Vogt, Majbritt

[["dc.bibliographiccitation.journal","Monthly Notices of the Royal Astronomical Society"],["dc.contributor.author","Toledo-Padrón, B"],["dc.contributor.author","Hernández, J I González"],["dc.contributor.author","Rodríguez-López, C"],["dc.contributor.author","Mascareño, A Suárez"],["dc.contributor.author","Rebolo, R"],["dc.contributor.author","Butler, R P"],["dc.contributor.author","Ribas, I"],["dc.contributor.author","Anglada-Escudé, G"],["dc.contributor.author","Johnson, E N"],["dc.contributor.author","Reiners, A"],["dc.contributor.author","Caballero, J A"],["dc.contributor.author","Quirrenbach, A"],["dc.contributor.author","Amado, P J"],["dc.contributor.author","Béjar, V J S"],["dc.contributor.author","Morales, J C"],["dc.contributor.author","Perger, M"],["dc.contributor.author","Jeffers, S V"],["dc.contributor.author","Vogt, S"],["dc.contributor.author","Teske, J"],["dc.contributor.author","Shectman, S"],["dc.contributor.author","Crane, J"],["dc.contributor.author","Díaz, M"],["dc.contributor.author","Arriagada, P"],["dc.contributor.author","Holden, B"],["dc.contributor.author","Burt, J"],["dc.contributor.author","Rodríguez, E"],["dc.contributor.author","Herrero, E"],["dc.contributor.author","Murgas, F"],["dc.contributor.author","Pallé, E"],["dc.contributor.author","Morales, N"],["dc.contributor.author","López-González, M J"],["dc.contributor.author","Alonso, E Díez"],["dc.contributor.author","Tuomi, M"],["dc.contributor.author","Kiraga, M"],["dc.contributor.author","Engle, S G"],["dc.contributor.author","Guinan, E F"],["dc.contributor.author","Strachan, J B P"],["dc.contributor.author","Aceituno, F J"],["dc.contributor.author","Aceituno, J"],["dc.contributor.author","Casanova, V M"],["dc.contributor.author","Martín-Ruiz, S"],["dc.contributor.author","Montes, D"],["dc.contributor.author","Ortiz, J L"],["dc.contributor.author","Sota, A"],["dc.contributor.author","Briol, J"],["dc.contributor.author","Barbieri, L"],["dc.contributor.author","Cervini, I"],["dc.contributor.author","Deldem, M"],["dc.contributor.author","Dubois, F"],["dc.contributor.author","Hambsch, F-J"],["dc.contributor.author","Harris, B"],["dc.contributor.author","Kotnik, C"],["dc.contributor.author","Logie, L"],["dc.contributor.author","Lopez, J"],["dc.contributor.author","McNeely, M"],["dc.contributor.author","Ogmen, Y"],["dc.contributor.author","Pérez, L"],["dc.contributor.author","Rau, S"],["dc.contributor.author","Rodríguez, D"],["dc.contributor.author","Urquijo, F S"],["dc.contributor.author","Vanaverbeke, S"],["dc.date.accessioned","2020-12-10T18:19:31Z"],["dc.date.available","2020-12-10T18:19:31Z"],["dc.date.issued","2019"],["dc.identifier.doi","10.1093/mnras/stz1975"],["dc.identifier.eissn","1365-2966"],["dc.identifier.issn","0035-8711"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/75278"],["dc.language.iso","en"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Stellar activity analysis of Barnard’s Star: Very slow rotation and evidence for long-term activity cycle"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","33"],["dc.bibliographiccitation.issue","1-2"],["dc.bibliographiccitation.journal","Journal of Hydrology"],["dc.bibliographiccitation.lastpage","45"],["dc.bibliographiccitation.volume","384"],["dc.contributor.author","Brauchler, R."],["dc.contributor.author","Hu, R."],["dc.contributor.author","Vogt, T."],["dc.contributor.author","Al-Halbouni, D."],["dc.contributor.author","Heinrich, Steffen"],["dc.contributor.author","Ptak, Thomas"],["dc.contributor.author","Sauter, M."],["dc.date.accessioned","2018-11-07T08:44:03Z"],["dc.date.available","2018-11-07T08:44:03Z"],["dc.date.issued","2010"],["dc.description.abstract","In this study the potential of cross-well slug interference tests for high resolution aquifer characterization of hydraulic heterogeneity was assessed. The cross-well slug interference tests were performed at the research site \"Stegemuhle\", located in the Leine River valley near Gottingen, Germany. The geological composition of the subsurface, consisting mainly of 3.5 m silt and clay overlying 2.5 m sand and gravel, was determined by geophysical well logging and bore core data. To account for lateral changes a refraction seismic survey was conducted. Based on these data an area, characterized by an aquifer thickness of approximately 2 m and an average hydraulic conductivity of 5.0 x 10(-4) m/s (determined by pumping tests), most appropriate for cross-well slug interference tests, was chosen. Altogether 196 cross-well slug interference tests were performed using a tomographic measurement array. The cross-well slug interference