@article{HofmanHaywardHeimetal.2019,
  author    = {Hofman, Maarten P. G. and Hayward, M. W. and Heim, M. and Marchand, P. and Rolandsen, C. M. and Mattisson, Jenny and Urbano, F. and Heurich, M. and Mysterud, A. and Melzheimer, J. and Morellet, N. and Voigt, Ulrich and Allen, B. L. and Gehr, Benedikt and Rouco Zufiaurre, Carlos and Ullmann, Wiebke and Holand, O. and Jorgensen, n H. and Steinheim, G. and Cagnacci, F. and Kroeschel, M. and Kaczensky, P. and Buuveibaatar, B. and Payne, J. C. and Palmegiani, I and Jerina, K. and Kjellander, P. and Johansson, O. and LaPoint, S. and Bayrakcismith, R. and Linnell, J. D. C. and Zaccaroni, M. and Jorge, M. L. S. and Oshima, J. E. F. and Songhurst, A. and Fischer, C. and Mc Bride, R. T. and Thompson, J. J. and Streif, S. and Sandfort, R. and Bonenfant, Christophe and Drouilly, M. and Klapproth, M. and Zinner, Dietmar and Yarnell, Richard and Stronza, A. and Wilmott, L. and Meisingset, E. and Thaker, Maria and Vanak, A. T. and Nicoloso, S. and Graeber, R. and Said, S. and Boudreau, M. R. and Devlin, A. and Hoogesteijn, R. and May-Junior, J. A. and Nifong, J. C. and Odden, J. and Quigley, H. B. and Tortato, F. and Parker, D. M. and Caso, A. and Perrine, J. and Tellaeche, C. and Zieba, F. and Zwijacz-Kozica, T. and Appel, C. L. and Axsom, I and Bean, W. T. and Cristescu, B. and Periquet, S. and Teichman, K. J. and Karpanty, S. and Licoppe, A. and Menges, V and Black, K. and Scheppers, Thomas L. and Schai-Braun, S. C. and Azevedo, F. C. and Lemos, F. G. and Payne, A. and Swanepoel, L. H. and Weckworth, B. and Berger, A. and Bertassoni, Alessandra and McCulloch, G. and Sustr, P. and Athreya, V and Bockmuhl, D. and Casaer, J. and Ekori, A. and Melovski, D. and Richard-Hansen, C. and van de Vyver, D. and Reyna-Hurtado, R. and Robardet, E. and Selva, N. and Sergiel, A. and Farhadinia, M. S. and Sunde, P. and Portas, R. and Ambarli, H{\"u}seyin and Berzins, R. and Kappeler, P. M. and Mann, G. K. and Pyritz, L. and Bissett, C. and Grant, T. and Steinmetz, R. and Swedell, Larissa and Welch, R. J. and Armenteras, D. and Bidder, O. R. and Gonzalez, T. M. and Rosenblatt, A. and Kachel, S. and Balkenhol, N.},
  title     = {Right on track?},
  series = {PLoS one},
  volume    = {14},
  journal   = {PLoS one},
  number    = {5},
  publisher = {PLoS},
  address   = {San Fransisco},
  issn      = {1932-6203},
  doi       = {10.1371/journal.pone.0216223},
  pages     = {26},
  year      = {2019},
  abstract  = {Satellite telemetry is an increasingly utilized technology in wildlife research, and current devices can track individual animal movements at unprecedented spatial and temporal resolutions. However, as we enter the golden age of satellite telemetry, we need an in-depth understanding of the main technological, species-specific and environmental factors that determine the success and failure of satellite tracking devices across species and habitats. Here, we assess the relative influence of such factors on the ability of satellite telemetry units to provide the expected amount and quality of data by analyzing data from over 3,000 devices deployed on 62 terrestrial species in 167 projects worldwide. We evaluate the success rate in obtaining GPS fixes as well as in transferring these fixes to the user and we evaluate failure rates. Average fix success and data transfer rates were high and were generally better predicted by species and unit characteristics, while environmental characteristics influenced the variability of performance. However, 48\% of the unit deployments ended prematurely, half of them due to technical failure. Nonetheless, this study shows that the performance of satellite telemetry applications has shown improvements over time, and based on our findings, we provide further recommendations for both users and manufacturers.},
  language  = {en}
}
@article{CharpinetBrassardFontaineetal.2019,
