--- _id: '1212' abstract: - lang: eng text: 'Plants adjust their growth according to gravity. Gravitropism involves gravity perception, signal transduction, and asymmetric growth response, with organ bending as a consequence [1]. Asymmetric growth results from the asymmetric distribution of the plant-specific signaling molecule auxin [2] that is generated by lateral transport, mediated in the hypocotyl predominantly by the auxin transporter PIN-FORMED3 (PIN3) [3–5]. Gravity stimulation polarizes PIN3 to the bottom sides of endodermal cells, correlating with increased auxin accumulation in adjacent tissues at the lower side of the stimulated organ, where auxin induces cell elongation and, hence, organ bending. A curvature response allows the hypocotyl to resume straight growth at a defined angle [6], implying that at some point auxin symmetry is restored to prevent overbending. Here, we present initial insights into cellular and molecular mechanisms that lead to the termination of the tropic response. We identified an auxin feedback on PIN3 polarization as underlying mechanism that restores symmetry of the PIN3-dependent auxin flow. Thus, two mechanistically distinct PIN3 polarization events redirect auxin fluxes at different time points of the gravity response: first, gravity-mediated redirection of PIN3-mediated auxin flow toward the lower hypocotyl side, where auxin gradually accumulates and promotes growth, and later PIN3 polarization to the opposite cell side, depleting this auxin maximum to end the bending. Accordingly, genetic or pharmacological interference with the late PIN3 polarization prevents termination of the response and leads to hypocotyl overbending. This observation reveals a role of auxin feedback on PIN polarity in the termination of the tropic response. © 2016 Elsevier Ltd' acknowledgement: "We thank Dr. Jie Li (Key Laboratory of Plant Molecular Physiology, Chinese Academy of Science, China) for the pPIN3::PIN3-GFP/DII::VENUS line and Martine De Cock for help in preparing the manuscript. This work was supported by the European Research Council (project ERC-2011-StG-20101109-PSDP), by the Czech Science Foundation GAČR (GA13-40637S) to J.F., and by the Ministry of Education, Youth and Sports of the Czech Republic under the project CEITEC 2020 (LQ1601) to H.S.R. H.R. is indebted to the Agency for Innovation by Science and Technology (IWT) for a predoctoral fellowship.\r\n" article_processing_charge: No author: - first_name: Hana full_name: Rakusová, Hana last_name: Rakusová - first_name: Mohamad full_name: Abbas, Mohamad id: 47E8FC1C-F248-11E8-B48F-1D18A9856A87 last_name: Abbas - first_name: Huibin full_name: Han, Huibin id: 31435098-F248-11E8-B48F-1D18A9856A87 last_name: Han - first_name: Siyuan full_name: Song, Siyuan last_name: Song - first_name: Hélène full_name: Robert, Hélène last_name: Robert - first_name: Jirí full_name: Friml, Jirí id: 4159519E-F248-11E8-B48F-1D18A9856A87 last_name: Friml orcid: 0000-0002-8302-7596 citation: ama: Rakusová H, Abbas M, Han H, Song S, Robert H, Friml J. Termination of shoot gravitropic responses by auxin feedback on PIN3 polarity. Current Biology. 2016;26(22):3026-3032. doi:10.1016/j.cub.2016.08.067 apa: Rakusová, H., Abbas, M., Han, H., Song, S., Robert, H., & Friml, J. (2016). Termination of shoot gravitropic responses by auxin feedback on PIN3 polarity. Current Biology. Cell Press. https://doi.org/10.1016/j.cub.2016.08.067 chicago: Rakusová, Hana, Mohamad Abbas, Huibin Han, Siyuan Song, Hélène Robert, and Jiří Friml. “Termination of Shoot Gravitropic Responses by Auxin Feedback on PIN3 Polarity.” Current Biology. Cell Press, 2016. https://doi.org/10.1016/j.cub.2016.08.067. ieee: H. Rakusová, M. Abbas, H. Han, S. Song, H. Robert, and J. Friml, “Termination of shoot gravitropic responses by auxin feedback on PIN3 polarity,” Current Biology, vol. 26, no. 22. Cell Press, pp. 3026–3032, 2016. ista: Rakusová H, Abbas M, Han H, Song S, Robert H, Friml J. 2016. Termination of shoot gravitropic responses by auxin feedback on PIN3 polarity. Current Biology. 26(22), 3026–3032. mla: Rakusová, Hana, et al. “Termination of Shoot Gravitropic Responses by Auxin Feedback on PIN3 Polarity.” Current Biology, vol. 26, no. 22, Cell Press, 2016, pp. 3026–32, doi:10.1016/j.cub.2016.08.067. short: H. Rakusová, M. Abbas, H. Han, S. Song, H. Robert, J. Friml, Current Biology 26 (2016) 3026–3032. date_created: 2018-12-11T11:50:44Z date_published: 2016-11-21T00:00:00Z date_updated: 2026-04-28T08:29:26Z day: '21' ddc: - '581' department: - _id: JiFr doi: 10.1016/j.cub.2016.08.067 ec_funded: 1 external_id: isi: - '000388545900020' file: - access_level: open_access checksum: 79ed2498185a027cf51a8f88100379e6 content_type: application/pdf creator: system date_created: 2018-12-12T10:09:33Z date_updated: 2020-07-14T12:44:39Z file_id: '4757' file_name: IST-2018-1008-v1+1_Rakusova_CurrBiol_2016_proof.pdf file_size: 5391923 relation: main_file file_date_updated: 2020-07-14T12:44:39Z has_accepted_license: '1' intvolume: ' 26' isi: 1 issue: '22' language: - iso: eng month: '11' oa: 1 oa_version: Submitted Version page: 3026 - 3032 project: - _id: 25716A02-B435-11E9-9278-68D0E5697425 call_identifier: FP7 grant_number: '282300' name: Polarity and subcellular dynamics in plants publication: Current Biology publication_status: published publisher: Cell Press publist_id: '6138' pubrep_id: '1008' quality_controlled: '1' scopus_import: '1' status: public title: Termination of shoot gravitropic responses by auxin feedback on PIN3 polarity type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 26 year: '2016' ... --- _id: '1222' abstract: - lang: eng text: We consider packings of congruent circles on a square flat torus, i.e., periodic (w.r.t. a square lattice) planar circle packings, with the maximal circle radius. This problem is interesting due to a practical reason—the problem of “super resolution of images.” We have found optimal arrangements for N=6, 7 and 8 circles. Surprisingly, for the case N=7 there are three different optimal arrangements. Our proof is based on a computer enumeration of toroidal irreducible contact graphs. acknowledgement: We wish to thank Alexey Tarasov, Vladislav Volkov and Brittany Fasy for some useful comments and remarks, and especially Thom Sulanke for modifying surftri to suit our purposes. Oleg R. Musin was partially supported by the NSF Grant DMS-1400876 and by the RFBR Grant 15-01-99563. Anton V. Nikitenko was supported by the Chebyshev Laboratory (Department of Mathematics and Mechanics, St. Petersburg State University) under RF Government Grant 11.G34.31.0026. article_processing_charge: No arxiv: 1 author: - first_name: Oleg full_name: Musin, Oleg last_name: Musin - first_name: Anton full_name: Nikitenko, Anton id: 3E4FF1BA-F248-11E8-B48F-1D18A9856A87 last_name: Nikitenko orcid: 0000-0002-0659-3201 citation: ama: Musin O, Nikitenko A. Optimal packings of congruent circles on a square flat torus. Discrete & Computational Geometry. 2016;55(1):1-20. doi:10.1007/s00454-015-9742-6 apa: Musin, O., & Nikitenko, A. (2016). Optimal packings of congruent circles on a square flat torus. Discrete & Computational Geometry. Springer. https://doi.org/10.1007/s00454-015-9742-6 chicago: Musin, Oleg, and Anton Nikitenko. “Optimal Packings of Congruent Circles on a Square Flat Torus.” Discrete & Computational Geometry. Springer, 2016. https://doi.org/10.1007/s00454-015-9742-6. ieee: O. Musin and A. Nikitenko, “Optimal packings of congruent circles on a square flat torus,” Discrete & Computational Geometry, vol. 55, no. 1. Springer, pp. 1–20, 2016. ista: Musin O, Nikitenko A. 2016. Optimal packings of congruent circles on a square flat torus. Discrete & Computational Geometry. 55(1), 1–20. mla: Musin, Oleg, and Anton Nikitenko. “Optimal Packings of Congruent Circles on a Square Flat Torus.” Discrete & Computational Geometry, vol. 55, no. 1, Springer, 2016, pp. 1–20, doi:10.1007/s00454-015-9742-6. short: O. Musin, A. Nikitenko, Discrete & Computational Geometry 55 (2016) 1–20. date_created: 2018-12-11T11:50:48Z date_published: 2016-01-01T00:00:00Z date_updated: 2025-09-22T09:32:23Z day: '01' department: - _id: HeEd doi: 10.1007/s00454-015-9742-6 external_id: arxiv: - '1212.0649' isi: - '000367625500001' intvolume: ' 55' isi: 1 issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1212.0649 month: '01' oa: 1 oa_version: Preprint page: 1 - 20 publication: Discrete & Computational Geometry publication_status: published publisher: Springer publist_id: '6111' quality_controlled: '1' scopus_import: '1' status: public title: Optimal packings of congruent circles on a square flat torus type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 55 year: '2016' ... --- _id: '12615' abstract: - lang: eng text: 'We apply the process-based, distributed TOPKAPI-ETH glacio-hydrological model to a glacierized catchment (19% glacierized) in the semiarid Andes of central Chile. The semiarid Andes provides vital freshwater resources to valleys in Chile and Argentina, but only few glacio-hydrological modelling studies have been conducted, and its dominant hydrological processes remain poorly understood. The catchment contains two debris-free glaciers reaching down to 3900 m asl (Bello and Yeso glaciers) and one debris-covered avalanche-fed glacier reaching to 3200 m asl (Piramide Glacier). Our main objective is to compare the mass balance and runoff contributions of both glacier types under current climatic conditions. We use a unique dataset of field measurements collected over two ablation seasons combined with the distributed TOPKAPI-ETH model that includes physically oriented parameterizations of snow and ice ablation, gravitational distribution of snow, snow albedo evolution and the ablation of debris-covered ice. Model outputs indicate that while the mass balance of Bello and Yeso glaciers is mostly explained by temperature gradients, the Piramide Glacier mass balance is governed by debris thickness and avalanches and has a clear non-linear profile with elevation as a result. Despite the thermal insulation effect of the debris cover, the mass balance and contribution to runoff from debris-free and debris-covered glaciers are similar in magnitude, mainly because of elevation differences. However, runoff contributions are distinct in time and seasonality with ice melt starting approximately four weeks earlier from the debris-covered glacier, what is of relevance for water resources management. At the catchment scale, snowmelt is the dominant contributor to runoff during both years. However, during the driest year of our simulations, ice melt contributes 42 ± 8% and 67 ± 6% of the annual and summer runoff, respectively. Sensitivity analyses show that runoff is most sensitive to temperature and precipitation gradients, melt factors and debris cover thickness. ' article_processing_charge: No article_type: original author: - first_name: A. full_name: Ayala, A. last_name: Ayala - first_name: Francesca full_name: Pellicciotti, Francesca id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70 last_name: Pellicciotti - first_name: S. full_name: MacDonell, S. last_name: MacDonell - first_name: J. full_name: McPhee, J. last_name: McPhee - first_name: S. full_name: Vivero, S. last_name: Vivero - first_name: C. full_name: Campos, C. last_name: Campos - first_name: P. full_name: Egli, P. last_name: Egli citation: ama: Ayala A, Pellicciotti F, MacDonell S, et al. Modelling the hydrological response of debris-free and debris-covered glaciers to present climatic conditions in the semiarid Andes of central Chile. Hydrological Processes. 