Institution
University of Crete
Education•Rethymno, Greece•
About: University of Crete is a education organization based out in Rethymno, Greece. It is known for research contribution in the topics: Population & Galaxy. The organization has 8681 authors who have published 21684 publications receiving 709078 citations. The organization is also known as: Panepistimio Kritis.
Topics: Population, Galaxy, Cancer, Active galactic nucleus, Luminosity
Papers published on a yearly basis
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TL;DR: It has been shown directly that various extracellular proteins involved in pathogenesis and defence elicitation by plantpathogenic bacteria utilize this pathway, and the pathway is known to function in the export of virulence factors from the animal pathogens.
Abstract: Genes of plant-pathogenic bacteria controlling hypersensitive response (HR) elicitation and pathogenesis were designated ‘hrp’ by Lindgren et al. in 1986 (J Bacteriol 168: 512–522). hrp genes have been characterized in several species of the four major genera of Gramnegative plant pathogens, Erwinia, Pseudomonas, Ralstonia (a new proposed genus including Pseudomonas solanacearum) and Xanthomonas. To date, hrp genes have been found mainly in large clusters, and they have been shown to be conserved physically and, in many cases, functionally among different bacteria. Hybridization studies and genetic analyses have revealed the presence of functional hrp genes even in species that are not typically observed to elicit an HR, such as Erwinia chrysanthemi and Erwinia stewartii, suggesting that hrp genes may be common to all Gram-negative plant pathogens, possibly excluding Agrobacterium spp. Current knowledge of hrp genes has been reviewed by Bonas (1994, Curr Top Microbiol Immunol 192: 79–98) and by Van Gijsegem et al. (1995, In Pathogenesis and Host–Parasite Specificity in Plant Diseases: Histopathological, Biochemical, Genetic and Molecular Basis. Volume 1. (Kohmoto et al., eds); Oxford: Pergamon Press, pp. 273–292). The nucleotide sequences of four hrp gene clusters, those of Ralstonia solanacearum (previously P. solanacearum) (Genin et al., 1992, Mol Microbiol 6: 3065–3076; Gough et al., 1992, Mol Plant–Microbe Interact 5: 384–389; Gough et al., 1993, Mol Gen Genet 239: 378–392; Van Gijsegem et al., 1995, Mol Microbiol 15: 1095–1114), Erwinia amylovora (Bogdanove et al., 1996, J Bacteriol 178: 1720– 1730; Wei and Beer, 1993, J Bacteriol 175: 7958–7967; Wei and Beer, 1995, J Bacteriol 177: 6201–6210; Wei et al., 1992, Science 257: 85–88; S. V. Beer, unpublished), Pseudomonas syringae pv. syringae (Huang et al., 1992, J Bacteriol 174: 6878–6885; Huang et al., 1993, Mol Plant–Microbe Interact 6: 515–520; Huang et al., 1995, Mol Plant–Microbe Interact 8: 733–746; Lidell and Hutcheson, 1994, Mol Plant–Microbe Interact 7: 488–497; Preston et al., 1995, Mol Plant–Microbe Interact 8: 717–732; Xiao et al., 1994, J Bacteriol 176: 1025–1036), and Xanthomonas campestris pv. vesicatoria (Fenselau et al., 1992, Mol Plant–Microbe Interact 5: 390–396; Fenselau and Bonas, 1995, Mol Plant–Microbe Interact 8: 845–854; U. Bonas, unpublished), have been largely determined. These clusters each contain more than twenty genes, many of which encode components of a novel proteinsecretion pathway designated ‘type III’. It has been shown directly that various extracellular proteins involved in pathogenesis and defence elicitation by plantpathogenic bacteria utilize this pathway (Arlat et al., 1994, EMBO J 13: 543–553; He et al., 1993, Cell 73: 1255–1266; Wei and Beer, 1993, ibid.), and the pathway is known to function in the export of virulence factors from the animal pathogens Salmonella typhimurium, Shigella flexneri, and Yersinia entercolitica, Yersinia pestis, and Yersinia pseudotuberculosis (for reviews, see Salmond and Reeves, 1993, Trends Biochem Sci 18: 7–12; and Van Gijsegem et al., 1993, Trends Microbiol 1: 175– 180). Nine type III secretion genes are conserved among all four of the plant pathogens listed above and among the animal pathogens. Based on sequence analysis and some experimental evidence, they are believed to encode one outer-membrane protein, one outer-membrane-associated lipoprotein, five inner-membrane proteins, and two cytoplasmic proteins, one of which is a putative ATPase. All of the predicted gene products, except the outer-membrane protein, show significant similarity to components of the flagellar biogenesis complex (for reviews see Blair, 1995, Annu Rev Microbiol 49: 489–522; and Bischoff and Ordal, 1992, Mol Microbiol 6: 23–28). We herein refer to the hrp-encoded type III pathway as the ‘Hrp pathway’. Because hrp genes have been characterized independently in diverse plant-pathogenic bacteria, hrp gene nomenclature differs in different species, and it is not always consistent even within the same organism. Different designations are used for homologous genes, and, even worse, the same designation is used for different genes in different organisms. For example, hrpI of E. amylovora is homologous with hrpC2 of X. campestris pv. vesicatoria and hrpO of R. solanacearum, and the homologue in P. syringae pv. syringae appears in the literature both as hrpI and as hrpJ2. Also, ‘hrpN ’ in R. solanacearum designates a secretion-pathway gene, whereas in E. amylovora, ‘hrpN ’ designates the gene encoding the elicitor harpin. Furthermore, in many bacteria the number of known hrp genes approaches 26. In anticipation of exhausting the alphabet, some authors chose to designate hrp genes with a letter and a number, creating the potential for confusion of distinct genes with alleles of the same gene. For hrp gene researchers, the current nomenclature is at best inconvenient; for other scientists, it is bewildering. Another problem exists: accumulation of knowledge about the structure of hrp loci has outpaced the accumulation of Molecular Microbiology (1996) 20(3), 681–683
253 citations
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TL;DR: Shift in gas/particle distribution due to difference in ambient temperature elucidated to some extent the seasonal variation of the concentration of PAHs in particles.