  author    = {Charpinet, St{\´e}phane and Brassard, P. and Fontaine, G. and Van Grootel, Valerie and Zong, Weika and Giammichele, N. and Heber, Ulrich and Bogn{\´a}r, Zs{\´o}fia and Geier, Stephan and Green, Elizabeth M. and Hermes, J. J. and Kilkenny, D. and Ostensen, R. H. and Pelisoli, Ingrid Domingos and Silvotti, R. and Telting, J. H. and Vuckovic, Maja and Worters, H. L. and Baran, Andrzej S. and Bell, Keaton J. and Bradley, Paul A. and Debes, J. H. and Kawaler, S. D. and Kolaczek-Szymanski, P. and Murphy, S. J. and Pigulski, A. and Sodor, A. and Uzundag, Murat and Handberg, R. and Kjeldsen, H. and Ricker, G. R. and Vanderspek, R. K.},
  title     = {TESS first look at evolved compact pulsators Discovery and asteroseismic probing of the g-mode hot B subdwarf pulsator EC 21494-7018},
  series = {Astronomy and astrophysics : an international weekly journal},
  volume    = {632},
  journal   = {Astronomy and astrophysics : an international weekly journal},
  publisher = {EDP Sciences},
  address   = {Les Ulis},
  issn      = {0004-6361},
  doi       = {10.1051/0004-6361/201935395},
  pages     = {23},
  year      = {2019},
  abstract  = {Context. The TESS satellite was launched in 2018 to perform high-precision photometry from space over almost the whole sky in a search for exoplanets orbiting bright stars. This instrument has opened new opportunities to study variable hot subdwarfs, white dwarfs, and related compact objects. Targets of interest include white dwarf and hot subdwarf pulsators, both carrying high potential for asteroseismology. Aims. We present the discovery and detailed asteroseismic analysis of a new g-mode hot B subdwarf (sdB) pulsator, EC 21494-7018 (TIC 278659026), monitored in TESS first sector using 120-s cadence. Methods. The TESS light curve was analyzed with standard prewhitening techniques, followed by forward modeling using our latest generation of sdB models developed for asteroseismic investigations. By simultaneously best-matching all the observed frequencies with those computed from models, we identified the pulsation modes detected and, more importantly, we determined the global parameters and structural configuration of the star. Results. The light curve analysis reveals that EC 21494-7018 is a sdB pulsator counting up to 20 frequencies associated with independent g-modes. The seismic analysis singles out an optimal model solution in full agreement with independent measurements provided by spectroscopy (atmospheric parameters derived from model atmospheres) and astrometry (distance evaluated from Gaia DR2 trigonometric parallax). Several key parameters of the star are derived. Its mass (0.391 +/- 0.009x2006;M-circle dot) is significantly lower than the typical mass of sdB stars and suggests that its progenitor has not undergone the He-core flash; therefore this progenitor could originate from a massive (greater than or similar to 2;M-circle dot) red giant, which is an alternative channel for the formation of sdBs. Other derived parameters include the H-rich envelope mass (0.0037 +/- 0.0010;M-circle dot), radius (0.1694 +/- 0.0081;R-circle dot), and luminosity (8.2 +/- 1.1;L-circle dot). The optimal model fit has a double-layered He+H composition profile, which we interpret as an incomplete but ongoing process of gravitational settling of helium at the bottom of a thick H-rich envelope. Moreover, the derived properties of the core indicate that EC 21494-7018 has burnt similar to 43\% (in mass) of its central helium and possesses a relatively large mixed core (M-core;=;0.198 +/- 0.010;M-circle dot), in line with trends already uncovered from other g-mode sdB pulsators analyzed with asteroseismology. Finally, we obtain for the first time an estimate of the amount of oxygen (in mass; X(O)(core) = 0.16(-0.05)(+0.13)X(O)core=0.16-0.05+0.13\$ X(mathrm{O})_{mathrm{core}}=0.16_{-0.05}<^>{+0.13} \$) produced at this stage of evolution by an helium-burning core. This result, along with the core-size estimate, is an interesting constraint that may help to narrow down the still uncertain C-12(alpha,;gamma)O-16 nuclear reaction rate.},