2016;30(22):4036-4058. doi:10.1002/hyp.10971 apa: Ayala, A., Pellicciotti, F., MacDonell, S., McPhee, J., Vivero, S., Campos, C., & Egli, P. (2016). Modelling the hydrological response of debris-free and debris-covered glaciers to present climatic conditions in the semiarid Andes of central Chile. Hydrological Processes. Wiley. https://doi.org/10.1002/hyp.10971 chicago: Ayala, A., Francesca Pellicciotti, S. MacDonell, J. McPhee, S. Vivero, C. Campos, and P. Egli. “Modelling the Hydrological Response of Debris-Free and Debris-Covered Glaciers to Present Climatic Conditions in the Semiarid Andes of Central Chile.” Hydrological Processes. Wiley, 2016. https://doi.org/10.1002/hyp.10971. ieee: A. Ayala et al., “Modelling the hydrological response of debris-free and debris-covered glaciers to present climatic conditions in the semiarid Andes of central Chile,” Hydrological Processes, vol. 30, no. 22. Wiley, pp. 4036–4058, 2016. ista: Ayala A, Pellicciotti F, MacDonell S, McPhee J, Vivero S, Campos C, Egli P. 2016. Modelling the hydrological response of debris-free and debris-covered glaciers to present climatic conditions in the semiarid Andes of central Chile. Hydrological Processes. 30(22), 4036–4058. mla: Ayala, A., et al. “Modelling the Hydrological Response of Debris-Free and Debris-Covered Glaciers to Present Climatic Conditions in the Semiarid Andes of Central Chile.” Hydrological Processes, vol. 30, no. 22, Wiley, 2016, pp. 4036–58, doi:10.1002/hyp.10971. short: A. Ayala, F. Pellicciotti, S. MacDonell, J. McPhee, S. Vivero, C. Campos, P. Egli, Hydrological Processes 30 (2016) 4036–4058. date_created: 2023-02-20T08:14:40Z date_published: 2016-07-28T00:00:00Z date_updated: 2023-02-24T11:29:28Z day: '28' doi: 10.1002/hyp.10971 extern: '1' intvolume: ' 30' issue: '22' keyword: - Water Science and Technology language: - iso: eng month: '07' oa_version: None page: 4036-4058 publication: Hydrological Processes publication_identifier: issn: - 0885-6087 publication_status: published publisher: Wiley quality_controlled: '1' scopus_import: '1' status: public title: Modelling the hydrological response of debris-free and debris-covered glaciers to present climatic conditions in the semiarid Andes of central Chile type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 30 year: '2016' ... --- _id: '12617' abstract: - lang: eng text: This study presents volume and mass changes of seven (five partially debris-covered, two debris-free) glaciers in the upper Langtang catchment in Nepal. We use a digital elevation model (DEM) from 1974 stereo Hexagon satellite data and seven DEMs derived from 2006–2015 stereo or tri-stereo satellite imagery (e.g., SPOT6/7). The availability of multiple independent DEM differences allows the identification of a robust signal and narrowing down of the uncertainty about recent volume changes. The volume changes calculated over several multiyear periods between 2006 and 2015 consistently indicate that glacier thinning has accelerated with respect to the period 1974–2006. We calculate an ensemble-mean elevation change rate of –0.45 ± 0.18 m a−1 for 2006–2015, while for the period 1974–2006 we compute a rate of −0.24 ± 0.08 m a−1. However, the behavior of glaciers in the study area is heterogeneous, and the presence or absence of debris does not seem to be a good predictor for mass balance trends. Debris-covered tongues have nonlinear thinning profiles, and we show that recent accelerations in thinning correlate with the presence of supraglacial cliffs and lakes. At stagnating glacier areas near the glacier front, however, thinning rates decreased with time or remained constant. The April 2015 Nepal earthquake triggered large avalanches in the study catchment. Analysis of two post-earthquake DEMs revealed that the avalanche deposit volumes remaining 6 months after the earthquake are negligible in comparison to 2006–2015 elevation changes. However, the deposits compensate about 40 % the mass loss of debris-covered tongues of 1 average year. article_processing_charge: No article_type: original author: - first_name: Silvan full_name: Ragettli, Silvan last_name: Ragettli - first_name: Tobias full_name: Bolch, Tobias last_name: Bolch - first_name: Francesca full_name: Pellicciotti, Francesca id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70 last_name: Pellicciotti citation: ama: Ragettli S, Bolch T, Pellicciotti F. Heterogeneous glacier thinning patterns over the last 40 years in Langtang Himal, Nepal. The Cryosphere. 2016;10(5):2075-2097. doi:10.5194/tc-10-2075-2016 apa: Ragettli, S., Bolch, T., & Pellicciotti, F. (2016). Heterogeneous glacier thinning patterns over the last 40 years in Langtang Himal, Nepal. The Cryosphere. Copernicus Publications. https://doi.org/10.5194/tc-10-2075-2016 chicago: Ragettli, Silvan, Tobias Bolch, and Francesca Pellicciotti. “Heterogeneous Glacier Thinning Patterns over the Last 40 Years in Langtang Himal, Nepal.” The Cryosphere. Copernicus Publications, 2016. https://doi.org/10.5194/tc-10-2075-2016. ieee: S. Ragettli, T. Bolch, and F. Pellicciotti, “Heterogeneous glacier thinning patterns over the last 40 years in Langtang Himal, Nepal,” The Cryosphere, vol. 10, no. 5. Copernicus Publications, pp. 2075–2097, 2016. ista: Ragettli S, Bolch T, Pellicciotti F. 2016. Heterogeneous glacier thinning patterns over the last 40 years in Langtang Himal, Nepal. The Cryosphere. 10(5), 2075–2097. mla: Ragettli, Silvan, et al. “Heterogeneous Glacier Thinning Patterns over the Last 40 Years in Langtang Himal, Nepal.” The Cryosphere, vol. 10, no. 5, Copernicus Publications, 2016, pp. 2075–97, doi:10.5194/tc-10-2075-2016. short: S. Ragettli, T. Bolch, F. Pellicciotti, The Cryosphere 10 (2016) 2075–2097. date_created: 2023-02-20T08:14:51Z date_published: 2016-09-14T00:00:00Z date_updated: 2023-02-24T10:54:02Z day: '14' doi: 10.5194/tc-10-2075-2016 extern: '1' intvolume: ' 10' issue: '5' keyword: - Earth-Surface Processes - Water Science and Technology language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.5194/tc-10-2075-2016 month: '09' oa: 1 oa_version: Published Version page: 2075-2097 publication: The Cryosphere publication_identifier: issn: - 1994-0424 publication_status: published publisher: Copernicus Publications quality_controlled: '1' scopus_import: '1' status: public title: Heterogeneous glacier thinning patterns over the last 40 years in Langtang Himal, Nepal type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 10 year: '2016' ... --- _id: '12625' abstract: - lang: eng text: Debris-covered glaciers play an important role in the high-altitude water cycle in the Himalaya, yet their dynamics are poorly understood, partly because of the difficult fieldwork conditions. In this study we therefore deploy an unmanned aerial vehicle (UAV) three times (May 2013, October 2013 and May 2014) over the debris-covered Lirung Glacier in Nepal. The acquired data are processed into orthomosaics and elevation models by a Structure from Motion workflow, and seasonal surface velocity is derived using frequency cross-correlation. In order to obtain optimal surface velocity products, the effects of different input data and correlator configurations are evaluated, which reveals that the orthomosaic as input paired with moderate correlator settings provides the best results. The glacier has considerable spatial and seasonal differences in surface velocity, with maximum summer and winter velocities 6 and 2.5 m a-1, respectively, in the upper part of the tongue, while the lower part is nearly stagnant. It is hypothesized that the higher velocities during summer are caused by basal sliding due to increased lubrication of the bed. We conclude that UAVs have great potential to quantify seasonal and annual variations in flow and can help to further our understanding of debris-covered glaciers. article_processing_charge: No article_type: original author: - first_name: Philip full_name: Kraaijenbrink, Philip last_name: Kraaijenbrink - first_name: Sander W. full_name: Meijer, Sander W. last_name: Meijer - first_name: Joseph M. full_name: Shea, Joseph M. last_name: Shea - first_name: Francesca full_name: Pellicciotti, Francesca id: b28f055a-81ea-11ed-b70c-a9fe7f7b0e70 last_name: Pellicciotti - first_name: Steven M. full_name: De Jong, Steven M. last_name: De Jong - first_name: Walter W. full_name: Immerzeel, Walter W. last_name: Immerzeel citation: ama: Kraaijenbrink P, Meijer SW, Shea JM, Pellicciotti F, De Jong SM, Immerzeel WW. Seasonal surface velocities of a Himalayan glacier derived by automated correlation of unmanned aerial vehicle imagery. Annals of Glaciology. 2016;57(71):103-113. doi:10.3189/2016aog71a072 apa: Kraaijenbrink, P., Meijer, S. W., Shea, J. M., Pellicciotti, F., De Jong, S. M., & Immerzeel, W. W. (2016). Seasonal surface velocities of a Himalayan glacier derived by automated correlation of unmanned aerial vehicle imagery. Annals of Glaciology. International Glaciological Society. https://doi.org/10.3189/2016aog71a072 chicago: Kraaijenbrink, Philip, Sander W. Meijer, Joseph M. Shea, Francesca Pellicciotti, Steven M. De Jong, and Walter W. Immerzeel. “Seasonal Surface Velocities of a Himalayan Glacier Derived by Automated Correlation of Unmanned Aerial Vehicle Imagery.” Annals of Glaciology. International Glaciological Society, 2016. https://doi.org/10.3189/2016aog71a072. ieee: P. Kraaijenbrink, S. W. Meijer, J. M. Shea, F. Pellicciotti, S. M. De Jong, and W. W. Immerzeel, “Seasonal surface velocities of a Himalayan glacier derived by automated correlation of unmanned aerial vehicle imagery,” Annals of Glaciology, vol. 57, no. 71. International Glaciological Society, pp. 103–113, 2016. ista: Kraaijenbrink P, Meijer SW, Shea JM, Pellicciotti F, De Jong SM, Immerzeel WW. 2016. Seasonal surface velocities of a Himalayan glacier derived by automated correlation of unmanned aerial vehicle imagery. Annals of Glaciology. 