Santander-Martinez, Petra Maria

[["dc.bibliographiccitation.artnumber","8940"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Scientific Reports"],["dc.bibliographiccitation.volume","12"],["dc.contributor.author","Dieks, Jana-K."],["dc.contributor.author","Jünemann, Laura"],["dc.contributor.author","Hensel, Kai O."],["dc.contributor.author","Bergmann, Charlotte"],["dc.contributor.author","Schmidt, Stefan"],["dc.contributor.author","Quast, Anja"],["dc.contributor.author","Horn, Sebastian"],["dc.contributor.author","Sigler, Matthias"],["dc.contributor.author","Meyer-Marcotty, Philipp"],["dc.contributor.author","Santander, Petra"],["dc.date.accessioned","2022-06-01T09:39:11Z"],["dc.date.available","2022-06-01T09:39:11Z"],["dc.date.issued","2022"],["dc.description.abstract","Head development is a surrogate for brain development in infants and is related to neurocognitive outcome. There is only limited knowledge on early extra-uterine head shape and size assessment in very preterm infants. Here, 26 very preterm infants with a mean gestational age of 29.1 ± 2.2 weeks and a mean birth weight of 1273.8 ± 427.7 g underwent serial stereophotogrammetric 3D head imaging in weekly intervals from birth to term-equivalent age. The main outcome was the longitudinal assessment of the ‘physiological’ preterm head development with cephalometric size (head circumference, cranial volume) and shape parameters (cranial index, cranial vault asymmetry index) according to chronological and postmenstrual age (PMA). Potential clinical risk factors for the development of an abnormal low cranial index (dolichocephaly) were analysed. In serial measurements of 26 infants, the estimated head volume (95% confidence interval) increased from 244 (226–263) cm 3 at 28 weeks PMA to 705 (688–721) cm 3 at 40 weeks PMA. Moderate or severe dolichocephaly occurred in 21/26 infants (80.8%). Cranial index decreased over time (72.4%; 70.7–74 95% confidence interval). Brachycephaly and plagiocephaly were uncommon. No risk factors for severe dolichocephaly were identified. Our study shows that early detection of head shape and size anomalies utilizing 3D stereophotogrammetry is feasible and safe even in very preterm infants < 1500 g and/or < 32 weeks. 3D stereophotogrammetry could be used for timely identification of infants at risk for head shape anomalies. No specific risk factors for head shape anomalies were identified, especially not mode and duration of respiratory support."],["dc.description.sponsorship","Open-Access-Publikationsfonds 2022"],["dc.identifier.doi","10.1038/s41598-022-12887-x"],["dc.identifier.pii","12887"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/108408"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-572"],["dc.relation.eissn","2045-2322"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.title","Stereophotogrammetry can feasibly assess ‘physiological’ longitudinal three-dimensional head development of very preterm infants from birth to term"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.subtype","original_ja"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","clr.13820"],["dc.bibliographiccitation.firstpage","1228"],["dc.bibliographiccitation.issue","10"],["dc.bibliographiccitation.journal","Clinical Oral Implants Research"],["dc.bibliographiccitation.lastpage","1240"],["dc.bibliographiccitation.volume","32"],["dc.contributor.affiliation","Raschke, David; 1Department for Oral & Maxillofacial Surgery Universitätsmedizin Goettingen Goettingen Germany"],["dc.contributor.affiliation","Tröltzsch, Markus; 2Private Office Ansbach Germany & Department for Oral & Maxillofacial Surgery Universitätsmedizin Goettingen Goettingen Germany"],["dc.contributor.affiliation","Santander, Petra; 3Department of Orthodontics Universitätsmedizin Göttingen Goettingen Germany"],["dc.contributor.affiliation","Brockmeyer, Phillip; 1Department for Oral & Maxillofacial Surgery Universitätsmedizin Goettingen Goettingen Germany"],["dc.contributor.affiliation","Schliephake, Henning; 