  language  = {en}
}
@article{ZornLeCorvecVarleyetal.2019,
  author    = {Zorn, Edgar Ulrich and Le Corvec, Nicolas and Varley, Nick R. and Salzer, Jacqueline T. and Walter, Thomas R. and Navarro-Ochoa, Carlos and Vargas-Bracamontes, Dulce M. and Thiele, Samuel T. and Ar{\´a}mbula Mendoza, Ra{\´u}l},
  title     = {Load stress controls on directional lava dome growth at Volcan de Colima, Mexico},
  series = {Frontiers in Earth Science},
  volume    = {7},
  journal   = {Frontiers in Earth Science},
  publisher = {Frontiers Media},
  address   = {Lausanne},
  issn      = {2296-6463},
  doi       = {10.3389/feart.2019.00084},
  pages     = {18},
  year      = {2019},
  abstract  = {During eruptive activity of andesitic stratovolcanoes, the extrusion of lava domes, their collapse and intermittent explosions are common volcanic hazards. Many lava domes grow in a preferred direction, in turn affecting the direction of lava flows and pyroclastic density currents. Access to active lava domes is difficult and hazardous, so detailed data characterizing lava dome growth are typically limited, keeping the processes controlling the directionality of extrusions unclear. Here we combine TerraSAR-X satellite radar observations with high-resolution airborne photogrammetry to assess morphological changes, and perform finite element modeling to investigate the impact of loading stress on shallow magma ascent directions associated with lava dome extrusion and crater formation at Volcan de Colima, Mexico. The TerraSAR-X data, acquired in similar to 1-m resolution spotlight mode, enable us to derive a chronology of the eruptive processes from intensity-based time-lapse observations of the general crater and dome evolution. The satellite images are complemented by close-range airborne photos, processed by the Structure-from-Motion workflow. This allows the derivation of high-resolution digital elevation models, providing insight into detailed loading and unloading features. During the observation period from Jan-2013 to Feb-2016, we identify a dominantly W-directed dome growth and lava flow production until Jan-2015. In Feb-2015, following the removal of the active summit dome, the surface crater widened and elongated along a NE-SW axis. Later in May-2015, a new dome grew toward the SW of the crater while a separate vent developed in the NE of the crater, reflecting a change in the direction of magma ascent and possible conduit bifurcation. Finite element models show a significant stress change in agreement with the observed magma ascent direction changes in response to the changing surface loads, both for loading (dome growth) and unloading (crater forming excavation) cases. These results allow insight into shallow dome growth dynamics and the migration of magma ascent in response to changing volcano summit morphology. They further highlight the importance of detailed volcano summit morphology surveillance, as changes in direction or location of dome extrusion may have major implications regarding the directions of potential volcanic hazards, such as pyroclastic density currents generated by dome collapse.},
  language  = {en}
}
@article{TuckerBoehningGaeseFaganetal.2018,