57(71), 103–113. mla: Kraaijenbrink, Philip, et al. “Seasonal Surface Velocities of a Himalayan Glacier Derived by Automated Correlation of Unmanned Aerial Vehicle Imagery.” Annals of Glaciology, vol. 57, no. 71, International Glaciological Society, 2016, pp. 103–13, doi:10.3189/2016aog71a072. short: P. Kraaijenbrink, S.W. Meijer, J.M. Shea, F. Pellicciotti, S.M. De Jong, W.W. Immerzeel, Annals of Glaciology 57 (2016) 103–113. date_created: 2023-02-20T08:15:56Z date_published: 2016-03-01T00:00:00Z date_updated: 2023-02-24T10:11:46Z day: '01' doi: 10.3189/2016aog71a072 extern: '1' intvolume: ' 57' issue: '71' keyword: - Earth-Surface Processes language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3189/2016AoG71A072 month: '03' oa: 1 oa_version: Published Version page: 103-113 publication: Annals of Glaciology publication_identifier: eissn: - 1727-5644 issn: - 0260-3055 publication_status: published publisher: International Glaciological Society quality_controlled: '1' scopus_import: '1' status: public title: Seasonal surface velocities of a Himalayan glacier derived by automated correlation of unmanned aerial vehicle imagery type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 57 year: '2016' ... --- _id: '1331' abstract: - lang: eng text: 'Cytokinin is a phytohormone that is well known for its roles in numerous plant growth and developmental processes, yet it has also been linked to abiotic stress response in a less defined manner. Arabidopsis (Arabidopsis thaliana) Cytokinin Response Factor 6 (CRF6) is a cytokinin-responsive AP2/ERF-family transcription factor that, through the cytokinin signaling pathway, plays a key role in the inhibition of dark-induced senescence. CRF6 expression is also induced by oxidative stress, and here we show a novel function for CRF6 in relation to oxidative stress and identify downstream transcriptional targets of CRF6 that are repressed in response to oxidative stress. Analysis of transcriptomic changes in wild-type and crf6 mutant plants treated with H2O2 identified CRF6-dependent differentially expressed transcripts, many of which were repressed rather than induced. Moreover, many repressed genes also show decreased expression in 35S:CRF6 overexpressing plants. Together, these findings suggest that CRF6 functions largely as a transcriptional repressor. Interestingly, among the H2O2 repressed CRF6-dependent transcripts was a set of five genes associated with cytokinin processes: (signaling) ARR6, ARR9, ARR11, (biosynthesis) LOG7, and (transport) ABCG14. We have examined mutants of these cytokinin-associated target genes to reveal novel connections to oxidative stress. Further examination of CRF6-DNA interactions indicated that CRF6 may regulate its targets both directly and indirectly. Together, this shows that CRF6 functions during oxidative stress as a negative regulator to control this cytokinin-associated module of CRF6- dependent genes and establishes a novel connection between cytokinin and oxidative stress response.' acknowledgement: "This work was financially supported by the following: The Alabama Agricultural Experiment Station HATCH grants 370222-310010-2055 and 370225-310006-2055 for funding to P.J.Z., E.A.K, A.M.P., and A.M.R. P.J.Z. and E.A.K were supported by an Auburn University Cellular and Molecular Biosciences Research Fellowship. I.D.C. is a postdoctoral fellow of the Research Foundation Flanders (FWO) (FWO/PDO14/043) and is also supported by FWO travel\r\ngrant 12N2415N. F.V.B. was supported by grants from the Interuniversity Attraction Poles Programme (IUAP P7/29 MARS) initiated by the Belgian Science Policy Office and Ghent University (Multidisciplinary Research Partnership Biotechnology for a Sustainable Economy, grant 01MRB510W)." article_processing_charge: No article_type: original author: - first_name: Paul full_name: Zwack, Paul last_name: Zwack - first_name: Inge full_name: De Clercq, Inge last_name: De Clercq - first_name: Timothy full_name: Howton, Timothy last_name: Howton - first_name: H Tucker full_name: Hallmark, H Tucker last_name: Hallmark - first_name: Andrej full_name: Hurny, Andrej id: 4DC4AF46-F248-11E8-B48F-1D18A9856A87 last_name: Hurny orcid: 0000-0003-3638-1426 - first_name: Erika full_name: Keshishian, Erika last_name: Keshishian - first_name: Alyssa full_name: Parish, Alyssa last_name: Parish - first_name: Eva full_name: Benková, Eva id: 38F4F166-F248-11E8-B48F-1D18A9856A87 last_name: Benková orcid: 0000-0002-8510-9739 - first_name: M Shahid full_name: Mukhtar, M Shahid last_name: Mukhtar - first_name: Frank full_name: Van Breusegem, Frank last_name: Van Breusegem - first_name: Aaron full_name: Rashotte, Aaron last_name: Rashotte citation: ama: Zwack P, De Clercq I, Howton T, et al. Cytokinin response factor 6 represses cytokinin-associated genes during oxidative stress. Plant Physiology. 2016;172(2):1249-1258. doi:10.1104/pp.16.00415 apa: Zwack, P., De Clercq, I., Howton, T., Hallmark, H. T., Hurny, A., Keshishian, E., … Rashotte, A. (2016). Cytokinin response factor 6 represses cytokinin-associated genes during oxidative stress. Plant Physiology. American Society of Plant Biologists. https://doi.org/10.1104/pp.16.00415 chicago: Zwack, Paul, Inge De Clercq, Timothy Howton, H Tucker Hallmark, Andrej Hurny, Erika Keshishian, Alyssa Parish, et al. “Cytokinin Response Factor 6 Represses Cytokinin-Associated Genes during Oxidative Stress.” Plant Physiology. American Society of Plant Biologists, 2016. https://doi.org/10.1104/pp.16.00415. ieee: P. Zwack et al., “Cytokinin response factor 6 represses cytokinin-associated genes during oxidative stress,” Plant Physiology, vol. 172, no. 2. American Society of Plant Biologists, pp. 1249–1258, 2016. ista: Zwack P, De Clercq I, Howton T, Hallmark HT, Hurny A, Keshishian E, Parish A, Benková E, Mukhtar MS, Van Breusegem F, Rashotte A. 2016. Cytokinin response factor 6 represses cytokinin-associated genes during oxidative stress. Plant Physiology. 172(2), 1249–1258. mla: Zwack, Paul, et al. “Cytokinin Response Factor 6 Represses Cytokinin-Associated Genes during Oxidative Stress.” Plant Physiology, vol. 172, no. 2, American Society of Plant Biologists, 2016, pp. 1249–58, doi:10.1104/pp.16.00415. short: P. Zwack, I. De Clercq, T. Howton, H.T. Hallmark, A. Hurny, E. Keshishian, A. Parish, E. Benková, M.S. Mukhtar, F. Van Breusegem, A. Rashotte, Plant Physiology 172 (2016) 1249–1258. date_created: 2018-12-11T11:51:25Z date_published: 2016-10-02T00:00:00Z date_updated: 2026-06-18T17:30:26Z day: '02' ddc: - '580' department: - _id: EvBe doi: 10.1104/pp.16.00415 external_id: isi: - '000391147700047' intvolume: ' 172' isi: 1 issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1104/pp.16.00415 month: '10' oa: 1 oa_version: Published Version page: 1249 - 1258 publication: Plant Physiology publication_identifier: eissn: - 1532-2548 issn: - 0032-0889 publication_status: published publisher: American Society of Plant Biologists publist_id: '5937' quality_controlled: '1' scopus_import: '1' status: public title: Cytokinin response factor 6 represses cytokinin-associated genes during oxidative stress type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 172 year: '2016' ... --- _id: '1522' abstract: - lang: eng text: 'We classify smooth Brunnian (i.e., unknotted on both components) embeddings (S2 × S1) ⊔ S3 → ℝ6. Any Brunnian embedding (S2 × S1) ⊔ S3 → ℝ6 is isotopic to an explicitly constructed embedding fk,m,n for some integers k, m, n such that m ≡ n (mod 2). Two embeddings fk,m,n and fk′ ,m′,n′ are isotopic if and only if k = k′, m ≡ m′ (mod 2k) and n ≡ n′ (mod 2k). We use Haefliger’s classification of embeddings S3 ⊔ S3 → ℝ6 in our proof. The relation between the embeddings (S2 × S1) ⊔ S3 → ℝ6 and S3 ⊔ S3 → ℝ6 is not trivial, however. For example, we show that there exist embeddings f: (S2 ×S1) ⊔ S3 → ℝ6 and g, g′ : S3 ⊔ S3 → ℝ6 such that the componentwise embedded connected sum f # g is isotopic to f # g′ but g is not isotopic to g′.' acknowledgement: "I thank A. Skopenkov for telling me about the problem and for his useful remarks. I also thank A. Sossinsky,\r\nA. Zhubr, M. Skopenkov, P. Akhmetiev, and an anonymous referee for their feedback. Author was partially\r\nsupported by Dobrushin fellowship, 2013, and by RFBR grant 15-01-06302." article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Serhii full_name: Avvakumov, Serhii id: 3827DAC8-F248-11E8-B48F-1D18A9856A87 last_name: Avvakumov citation: ama: Avvakumov S. The classification of certain linked 3-manifolds in 6-space. Moscow Mathematical Journal. 2016;16(1):1-25. doi:10.17323/1609-4514-2016-16-1-1-25 apa: Avvakumov, S. (2016). The classification of certain linked 3-manifolds in 6-space. Moscow Mathematical Journal. Independent University of Moscow. https://doi.org/10.17323/1609-4514-2016-16-1-1-25 chicago: Avvakumov, Sergey. “The Classification of Certain Linked 3-Manifolds in 6-Space.” Moscow Mathematical Journal. Independent University of Moscow, 2016. https://doi.org/10.17323/1609-4514-2016-16-1-1-25. ieee: S. Avvakumov, “The classification of certain linked 3-manifolds in 6-space,” Moscow Mathematical Journal, vol. 16, no. 1. Independent University of Moscow, pp. 1–25, 2016. ista: Avvakumov S. 2016. The classification of certain linked 3-manifolds in 6-space. Moscow Mathematical Journal. 16(1), 1–25. mla: Avvakumov, Sergey. “The Classification of Certain Linked 3-Manifolds in 6-Space.” Moscow Mathematical Journal, vol. 16, no. 1, Independent University of Moscow, 2016, pp. 1–25, doi:10.17323/1609-4514-2016-16-1-1-25. short: S. Avvakumov, Moscow Mathematical Journal 16 (2016) 1–25. corr_author: '1' date_created: 2018-12-11T11:52:30Z date_published: 2016-01-01T00:00:00Z date_updated: 2024-10-09T20:56:44Z day: '01' department: - _id: UlWa doi: 10.17323/1609-4514-2016-16-1-1-25 external_id: arxiv: - '1408.3918' intvolume: ' 16' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: http://arxiv.org/abs/1408.3918 month: '01' oa: 1 oa_version: Preprint page: 1 - 25 publication: Moscow Mathematical Journal publication_identifier: eissn: - 1609-4514 publication_status: published publisher: Independent University of Moscow publist_id: '5652' quality_controlled: '1' scopus_import: '1' status: public title: The classification of certain linked 3-manifolds in 6-space type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 16 year: '2016' ... --- _id: '15245' abstract: - lang: eng text: 'eXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary goals are the determination of the equation of state of matter at supra-nuclear density, the measurement of QED effects in highly magnetized star, and the study of accretion in the strong-field regime of gravity. Primary targets include isolated and binary neutron stars, strong magnetic field systems like magnetars, and stellar-mass and supermassive black holes. The mission carries a unique and unprecedented suite of state-of-the-art scientific instruments enabling for the first time ever the simultaneous spectral-timing-polarimetry studies of cosmic sources in the energy range from 0.5-30 keV (and beyond). Key elements of the payload are: the Spectroscopic Focusing Array (SFA) - a set of 11 X-ray optics for a total effective area of ∼0.9 m2 and 0.6 m2 at 2 keV and 6 keV respectively, equipped with Silicon Drift Detectors offering <180 eV spectral resolution; the Large Area Detector (LAD) - a deployable set of 640 Silicon Drift Detectors, for a total effective area of ∼3.4 m2, between 6 and 10 keV, and spectral resolution better than 250 eV; the Polarimetry Focusing Array (PFA) - a set of 2 X-ray telescope, for a total effective area of 250 cm2 at 2 keV, equipped with imaging gas pixel photoelectric polarimeters; the Wide Field Monitor (WFM) - a set of 3 coded mask wide field units, equipped with position-sensitive Silicon Drift Detectors, each covering a 90 degrees x 90 degrees field of view. The eXTP international consortium includes major institutions of the Chinese Academy of Sciences and Universities in China, as well as major institutions in several European countries and the United States. The predecessor of eXTP, the XTP mission concept, has been selected and funded as one of the so-called background missions in the Strategic Priority Space Science Program of the Chinese Academy of Sciences since 2011. The strong European participation has significantly enhanced the scientific capabilities of eXTP. The planned launch date of the mission is earlier than 2025.' article_number: '99051Q ' article_processing_charge: No arxiv: 1 author: - first_name: S. N. full_name: Zhang, S. N. last_name: Zhang - first_name: M. full_name: Feroci, M. last_name: Feroci - first_name: A. full_name: Santangelo, A. last_name: Santangelo - first_name: Y. W. full_name: Dong, Y. W. last_name: Dong - first_name: H. full_name: Feng, H. last_name: Feng - first_name: F. J. full_name: Lu, F. J. last_name: Lu - first_name: K. full_name: Nandra, K. last_name: Nandra - first_name: Z. S. full_name: Wang, Z. S. last_name: Wang - first_name: S. full_name: Zhang, S. last_name: Zhang - first_name: E. full_name: Bozzo, E. last_name: Bozzo - first_name: S. full_name: Brandt, S. last_name: Brandt - first_name: A. full_name: De Rosa, A. last_name: De Rosa - first_name: L. J. full_name: Gou, L. J. last_name: Gou - first_name: M. full_name: Hernanz, M. last_name: Hernanz - first_name: M. full_name: van der Klis, M. last_name: van der Klis - first_name: X. D. full_name: Li, X. D. last_name: Li - first_name: Y. full_name: Liu, Y. last_name: Liu - first_name: P. full_name: Orleanski, P. last_name: Orleanski - first_name: G. full_name: Pareschi, G. last_name: Pareschi - first_name: M. full_name: Pohl, M. last_name: Pohl - first_name: J. full_name: Poutanen, J. last_name: Poutanen - first_name: J. L. full_name: Qu, J. 