1Department for Oral & Maxillofacial Surgery Universitätsmedizin Goettingen Goettingen Germany"],["dc.contributor.author","Kauffmann, Philipp"],["dc.contributor.author","Raschke, David"],["dc.contributor.author","Tröltzsch, Markus"],["dc.contributor.author","Santander, Petra"],["dc.contributor.author","Brockmeyer, Phillip"],["dc.contributor.author","Schliephake, Henning"],["dc.date.accessioned","2021-09-01T06:42:53Z"],["dc.date.available","2021-09-01T06:42:53Z"],["dc.date.issued","2021"],["dc.date.updated","2022-03-21T09:20:33Z"],["dc.description.abstract","Abstract Aim To test the hypothesis that the use of rhBMP2 in established defects requires additional growth factors such as rhVEGF to accomplish effective bone repair. Materials and Methods Horizontal/vertical defects of 2 cm length and 1 cm height were created bilaterally in the alveolar crest of the maxillae of 18 minipigs together with the extraction of all premolar teeth and one molar tooth on both sides. After 3 months of healing, defects were augmented with 0.5 g particulate PDLLA/CaCO3 composite loaded with 400 µg rhBMP2/50 µg rhVEGF165 on one side and 800 µg rhBMP2 on the other in 12 test animals, whereas defects in six control animals were sham operated and left unfilled on one side and augmented with blank carriers on the other. After 4 and 13 weeks, the animals were evaluated each for area of new bone formation (mm²) and bone density (area %). Results Augmentations with carriers loaded with 800 g µrhBMP2 failed to induce significantly more bone than in the augmentations with unloaded carrier after 4 and 13 weeks (p = .1000, p = .381). Augmentations with carriers loaded with 400 µg rhBMP2 and 50 µg erhVEGF165 resulted in significantly increased bone formation after 13 weeks (p = .024) compared to blank carriers. Soft tissue in augmentations with combined rhBMP2/rhVEGF165 loading exhibited numerous microvessels compared to soft tissue in augmentations with rhBMP2. Conclusions It is concluded that effective bone regeneration in augmentations of established alveolar ridge defects may require the application of rhVEGF additionally to rhBMP2."],["dc.description.sponsorship","KLS MARTIN"],["dc.identifier.doi","10.1111/clr.13820"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/89167"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-455"],["dc.relation.eissn","1600-0501"],["dc.relation.issn","0905-7161"],["dc.rights","This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes."],["dc.title","The use of rhBMP2 for augmentation of established horizontal/vertical defects may require additional use of rhVEGF to achieve significant bone regeneration: An in vivo experimental study"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","627"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","640"],["dc.bibliographiccitation.volume","477"],["dc.contributor.author","Costa, J. E. S."],["dc.contributor.author","Kepler, S. O."],["dc.contributor.author","Winget, D. E."],["dc.contributor.author","O'Brien, M. S."],["dc.contributor.author","Kawaler, S. D."],["dc.contributor.author","Costa, A. F. M."],["dc.contributor.author","Giovannini, O."],["dc.contributor.author","Kanaan, A."],["dc.contributor.author","Mukadam, A. S."],["dc.contributor.author","Mullally, F."],["dc.contributor.author","Nitta, A."],["dc.contributor.author","Provençal, J. L."],["dc.contributor.author","Shipman, H."],["dc.contributor.author","Wood, M. A."],["dc.contributor.author","Ahrens, T. J."],["dc.contributor.author","Grauer, A."],["dc.contributor.author","Kilic, M."],["dc.contributor.author","Bradley, P. A."],["dc.contributor.author","Sekiguchi, K."],["dc.contributor.author","Crowe, R."],["dc.contributor.author","Jiang, X. J."],["dc.contributor.author","Sullivan, D."],["dc.contributor.author","Sullivan, T."],["dc.contributor.author","Rosen, R."],["dc.contributor.author","Clemens, J. C."],["dc.contributor.author","Janulis, R."],["dc.contributor.author","O'Donoghue, D."],["dc.contributor.author","Ogloza, W."],["dc.contributor.author","Baran, A."],["dc.contributor.author","Silvotti, R."],["dc.contributor.author","Marinoni, S."],["dc.contributor.author","Vauclair, G."],["dc.contributor.author","Dolez, N."],["dc.contributor.author","Chevreton, M."],["dc.contributor.author","Dreizler, S."],["dc.contributor.author","Schuh, S."],["dc.contributor.author","Deetjen, J."],["dc.contributor.author","Nagel, T."],["dc.contributor.author","Solheim, J.