  author    = {Tucker, Marlee A. and Boehning-Gaese, Katrin and Fagan, William F. and Fryxell, John M. and Van Moorter, Bram and Alberts, Susan C. and Ali, Abdullahi H. and Allen, Andrew M. and Attias, Nina and Avgar, Tal and Bartlam-Brooks, Hattie and Bayarbaatar, Buuveibaatar and Belant, Jerrold L. and Bertassoni, Alessandra and Beyer, Dean and Bidner, Laura and van Beest, Floris M. and Blake, Stephen and Blaum, Niels and Bracis, Chloe and Brown, Danielle and de Bruyn, P. J. Nico and Cagnacci, Francesca and Calabrese, Justin M. and Camilo-Alves, Constanca and Chamaille-Jammes, Simon and Chiaradia, Andre and Davidson, Sarah C. and Dennis, Todd and DeStefano, Stephen and Diefenbach, Duane and Douglas-Hamilton, Iain and Fennessy, Julian and Fichtel, Claudia and Fiedler, Wolfgang and Fischer, Christina and Fischhoff, Ilya and Fleming, Christen H. and Ford, Adam T. and Fritz, Susanne A. and Gehr, Benedikt and Goheen, Jacob R. and Gurarie, Eliezer and Hebblewhite, Mark and Heurich, Marco and Hewison, A. J. Mark and Hof, Christian and Hurme, Edward and Isbell, Lynne A. and Janssen, Rene and Jeltsch, Florian and Kaczensky, Petra and Kane, Adam and Kappeler, Peter M. and Kauffman, Matthew and Kays, Roland and Kimuyu, Duncan and Koch, Flavia and Kranstauber, Bart and LaPoint, Scott and Leimgruber, Peter and Linnell, John D. C. and Lopez-Lopez, Pascual and Markham, A. Catherine and Mattisson, Jenny and Medici, Emilia Patricia and Mellone, Ugo and Merrill, Evelyn and Mourao, Guilherme de Miranda and Morato, Ronaldo G. and Morellet, Nicolas and Morrison, Thomas A. and Diaz-Munoz, Samuel L. and Mysterud, Atle and Nandintsetseg, Dejid and Nathan, Ran and Niamir, Aidin and Odden, John and Oliveira-Santos, Luiz Gustavo R. and Olson, Kirk A. and Patterson, Bruce D. and de Paula, Rogerio Cunha and Pedrotti, Luca and Reineking, Bjorn and Rimmler, Martin and Rogers, Tracey L. and Rolandsen, Christer Moe and Rosenberry, Christopher S. and Rubenstein, Daniel I. and Safi, Kamran and Said, Sonia and Sapir, Nir and Sawyer, Hall and Schmidt, Niels Martin and Selva, Nuria and Sergiel, Agnieszka and Shiilegdamba, Enkhtuvshin and Silva, Joao Paulo and Singh, Navinder and Solberg, Erling J. and Spiegel, Orr and Strand, Olav and Sundaresan, Siva and Ullmann, Wiebke and Voigt, Ulrich and Wall, Jake and Wattles, David and Wikelski, Martin and Wilmers, Christopher C. and Wilson, John W. and Wittemyer, George and Zieba, Filip and Zwijacz-Kozica, Tomasz and Mueller, Thomas},
  title     = {Moving in the Anthropocene},
  series = {Science},
  volume    = {359},
  journal   = {Science},
  number    = {6374},
  publisher = {American Assoc. for the Advancement of Science},
  address   = {Washington},
  issn      = {0036-8075},
  doi       = {10.1126/science.aam9712},
  pages     = {466 -- 469},
  year      = {2018},
  abstract  = {Animal movement is fundamental for ecosystem functioning and species survival, yet the effects of the anthropogenic footprint on animal movements have not been estimated across species. Using a unique GPS-tracking database of 803 individuals across 57 species, we found that movements of mammals in areas with a comparatively high human footprint were on average one-half to one-third the extent of their movements in areas with a low human footprint. We attribute this reduction to behavioral changes of individual animals and to the exclusion of species with long-range movements from areas with higher human impact. Global loss of vagility alters a key ecological trait of animals that affects not only population persistence but also ecosystem processes such as predator-prey interactions, nutrient cycling, and disease transmission.},
  language  = {en}
}
@article{KupferBauervanRoesteletal.2022,
  author    = {Kupfer, Thomas and Bauer, Evan B. and van Roestel, Jan and Bellm, Eric C. and Bildsten, Lars and Fuller, Jim and Prince, Thomas A. and Heber, Ulrich and Geier, Stephan and Green, Matthew J. and Kulkarni, Shrinivas R. and Bloemen, Steven and Laher, Russ R. and Rusholme, Ben and Schneider, David},
  title     = {Discovery of a Double-detonation Thermonuclear Supernova Progenitor},
  series = {The astrophysical journal : an international review of spectroscopy and astronomical physics ; Part 2, Letters},
  volume    = {925},