252 citations
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TL;DR: The state of the art on the possible nitrogen flow in PAs, their interconnection with nitrogen metabolism, as well as the signalling roles of PA-derived H( 2)O(2) during some developmental processes and stress responses are discussed.
Abstract: Polyamines (PAs) are nitrogenous molecules which play a well-established role in most cellular processes during growth and development under physiological or biotic/abiotic stress conditions. The molecular mode(s) of PA action have only recently started to be unveiled, and comprehensive models for their molecular interactions have been proposed. Their multiple roles are exerted, at least partially, through signalling by hydrogen peroxide (H(2)O(2)), which is generated by the oxidation/back-conversion of PAs by copper amine oxidases and PA oxidases. Accumulating evidence suggests that in plants the cellular titres of PAs are affected by other nitrogenous compounds. Here, we discuss the state of the art on the possible nitrogen flow in PAs, their interconnection with nitrogen metabolism, as well as the signalling roles of PA-derived H(2)O(2) during some developmental processes and stress responses.
252 citations
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University of Nottingham1, Cardiff University2, Max Planck Society3, University of Crete4, Institut d'Astrophysique de Paris5, Ghent University6, University of Hertfordshire7, INAF8, Complutense University of Madrid9, University of California, Irvine10, McGill University11, Durham University12, Imperial College London13, International School for Advanced Studies14, University of St Andrews15, UK Astronomy Technology Centre16, University of Edinburgh17, University of Central Lancashire18, University of Padua19, Ames Research Center20, Open University21, Leiden University22, University of Chile23
TL;DR: The first direct and unbiased measurement of the evolution of the dust mass function of galaxies over the past 5 billion years of cosmic history using data from the Science Demonstration Phase of the Herschel-Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) is presented in this paper.
Abstract: We present the first direct and unbiased measurement of the evolution of the dust mass function of galaxies over the past 5 billion years of cosmic history using data from the Science Demonstration Phase of the Herschel-Astrophysical Terahertz Large Area Survey (Herschel-ATLAS). The sample consists of galaxies selected at 250 m which have reliable counterparts from the Sloan Digital Sky Survey (SDSS) at z < 0.5, and contains 1867 sources. Dust masses are calculated using both a single-temperature grey-body model for the spectral energy distribution and also a model with multiple temperature components. The dust temperature for either model shows no trend with redshift. Splitting the sample into bins of redshift reveals a strong evolution in the dust properties of the most massive galaxies. At z= 0.4–0.5, massive galaxies had dust masses about five times larger than in the local Universe. At the same time, the dust-to-stellar mass ratio was about three to four times larger, and the optical depth derived from fitting the UV-sub-mm data with an energy balance model was also higher. This increase in the dust content of massive galaxies at high redshift is difficult to explain using standard dust evolution models and requires a rapid gas consumption time-scale together with either a more top-heavy initial mass function (IMF), efficient mantle growth, less dust destruction or combinations of all three. This evolution in dust mass is likely to be associated with a change in overall interstellar medium mass, and points to an enhanced supply of fuel for star formation at earlier cosmic epochs.
251 citations
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TL;DR: In this article, a unified model is presented to account for crater and subwavelength ripple formation based on a synergy of electron excitation and capillary wave solidification, and details of the surface morphology attained are elaborated as a function of the imposed conditions, and results are tested against experimental data.
Abstract: An investigation of ultrashort pulsed laser--induced surface modification due to conditions that result in a superheated melted liquid layer and material evaporation are considered. To describe the surface modification occurring after cooling and resolidification of the melted layer and understand the underlying physical fundamental mechanisms, a unified model is presented to account for crater and subwavelength ripple formation based on a synergy of electron excitation and capillary wave solidification. The proposed theoretical framework aims to address the laser--material interaction in subablation conditions and thus the minimal mass removal in combination with a hydrodynamics-based scenario of the crater creation and ripple formation following surface irradiation with single and multiple pulses, respectively. The development of the periodic structures is attributed to the interference of the incident wave with a surface plasmon wave. Details of the surface morphology attained are elaborated as a function of the imposed conditions, and results are tested against experimental data.
251 citations
Authors
Showing all 8725 results
Name | H-index | Papers | Citations |
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Mercouri G. Kanatzidis | 152 | 1854 | 113022 |
T. J. Pearson | 150 | 895 | 126533 |
Stylianos E. Antonarakis | 138 | 746 | 93605 |
William Wijns | 127 | 752 | 95517 |
Andrea Comastri | 111 | 706 | 49119 |
Costas M. Soukoulis | 108 | 644 | 50208 |
Elias Anaissie | 107 | 372 | 42808 |
Jian Zhang | 107 | 3064 | 69715 |
Emmanouil T. Dermitzakis | 101 | 294 | 82496 |
Andreas Engel | 99 | 448 | 33494 |
Nikos C. Kyrpides | 96 | 711 | 62360 |
David J. Kerr | 95 | 544 | 39408 |
Manolis Kogevinas | 95 | 623 | 28521 |
Thomas Walz | 92 | 255 | 29981 |
Jean-Paul Latgé | 91 | 343 | 29152 |