-E."],["dc.contributor.author","Gonzalez Perez, J. M."],["dc.contributor.author","Ulla, A."],["dc.contributor.author","Barstow, M."],["dc.contributor.author","Burleigh, M."],["dc.contributor.author","Good, S."],["dc.contributor.author","Metcalfe, T. S."],["dc.contributor.author","Kim, S.-L."],["dc.contributor.author","Lee, H."],["dc.contributor.author","Sergeev, A."],["dc.contributor.author","Akan, M. C."],["dc.contributor.author","Çakırlı, Ö."],["dc.contributor.author","Paparo, M."],["dc.contributor.author","Viraghalmy, G."],["dc.contributor.author","Ashoka, B. N."],["dc.contributor.author","Handler, G."],["dc.contributor.author","Hürkal, Ö."],["dc.contributor.author","Johannessen, F."],["dc.contributor.author","Kleinman, S. J."],["dc.contributor.author","Kalytis, R."],["dc.contributor.author","Krzesinski, J."],["dc.contributor.author","Klumpe, E."],["dc.contributor.author","Larrison, J."],["dc.contributor.author","Lawrence, T."],["dc.contributor.author","Meištas, E."],["dc.contributor.author","Martinez, P."],["dc.contributor.author","Nather, R. E."],["dc.contributor.author","Fu, J.-N."],["dc.contributor.author","Pakštienė, E."],["dc.contributor.author","Romero-Colmenero, E."],["dc.contributor.author","Riddle, R."],["dc.contributor.author","Seetha, S."],["dc.contributor.author","Silvestri, N. M."],["dc.contributor.author","Vučković, M."],["dc.contributor.author","Warner, B."],["dc.contributor.author","Zola, S."],["dc.contributor.author","Althaus, L. G."],["dc.contributor.author","Córsico, A. H."],["dc.contributor.author","Montgomery, M. H."],["dc.date.accessioned","2019-07-09T11:53:29Z"],["dc.date.available","2019-07-09T11:53:29Z"],["dc.date.issued","2008"],["dc.description.abstract","Context. PG 1159-035, a pre-white dwarf with Teff 140 000 K, is the prototype of both two classes: the PG 1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-035 photometric data obtained with the Whole Earth Telescope (WET) showed a rich frequency spectrum allowing the identification of 122 pulsation modes. Analyzing the periods of pulsation, it is possible to measure the stellar mass, the rotational period and the inclination of the rotation axis, to estimate an upper limit for the magnetic field, and even to obtain information about the inner stratification of the star. Aims. We have three principal aims: to increase the number of detected and identified pulsation modes in PG 1159-035, study trapping of the star’s pulsation modes, and to improve or constrain the determination of stellar parameters. Methods. We used all available WET photometric data from 1983, 1985, 1989, 1993 and 2002 to identify the pulsation periods. Results. We identified 76 additional pulsation modes, increasing to 198 the number of known pulsation modes in PG 1159-035, the largest number of modes detected in any star besides the Sun. From the period spacing we estimated a mass M/M = 0.59 ± 0.02 for PG 1159-035, with the uncertainty dominated by the models, not the observation. Deviations in the regular period spacing suggest that some of the pulsation modes are trapped, even though the star is a pre-white dwarf and the gravitational settling is ongoing. The position of the transition zone that causes the mode trapping was calculated at rc/R = 0.83 ± 0.05. From the multiplet splitting, we calculated the rotational period Prot = 1.3920 ± 0.0008 days and an upper limit for the magnetic field, B < 2000 G. The total power of the pulsation modes at the stellar surface changed less than 30% for = 1 modes and less than 50% for = 2 modes. We find no evidence of linear combinations between the 198 pulsation mode