tests were evaluated using type curve analysis, which provided detailed information concerning the vertical changes of hydraulic conductivity and specific storage. To assess hydraulic strata connectivity a travel time based tomographic inversion approach was utilized. The potential of the inversion approach to determine lateral changes could be successfully demonstrated by the reconstruction of the pinch out of a high diffusivity layer close to the bottom of the aquifer. The results demonstrate that the combined evaluation of cross-well slug interference tests based on type curve analysis and travel time inversion allows for the development of a detailed model about subsurface hydraulic heterogeneity. (C) 2010 Elsevier B.V. All rights reserved."],["dc.description.sponsorship","German Research Foundation [BF3379/1-2]"],["dc.identifier.doi","10.1016/j.jhydrol.2010.01.004"],["dc.identifier.isi","000276444700004"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/20118"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Elsevier Science Bv"],["dc.relation.issn","0022-1694"],["dc.title","Cross-well slug interference tests: An effective characterization method for resolving aquifer heterogeneity"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","L8"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","602"],["dc.contributor.author","Trifonov, T."],["dc.contributor.author","Kürster, M."],["dc.contributor.author","Zechmeister, M."],["dc.contributor.author","Zakhozhay, O. V."],["dc.contributor.author","Reffert, S."],["dc.contributor.author","Lee, M. H."],["dc.contributor.author","Rodler, F."],["dc.contributor.author","Vogt, S. S."],["dc.contributor.author","Brems, S. S."],["dc.date.accessioned","2020-12-10T18:11:35Z"],["dc.date.available","2020-12-10T18:11:35Z"],["dc.date.issued","2017"],["dc.identifier.doi","10.1051/0004-6361/201731044"],["dc.identifier.eissn","1432-0746"],["dc.identifier.issn","0004-6361"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/16809"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/74070"],["dc.notes.intern","DOI Import GROB-354"],["dc.notes.intern","Merged from goescholar"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","Three planets around HD 27894"],["dc.title.alternative","A close-in pair with a 2:1 period ratio and an eccentric Jovian planet at 5.4 AU⋆"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","791"],["dc.bibliographiccitation.issue","9"],["dc.bibliographiccitation.journal","JDDG Journal der Deutschen Dermatologischen Gesellschaft"],["dc.bibliographiccitation.lastpage","792"],["dc.bibliographiccitation.volume","9"],["dc.contributor.author","Schaefer, A."],["dc.contributor.author","Emmert, Steffen"],["dc.contributor.author","Kruppa, Jochen"],["dc.contributor.author","Schubert, S."],["dc.contributor.author","Tzvetkov, Mladen Vassilev"],["dc.contributor.author","Moessner, R."],["dc.contributor.author","Reich, Kristian"],["dc.contributor.author","Berking, Carola"],["dc.contributor.author","Volkenandt, Matthias"],["dc.contributor.author","Pfoehler, Claudia"],["dc.contributor.author","Schoen, Michael Peter"],["dc.contributor.author","Vogt, T."],["dc.contributor.author","Koenig, Inke R."],["dc.contributor.author","Reichrath, Joerg"],["dc.date.accessioned","2018-11-07T08:52:36Z"],["dc.date.available","2018-11-07T08:52:36Z"],["dc.date.issued","2011"],["dc.identifier.isi","000294596900179"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/22212"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Wiley-blackwell"],["dc.publisher.place","Malden"],["dc.relation.issn","1610-0379"],["dc.title","No Associateion of Polymorphisms in Genes of the Vitamin D Metabolism and the Risk of Melanoma Development and Melanoma Prognosis: a Case-Control Study"],["dc.type","conference_abstract"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","123"],["dc.bibliographiccitation.lastpage","137"],["dc.contributor.author","Freitag, Gudrun"],["dc.contributor.author","Munk, Axel"],["dc.contributor.author","Vogt, Majbritt"],["dc.contributor.editor","Akritas, Michael G."],["dc.contributor.editor","politis, dimitris"],["dc.date.accessioned","2017-09-07T11:53:21Z"],["dc.date.available","2017-09-07T11:53:21Z"],["dc.date.issued","2003"],["dc.description.abstract","We suggest diagnostic tools for the assessment of shape similarity of distributions, i.e. whether several distributions are equal up to a pre-specified semiparametric deviation, such as a simple shift in location or a scale deviation. This will be called a structural relationship between distributions, and it is of importance, for instance, in an initial analysis within the (nonparametric) analysis of variance. Our approach is based on a modification of a trimmed version of Mallows distance between distribution functions. Asymptotic theory for the corresponding test statistics is provided and a bootstrap limit theorem is shown. In particular, the case of dependent samples is covered as well. A simulation study reveals the bias corrected and accelerated bootstrap as an adequate method for the assessment of shape similar distributions. A medical application is discussed."],["dc.identifier.doi","10.1016/b978-044451378-6/50009-0"],["dc.identifier.gro","3145075"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/2771"],["dc.language.iso","en"],["dc.notes.intern","Crossref Import"],["dc.notes.status","zu prüfen"],["dc.publisher","Elsevier B.V."],["dc.publisher.place","Amsterdam"],["dc.relation.isbn","978-0-44451-378-6"],["dc.relation.isbn","978-0-444-51378-6"],["dc.relation.ispartof","Recent Advances and Trends in Nonparametric Statistics"],["dc.title","Assessing structural relationships between distributions - a quantile process approach based on Mallows distance"],["dc.type","book_chapter"],["dc.type.internalPublication","unknown"],["dc.type.peerReviewed","no"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","L89"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Monthly Notices of the Royal Astronomical Society"],["dc.bibliographiccitation.lastpage","L93"],["dc.bibliographiccitation.volume","443"],["dc.contributor.author","Anglada-Escude, Guillem"],["dc.contributor.author","Arriagada, Pamela"],["dc.contributor.author","Tuomi, Mikko"],["dc.contributor.author","Zechmeister, Mathias"],["dc.contributor.author","Jenkins, S."],["dc.contributor.author","Ofir, Aviv"],["dc.contributor.author","Dreizler, Stefan"],["dc.contributor.author","Gerlach, Enrico"],["dc.contributor.author","Marvin, Christopher J."],["dc.contributor.author","Reiners, Ansgar"],["dc.contributor.author","Jeffers, Sandra V."],["dc.contributor.author","Butler, R. Paul"],["dc.contributor.author","Vogt, S. S."],["dc.contributor.author","Amado, Pedro J."],["dc.contributor.author","Rodriguez-Lopez, Cristina"],["dc.contributor.author","Berdinas, Zaira M."],["dc.contributor.author","Morin, Julien"],["dc.contributor.author","Crane, Jeffrey D."],["dc.contributor.author","Shectman, Stephen A."],["dc.contributor.author","Thompson, Ian B."],["dc.contributor.author","Diaz, M."],["dc.contributor.author","Rivera, Eugenio J."],["dc.contributor.author","Sarmiento, Luis F."],["dc.contributor.author","Jones, Hugh R. A."],["dc.date.accessioned","2018-11-07T09:35:24Z"],["dc.date.available","2018-11-07T09:35:24Z"],["dc.date.issued","2014"],["dc.description.abstract","Exoplanets of a few Earth masses can be now detected around nearby low-mass stars using Doppler spectroscopy. In this Letter, we investigate the radial velocity variations of Kapteyn's star, which is both a sub-dwarf M-star and the nearest halo object to the Sun. The observations comprise archival and new HARPS (High Accuracy Radial velocity Planet Searcher), High Resolution Echelle Spectrometer (HIRES) and Planet Finder Spectrograph (PFS) Doppler measurements. Two Doppler signals are detected at periods of 48 and 120 d using likelihood periodograms and a Bayesian analysis of the data. Using the same techniques, the activity indices and archival All Sky Automated Survey (ASAS-3) photometry show evidence for low-level activity periodicities of the order of several hundred days. However, there are no significant correlations with the radial velocity variations on the same time-scales. The inclusion of planetary Keplerian signals in the model results in levels of correlated and excess white noise that are remarkably low compared to younger G, K and M dwarfs. We conclude that Kapteyn's star is most probably orbited by two super-Earth mass planets, one of which is orbiting in its circumstellar habitable zone, becoming the oldest potentially habitable planet known to date. The presence and long-term survival of a planetary system seem a remarkable feat given the peculiar origin and kinematic history of Kapteyn's star. The detection of super-Earth mass planets around halo stars provides important insights into planet-formation processes in the early days of the Milky Way."],["dc.identifier.doi","10.1093/mnrasl/slu076"],["dc.identifier.isi","000357291900019"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/32376"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Oxford Univ Press"],["dc.relation.issn","1365-2966"],["dc.relation.issn","0035-8711"],["dc.title","Two planets around Kapteyn's star: a cold and a temperate