengths ranging from 40 kG to hundreds of MG, is still a topic of debate. In contrast, only one magnetic hot subdwarf star has been identified out of thousands of known systems. Hot subdwarfs are formed from binary interaction, a process often associated with the generation of magnetic fields, and will evolve to become white dwarfs, which makes the lack of detected magnetic hot subdwarfs a puzzling phenomenon. Here we report the discovery of three new magnetic hot subdwarfs with field strengths in the range 300-500 kG. Like the only previously known system, they are all helium-rich O-type stars (He-sdOs). We analysed multiple archival spectra of the three systems and derived their stellar properties. We find that they all lack radial velocity variability, suggesting formation via a merger channel. However, we derive higher than typical hydrogen abundances for their spectral type, which are in disagreement with current model predictions. Our findings suggest a lower limit to the magnetic fraction of hot subdwarfs of 0.147(+0.143)(-0.047) per cent, and provide evidence for merger-induced magnetic fields which could explain white dwarfs with field strengths of 50-150 MG, assuming magnetic flux conservation. KW - stars: magnetic field KW - subdwarfs Y1 - 2022 U6 - https://doi.org/10.1093/mnras/stac1069 SN - 0035-8711 SN - 1365-2966 VL - 515 IS - 2 SP - 2496 EP - 2510 PB - Oxford University Press CY - Oxford ER - TY - JOUR A1 - Geng, Rongwei A1 - Andreev, Andrei A1 - Kruse, Stefan A1 - Heim, Birgit A1 - van Geffen, Femke A1 - Pestryakova, Luidmila A1 - Zakharov, Evgenii A1 - Troeva, Elena I. A1 - Shevtsova, Iuliia A1 - Li, Furong A1 - Zhao, Yan A1 - Herzschuh, Ulrike T1 - Modern pollen assemblages from lake sediments and soil in East Siberia and relative pollen productivity estimates for Major Taxa JF - Frontiers in Ecology and Evolution N2 - Modern pollen-vegetation-climate relationships underpin palaeovegetation and palaeoclimate reconstructions from fossil pollen records. East Siberia is an ideal area for investigating the relationships between modern pollen assemblages and near natural vegetation under cold continental climate conditions. Reliable pollen-based quantitative vegetation and climate reconstructions are still scarce due to the limited number of modern pollen datasets. Furthermore, differences in pollen representation of samples from lake sediments and soils are not well understood. Here, we present a new pollen dataset of 48 moss/soil and 24 lake surface-sediment samples collected in Chukotka and central Yakutia in East Siberia. The pollen-vegetation-climate relationships were investigated by ordination analyses. Generally, tundra and taiga vegetation types can be well distinguished in the surface pollen assemblages. Moss/soil and lake samples contain generally similar pollen assemblages as revealed by a Procrustes comparison with some exceptions. Overall, modern pollen assemblages reflect the temperature and precipitation gradients in the study areas as revealed by constrained ordination analysis. We estimate the relative pollen productivity (RPP) of major taxa and the relevant source area of pollen (RSAP) for moss/soil samples from Chukotka and central Yakutia using Extended R-Value (ERV) analysis. The RSAP of the tundra-forest transition area in Chukotka and taiga area in central Yakutia are ca. 1300 and 360 m, respectively. For Chukotka, RPPs relative to both Poaceae and Ericaceae were estimated while RPPs for central Yakutia were relative only to Ericaceae. Relative to Ericaceae (reference taxon, RPP = 1), Larix, Betula, Picea, and Pinus are overrepresented while Alnus, Cyperaceae, Poaceae, and Salix are underrepresented in the pollen spectra. Our estimates are in general agreement with previously published values and provide the basis for reliable quantitative reconstructions of East Siberian vegetation. KW - modern pollen assemblages KW - pollen-vegetation-climate relationships KW - East Siberia KW - tundra KW - taiga KW - relative pollen productivity KW - quantitative vegetation reconstruction Y1 - 2022 U6 - https://doi.org/10.3389/fevo.2022.837857 SN - 2296-701X VL - 10 PB - Frontiers Media CY - Lausanne ER - TY - JOUR A1 - Kamali, Bahareh A1 - Lorite, Ignacio J. A1 - Webber, Heidi A. A1 - Rezaei, Ehsan Eyshi A1 - Gabaldon-Leal, Clara A1 - Nendel, Claas A1 - Siebert, Stefan A1 - Ramirez-Cuesta, Juan Miguel A1 - Ewert, Frank A1 - Ojeda, Jonathan J. T1 - Uncertainty in climate change impact studies for irrigated maize cropping systems in southern Spain JF - Scientific reports N2 - This study investigates the main drivers