frequencies. PG 1159-035 models have not significative convection zones, supporting the hypothesis that nonlinearity arises in the convection zones in cooler pulsating white dwarf stars."],["dc.identifier.doi","10.1051/0004-6361:20053470"],["dc.identifier.fs","513378"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/7676"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/60434"],["dc.language.iso","en"],["dc.notes.intern","Merged from goescholar"],["dc.relation.orgunit","Fakultät für Physik"],["dc.rights","Goescholar"],["dc.rights.access","openAccess"],["dc.rights.uri","https://goedoc.uni-goettingen.de/licenses"],["dc.title","The pulsation modes of the pre-white dwarf PG 1159-035"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","639"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","654"],["dc.bibliographiccitation.volume","401"],["dc.contributor.author","Kepler, S. O."],["dc.contributor.author","Nather, R. E."],["dc.contributor.author","Winget, D. E."],["dc.contributor.author","Nitta, A."],["dc.contributor.author","Kleinman, S. J."],["dc.contributor.author","Metcalfe, T."],["dc.contributor.author","Sekiguchi, K."],["dc.contributor.author","Xiaojun, Jiang"],["dc.contributor.author","Sullivan, D."],["dc.contributor.author","Sullivan, T."],["dc.contributor.author","Janulis, R."],["dc.contributor.author","Meistas, E."],["dc.contributor.author","Kalytis, R."],["dc.contributor.author","Krzesinski, J."],["dc.contributor.author","Ogloza, W."],["dc.contributor.author","Zola, S."],["dc.contributor.author","O'Donoghue, D."],["dc.contributor.author","Romero-Colmenero, E."],["dc.contributor.author","Martinez, P."],["dc.contributor.author","Dreizler, S."],["dc.contributor.author","Deetjen, J."],["dc.contributor.author","Nagel, T."],["dc.contributor.author","Schuh, S. L."],["dc.contributor.author","Vauclair, G."],["dc.contributor.author","Ning, Fu Jian"],["dc.contributor.author","Chevreton, M."],["dc.contributor.author","Solheim, J.-E."],["dc.contributor.author","Perez, J. M. Gonzalez"],["dc.contributor.author","Johannessen, F."],["dc.contributor.author","Kanaan, A."],["dc.contributor.author","Costa, J. E."],["dc.contributor.author","Murillo Costa, A. F."],["dc.contributor.author","Wood, M. A."],["dc.contributor.author","Silvestri, N."],["dc.contributor.author","Ahrens, T. J."],["dc.contributor.author","Jones, A. K."],["dc.contributor.author","Collins, A. E."],["dc.contributor.author","Boyer, M."],["dc.contributor.author","Shaw, J. S."],["dc.contributor.author","Mukadam, A."],["dc.contributor.author","Klumpe, E. W."],["dc.contributor.author","Larrison, J."],["dc.contributor.author","Kawaler, S."],["dc.contributor.author","Riddle, R."],["dc.contributor.author","Ulla, A."],["dc.contributor.author","Bradley, P."],["dc.date.accessioned","2019-07-09T11:53:31Z"],["dc.date.available","2019-07-09T11:53:31Z"],["dc.date.issued","2003"],["dc.description.abstract","We report 323 hours of nearly uninterrupted time series photometric observations of the DBV star GD 358 acquired with the Whole Earth Telescope (WET) during May 23rd to June 8th, 2000. We acquired more than 232 000 independent measurements. We also report on 48 hours of time-series photometric observations in Aug 1996. We detected the non-radial g-modes consistent with degree ` = 1 and radial order 8 to 20 and their linear combinations up to 6th order. We also detect, for the first time, a high amplitude ` = 2 mode, with a period of 796 s. In the 2000 WET data, the largest amplitude modes are similar to those detected with the WET observations of 1990 and 1994, but the highest combination order previously detected was 4th order. At one point during the 1996 observations, most of the pulsation energy was transferred into the radial order k = 8 mode, which displayed a sinusoidal pulse shape in spite of the large amplitude. The multiplet structure of the individual modes changes from year to year, and during the 2000 observations only the k = 9 mode displays clear normal triplet structure. Even though the pulsation