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S. last_name: Weng - first_name: J. full_name: Wilms, J. last_name: Wilms - first_name: B. full_name: Winter, B. last_name: Winter - first_name: X. full_name: Wu, X. last_name: Wu - first_name: X. F. full_name: Wu, X. F. last_name: Wu - first_name: S. L. full_name: Xiong, S. L. last_name: Xiong - first_name: Y. P. full_name: Xu, Y. P. last_name: Xu - first_name: Y. Q. full_name: Xue, Y. Q. last_name: Xue - first_name: Z. full_name: Yan, Z. last_name: Yan - first_name: S. full_name: Yang, S. last_name: Yang - first_name: X. full_name: Yang, X. last_name: Yang - first_name: Y. J. full_name: Yang, Y. J. last_name: Yang - first_name: F. full_name: Yuan, F. last_name: Yuan - first_name: W. M. full_name: Yuan, W. M. last_name: Yuan - first_name: Y. F. full_name: Yuan, Y. F. last_name: Yuan - first_name: G. full_name: Zampa, G. last_name: Zampa - first_name: N. full_name: Zampa, N. last_name: Zampa - first_name: A. full_name: Zdziarski, A. last_name: Zdziarski - first_name: C. full_name: Zhang, C. last_name: Zhang - first_name: C. L. full_name: Zhang, C. L. last_name: Zhang - first_name: L. full_name: Zhang, L. last_name: Zhang - first_name: X. full_name: Zhang, X. last_name: Zhang - first_name: Z. full_name: Zhang, Z. last_name: Zhang - first_name: W. D. full_name: Zhang, W. D. last_name: Zhang - first_name: S. J. full_name: Zheng, S. J. last_name: Zheng - first_name: P. full_name: Zhou, P. last_name: Zhou - first_name: X. L. full_name: Zhou, X. L. last_name: Zhou citation: ama: 'Zhang SN, Feroci M, Santangelo A, et al. eXTP: Enhanced X-ray timing and polarization mission. In: Proceedings of the SPIE. Vol 9905. SPIE; 2016. doi:10.1117/12.2232034' apa: 'Zhang, S. N., Feroci, M., Santangelo, A., Dong, Y. W., Feng, H., Lu, F. J., … Zhou, X. L. (2016). eXTP: Enhanced X-ray timing and polarization mission. In Proceedings of the SPIE (Vol. 9905). SPIE. https://doi.org/10.1117/12.2232034' chicago: 'Zhang, S. N., M. Feroci, A. Santangelo, Y. W. Dong, H. Feng, F. J. Lu, K. Nandra, et al. “EXTP: Enhanced X-Ray Timing and Polarization Mission.” In Proceedings of the SPIE, Vol. 9905. SPIE, 2016. https://doi.org/10.1117/12.2232034.' ieee: 'S. N. Zhang et al., “eXTP: Enhanced X-ray timing and polarization mission,” in Proceedings of the SPIE, 2016, vol. 9905.' ista: 'Zhang SN et al. 2016. eXTP: Enhanced X-ray timing and polarization mission. Proceedings of the SPIE. vol. 9905, 99051Q.' mla: 'Zhang, S. N., et al. “EXTP: Enhanced X-Ray Timing and Polarization Mission.” Proceedings of the SPIE, vol. 9905, 99051Q, SPIE, 2016, doi:10.1117/12.2232034.' short: S.N. Zhang, M. Feroci, A. Santangelo, Y.W. Dong, H. Feng, F.J. Lu, K. Nandra, Z.S. Wang, S. Zhang, E. Bozzo, S. Brandt, A. De Rosa, L.J. Gou, M. Hernanz, M. van der Klis, X.D. Li, Y. Liu, P. Orleanski, G. Pareschi, M. Pohl, J. Poutanen, J.L. Qu, S. Schanne, L. Stella, P. Uttley, A. Watts, R.X. Xu, W.F. Yu, J.J.M. in ’t Zand, S. Zane, L. Alvarez, L. Amati, L. Baldini, C. Bambi, S. Basso, S. Bhattacharyya, R. Bellazzini, T. Belloni, P. Bellutti, S. Bianchi, A. Brez, M. Bursa, V. Burwitz, C. Budtz-Jørgensen, I. Caiazzo, R. Campana, X.L. Cao, P. Casella, C.Y. Chen, L. Chen, T. Chen, Y. Chen, Y. Chen, Y.P. Chen, M. Civitani, F. Coti Zelati, W. Cui, W.W. Cui, Z.G. Dai, E. Del Monte, D. de Martino, S. Di Cosimo, S. Diebold, M. Dovciak, I. Donnarumma, V. Doroshenko, P. Esposito, Y. Evangelista, Y. Favre, P. Friedrich, F. Fuschino, J.L. Galvez, Z.L. Gao, M.Y. Ge, O. Gevin, D. Goetz, D.W. Han, J. Heyl, J. Horak, W. Hu, F. Huang, Q.S. Huang, R. Hudec, D. Huppenkothen, G.L. Israel, A. Ingram, V. Karas, D. Karelin, P.A. Jenke, L. Ji, S. Korpela, D. Kunneriath, C. Labanti, G. Li, X. Li, Z.S. Li, E.W. Liang, O. Limousin, L. Lin, Z.X. Ling, H.B. Liu, H.W. Liu, Z. Liu, B. Lu, N. Lund, D. Lai, B. Luo, T. Luo, B. Ma, S. Mahmoodifar, M. Marisaldi, A. Martindale, N. Meidinger, Y.P. Men, M. Michalska, R. Mignani, M. Minuti, S. Motta, F. Muleri, J. Neilsen, M. Orlandini, A.T. Pan, A. Patruno, E. Perinati, A. Picciotto, C. Piemonte, M. Pinchera, A. Rachevski, M. Rapisarda, N. Rea, E.M.R. Rossi, A. Rubini, G. Sala, X.W. Shu, C. Sgro, Z.X. Shen, P. Soffitta, L.M. Song, G. Spandre, G. Stratta, T.E. Strohmayer, L. Sun, J. Svoboda, G. Tagliaferri, C. Tenzer, T. Hong, R. Taverna, G. Torok, R. Turolla, S. Vacchi, J. Wang, D. Walton, K. Wang, J.F. Wang, R.J. Wang, Y.F. Wang, S.S. Weng, J. Wilms, B. Winter, X. Wu, X.F. Wu, S.L. Xiong, Y.P. Xu, Y.Q. Xue, Z. Yan, S. Yang, X. Yang, Y.J. Yang, F. Yuan, W.M. Yuan, Y.F. Yuan, G. Zampa, N. Zampa, A. Zdziarski, C. Zhang, C.L. Zhang, L. Zhang, X. Zhang, Z. Zhang, W.D. Zhang, S.J. Zheng, P. Zhou, X.L. Zhou, in:, Proceedings of the SPIE, SPIE, 2016. date_created: 2024-03-26T10:42:21Z date_published: 2016-07-01T00:00:00Z date_updated: 2024-03-27T08:23:11Z day: '01' doi: 10.1117/12.2232034 extern: '1' external_id: arxiv: - '1607.08823' intvolume: ' 9905' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.1607.08823 month: '07' oa: 1 oa_version: Preprint publication: Proceedings of the SPIE publication_identifier: issn: - 0277-786X publication_status: published publisher: SPIE quality_controlled: '1' scopus_import: '1' status: public title: 'eXTP: Enhanced X-ray timing and polarization mission' type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 9905 year: '2016' ... --- _id: '1616' abstract: - lang: eng text: The hippocampus plays a key role in learning and memory. Previous studies suggested that the main types of principal neurons, dentate gyrus granule cells (GCs), CA3 pyramidal neurons, and CA1 pyramidal neurons, differ in their activity pattern, with sparse firing in GCs and more frequent firing in CA3 and CA1 pyramidal neurons. It has been assumed but never shown that such different activity may be caused by differential synaptic excitation. To test this hypothesis, we performed high-resolution whole-cell patch-clamp recordings in anesthetized rats in vivo. In contrast to previous in vitro data, both CA3 and CA1 pyramidal neurons fired action potentials spontaneously, with a frequency of ∼3–6 Hz, whereas GCs were silent. Furthermore, both CA3 and CA1 cells primarily fired in bursts. To determine the underlying mechanisms, we quantitatively assessed the frequency of spontaneous excitatory synaptic input, the passive membrane properties, and the active membrane characteristics. Surprisingly, GCs showed comparable synaptic excitation to CA3 and CA1 cells and the highest ratio of excitation versus hyperpolarizing inhibition. Thus, differential synaptic excitation is not responsible for differences in firing. Moreover, the three types of hippocampal neurons markedly differed in their passive properties. While GCs showed the most negative membrane potential, CA3 pyramidal neurons had the highest input resistance and the slowest membrane time constant. The three types of neurons also differed in the active membrane characteristics. GCs showed the highest action potential threshold, but displayed the largest gain of the input-output curves. In conclusion, our results reveal that differential firing of the three main types of hippocampal principal neurons in vivo is not primarily caused by differences in the characteristics of the synaptic input, but by the distinct properties of synaptic integration and input-output transformation. acknowledgement: "The authors thank Jose Guzman for critically reading prior versions of the manuscript. They also thank T. Asenov for\r\nengineering mechanical devices, A. Schlögl for efficient pro-gramming, F. Marr for technical assistance, and E. Kramberger for manuscript editing." article_processing_charge: No author: - first_name: Janina full_name: Kowalski, Janina id: 3F3CA136-F248-11E8-B48F-1D18A9856A87 last_name: Kowalski - first_name: Jian full_name: Gan, Jian id: 3614E438-F248-11E8-B48F-1D18A9856A87 last_name: Gan - first_name: Peter M full_name: Jonas, Peter M id: 353C1B58-F248-11E8-B48F-1D18A9856A87 last_name: Jonas orcid: 0000-0001-5001-4804 - first_name: Alejandro full_name: Pernia-Andrade, Alejandro id: 36963E98-F248-11E8-B48F-1D18A9856A87 last_name: Pernia-Andrade citation: ama: Kowalski J, Gan J, Jonas PM, Pernia-Andrade A. Intrinsic membrane properties determine hippocampal differential firing pattern in vivo in anesthetized rats. Hippocampus. 2016;26(5):668-682. doi:10.1002/hipo.22550 apa: Kowalski, J., Gan, J., Jonas, P. M., & Pernia-Andrade, A. (2016). Intrinsic membrane properties determine hippocampal differential firing pattern in vivo in anesthetized rats. Hippocampus. Wiley. https://doi.org/10.1002/hipo.22550 chicago: Kowalski, Janina, Jian Gan, Peter M Jonas, and Alejandro Pernia-Andrade. “Intrinsic Membrane Properties Determine Hippocampal Differential Firing Pattern in Vivo in Anesthetized Rats.” Hippocampus. Wiley, 2016. https://doi.org/10.1002/hipo.22550. ieee: J. Kowalski, J. Gan, P. M. Jonas, and A. Pernia-Andrade, “Intrinsic membrane properties determine hippocampal differential firing pattern in vivo in anesthetized rats,” Hippocampus, vol. 26, no. 5. Wiley, pp. 668–682, 2016. ista: Kowalski J, Gan J, Jonas PM, Pernia-Andrade A. 2016. Intrinsic membrane properties determine hippocampal differential firing pattern in vivo in anesthetized rats. Hippocampus. 