of uncertainties in simulated irrigated maize yield under historical conditions as well as scenarios of increased temperatures and altered irrigation water availability. Using APSIM, MONICA, and SIMPLACE crop models, we quantified the relative contributions of three irrigation water allocation strategies, three sowing dates, and three maize cultivars to the uncertainty in simulated yields. The water allocation strategies were derived from historical records of farmer's allocation patterns in drip-irrigation scheme of the Genil-Cabra region, Spain (2014-2017). By considering combinations of allocation strategies, the adjusted R-2 values (showing the degree of agreement between simulated and observed yields) increased by 29% compared to unrealistic assumptions of considering only near optimal or deficit irrigation scheduling. The factor decomposition analysis based on historic climate showed that irrigation strategies was the main driver of uncertainty in simulated yields (66%). However, under temperature increase scenarios, the contribution of crop model and cultivar choice to uncertainty in simulated yields were as important as irrigation strategy. This was partially due to different model structure in processes related to the temperature responses. Our study calls for including information on irrigation strategies conducted by farmers to reduce the uncertainty in simulated yields at field scale. Y1 - 2022 U6 - https://doi.org/10.1038/s41598-022-08056-9 SN - 2045-2322 VL - 12 IS - 1 PB - Macmillan Publishers Limited, CY - London ER - TY - JOUR A1 - Tolomeev, Aleksandr P. A1 - Dubovskaya, Olga P. A1 - Kirillin, Georgiy A1 - Buseva, Zhanna A1 - Kolmakova, Olesya A1 - Grossart, Hans-Peter A1 - Tang, Kam W. A1 - Gladyšev, Michail I. T1 - Degradation of dead cladoceran zooplankton and their contribution to organic carbon cycling in stratified lakes BT - field observation and model prediction JF - Journal of plankton research N2 - The contribution of dead zooplankton biomass to carbon cycle in aquatic ecosystems is practically unknown. Using abundance data of zooplankton in water column and dead zooplankton in sediment traps in Lake Stechlin, an ecological-mathematical model was developed to simulate the abundance and sinking of zooplankton carcasses and predict the related release of labile organic matter (LOM) into the water column. We found species-specific differences in mortality rate of the dominant zooplankton: Daphnia cucullata, Bosmina coregoni and Diaphanosoma brachyurum (0.008, 0.129 and 0.020 day(-1), respectively) and differences in their carcass sinking velocities in metalimnion (and hypolimnion): 2.1 (7.64), 14.0 (19.5) and 1.1 (5.9) m day(-1), respectively. Our model simulating formation and degradation processes of dead zooplankton predicted a bimodal distribution of the released LOM: epilimnic and metalimnic peaks of comparable intensity, ca. 1 mg DW m(-3) day(-1). Maximum degradation of carcasses up to ca. 1.7 mg DW m(-3) day(-1) occurred in the density gradient zone of metalimnion. LOM released from zooplankton carcasses into the surrounding water may stimulate microbial activity and facilitate microbial degradation of more refractory organic matter; therefore, dead zooplankton are expected to be an integral part of water column carbon source/sink dynamics in stratified lakes. KW - zooplankton carcasses KW - non-predatory mortality KW - sinking velocities KW - microbial degradation KW - Lake Stechlin KW - simulation modeling Y1 - 2022 U6 - https://doi.org/10.1093/plankt/fbac023 SN - 0142-7873 SN - 1464-3774 VL - 44 IS - 3 SP - 386 EP - 400 PB - Oxford Univ. Press CY - Oxford ER - TY - JOUR A1 - Leong, Jia Xuan A1 - Raffeiner, Margot A1 - Spinti, Daniela A1 - Langin, Gautier A1 - Franz-Wachtel, Mirita A1 - Guzman, Andrew R. A1 - Kim, Jung-Gun A1 - Pandey, Pooja A1 - Minina, Alyona E. A1 - Macek, Boris A1 - Hafren, Anders A1 - Bozkurt, Tolga O. A1 - Mudgett, Mary Beth A1 - Börnke, Frederik A1 - Hofius, Daniel A1 - Uestuen, Suayib T1 - A bacterial effector counteracts host autophagy by promoting degradation of an autophagy component JF - The EMBO journal N2 - Beyond its role in cellular homeostasis, autophagy plays anti- and promicrobial roles in host-microbe interactions, both in animals and plants. One prominent role of antimicrobial autophagy is to degrade intracellular pathogens or microbial molecules, in a process termed xenophagy. Consequently, microbes evolved mechanisms to hijack or modulate autophagy to escape elimination. Although well-described in animals, the extent to which xenophagy contributes to plant-bacteria