amplitudes change on timescales of days and years, the eigenfrequencies remain essentially the same, showing the stellar structure is not changing on any dynamical timescale."],["dc.identifier.doi","10.1051/0004-6361:20030105"],["dc.identifier.fs","20311"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/7683"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/60437"],["dc.language.iso","en"],["dc.notes.intern","Merged from goescholar"],["dc.relation.orgunit","Fakultät für Physik"],["dc.rights","Goescholar"],["dc.rights.access","openAccess"],["dc.rights.uri","https://goedoc.uni-goettingen.de/licenses"],["dc.title","The everchanging pulsating white dwarf GD358"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Head & Face Medicine"],["dc.bibliographiccitation.volume","16"],["dc.contributor.author","Santander, Petra"],["dc.contributor.author","Quast, Anja"],["dc.contributor.author","Olbrisch, Carolin"],["dc.contributor.author","Rose, Marius"],["dc.contributor.author","Moser, Norman"],["dc.contributor.author","Schliephake, Henning"],["dc.contributor.author","Meyer-Marcotty, Philipp"],["dc.date.accessioned","2021-04-14T08:32:08Z"],["dc.date.available","2021-04-14T08:32:08Z"],["dc.date.issued","2020"],["dc.description.sponsorship","Open-Access-Publikationsfonds 2021"],["dc.identifier.doi","10.1186/s13005-020-00245-z"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/17690"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/83821"],["dc.language.iso","en"],["dc.notes.intern","DOI Import GROB-399"],["dc.notes.intern","Merged from goescholar"],["dc.relation.eissn","1746-160X"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.title","Comprehensive 3D analysis of condylar morphology in adults with different skeletal patterns – a cross-sectional study"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","1"],["dc.bibliographiccitation.journal","Case Reports in Dentistry"],["dc.bibliographiccitation.lastpage","8"],["dc.bibliographiccitation.volume","2018"],["dc.contributor.author","Santander, P."],["dc.contributor.author","Schwaibold, E. M. C."],["dc.contributor.author","Bremmer, F."],["dc.contributor.author","Batschkus, S."],["dc.contributor.author","Kauffmann, P."],["dc.date.accessioned","2019-07-09T11:45:55Z"],["dc.date.available","2019-07-09T11:45:55Z"],["dc.date.issued","2018"],["dc.description.abstract","We report a case of multiple keratocysts first diagnosed in an 8-year-old boy. Case report. The incidental radiographic finding of a cystic lesion in an 8-year-old boy led to the surgical enucleation and further diagnosis of a keratocyst associated with a tooth crown. In the course of dental maturation from deciduous to permanent teeth, the boy presented new lesions, always associated with the crowns of teeth. Gorlin-Goltz (nevoid basal-cell carcinoma) syndrome was suspected, and the genetic analysis detected a previously undescribed germline variant in the PTCH1 gene. Treatment. This included a surgical removal of the cystic lesions, as well as the affected teeth. Follow-up. Due to the high recurrence rate of the keratocysts, frequent radiological checks were performed over a 5-year period."],["dc.identifier.doi","10.1155/2018/7594840"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/15343"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/59336"],["dc.language.iso","en"],["dc.notes.intern","Merged from goescholar"],["dc.relation.issn","2090-6455"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.subject.ddc","610"],["dc.title","Multiple, Multiloculated, and Recurrent Keratocysts of the Mandible and Maxilla in Association with Gorlin-Goltz (Nevoid Basal-Cell Carcinoma) Syndrome: A Pediatric Case Report and Follow-up over 5 Years"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","1019"],["dc.bibliographiccitation.issue","3"],["dc.bibliographiccitation.journal","European Archives of Oto-Rhino-Laryngology"],["dc.bibliographiccitation.lastpage","1025"],["dc.bibliographiccitation.volume","270"],["dc.contributor.author","Santander, Petra"],["dc.contributor.author","Engelke, Wilfried