26(5), 668–682. mla: Kowalski, Janina, et al. “Intrinsic Membrane Properties Determine Hippocampal Differential Firing Pattern in Vivo in Anesthetized Rats.” Hippocampus, vol. 26, no. 5, Wiley, 2016, pp. 668–82, doi:10.1002/hipo.22550. short: J. Kowalski, J. Gan, P.M. Jonas, A. Pernia-Andrade, Hippocampus 26 (2016) 668–682. corr_author: '1' date_created: 2018-12-11T11:53:03Z date_published: 2016-05-01T00:00:00Z date_updated: 2025-09-18T10:58:31Z day: '01' ddc: - '570' department: - _id: PeJo doi: 10.1002/hipo.22550 external_id: isi: - '000374666700011' file: - access_level: open_access checksum: 284b72b12fbe15474833ed3d4549f86b content_type: application/pdf creator: system date_created: 2018-12-12T10:13:47Z date_updated: 2020-07-14T12:45:07Z file_id: '5033' file_name: IST-2016-469-v1+1_Kowalski_et_al-Hippocampus.pdf file_size: 905348 relation: main_file file_date_updated: 2020-07-14T12:45:07Z has_accepted_license: '1' intvolume: ' 26' isi: 1 issue: '5' language: - iso: eng license: https://creativecommons.org/licenses/by-nc-nd/4.0/ month: '05' oa: 1 oa_version: Published Version page: 668 - 682 publication: Hippocampus publication_identifier: eissn: - 1098-1063 issn: - 1050-9631 publication_status: published publisher: Wiley publist_id: '5550' pubrep_id: '469' quality_controlled: '1' scopus_import: '1' status: public title: Intrinsic membrane properties determine hippocampal differential firing pattern in vivo in anesthetized rats tmp: image: /images/cc_by_nc_nd.png legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) short: CC BY-NC-ND (4.0) type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 26 year: '2016' ... --- _id: '482' abstract: - lang: eng text: Nonlinear electro-optical conversion of microwave radiation into the optical telecommunication band is achieved within a crystalline whispering gallery mode resonator, reaching 0.1% photon number conversion efficiency with MHz bandwidth. alternative_title: - Optics InfoBase Conference Papers article_processing_charge: No author: - first_name: Alfredo full_name: Rueda, Alfredo last_name: Rueda - first_name: Florian full_name: Sedlmeir, Florian last_name: Sedlmeir - first_name: Michele full_name: Collodo, Michele last_name: Collodo - first_name: Ulrich full_name: Vogl, Ulrich last_name: Vogl - first_name: Birgit full_name: Stiller, Birgit last_name: Stiller - first_name: Gerhard full_name: Schunk, Gerhard last_name: Schunk - first_name: Dmitry full_name: Strekalov, Dmitry last_name: Strekalov - first_name: Christoph full_name: Marquardt, Christoph last_name: Marquardt - first_name: Johannes M full_name: Fink, Johannes M id: 4B591CBA-F248-11E8-B48F-1D18A9856A87 last_name: Fink orcid: 0000-0001-8112-028X - first_name: Oskar full_name: Painter, Oskar last_name: Painter - first_name: Gerd full_name: Leuchs, Gerd last_name: Leuchs - first_name: Harald full_name: Schwefel, Harald last_name: Schwefel citation: ama: 'Rueda A, Sedlmeir F, Collodo M, et al. Nonlinear single sideband microwave to optical conversion using an electro-optic WGM-resonator. In: Optica Publishing Group; 2016. doi:10.1364/NP.2016.NTh3A.6' apa: 'Rueda, A., Sedlmeir, F., Collodo, M., Vogl, U., Stiller, B., Schunk, G., … Schwefel, H. (2016). Nonlinear single sideband microwave to optical conversion using an electro-optic WGM-resonator. Presented at the NP: Nonlinear Photonics, Sydney, Australia: Optica Publishing Group. https://doi.org/10.1364/NP.2016.NTh3A.6' chicago: Rueda, Alfredo, Florian Sedlmeir, Michele Collodo, Ulrich Vogl, Birgit Stiller, Gerhard Schunk, Dmitry Strekalov, et al. “Nonlinear Single Sideband Microwave to Optical Conversion Using an Electro-Optic WGM-Resonator.” Optica Publishing Group, 2016. https://doi.org/10.1364/NP.2016.NTh3A.6. ieee: 'A. Rueda et al., “Nonlinear single sideband microwave to optical conversion using an electro-optic WGM-resonator,” presented at the NP: Nonlinear Photonics, Sydney, Australia, 2016.' ista: 'Rueda A, Sedlmeir F, Collodo M, Vogl U, Stiller B, Schunk G, Strekalov D, Marquardt C, Fink JM, Painter O, Leuchs G, Schwefel H. 2016. Nonlinear single sideband microwave to optical conversion using an electro-optic WGM-resonator. NP: Nonlinear Photonics, Optics InfoBase Conference Papers, .' mla: Rueda, Alfredo, et al. Nonlinear Single Sideband Microwave to Optical Conversion Using an Electro-Optic WGM-Resonator. Optica Publishing Group, 2016, doi:10.1364/NP.2016.NTh3A.6. short: A. Rueda, F. Sedlmeir, M. Collodo, U. Vogl, B. Stiller, G. Schunk, D. Strekalov, C. Marquardt, J.M. Fink, O. Painter, G. Leuchs, H. Schwefel, in:, Optica Publishing Group, 2016. conference: end_date: 2016-09-08 location: Sydney, Australia name: 'NP: Nonlinear Photonics' start_date: 2016-09-05 date_created: 2018-12-11T11:46:43Z date_published: 2016-08-29T00:00:00Z date_updated: 2023-10-17T12:16:43Z day: '29' department: - _id: JoFi doi: 10.1364/NP.2016.NTh3A.6 language: - iso: eng month: '08' oa_version: None publication_status: published publisher: Optica Publishing Group publist_id: '7339' quality_controlled: '1' scopus_import: '1' status: public title: Nonlinear single sideband microwave to optical conversion using an electro-optic WGM-resonator type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2016' ... --- _id: '5551' abstract: - lang: eng text: "Data from array experiments investigating pollinator behaviour on snapdragons in controlled conditions, and their effect on plant mating. Data were collected as part of Tom Ellis' PhD thesis , submitted February 2016.\r\n\r\nWe placed a total of 36 plants in a grid inside a closed organza tent, with a single hive of commercially bred bumblebees (Bombus hortorum). We used only the yellow-flowered Antirrhinum majus striatum and the magenta-flowered Antirrhinum majus pseudomajus, at ratios of 6:36, 12:24, 18:18, 24:12 and 30:6.\r\n\r\nAfter 24 hours to learn how to deal with snapdragons, I observed pollinators foraging on plants, and recorded the transitions between plants. Thereafter seeds on plants were allowed to develops. A sample of these were grown to maturity when their flower colour could be determined, and they were scored as yellow, magenta, or hybrid." article_processing_charge: No author: - first_name: Thomas full_name: Ellis, Thomas id: 3153D6D4-F248-11E8-B48F-1D18A9856A87 last_name: Ellis orcid: 0000-0002-8511-0254 citation: ama: Ellis T. Data on pollinator observations and offpsring phenotypes. 2016. doi:10.15479/AT:ISTA:35 apa: Ellis, T. (2016). Data on pollinator observations and offpsring phenotypes. Institute of Science and Technology Austria. https://doi.org/10.15479/AT:ISTA:35 chicago: Ellis, Thomas. “Data on Pollinator Observations and Offpsring Phenotypes.” Institute of Science and Technology Austria, 2016. https://doi.org/10.15479/AT:ISTA:35. ieee: T. Ellis, “Data on pollinator observations and offpsring phenotypes.” Institute of Science and Technology Austria, 2016. ista: Ellis T. 2016. Data on pollinator observations and offpsring phenotypes, Institute of Science and Technology Austria, 10.15479/AT:ISTA:35. mla: Ellis, Thomas. Data on Pollinator Observations and Offpsring Phenotypes. Institute of Science and Technology Austria, 2016, doi:10.15479/AT:ISTA:35. short: T. Ellis, (2016). contributor: - first_name: David id: 419049E2-F248-11E8-B48F-1D18A9856A87 last_name: Field - first_name: Nicholas H id: 4880FE40-F248-11E8-B48F-1D18A9856A87 last_name: Barton orcid: 0000-0002-8548-5240 datarep_id: '35' date_created: 2018-12-12T12:31:29Z date_published: 2016-02-19T00:00:00Z date_updated: 2026-04-09T10:52:07Z day: '19' department: - _id: NiBa doi: 10.15479/AT:ISTA:35 file: - access_level: open_access checksum: aa3eb85d52b110cd192aa23147c4d4f3 content_type: application/zip creator: system date_created: 2018-12-12T13:05:12Z date_updated: 2020-07-14T12:47:01Z file_id: '5640' file_name: IST-2016-35-v1+1_array_data.zip file_size: 32775 relation: main_file file_date_updated: 2020-07-14T12:47:01Z has_accepted_license: '1' license: https://creativecommons.org/publicdomain/zero/1.0/ month: '02' oa: 1 oa_version: Published Version publisher: Institute of Science and Technology Austria related_material: record: - id: '1398' relation: part_of_dissertation status: public status: public title: Data on pollinator observations and offpsring phenotypes tmp: image: /images/cc_0.png legal_code_url: https://creativecommons.org/publicdomain/zero/1.0/legalcode name: Creative Commons Public Domain Dedication (CC0 1.0) short: CC0 (1.0) type: research_data user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2016' ... --- _id: '5557' abstract: - lang: eng text: "Small synthetic discrete tomography problems.\r\nSizes are 32x32, 64z64 and 256x256.\r\nProjection angles are 2, 4, and 6.\r\nNumber of labels are 3 and 5." article_processing_charge: No author: - first_name: Paul full_name: Swoboda, Paul id: 446560C6-F248-11E8-B48F-1D18A9856A87 last_name: Swoboda citation: ama: Swoboda P. Synthetic discrete tomography problems. 2016. doi:10.15479/AT:ISTA:46 apa: Swoboda, P. (2016). Synthetic discrete tomography problems. Institute of Science and Technology Austria. https://doi.org/10.15479/AT:ISTA:46 chicago: Swoboda, Paul. “Synthetic Discrete Tomography Problems.” Institute of Science and Technology Austria, 2016. https://doi.org/10.15479/AT:ISTA:46. ieee: P. Swoboda, “Synthetic discrete tomography problems.” Institute of Science and Technology Austria, 2016. ista: Swoboda P. 2016. Synthetic discrete tomography problems, Institute of Science and Technology Austria, 10.15479/AT:ISTA:46. mla: Swoboda, Paul. Synthetic Discrete Tomography Problems. Institute of Science and Technology Austria, 2016, doi:10.15479/AT:ISTA:46. short: P. Swoboda, (2016). contributor: - contributor_type: data_collector first_name: Jan last_name: Kuske datarep_id: '46' date_created: 2018-12-12T12:31:31Z date_published: 2016-09-20T00:00:00Z date_updated: 2024-02-21T13:50:21Z day: '20' ddc: - '006' department: - _id: VlKo doi: 10.15479/AT:ISTA:46 file: - access_level: open_access checksum: aa5a16a0dc888da7186fb8fc45e88439 content_type: application/zip creator: system date_created: 2018-12-12T13:05:19Z date_updated: 2020-07-14T12:47:02Z file_id: '5645' file_name: IST-2016-46-v1+1_discrete_tomography_synthetic.zip file_size: 36058401 relation: main_file file_date_updated: 2020-07-14T12:47:02Z has_accepted_license: '1' keyword: - discrete tomography month: '09' oa: 1 oa_version: Published Version publisher: Institute of Science and Technology Austria status: public title: Synthetic discrete tomography problems tmp: image: /images/cc_0.png legal_code_url: https://creativecommons.org/publicdomain/zero/1.0/legalcode name: Creative Commons Public Domain Dedication (CC0 1.0) short: CC0 (1.0) type: research_data user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2016' ... --- _id: '5806' abstract: - lang: eng text: Although the concept of functional plane for naive plane is studied and reported in the literature in great detail, no similar study is yet found for naive sphere. This article exposes the first study in this line, opening up further prospects of analyzing the topological properties of sphere in the discrete space. We show that each quadraginta octant Q of a naive sphere forms a bijection with its projected pixel set on a unique coordinate plane, which thereby serves as the functional plane of Q, and hence gives rise to merely mono-jumps during back projection. The other two coordinate planes serve as para-functional and dia-functional planes for Q, as the former is ‘mono-jumping’ but not bijective, whereas the latter holds neither of the two. Owing to this, the quadraginta octants form symmetry groups and subgroups with equivalent jump conditions. We also show a potential application in generating a special class of discrete 3D circles based on back projection and jump bridging by Steiner voxels. A circle in this class possesses 4-symmetry, uniqueness, and bounded distance from the underlying real sphere and real plane. alternative_title: - LNCS article_processing_charge: No author: - first_name: Ranita full_name: Biswas, Ranita id: 3C2B033E-F248-11E8-B48F-1D18A9856A87 last_name: Biswas orcid: 0000-0002-5372-7890 - first_name: Partha full_name: Bhowmick, Partha last_name: Bhowmick citation: ama: 'Biswas R, Bhowmick P. On functionality of quadraginta octants of naive sphere with application to circle drawing. In: Discrete Geometry for Computer Imagery. Vol 9647. Cham: Springer Nature; 2016:256-267. doi:10.1007/978-3-319-32360-2_20' apa: 'Biswas, R., & Bhowmick, P. (2016). On functionality of quadraginta octants of naive sphere with application to circle drawing. In Discrete Geometry for Computer Imagery (Vol. 9647, pp. 256–267). Cham: Springer Nature. https://doi.org/10.1007/978-3-319-32360-2_20' chicago: 'Biswas, Ranita, and Partha Bhowmick. “On Functionality of Quadraginta Octants of Naive Sphere with Application to Circle Drawing.” In Discrete Geometry for Computer Imagery, 9647:256–67. Cham: Springer Nature, 2016. https://doi.org/10.1007/978-3-319-32360-2_20.' ieee: R. Biswas and P. Bhowmick, “On functionality of quadraginta octants of naive sphere with application to circle drawing,” in Discrete Geometry for Computer Imagery, Nantes, France, 2016, vol. 9647, pp. 256–267. ista: 'Biswas R, Bhowmick P. 2016. On functionality of quadraginta octants of naive sphere with application to circle drawing. Discrete Geometry for Computer Imagery. DGCI: International Conference on Discrete Geometry for Computer Imagery, LNCS, vol. 9647, 256–267.' mla: Biswas, Ranita, and Partha Bhowmick. “On Functionality of Quadraginta Octants of Naive Sphere with Application to Circle Drawing.” Discrete Geometry for Computer Imagery, vol. 9647, Springer Nature, 2016, pp. 256–67, doi:10.1007/978-3-319-32360-2_20. short: R. Biswas, P. Bhowmick, in:, Discrete Geometry for Computer Imagery, Springer Nature, Cham, 2016, pp. 256–267. conference: end_date: 2016-04-20 location: Nantes, France name: 'DGCI: International Conference on Discrete Geometry for Computer Imagery' start_date: 2016-04-18 date_created: 2019-01-08T20:44:37Z date_published: 2016-04-09T00:00:00Z date_updated: 2022-01-28T08:10:11Z day: '09' department: - _id: HeEd doi: 10.1007/978-3-319-32360-2_20 extern: '1' intvolume: ' 9647' language: - iso: eng month: '04' oa_version: None page: 256-267 place: Cham publication: Discrete Geometry for Computer Imagery publication_identifier: eisbn: - 978-3-319-32360-2 isbn: - 978-3-319-32359-6 issn: - 0302-9743 - 1611-3349 publication_status: published publisher: Springer Nature quality_controlled: '1' status: public title: On functionality of quadraginta octants of naive sphere with application to circle drawing type: conference user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9 volume: 9647 year: '2016' ... --- _id: '17618' abstract: - lang: eng text: The largest observed supermassive black holes (SMBHs) have a mass of M_BH ~ 10^{10} M_sun, nearly independent of redshift, from the local (z~0) to the early (z>6) Universe. We suggest that the growth of SMBHs above a few 10^{10} M_sun is prevented by small-scale accretion physics, independent of the properties of their host galaxies or of cosmology. Growing more massive BHs requires a gas supply rate from galactic scales onto a nuclear region as high as >10^3 M_sun/yr. At such a high accretion rate, most of the gas converts to stars at large radii (~10-100 pc), well before reaching the BH. We adopt a simple model (Thompson et al. 2005) for a star-forming accretion disk, and find that the accretion rate in the sub-pc nuclear region is reduced to the smaller value of at most a few M_sun/yr. This prevents SMBHs from growing above ~10^{11} M_sun in the age of the Universe. Furthermore, once a SMBH reaches a sufficiently high mass, this rate falls below the critical value at which the accretion flow becomes advection dominated. Once this transition occurs, BH feeding can be suppressed by strong outflows and jets from hot gas near the BH. We find that the maximum SMBH mass, given by this transition, is between M_{BH,max} ~ (1-6) * 10^{10} M_sun, depending primarily on the efficiency of angular momentum transfer inside the galactic disk, and not on other properties of the host galaxy. article_number: '110' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Kohei full_name: Inayoshi, Kohei last_name: Inayoshi - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Inayoshi K, Haiman Z. Is there a maximum mass for black holes in galactic nuclei? The Astrophysical Journal. 2016;828(2). doi:10.3847/0004-637x/828/2/110 apa: Inayoshi, K., & Haiman, Z. (2016). Is there a maximum mass for black holes in galactic nuclei? The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/0004-637x/828/2/110 chicago: Inayoshi, Kohei, and Zoltán Haiman. “Is There a Maximum Mass for Black Holes in Galactic Nuclei?” The Astrophysical Journal. American Astronomical Society, 2016. https://doi.org/10.3847/0004-637x/828/2/110. ieee: K. Inayoshi and Z. Haiman, “Is there a maximum mass for black holes in galactic nuclei?,” The Astrophysical Journal, vol. 828, no. 2. American Astronomical Society, 2016. ista: Inayoshi K, Haiman Z. 2016. Is there a maximum mass for black holes in galactic nuclei? The Astrophysical Journal. 828(2), 110. mla: Inayoshi, Kohei, and Zoltán Haiman. “Is There a Maximum Mass for Black Holes in Galactic Nuclei?” The Astrophysical Journal, vol. 828, no. 2, 110, American Astronomical Society, 2016, doi:10.3847/0004-637x/828/2/110. short: K. Inayoshi, Z. Haiman, The Astrophysical Journal 828 (2016). date_created: 2024-09-05T13:44:44Z date_published: 2016-09-12T00:00:00Z date_updated: 2024-09-24T08:11:51Z day: '12' doi: 10.3847/0004-637x/828/2/110 extern: '1' external_id: arxiv: - '1601.02611' intvolume: ' 828' issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: ' https://doi.org/10.48550/arXiv.1601.02611' month: '09' oa: 1 oa_version: Preprint publication: The Astrophysical Journal publication_identifier: issn: - 0004-637X - 1538-4357 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: Is there a maximum mass for black holes in galactic nuclei? type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 828 year: '2016' ... --- _id: '17709' abstract: - lang: eng text: 'We study very-high rate spherically symmetric accretion flows onto a massive black hole (BH; 10^2 < M_BH < 10^6 Msun) embedded in a dense gas cloud with a low abundance of metals, performing one-dimensional hydrodynamical simulations which include multi-frequency radiation transfer and non-equilibrium primordial chemistry. We find that rapid gas supply from the Bondi radius at a hyper-Eddington rate can occur without being impeded by radiation feedback when (n/10^5 cm^-3) > (M_BH/10^4Msun)^{-1}(T/10^4 K)^{3/2}, where n and T are the density and temperature of ambient gas outside of the Bondi radius. The resulting accretion rate in this regime is steady, and larger than 3000 times the Eddington rate. At lower Bondi rates, the accretion is episodic due to radiative feedback and the average rate is limited below the Eddington rate. For the hyper-Eddington case, the steady solution consists of two parts: a radiation-dominated central core, where photon trapping due to electron scattering is important, and an accreting envelope which follows a Bondi profile with T~8000 K. When the emergent luminosity is limited below the Eddington luminosity because of photon trapping, radiation from the central region does not affect the gas dynamics at larger scales. We apply our result to the rapid formation of massive BHs in protogalaxies with a virial temperature of T_vir> 10^4 K. Once a seed BH forms at the center of the galaxy, it can grow up to a maximum ~10^5 (T_vir/10^4 K) Msun via gas accretion independent of the initial BH mass. Finally, we discuss possible observational signatures of rapidly accreting BHs with/without allowance for dust. We suggest that these systems could explain Lya emitters without X-rays and luminous infrared sources with hot dust emission, respectively.' article_processing_charge: No article_type: original author: - first_name: Kohei full_name: Inayoshi, Kohei last_name: Inayoshi - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Jeremiah P. full_name: Ostriker, Jeremiah P. last_name: Ostriker citation: ama: Inayoshi K, Haiman Z, Ostriker JP. Hyper-Eddington accretion flows on to massive black holes. Monthly Notices of the Royal Astronomical Society. 2016;459(4):3738-3755. doi:10.1093/mnras/stw836 apa: Inayoshi, K., Haiman, Z., & Ostriker, J. P. (2016). Hyper-Eddington accretion flows on to massive black holes. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stw836 chicago: Inayoshi, Kohei, Zoltán Haiman, and Jeremiah P. Ostriker. “Hyper-Eddington Accretion Flows on to Massive Black Holes.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2016. https://doi.org/10.1093/mnras/stw836. ieee: K. Inayoshi, Z. Haiman, and J. P. Ostriker, “Hyper-Eddington accretion flows on to massive black holes,” Monthly Notices of the Royal Astronomical Society, vol. 459, no. 4. Oxford University Press, pp. 3738–3755, 2016. ista: Inayoshi K, Haiman Z, Ostriker JP. 2016. Hyper-Eddington accretion flows on to massive black holes. Monthly Notices of the Royal Astronomical Society. 459(4), 3738–3755. mla: Inayoshi, Kohei, et al. “Hyper-Eddington Accretion Flows on to Massive Black Holes.” Monthly Notices of the Royal Astronomical Society, vol. 459, no. 4, Oxford University Press, 2016, pp. 3738–55, doi:10.1093/mnras/stw836. short: K. Inayoshi, Z. Haiman, J.P. Ostriker, Monthly Notices of the Royal Astronomical Society 459 (2016) 3738–3755. date_created: 2024-09-06T08:54:12Z date_published: 2016-04-12T00:00:00Z date_updated: 2024-09-25T12:00:22Z day: '12' doi: 10.1093/mnras/stw836 extern: '1' intvolume: ' 459' issue: '4' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stw836 month: '04' oa: 1 oa_version: Published Version page: 3738-3755 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: Hyper-Eddington accretion flows on to massive black holes type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 459 year: '2016' ... --- _id: '8452' abstract: - lang: eng text: During spore formation in Bacillus subtilis a transenvelope complex is assembled across the double membrane that separates the mother cell and forespore. This complex (called the “A–Q complex”) is required to maintain forespore development and is composed of proteins with remote homology to components of type II, III, and IV secretion systems found in Gram-negative bacteria. Here, we show that one of these proteins, SpoIIIAG, which has remote homology to ring-forming proteins found in type III secretion systems, assembles into an oligomeric ring in the periplasmic-like space between the two membranes. Three-dimensional reconstruction of images generated by cryo-electron microscopy indicates that the SpoIIIAG ring has a cup-and-saucer architecture with a 6-nm central pore. Structural modeling of SpoIIIAG generated a 24-member ring with dimensions similar to those of the EM-derived saucer. Point mutations in the predicted oligomeric interface disrupted ring formation in vitro and impaired forespore gene expression and efficient spore formation in vivo. Taken together, our data provide strong support for the model in which the A–Q transenvelope complex contains a conduit that connects the mother cell and forespore. We propose that a set of stacked rings spans the intermembrane space, as has been found for type III secretion systems. article_processing_charge: No article_type: original author: - first_name: Christopher D. A. full_name: Rodrigues, Christopher D. A. last_name: Rodrigues - first_name: Xavier full_name: Henry, Xavier last_name: Henry - first_name: Emmanuelle full_name: Neumann, Emmanuelle last_name: Neumann - first_name: Vilius full_name: Kurauskas, Vilius last_name: Kurauskas - first_name: Laure full_name: Bellard, Laure last_name: Bellard - first_name: Yann full_name: Fichou, Yann last_name: Fichou - first_name: Paul full_name: Schanda, Paul id: 7B541462-FAF6-11E9-A490-E8DFE5697425 last_name: Schanda orcid: 0000-0002-9350-7606 - first_name: Guy full_name: Schoehn, Guy last_name: Schoehn - first_name: David Z. full_name: Rudner, David Z. last_name: Rudner - first_name: Cecile full_name: Morlot, Cecile last_name: Morlot citation: ama: Rodrigues CDA, Henry X, Neumann E, et al. A ring-shaped conduit connects the mother cell and forespore during sporulation in Bacillus subtilis. Proceedings of the National Academy of Sciences. 