interactions remains unknown. Here, we provide evidence that Xanthomonas campestris pv. vesicatoria (Xcv) suppresses host autophagy by utilizing type-III effector XopL. XopL interacts with and degrades the autophagy component SH3P2 via its E3 ligase activity to promote infection. Intriguingly, XopL is targeted for degradation by defense-related selective autophagy mediated by NBR1/Joka2, revealing a complex antagonistic interplay between XopL and the host autophagy machinery. Our results implicate plant antimicrobial autophagy in the depletion of a bacterial virulence factor and unravel an unprecedented pathogen strategy to counteract defense-related autophagy in plant-bacteria interactions. KW - autophagy KW - effectors KW - immunity KW - ubiquitination KW - xenophagy Y1 - 2022 U6 - https://doi.org/10.15252/embj.2021110352 SN - 0261-4189 SN - 1460-2075 VL - 41 IS - 13 PB - Wiley CY - Hoboken ER - TY - JOUR A1 - Agne, Stefanie A1 - Naylor, Gavin J. P. A1 - Preick, Michaela A1 - Yang, Lei A1 - Thiel, Ralf A1 - Weigmann, Simon A1 - Paijmans, Johanna L. A. A1 - Barlow, Axel A1 - Hofreiter, Michael A1 - Straube, Nicolas T1 - Taxonomic identification of two poorly known lantern shark species based on mitochondrial DNA from wet-collection paratypes JF - Frontiers in Ecology and Evolution N2 - Etmopteridae (lantern sharks) is the most species-rich family of sharks, comprising more than 50 species. Many species are described from few individuals, and re-collection of specimens is often hindered by the remoteness of their sampling sites. For taxonomic studies, comparative morphological analysis of type specimens housed in natural history collections has been the main source of evidence. In contrast, DNA sequence information has rarely been used. Most lantern shark collection specimens, including the types, were formalin fixed before long-term storage in ethanol solutions. The DNA damage caused by both fixation and preservation of specimens has excluded these specimens from DNA sequence-based phylogenetic analyses so far. However, recent advances in the field of ancient DNA have allowed recovery of wet-collection specimen DNA sequence data. Here we analyse archival mitochondrial DNA sequences, obtained using ancient DNA approaches, of two wet-collection lantern shark paratype specimens, namely Etmopterus litvinovi and E. pycnolepis, for which the type series represent the only known individuals. Target capture of mitochondrial markers from single-stranded DNA libraries allows for phylogenetic placement of both species. Our results suggest synonymy of E. benchleyi with E. litvinovi but support the species status of E. pycnolepis. This revised taxonomy is helpful for future conservation and management efforts, as our results indicate a larger distribution range of E. litvinovi. This study further demonstrates the importance of wet-collection type specimens as genetic resource for taxonomic research. KW - type specimens KW - Etmopterus litvinovi KW - Etmopterus pycnolepis KW - deep-sea KW - sharks KW - archival DNA Y1 - 2022 U6 - https://doi.org/10.3389/fevo.2022.910009 SN - 2296-701X VL - 10 PB - Frontiers Media CY - Lausanne ER - TY - JOUR A1 - Born, Artur A1 - Johansson, Fredrik O. L. A1 - Leitner, Torsten A1 - Bidermane, Ieva A1 - Kuehn, Danilo A1 - Martensson, Nils A1 - Föhlisch, Alexander T1 - The degree of electron itinerancy and shell closing in the core-ionized state of transition metals probed by Auger-photoelectron coincidence spectroscopy JF - Physical chemistry, chemical physics : a journal of European Chemical Societies N2 - Auger-photoelectron coincidence spectroscopy (APECS) has been used to examine the electron correlation and itinerance effects in transition metals Cu, Ni and Co. It is shown that the LVV Auger, in coincidence with 2p photoelectrons, spectra can be represented using atomic multiplet positions if the 3d-shell is localized (atomic-like) and with a self-convoluted valence band for band-like (itinerant) materials as explained using the Cini-Sawatzky model. For transition metals, the 3d band changes from band-like to localized with increasing atomic number, with the possibility of a mixed behavior. Our result shows that the LVV spectra of Cu can be represented by atomic multiplet calculations, those of Co resemble the self-convolution of the valence band and those of Ni are a mixture of both, consistent with the Cini-Sawatzky model. KW - spectra KW - Ni Y1 - 2022 U6 - https://doi.org/10.1039/d2cp02477b SN - 1463-9076 SN - 1463-9084 VL - 24 IS - 32 SP - 19218 EP - 19222 PB - Royal Society of Chemistry CY - Cambridge ER -