G. H."],["dc.contributor.author","Olthoff, Arno"],["dc.contributor.author","Voelter, Christiane"],["dc.date.accessioned","2018-11-07T09:27:42Z"],["dc.date.available","2018-11-07T09:27:42Z"],["dc.date.issued","2013"],["dc.description.abstract","Swallowing disturbances are common after neurological disease and oropharyngeal tumor resection. In this case the oral stage is often affected. So far the clinical evaluation of the oral phase is limited. Recently the role of pressure changes during oropharyngeal swallowing has been pointed out, but until now there are not enough data. Thereby 52 healthy adults aged between 20 and 45 years were examined using an oral shield (Silencos(A (R)), Bredent, Senden, Germany) connected to a digital manometer (GDUSB 1000(A (R)), Greisinger electronics, Regenstauf, Germany) able to record pressures in a range of 2,000 to -1,000 mbar at a frequency of 1 kHz. Three swallowing conditions were measured: an active bolus intake (ABI) of water, a passive bolus application of a water-bolus (PWA) and a passive application of a gel-bolus (PGA). We found negative pressures with a median value of -278.9 mbar during ABI, of -24.2 mbar during PWA and of -29.4 mbar during PGA. Significant differences in pressure amplitudes and the pressure pattern were observed depending on the kind of bolus application and its consistency. The used test presents a simple and easy to handle method to assess the oral phase of swallowing."],["dc.identifier.doi","10.1007/s00405-012-2299-6"],["dc.identifier.isi","000315443000033"],["dc.identifier.pmid","23238701"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/10305"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/30600"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Springer"],["dc.relation.issn","0937-4477"],["dc.rights","Goescholar"],["dc.rights.uri","https://goescholar.uni-goettingen.de/licenses"],["dc.title","Intraoral pressure patterns during swallowing"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","219"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","224"],["dc.bibliographiccitation.volume","432"],["dc.contributor.author","Kanaan, A."],["dc.contributor.author","Nitta, A."],["dc.contributor.author","Winget, D. E."],["dc.contributor.author","Kepler, S. O."],["dc.contributor.author","Montgomery, M. H."],["dc.contributor.author","Metcalfe, T. S."],["dc.contributor.author","Oliveira, H."],["dc.contributor.author","Fraga, L."],["dc.contributor.author","da Costa, AFM"],["dc.contributor.author","Costa, JES"],["dc.contributor.author","Castanheira, B. G."],["dc.contributor.author","Giovannini, O."],["dc.contributor.author","Nather, R. E."],["dc.contributor.author","Mukadam, A. S."],["dc.contributor.author","Kawaler, Steven D."],["dc.contributor.author","O'Brien, M. S."],["dc.contributor.author","Reed, M. D."],["dc.contributor.author","Kleinman, S. J."],["dc.contributor.author","Provencal, J. L."],["dc.contributor.author","Watson, T. K."],["dc.contributor.author","Kilkenny, D."],["dc.contributor.author","Sullivan, D. J."],["dc.contributor.author","Sullivan, T."],["dc.contributor.author","Shobbrook, B."],["dc.contributor.author","Jiang, X. J."],["dc.contributor.author","Ashoka, B. N."],["dc.contributor.author","Seetha, S."],["dc.contributor.author","Leibowitz, E. M."],["dc.contributor.author","Ibbetson, P."],["dc.contributor.author","Mendelson, H."],["dc.contributor.author","Meistas, E. G."],["dc.contributor.author","Kalytis, R."],["dc.contributor.author","Alisauskas, D."],["dc.contributor.author","O'Donoghue, D."],["dc.contributor.author","Buckley, D."],["dc.contributor.author","Martinez, P."],["dc.contributor.author","van Wyk, F."],["dc.contributor.author","Stobie, R."],["dc.contributor.author","Marang, F."],["dc.contributor.author","van