super-Earth orbiting the nearest halo red dwarf"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","74"],["dc.bibliographiccitation.firstpage","74"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","The Astrophysical Journal"],["dc.bibliographiccitation.volume","830"],["dc.contributor.author","Anglada-Escude, Guillem"],["dc.contributor.author","Tuomi, Mikko"],["dc.contributor.author","Arriagada, Pamela"],["dc.contributor.author","Zechmeister, Mathias"],["dc.contributor.author","Jenkins, J. S."],["dc.contributor.author","Ofir, Aviv"],["dc.contributor.author","Dreizler, Stefan"],["dc.contributor.author","Gerlach, Enrico"],["dc.contributor.author","Marvin, Christopher J."],["dc.contributor.author","Reiners, Ansgar"],["dc.contributor.author","Jeffers, Sandra V."],["dc.contributor.author","Butler, R. Paul"],["dc.contributor.author","Vogt, S. S."],["dc.contributor.author","Amado, Pedro J."],["dc.contributor.author","Rodriguez-Lopez, Cristina"],["dc.contributor.author","Berdinas, Zaira M."],["dc.contributor.author","Morin, Julien"],["dc.contributor.author","Crane, Jeffrey D."],["dc.contributor.author","Shectman, Stephen A."],["dc.contributor.author","Diaz, M. R."],["dc.contributor.author","Sarmiento, Luis F."],["dc.contributor.author","Jones, Hugh R. A."],["dc.date.accessioned","2018-11-07T10:06:54Z"],["dc.date.available","2018-11-07T10:06:54Z"],["dc.date.issued","2016"],["dc.description.abstract","Stellar activity may induce Doppler variability at the level of a few m s(-1) which can then be confused by the Doppler signal of an exoplanet orbiting the star. To first order, linear correlations between radial velocity measurements and activity indices have been proposed to account for any such correlation. The likely presence of two super-Earths orbiting Kapteyn's star was reported in Anglada-Escude et al., but this claim was recently challenged by Robertson et al., who argued for evidence of a rotation period (143 days) at three times the orbital period of one of the proposed planets (Kapteyn's b, P = 48.6 days) and the existence of strong linear correlations between its Doppler signal and activity data. By re-analyzing the data using global statistics and model comparison, we show that such a claim is incorrect given that (1) the choice of a rotation period at 143 days is unjustified, and (2) the presence of linear correlations is not supported by the data. We conclude that the radial velocity signals of Kapteyn's star remain more simply explained by the presence of two super-Earth candidates orbiting it. We note that analysis of time series of activity indices must be executed with the same care as Doppler time series. We also advocate for the use of global optimization procedures and objective arguments, instead of claims based on residual analyses which are prone to biases and incorrect interpretations."],["dc.identifier.doi","10.3847/0004-637X/830/2/74"],["dc.identifier.eissn","1538-4357"],["dc.identifier.isi","000396001400001"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/39187"],["dc.notes.intern","DOI Import GROB-354"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Iop Publishing Ltd"],["dc.relation.issn","1538-4357"],["dc.relation.issn","0004-637X"],["dc.title","No Evidence for Activity Correlations in the Radial Velocities of Kapteyn's Star"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","2881"],["dc.bibliographiccitation.issue","14"],["dc.bibliographiccitation.journal","Journal of Cell Science"],["dc.bibliographiccitation.lastpage","2891"],["dc.bibliographiccitation.volume","115"],["dc.contributor.author","Jedrusik, M. A."],["dc.contributor.author","Vogt, S."],["dc.contributor.author","Claus, P."],["dc.contributor.author","Schulze, E."],["dc.date.accessioned","2018-11-07T10:18:55Z"],["dc.date.available","2018-11-07T10:18:55Z"],["dc.date.issued","2002"],["dc.description.abstract","The histone Ell complement of Caenorhabditis elegans contains a single unusual protein, H1.X. Although H1.X possesses the globular domain and the canonical three-domain structure of linker histones, the amino acid composition of H1.X is distinctly different from conventional linker histones in both terminal domains. We have characterized H1.X in C elegans by antibody labeling, green fluorescent protein fusion protein expression and RNA interference. Unlike normal linker histones, H1.X is a cytoplasmic as well as a nuclear protein and is not associated with chromosomes. H1.X is most prominently expressed in the marginal cells of the pharynx and is associated with a peculiar cytoplasmic cytoskeletal structure therein, the tonofilaments. Additionally H1.X::GFP