2016;113(41):11585-11590. doi:10.1073/pnas.1609604113 apa: Rodrigues, C. D. A., Henry, X., Neumann, E., Kurauskas, V., Bellard, L., Fichou, Y., … Morlot, C. (2016). A ring-shaped conduit connects the mother cell and forespore during sporulation in Bacillus subtilis. Proceedings of the National Academy of Sciences. National Academy of Sciences. https://doi.org/10.1073/pnas.1609604113 chicago: Rodrigues, Christopher D. A., Xavier Henry, Emmanuelle Neumann, Vilius Kurauskas, Laure Bellard, Yann Fichou, Paul Schanda, Guy Schoehn, David Z. Rudner, and Cecile Morlot. “A Ring-Shaped Conduit Connects the Mother Cell and Forespore during Sporulation in Bacillus Subtilis.” Proceedings of the National Academy of Sciences. National Academy of Sciences, 2016. https://doi.org/10.1073/pnas.1609604113. ieee: C. D. A. Rodrigues et al., “A ring-shaped conduit connects the mother cell and forespore during sporulation in Bacillus subtilis,” Proceedings of the National Academy of Sciences, vol. 113, no. 41. National Academy of Sciences, pp. 11585–11590, 2016. ista: Rodrigues CDA, Henry X, Neumann E, Kurauskas V, Bellard L, Fichou Y, Schanda P, Schoehn G, Rudner DZ, Morlot C. 2016. A ring-shaped conduit connects the mother cell and forespore during sporulation in Bacillus subtilis. Proceedings of the National Academy of Sciences. 113(41), 11585–11590. mla: Rodrigues, Christopher D. A., et al. “A Ring-Shaped Conduit Connects the Mother Cell and Forespore during Sporulation in Bacillus Subtilis.” Proceedings of the National Academy of Sciences, vol. 113, no. 41, National Academy of Sciences, 2016, pp. 11585–90, doi:10.1073/pnas.1609604113. short: C.D.A. Rodrigues, X. Henry, E. Neumann, V. Kurauskas, L. Bellard, Y. Fichou, P. Schanda, G. Schoehn, D.Z. Rudner, C. Morlot, Proceedings of the National Academy of Sciences 113 (2016) 11585–11590. date_created: 2020-09-18T10:06:58Z date_published: 2016-09-28T00:00:00Z date_updated: 2021-01-12T08:19:22Z day: '28' doi: 10.1073/pnas.1609604113 extern: '1' intvolume: ' 113' issue: '41' language: - iso: eng month: '09' oa_version: None page: 11585-11590 publication: Proceedings of the National Academy of Sciences publication_identifier: issn: - 0027-8424 - 1091-6490 publication_status: published publisher: National Academy of Sciences quality_controlled: '1' status: public title: A ring-shaped conduit connects the mother cell and forespore during sporulation in Bacillus subtilis type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 113 year: '2016' ... --- _id: '7294' abstract: - lang: eng text: Mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres were prepared by non-hydrolytic sol–gel from TiCl4, VOCl3, and iPr2O at 110 °C without any solvent or additives. The samples were characterized by elemental analysis, X-ray diffraction, Raman spectroscopy, scanning electron microscopy, nitrogen physisorption, and impedance measurements. At low vanadium loadings, only TiO2 anatase was detected, and V2O5 scherbinaite was also detected at high vanadium loadings. The texture of the samples depended on the V loading, but all the samples appeared built of primary nanoparticles (≈10–20 nm in size) that aggregate to form mesoporous micron-sized spheres. The lithium insertion properties of these materials were evaluated by galvanostatic measurements taken using coin-type cells, in view of their application as electrode for rechargeable Li-ion batteries. The mesoporous TiO2 microspheres showed good performances, with a specific reversible capacity of 145 and 128 mAh g−1 at C/2 and C, respectively (C = 335.6 mA g−1), good coulombic efficiency, and a moderate capacity fade (6 %) from the 2nd to the 20th cycle at C/20. Although the addition of V effectively increased the electronic conductivity of the powders, the specific reversible capacity and cycling performances of the TiO2–V2O5 samples were only minimally improved for a 5 at% V loading and were lower at higher V loading. article_processing_charge: No article_type: original author: - first_name: A. M. full_name: Escamilla-Pérez, A. M. last_name: Escamilla-Pérez - first_name: N. full_name: Louvain, N. last_name: Louvain - first_name: M. full_name: Kaschowitz, M. last_name: Kaschowitz - first_name: Stefan Alexander full_name: Freunberger, Stefan Alexander id: A8CA28E6-CE23-11E9-AD2D-EC27E6697425 last_name: Freunberger orcid: 0000-0003-2902-5319 - first_name: O. full_name: Fontaine, O. last_name: Fontaine - first_name: B. full_name: Boury, B. last_name: Boury - first_name: N. full_name: Brun, N. last_name: Brun - first_name: P. H. full_name: Mutin, P. H. last_name: Mutin citation: ama: Escamilla-Pérez AM, Louvain N, Kaschowitz M, et al. Lithium insertion properties of mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres prepared by non-hydrolytic sol–gel. Journal of Sol-Gel Science and Technology. 2016;79(2):270-278. doi:10.1007/s10971-016-4037-9 apa: Escamilla-Pérez, A. M., Louvain, N., Kaschowitz, M., Freunberger, S. A., Fontaine, O., Boury, B., … Mutin, P. H. (2016). Lithium insertion properties of mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres prepared by non-hydrolytic sol–gel. Journal of Sol-Gel Science and Technology. Springer Nature. https://doi.org/10.1007/s10971-016-4037-9 chicago: Escamilla-Pérez, A. M., N. Louvain, M. Kaschowitz, Stefan Alexander Freunberger, O. Fontaine, B. Boury, N. Brun, and P. H. Mutin. “Lithium Insertion Properties of Mesoporous Nanocrystalline TiO2 and TiO2–V2O5 Microspheres Prepared by Non-Hydrolytic Sol–Gel.” Journal of Sol-Gel Science and Technology. Springer Nature, 2016. https://doi.org/10.1007/s10971-016-4037-9. ieee: A. M. Escamilla-Pérez et al., “Lithium insertion properties of mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres prepared by non-hydrolytic sol–gel,” Journal of Sol-Gel Science and Technology, vol. 79, no. 2. Springer Nature, pp. 270–278, 2016. ista: Escamilla-Pérez AM, Louvain N, Kaschowitz M, Freunberger SA, Fontaine O, Boury B, Brun N, Mutin PH. 2016. Lithium insertion properties of mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres prepared by non-hydrolytic sol–gel. Journal of Sol-Gel Science and Technology. 79(2), 270–278. mla: Escamilla-Pérez, A. M., et al. “Lithium Insertion Properties of Mesoporous Nanocrystalline TiO2 and TiO2–V2O5 Microspheres Prepared by Non-Hydrolytic Sol–Gel.” Journal of Sol-Gel Science and Technology, vol. 79, no. 2, Springer Nature, 2016, pp. 270–78, doi:10.1007/s10971-016-4037-9. short: A.M. Escamilla-Pérez, N. Louvain, M. Kaschowitz, S.A. Freunberger, O. Fontaine, B. Boury, N. Brun, P.H. Mutin, Journal of Sol-Gel Science and Technology 79 (2016) 270–278. date_created: 2020-01-15T12:16:08Z date_published: 2016-04-08T00:00:00Z date_updated: 2021-01-12T08:12:49Z day: '08' doi: 10.1007/s10971-016-4037-9 extern: '1' intvolume: ' 79' issue: '2' language: - iso: eng month: '04' oa_version: None page: 270-278 publication: Journal of Sol-Gel Science and Technology publication_identifier: issn: - 0928-0707 - 1573-4846 publication_status: published publisher: Springer Nature quality_controlled: '1' status: public title: Lithium insertion properties of mesoporous nanocrystalline TiO2 and TiO2–V2O5 microspheres prepared by non-hydrolytic sol–gel type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 79 year: '2016' ... --- _id: '11519' abstract: - lang: eng text: 'Faint Lyα emitters become increasingly rarer toward the reionization epoch (z ∼ 6–7). However, observations from a very large (∼5 deg2) Lyα narrow-band survey at z = 6.6 show that this is not the case for the most luminous emitters, capable of ionizing their own local bubbles. Here we present follow-up observations of the two most luminous Lyα candidates in the COSMOS field: “MASOSA” and “CR7.” We used X-SHOOTER, SINFONI, and FORS2 on the Very Large Telescope, and DEIMOS on Keck, to confirm both candidates beyond any doubt. We find redshifts of z = 6.541 and z = 6.604 for “MASOSA” and “CR7,” respectively. MASOSA has a strong detection in Lyα with a line width of 386 ± 30 km s−1 (FWHM) and with very high EW0 (>200 Å), but undetected in the continuum, implying very low stellar mass and a likely young, metal-poor stellar population. “CR7,” with an observed Lyα luminosity of 1043.92±0.05 erg s−1 is the most luminous Lyα emitter ever found at z > 6 and is spatially extended (∼16 kpc). “CR7” reveals a narrow Lyα line with 266 ± 15 km s−1 FWHM, being detected in the near-infrared (NIR) (rest-frame UV; β = −2.3 ± 0.1) and in IRAC/Spitzer. We detect a narrow He II 1640 Å emission line (6σ, FWHM = 130 ± 30 km s−1 ) in CR7 which can explain the clear excess seen in the J-band photometry (EW0 ∼ 80 Å). We find no other emission lines from the UV to the NIR in our X-SHOOTER spectra (He II/O III] 1663 Å > 3 and He II/C III] 1908 Å > 2.5). We conclude that CR7 is best explained by a combination of a PopIII-like population, which dominates the rest-frame UV and the nebular emission, and a more normal stellar population, which presumably dominates the mass. Hubble Space Telescope/WFC3 observations show that the light is indeed spatially separated between a very blue component, coincident with Lyα and He II emission, and two red components (∼5 kpc away), which dominate the mass. Our findings are consistent with theoretical predictions of a PopIII wave, with PopIII star formation migrating away from the original sites of star formation.' acknowledgement: We thank the anonymous reviewer for useful and constructive comments and suggestions which greatly improved the quality and clarity of our work. D.S. acknowledges financial support from the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship, from FCT through a FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010), from FCT grant UID/FIS/04434/2013, and from LSF and LKBF. J.M. acknowledges the award of a Huygens PhD fellowship. H.R. acknowledges support from the ERC Advanced Investigator program NewClusters 321271. The authors thank Mark Dijkstra, Bhaskar Agarwal, Jarrett Johnson, Andrea Ferrara, Jarle Brinchmann, Rebecca Bowler, George Becker, Emma Curtis-Lake, Milos Milosavljevic, Raffaella Schneider, Paul Shapiro, and Erik Zackrisson for interesting, stimulating and helpful discussions. The authors are extremely grateful to ESO for the award of ESO DDT time (294.A-5018 and 294.A-5039) which allowed the spectroscopic confirmation of both sources and the detailed investigation of their nature. Observations are also based on data from W.M. Keck Observatory. The W.M. Keck Observatory is operated as a scientific partnership of Caltech, the University of California and the National Aeronautics and Space Administration. Based on observations obtained with MegaPrime/Megacam, a joint project of CFHT and CEA/IRFU, at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de lUnivers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada–France–Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO programme IDs 294.A-5018, 294.A-5039, and 179.A-2005, and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. The authors acknowledge the award of service time (SW2014b20) on the William Herschel Telescope (WHT). WHT and its service programme are operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: David full_name: Sobral, David last_name: Sobral - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X - first_name: Behnam full_name: Darvish, Behnam last_name: Darvish - first_name: Daniel full_name: Schaerer, Daniel last_name: Schaerer - first_name: Bahram full_name: Mobasher, Bahram last_name: Mobasher - first_name: Huub full_name: Röttgering, Huub last_name: Röttgering - first_name: Sérgio full_name: Santos, Sérgio last_name: Santos - first_name: Shoubaneh full_name: Hemmati, Shoubaneh last_name: Hemmati citation: ama: 'Sobral D, Matthee JJ, Darvish B, et al. Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. The Astrophysical Journal. 2015;808(2):139. doi:10.1088/0004-637X/808/2/139' apa: 'Sobral, D., Matthee, J. J., Darvish, B., Schaerer, D., Mobasher, B., Röttgering, H., … Hemmati, S. (2015). Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. The Astrophysical Journal. IOP Publishing. https://doi.org/10.1088/0004-637X/808/2/139' chicago: 'Sobral, David, Jorryt J Matthee, Behnam Darvish, Daniel Schaerer, Bahram Mobasher, Huub Röttgering, Sérgio Santos, and Shoubaneh Hemmati. “Evidence for PopIII-like Stellar Populations in the Most Luminous Lyα Emitters at the Epoch of Reionisation: Spectroscopic Confirmation.” The Astrophysical Journal. IOP Publishing, 2015. https://doi.org/10.1088/0004-637X/808/2/139.' ieee: 'D. Sobral et al., “Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation,” The Astrophysical Journal, vol. 808, no. 2. IOP Publishing, p. 139, 2015.' ista: 'Sobral D, Matthee JJ, Darvish B, Schaerer D, Mobasher B, Röttgering H, Santos S, Hemmati S. 2015. Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. The Astrophysical Journal. 808(2), 139.' mla: 'Sobral, David, et al. “Evidence for PopIII-like Stellar Populations in the Most Luminous Lyα Emitters at the Epoch of Reionisation: Spectroscopic Confirmation.” The Astrophysical Journal, vol. 808, no. 2, IOP Publishing, 2015, p. 139, doi:10.1088/0004-637X/808/2/139.' short: D. Sobral, J.J. Matthee, B. Darvish, D. Schaerer, B. Mobasher, H. Röttgering, S. Santos, S. Hemmati, The Astrophysical Journal 808 (2015) 139. date_created: 2022-07-07T09:00:58Z date_published: 2015-07-28T00:00:00Z date_updated: 2022-08-18T10:30:13Z day: '28' doi: 10.1088/0004-637X/808/2/139 extern: '1' external_id: arxiv: - '1504.01734' intvolume: ' 808' issue: '2' keyword: - Space and Planetary Science - Astronomy and Astrophysics - dark ages - reionization - 'first stars – early universe – galaxies: evolution' language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1504.01734 month: '07' oa: 1 oa_version: Preprint page: '139' publication: The Astrophysical Journal publication_identifier: eissn: - 1538-4357 issn: - 0004-637X publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: 'Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation' type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 808 year: '2015' ... --- _id: '11837' abstract: - lang: eng text: "Online social networks allow the collection of large amounts of data about the influence between users connected by a friendship-like relationship. When distributing items among agents forming a social network, this information allows us to exploit network externalities that each agent receives from his neighbors that get the same item. In this paper we consider Friends-of-Friends (2-hop) network externalities, i.e., externalities that not only depend on the neighbors that get the same item but also on neighbors of neighbors. For these externalities we study a setting where multiple different items are assigned to unit-demand agents. Specifically, we study the problem of welfare maximization under different types of externality functions. Let n be the number of agents and m be the number of items. Our contributions are the following: (1) We show that welfare maximization is APX-hard; we show that even for step functions with 2-hop (and also with 1-hop) externalities it is NP-hard to approximate social welfare better than (1-1/e). (2) On the positive side we present (i) an O(sqrt n)-approximation algorithm for general concave externality functions,\r\n(ii) an O(\\log m)-approximation algorithm for linear externality functions, and (iii) an (1-1/e)\\frac{1}{6}-approximation algorithm for 2-hop step function externalities. We also improve the result from [6] for 1-hop step function externalities by giving a (1-1/e)/2-approximation algorithm." alternative_title: - LIPIcs article_processing_charge: No author: - first_name: Sayan full_name: Bhattacharya, Sayan last_name: Bhattacharya - first_name: Wolfgang full_name: Dvorák, Wolfgang last_name: Dvorák - first_name: Monika H full_name: Henzinger, Monika H id: 540c9bbd-f2de-11ec-812d-d04a5be85630 last_name: Henzinger orcid: 0000-0002-5008-6530 - first_name: ' Martin' full_name: Starnberger, Martin last_name: Starnberger citation: ama: 'Bhattacharya S, Dvorák W, Henzinger M, Starnberger Martin. Welfare maximization with friends-of-friends network externalities. In: 32nd International Symposium on Theoretical Aspects of Computer Science. Vol 30. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2015:90-102. doi:10.4230/LIPICS.STACS.2015.90' apa: 'Bhattacharya, S., Dvorák, W., Henzinger, M., & Starnberger, Martin. (2015). Welfare maximization with friends-of-friends network externalities. In 32nd International Symposium on Theoretical Aspects of Computer Science (Vol. 30, pp. 90–102). Garching, Germany: Schloss Dagstuhl - Leibniz-Zentrum für Informatik. https://doi.org/10.4230/LIPICS.STACS.2015.90' chicago: Bhattacharya, Sayan, Wolfgang Dvorák, Monika Henzinger, and Martin Starnberger. “Welfare Maximization with Friends-of-Friends Network Externalities.” In 32nd International Symposium on Theoretical Aspects of Computer Science, 30:90–102. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2015. https://doi.org/10.4230/LIPICS.STACS.2015.90. ieee: S. Bhattacharya, W. Dvorák, M. Henzinger, and Martin Starnberger, “Welfare maximization with friends-of-friends network externalities,” in 32nd International Symposium on Theoretical Aspects of Computer Science, Garching, Germany, 2015, vol. 30, pp. 90–102. ista: 'Bhattacharya S, Dvorák W, Henzinger M, Starnberger Martin. 2015. Welfare maximization with friends-of-friends network externalities. 32nd International Symposium on Theoretical Aspects of Computer Science. STACS: Symposium on Theoretical Aspects of Computer Science, LIPIcs, vol. 30, 90–102.' mla: Bhattacharya, Sayan, et al. “Welfare Maximization with Friends-of-Friends Network Externalities.” 32nd International Symposium on Theoretical Aspects of Computer Science, vol. 30, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2015, pp. 90–102, doi:10.4230/LIPICS.STACS.2015.90. short: S. Bhattacharya, W. Dvorák, M. Henzinger, Martin Starnberger, in:, 32nd International Symposium on Theoretical Aspects of Computer Science, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2015, pp. 90–102. conference: end_date: 2015-03-07 location: Garching, Germany name: 'STACS: Symposium on Theoretical Aspects of Computer Science' start_date: 2015-03-04 date_created: 2022-08-12T11:39:40Z date_published: 2015-02-26T00:00:00Z date_updated: 2024-11-06T12:24:23Z day: '26' doi: 10.4230/LIPICS.STACS.2015.90 extern: '1' intvolume: ' 30' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.4230/LIPICS.STACS.2015.90 month: '02' oa: 1 oa_version: Published Version page: 90-102 publication: 32nd International Symposium on Theoretical Aspects of Computer Science publication_identifier: isbn: - 978-3-939897-78-1 issn: - 1868-8969 publication_status: published publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik quality_controlled: '1' related_material: record: - id: '11903' relation: later_version status: public scopus_import: '1' status: public title: Welfare maximization with friends-of-friends network externalities type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 30 year: '2015' ... --- OA_place: repository OA_type: green _id: '259' abstract: - lang: eng text: "The Hasse principle and weak approximation is established for\r\nnon-singular cubic hypersurfaces X over the function field Fq(t), provided that\r\nchar(Fq) > 3 and X has dimension at least 6." acknowledgement: "EP/J018260/1\tEngineering and Physical Sciences Research Council EPSRC" article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Timothy D full_name: Browning, Timothy D id: 35827D50-F248-11E8-B48F-1D18A9856A87 last_name: Browning orcid: 0000-0002-8314-0177 - first_name: Pankaj full_name: Vishe, Pankaj last_name: Vishe citation: ama: Browning TD, Vishe P. Rational points on cubic hypersurfaces over F_q(t) . Geometric and Functional Analysis. 2015;25(3):671-732. doi:10.1007/s00039-015-0328-5 apa: Browning, T. D., & Vishe, P. (2015). Rational points on cubic hypersurfaces over F_q(t) . Geometric and Functional Analysis. Springer Nature. https://doi.org/10.1007/s00039-015-0328-5 chicago: Browning, Timothy D, and Pankaj Vishe. “Rational Points on Cubic Hypersurfaces over F_q(T) .” Geometric and Functional Analysis. Springer Nature, 2015. https://doi.org/10.1007/s00039-015-0328-5. ieee: T. D. Browning and P. Vishe, “Rational points on cubic hypersurfaces over F_q(t) ,” Geometric and Functional Analysis, vol. 25, no. 3. Springer Nature, pp. 671–732, 2015. ista: Browning TD, Vishe P. 2015. Rational points on cubic hypersurfaces over F_q(t) . Geometric and Functional Analysis. 25(3), 671–732. mla: Browning, Timothy D., and Pankaj Vishe. “Rational Points on Cubic Hypersurfaces over F_q(T) .” Geometric and Functional Analysis, vol. 25, no. 3, Springer Nature, 2015, pp. 671–732, doi:10.1007/s00039-015-0328-5. short: T.D. Browning, P. Vishe, Geometric and Functional Analysis 25 (2015) 671–732. date_created: 2018-12-11T11:45:29Z date_published: 2015-06-11T00:00:00Z date_updated: 2026-05-19T09:46:04Z day: '11' doi: 10.1007/s00039-015-0328-5 extern: '1' external_id: arxiv: - '1502.00772' intvolume: ' 25' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: ' https://doi.org/10.48550/arXiv.1502.00772' month: '06' oa: 1 oa_version: Preprint page: 671 - 732 publication: Geometric and Functional Analysis publication_identifier: eissn: - 1420-8970 issn: - 1016-443X publication_status: published publisher: Springer Nature publist_id: '7643' quality_controlled: '1' scopus_import: '1' status: public title: 'Rational points on cubic hypersurfaces over F_q(t) ' type: journal_article user_id: ba8df636-2132-11f1-aed0-ed93e2281fdd volume: 25 year: '2015' ...