Zyl, L."],["dc.contributor.author","Ogloza, W."],["dc.contributor.author","Krzesinski, J."],["dc.contributor.author","Zola, S."],["dc.contributor.author","Moskalik, P."],["dc.contributor.author","Breger, M."],["dc.contributor.author","Stankov, A."],["dc.contributor.author","Silvotti, Roberto"],["dc.contributor.author","Piccioni, A."],["dc.contributor.author","Vauclair, G."],["dc.contributor.author","Dolez, N."],["dc.contributor.author","Chevreton, M."],["dc.contributor.author","Deetjen, J."],["dc.contributor.author","Dreizler, Stefan"],["dc.contributor.author","Schuh, Sonja"],["dc.contributor.author","Perez, JMG"],["dc.contributor.author","Ostensen, Roy H."],["dc.contributor.author","Ulla, A."],["dc.contributor.author","Manteiga, M."],["dc.contributor.author","Suarez, O."],["dc.contributor.author","Burleigh, M. R."],["dc.contributor.author","Barstow, M. A."],["dc.date.accessioned","2018-11-07T11:18:05Z"],["dc.date.available","2018-11-07T11:18:05Z"],["dc.date.issued","2005"],["dc.description.abstract","BPM 37093 is the only hydrogen-atmosphere white dwarf currently known which has sufficient mass (similar to 1.1 M-.) to theoretically crystallize while still inside the ZZ Ceti instability strip (T-eff similar to 12 000 K). As a consequence, this star represents our first opportunity to test crystallization theory directly. If the core is substantially crystallized, then the inner boundary for each pulsation mode will be located at the top of the solid core rather than at the center of the star, affecting mainly the average period spacing. This is distinct from the \"mode trapping\" caused by the stratified surface layers, which modifies the pulsation periods more selectively. In this paper we report on Whole Earth Telescope observations of BPM 37093 obtained in 1998 and 1999. Based on a simple analysis of the average period spacing we conclude that a large fraction of the total stellar mass is likely to be crystallized."],["dc.identifier.doi","10.1051/0004-6361:20041125"],["dc.identifier.fs","38252"],["dc.identifier.isi","227493100024"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9872"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/54959"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","E D P Sciences"],["dc.relation.issn","0004-6361"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","Whole Earth Telescope observations of BPM 37093: A seismological test of crystallization theory in white dwarfs"],["dc.title.original","9872"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","27"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Head & Face Medicine"],["dc.bibliographiccitation.volume","17"],["dc.contributor.author","Quast, Anja"],["dc.contributor.author","Santander, Petra"],["dc.contributor.author","Kahlmeier, Timon"],["dc.contributor.author","Moser, Norman"],["dc.contributor.author","Schliephake, Henning"],["dc.contributor.author","Meyer-Marcotty, Philipp"],["dc.date.accessioned","2021-11-25T11:13:00Z"],["dc.date.available","2021-11-25T11:13:00Z"],["dc.date.issued","2021-07-13"],["dc.date.updated","2021-11-19T12:47:38Z"],["dc.description.abstract","Abstract Background Virtual surgery planning (VSP) is believed to reduce inaccuracies in maxillary positioning compared to conventional surgery planning (CSP) due to the elimination of face-bow transfer and laboratory steps. However, there is still a lack of comparative studies for the accuracy of splint-based maxillary positioning in CSP versus VSP. Therefore, the objective of this retrospective, observational study was to compare if splints produced by VSP and CSP reach postoperative outcomes within clinically acceptable limits. Methods The planned and actual postoperative results of 52 patients (VSP: n = 26; CSP: n = 26) with a mean age of 24.4 ± 6.2 years were investigated by three-dimensional (3D) alignment with planning software. The conventional treatment plan was digitized, so that the evaluation of both methods was performed in the same manner using the same coordinate system. Inaccuracies were measured by sagittal, vertical and transversal deviations of the upper central incisors and the inclination of the maxillary occlusal plane between the planned and achieved maxillary positions. Results Both methods demonstrated significant differences between the planned and actual outcome. The highest inaccuracies were observed in vertical impaction and midline correction. No significant differences between CSP and VSP were observed in any dimension. Errors in vertical and sagittal dimension intensified each other. Conclusions In conclusion, splint-based surgeries reached similar results regardless of the applied planning method and splint production."],["dc.description.sponsorship","Open-Access-Publikationsfonds 2021"],["dc.identifier.citation","Head & Face Medicine. 