is expressed in the cytoplasm of body and vulva muscle cells, neurons, excretory cells and in the nucleoli of embryonic blastomeres; and adult gut cells. RNA interference with H1.X results in uncoordinated and egg laying defective animals, as well as in a longitudinally enlarged pharynx. These phenotypes indicate a cytoplasmic role of H1.X in muscle growth and muscle function."],["dc.identifier.isi","000177308300009"],["dc.identifier.pmid","12082149"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/41549"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Company Of Biologists Ltd"],["dc.relation.issn","0021-9533"],["dc.title","A novel linker histone-like protein is associated with cytoplasmic filaments in Caenorhabditis elegans"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","012002"],["dc.contributor.author","Stefani, F"],["dc.contributor.author","Albrecht, T"],["dc.contributor.author","Arlt, R"],["dc.contributor.author","Christen, M"],["dc.contributor.author","Gailitis, A"],["dc.contributor.author","Gellert, M"],["dc.contributor.author","Giesecke, A"],["dc.contributor.author","Goepfert, O"],["dc.contributor.author","Herault, J"],["dc.contributor.author","Kirillov, O N"],["dc.contributor.author","Mamatsashvili, G."],["dc.contributor.author","Priede, J"],["dc.contributor.author","Rüdiger, G"],["dc.contributor.author","Seilmayer, M"],["dc.contributor.author","Tilgner, A"],["dc.contributor.author","Vogt, T"],["dc.date.accessioned","2020-12-10T18:15:59Z"],["dc.date.available","2020-12-10T18:15:59Z"],["dc.date.issued","2017"],["dc.identifier.doi","10.1088/1757-899X/228/1/012002"],["dc.identifier.eissn","1757-899X"],["dc.identifier.issn","1757-8981"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/75016"],["dc.notes.intern","DOI Import GROB-354"],["dc.relation.conference","LIMTECH Colloquium and International Symposium on Liquid Metal Technologies"],["dc.relation.eventend","2017-09-20"],["dc.relation.eventlocation","Dresden"],["dc.relation.eventstart","2017-09-19"],["dc.relation.ispartof","Final"],["dc.title","Magnetic field dynamos and magnetically triggered flow instabilities"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","607"],["dc.bibliographiccitation.journal","Journal de Physique. IV, Proceedings"],["dc.bibliographiccitation.lastpage","613"],["dc.bibliographiccitation.volume","104"],["dc.contributor.author","Schneider, G."],["dc.contributor.author","Denbeaux, G."],["dc.contributor.author","Anderson, E."],["dc.contributor.author","Pearson, A."],["dc.contributor.author","Bates, W."],["dc.contributor.author","Vogt, S."],["dc.contributor.author","Knochel, C."],["dc.contributor.author","Meyer, M. A."],["dc.contributor.author","Zschech, E."],["dc.date.accessioned","2018-11-07T10:40:32Z"],["dc.date.available","2018-11-07T10:40:32Z"],["dc.date.issued","2003"],["dc.description.abstract","With the new tomography setup developed for the x-ray microscope XM-1 installed at the Advanced Light Source, tomography of immunolabelled frozen-hydrated cells to detect protein distributions inside of cells was performed. The distribution of the nuclear protein, male specific lethal 1 (MSL-1) in the Drosophila melanogaster cell was studied. Another application field for high resolution tomography which is of fundamental interest in materials science is electromigration in advanced copper interconnects. In this work, quantitative time-resolved x-ray microscopy mass transport studies of the early stages of electromigration in an inlaid Cu line/via structure were performed with 40 nm spatial resolution at 1.8 keV photon energy. Correlation of the real time x-ray microscopy images with post mortem high voltage electron micrographs of the sample shows that the void nucleation occurs at the site of grain boundaries in Cu and that the voids migrate along these grain boundaries during electromigration. To provide 3D information about the exact location (bulk or interface) of void nucleation and migration during an EM experiment, as well as to measure quantitatively the mass transport in the volume, future experiments must be based on time-resolved x-ray tomography."],["dc.identifier.doi","10.1051/jp4:20030155"],["dc.identifier.isi","000183273900142"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/46323"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.relation.conference","7th International Conference on X-Ray Microscopy"],["dc.relation.eventlocation","GRENOBLE, FRANCE"],["dc.relation.issn","1155-4339"],["dc.title","High resolution X-ray tomography with applications in biology and materials science"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]