  journal   = {The astrophysical journal : an international review of spectroscopy and astronomical physics ; Part 2, Letters},
  number    = {2},
  publisher = {IOP Publ. Ltd.},
  address   = {Bristol},
  issn      = {2041-8205},
  doi       = {10.3847/2041-8213/ac48f1},
  pages     = {10},
  year      = {2022},
  abstract  = {We present the discovery of a new double-detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with a P (orb) = 76.34179(2) minutes orbital period. Spectroscopic observations are consistent with an sdB star during helium core burning residing on the extreme horizontal branch. Chimera light curves are dominated by ellipsoidal deformation of the sdB star and a weak eclipse of the companion white dwarf. Combining spectroscopic and light curve fits, we find a low-mass sdB star, M (sdB) = 0.383 +/- 0.028 M (circle dot) with a massive white dwarf companion, M (WD) = 0.725 +/- 0.026 M (circle dot). From the eclipses we find a blackbody temperature for the white dwarf of 26,800 K resulting in a cooling age of approximate to 25 Myr whereas our MESA model predicts an sdB age of approximate to 170 Myr. We conclude that the sdB formed first through stable mass transfer followed by a common envelope which led to the formation of the white dwarf companion approximate to 25 Myr ago. Using the MESA stellar evolutionary code we find that the sdB star will start mass transfer in approximate to 6 Myr and in approximate to 60 Myr the white dwarf will reach a total mass of 0.92 M (circle dot) with a thick helium layer of 0.17 M (circle dot). This will lead to a detonation that will likely destroy the white dwarf in a peculiar thermonuclear supernova. PTF1 J2238+7430 is only the second confirmed candidate for a double-detonation thermonuclear supernova. Using both systems we estimate that at least approximate to 1\% of white dwarf thermonuclear supernovae originate from sdB+WD binaries with thick helium layers, consistent with the small number of observed peculiar thermonuclear explosions.},
  language  = {en}
}
@article{BhatMilicicThieulinPardoetal.2017,
  author    = {Bhat, Javaid Y. and Milicic, Goran and Thieulin-Pardo, Gabriel and Bracher, Andreas and Maxwell, Andrew and Ciniawsky, Susanne and M{\"u}ller-Cajar, Oliver and Engen, John R. and Hartl, F. Ulrich and Wendler, Petra and Hayer-Hartl, Manajit},
  title     = {Mechanism of Enzyme Repair by the AAA(+) Chaperone Rubisco Activase},
  series = {Molecular cell},
  volume    = {67},
  journal   = {Molecular cell},
  publisher = {Cell Press},
  address   = {Cambridge},
  issn      = {1097-2765},
  doi       = {10.1016/j.molcel.2017.07.004},
  pages     = {744 -- 756},
  year      = {2017},
  abstract  = {How AAA(+) chaperones conformationally remodel specific target proteins in an ATP-dependent manner is not well understood. Here, we investigated the mechanism of the AAA(+) protein Rubisco activase (Rca) in metabolic repair of the photosynthetic enzyme Rubisco, a complex of eight large (RbcL) and eight small (RbcS) subunits containing eight catalytic sites. Rubisco is prone to inhibition by tight-binding sugar phosphates, whose removal is catalyzed by Rca. We engineered a stable Rca hexamer ring and analyzed its functional interaction with Rubisco. Hydrogen/deuterium exchange and chemical crosslinking showed that Rca structurally destabilizes elements of the Rubisco active site with remarkable selectivity. Cryo-electron microscopy revealed that Rca docks onto Rubisco over one active site at a time, positioning the C-terminal strand of RbcL, which stabilizes the catalytic center, for access to the Rca hexamer pore. The pulling force of Rca is fine-tuned to avoid global destabilization and allow for precise enzyme repair.},
  language  = {en}
}
@article{FrijiaForknerMinisinietal.2019,
  author    = {Frijia, Gianluca and Forkner, R. and Minisini, D. and Pacton, M. and Struck, Ulrich and Mutti, Maria},