2021 Jul 13;17(1):27"],["dc.identifier.doi","10.1186/s13005-021-00279-x"],["dc.identifier.pii","279"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/93539"],["dc.language.iso","en"],["dc.notes.intern","DOI Import GROB-448"],["dc.publisher","BioMed Central"],["dc.relation.eissn","1746-160X"],["dc.rights","CC BY 4.0"],["dc.rights.holder","The Author(s)"],["dc.subject","Orthognathic surgery"],["dc.subject","Orthodontic-surgical treatment"],["dc.subject","Osteotomy"],["dc.subject","BSSO"],["dc.subject","Le Fort I"],["dc.subject","Accuracy"],["dc.subject","Maxillary positioning"],["dc.title","Predictability of maxillary positioning: a 3D comparison of virtual and conventional orthognathic surgery planning"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.subtype","original_ja"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","21155"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Scientific Reports"],["dc.bibliographiccitation.volume","11"],["dc.contributor.author","Santander, Petra"],["dc.contributor.author","Quast, Anja"],["dc.contributor.author","Hubbert, Johanna"],["dc.contributor.author","Juenemann, Laura"],["dc.contributor.author","Horn, Sebastian"],["dc.contributor.author","Hensel, Kai O."],["dc.contributor.author","Meyer-Marcotty, Philipp"],["dc.contributor.author","Dieks, Jana-Katharina"],["dc.date.accessioned","2021-12-01T09:23:10Z"],["dc.date.available","2021-12-01T09:23:10Z"],["dc.date.issued","2021"],["dc.description.abstract","The development of head shape and volume may reflect neurodevelopmental outcome and therefore is of paramount importance in neonatal care. Here, we compare head morphology in 25 very preterm infants with a birth weight of below 1500 g and / or a gestational age (GA) before 32 completed weeks to 25 term infants with a GA of 37–42 weeks at term equivalent age (TEA) and identify possible risk factors for non-synostotic head shape deformities. For three-dimensional head assessments, a portable stereophotogrammetric device was used. The most common and distinct head shape deformity in preterm infants was dolichocephaly. Severity of dolichocephaly correlated with GA and body weight at TEA but not with other factors such as neonatal morbidity, sex or total duration of respiratory support. Head circumference (HC) and cranial volume (CV) were not significantly different between the preterm and term infant group. Digitally measured HC and the CV significantly correlated even in infants with head shape deformities. Our study shows that stereophotogrammetric head assessment is feasible in all preterm and term infants and provides valuable information on volumetry and comprehensive head shape characteristics. In a small sample of preterm infants, body weight at TEA was identified as a specific risk factor for the development of dolichocephaly."],["dc.description.sponsorship","Open-Access-Publikationsfonds 2022"],["dc.identifier.doi","10.1038/s41598-021-00680-1"],["dc.identifier.pii","680"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/94581"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-478"],["dc.relation.eissn","2045-2322"],["dc.rights","CC BY 4.0"],["dc.title","Stereophotogrammetric head shape assessment in neonates is feasible and can identify distinct differences between term-born and very preterm infants at term equivalent age"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.subtype","original_ja"],["dspace.entity.type","Publication"]]