  title     = {Cyanobacteria proliferation in the cenomanian-turonian boundary interval of the apennine carbonate platform:},
  series = {Geochemistry, geophysics, geosystems},
  volume    = {20},
  journal   = {Geochemistry, geophysics, geosystems},
  number    = {6},
  publisher = {American Geophysical Union},
  address   = {Washington},
  issn      = {1525-2027},
  doi       = {10.1029/2019GC008306},
  pages     = {2698 -- 2716},
  year      = {2019},
  abstract  = {Oceanic Anoxic Event-2 (OAE-2; Cenomanian-Turonian) is characterized by extensive deposition of organic carbon-rich deposits (black shales) in ocean basins worldwide as result of a major perturbation of the global carbon cycle. While the sedimentological, geochemical, and paleontological aspects of deep water expressions of OAE-2 have been intensively studied in the last few decades, much less attention has been given to the coeval shallow water deposits. In this study, we present the results of a detailed facies and petrographic (optical microscope and scanning electron microscopy) and geochemical studies (delta C-13(carb), delta C-13 (org), delta N-15(bulk), TOC, and Rock-Eval pyrolysis) on two key shallow marine sections from the Apennine Carbonate Platform (ACP; Italy). Here a continuous record of shallow water carbonates through the OAE-2 interval is preserved, offering the unique opportunity to document the archive of paleoenvironmental changes in a neritic setting, at a tropical latitude and far from the influence of a large continental block. Two conspicuous intervals are characterized by abundant and closely spaced dark microbial laminites found at correlative stratigraphic horizons in the two stratigraphic sections. These laminites contain elevated concentrations of TOC (up to 1\%) relative to microbial capping cycles laminites stratigraphically above and below. The organic matter preserved in these fine-grained laminites is dominated by cyanobacteria remains, which accounted for most of the organic matter produced on the ACP in these intervals. Our study suggests that Tethyan carbonate platforms experienced significant biological changes during OAE-2, alternating, in few kiloyears, between eutrophic phases dominated by microbial communities and mesotrophic/oligotrophic conditions favoring normal carbonate production/sedimentation. The synchronous occurrence of microbialite facies at different locations across the ACP and on other platforms worldwide (e.g., Mexico and Croatia) suggests a causal link between Large Igneous Province volcanism and the environmental conditions necessary to trigger cyanobacterial proliferation on shallow carbonate platforms.},
  language  = {en}
}
@article{BarthelSchollwockWhite2009,
  author    = {Barthel, Thomas and Schollwock, Ulrich and White, Steven R.},
  title     = {Spectral functions in one-dimensional quantum systems at finite temperature using the density matrix renormalization group},
  issn      = {1098-0121},
  doi       = {10.1103/Physrevb.79.245101},
  year      = {2009},
  abstract  = {We present time-dependent density matrix renormalization group simulations (t-DMRG) at finite temperatures. It is demonstrated how a combination of finite-temperature t-DMRG and time-series prediction allows for an easy and very accurate calculation of spectral functions in one-dimensional quantum systems, irrespective of their statistics for arbitrary temperatures. This is illustrated with spin structure factors of XX and XXX spin-1/2 chains. For the XX model we can compare against an exact solution, and for the XXX model (Heisenberg antiferromagnet) against a Bethe ansatz solution and quantum Monte Carlo data.},
  language  = {en}
}
@article{GedvilaiteFroemmelSasnauskasetal.2000,
  author    = {Gedvilaite, Alma and Fr{\"o}mmel, C. and Sasnauskas, K. and Micheel, Burkhard and {\"O}zel, M. and Behrsing, Olaf and Staniulis, J. and Jandrig, Burkhard and Scherneck, Siegfried and Ulrich, R.},
  title     = {Formation of immunogenic virus-like particles by inserting epitopes into surface-exposed regions of hamster polyomavirus major capsid protein},
  year      = {2000},
  language  = {en}
}
@book{AckermannAhlgrimmApelojgetal.2018,
  author    = {Ackermann, Peter and Ahlgrimm, Frederik and Apelojg, Benjamin and B{\"o}rnert-Ringleb, Moritz and Borowski, Andreas and Ehlert, Antje and Eichler, Constanze and Frohn, Julia and Gehrmann, Marie-Luise and Gerlach, Erin and Goetz, Ilka and Goral, Johanna and Gronostaj, Anna and Grubert, Jana and G{\"u}lery{\"u}z, Burak and Hacke, Alexander and Heck, Sebastian and Hermanns, Jolanda and Hochmuth, J{\"o}rg and Jennek, Julia and Jostes, Brigitte and Jurczok, Anne and Kleemann, Katrin and Kortenkamp, Ulrich and Krauskopf, Karsten and K{\"u}choll, Denise and Kulawiak, Pawel R. and Lauterbach, Wolfgang and Lazarides, Rebecca and Linka, Tim and L{\"o}weke, Sebastian and Lohse-Bossenz, Hendrik and Maar, Verena and Nowak, Anna and Ratzlaff, Olaf and Reitz-Koncebovski, Karen and Rother, Stefanie and Scherreiks, Lynn and Schroeder, Christoph and Schwalbe, Anja and Schwill, Andreas and Tosch, Frank and Vock, Miriam and Wagner, Luisa and Westphal, Andrea and Wilbert, J{\"u}rgen},
  title     = {PSI-Potsdam},
  series = {Potsdamer Beitr{\"a}ge zur Lehrerbildung und Bildungsforschung},
  journal   = {Potsdamer Beitr{\"a}ge zur Lehrerbildung und Bildungsforschung},
  number    = {1},
  editor    = {Borowski, Andreas and Ehlert, Antje and Prechtl, Helmut},
  publisher = {Universit{\"a}tsverlag Potsdam},
  address   = {Potsdam},
  isbn      = {978-3-86956-442-5},
  issn      = {2626-3556},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-414542},
  publisher      = {Universit{\"a}t Potsdam},
  pages     = {354},
  year      = {2018},
  abstract  = {In Brandenburg kommt der Universit{\"a}t Potsdam eine besondere Rolle zu: Sie ist die einzige, an der zuk{\"u}nftige Lehrerinnen und Lehrer die erste Phase ihres Werdegangs - das Lehramtsstudium - absolvieren k{\"o}nnen. Vor diesem Hintergrund wurde bereits kurz nach der Gr{\"u}ndung im Jahr 1991 das „Potsdamer Modell der Lehrerbildung" entwickelt. Dieses Modell strebt fortlaufend eine enge Verzahnung von Theorie und Praxis {\"u}ber das gesamte Studium hinweg an und bindet hierf{\"u}r die schulpraktischen Studienanteile in besonderer Weise ein. Eine erneute St{\"a}rkung erfuhr die Lehrerbildung im Dezember 2014 mit der Gr{\"u}ndung des Zentrums f{\"u}r Lehrerbildung und Bildungsforschung (ZeLB). Aus der koordinierenden Arbeit des Zentrums entstand das fakult{\"a}ts{\"u}bergreifende Projekt „Professionalisierung - Schulpraktische Studien - Inklusion" (PSI-Potsdam) das im Rahmen der Qualit{\"a}tsoffensive Lehrerbildung des Bundesministeriums f{\"u}r Bildung und Forschung erfolgreich gef{\"o}rdert wurde (2015-2018) und dessen Verl{\"a}ngerung (2019-2023) bewilligt ist. Der vorliegende Band vermittelt in den drei großen Kapiteln „Erhebungsinstrumente", „Seminarkonzepte" und „Vernetzungen" einen {\"U}berblick {\"u}ber einige der praxisnahen Forschungszug{\"a}nge, hochschuldidaktischen Ans{\"a}tze und Strategien zur Vernetzung innerhalb der Lehrerbildung, die im Rahmen von PSI-Potsdam entwickelt und umgesetzt wurden. Die Beitr{\"a}ge wurden mit dem Ziel verfasst, Kolleginnen und Kollegen an Universit{\"a}ten und Hochschulen, Akteur_innen des Vorbereitungsdiensts sowie der Fort- und Weiterbildung von Lehrkr{\"a}ften m{\"o}glichst konkrete Einblicke zu gew{\"a}hren. Unter der Herausgeberschaft von Prof. Dr. Andreas Borowski (Fachdidaktik Physik), Prof. Dr. Antje Ehlert (Inklusionsp{\"a}dagogik mit dem F{\"o}rderschwerpunkt Lernen) und Prof. Dr. Helmut Prechtl (Fachdidaktik Biologie) vereinen sich Autor_innen mit breit gestreuter fachdidaktischer und bildungswissenschaftlicher Expertise.},
  language  = {de}
}