Selection and characterization of conditionally active promotors in Lactobacillus plantarum, using alanine racemase as a promotor probe

This paper describes the use of the alr gene, encoding alanine racemase, as a promoter-screening tool for the identification of conditional promoters in Lactobacillus plantarum. Random fragments of the L. plantarum WCFS1 genome were cloned upstream of the promoterless alr gene of Lactococcus lactis in a low-copy-number plasmid vector. The resulting plasmid library was introduced into an L. plantarum Deltaalr strain (MD007), and 40,000 clones were selected. The genome coverage of the library was estimated to be 98%, based on nucleotide insert sequence and restriction analyses of the inserts of randomly selected clones. The library was screened for clones that were capable of complementing the D-alanine auxotroph phenotype of MD007 in media containing up to 10, 100, or 300 mug of the competitive Air inhibitor D-cycloserine per ml. Western blot analysis with polyclonal antibodies raised against lactococcal Air revealed that the Air production level required for growth increased in the presence of increasing concentrations Of D-cycloserine, adding a quantitative factor to the primarily qualitative nature of the alr complementation screen. Screening of the alr complementation library for clones that could grow only in the presence of 0.8 M NaCl resulted in the identification of eight clones that upon Western blot analysis showed significantly higher Air production under high-salt conditions than under low-salt conditions. These results established the effectiveness of the alanine racemase complementation screening method for the identification of promoters on their conditional or constitutive activity

Ku70 Serine 155 mediates Aurora B inhibition and activation of the DNA damage response

The Ku heterodimer (Ku70/Ku80) is the central DNA binding component of the classical non-homologous end joining (NHEJ) pathway that repairs DNA double-stranded breaks (DSBs), serving as the scaffold for the formation of the NHEJ complex. Here we show that Ku70 is phosphorylated on Serine 155 in response to DNA damage. Expression of Ku70 bearing a S155 phosphomimetic substitution (Ku70 S155D) in Ku70-deficient mouse embryonic fibroblasts (MEFs) triggered cell cycle arrest at multiple checkpoints and altered expression of several cell cycle regulators in absence of DNA damage. Cells expressing Ku70 S155D exhibited a constitutive DNA damage response, including ATM activation, H2AX phosphorylation and 53BP1 foci formation. Ku70 S155D was found to interact with Aurora B and to have an inhibitory effect on Aurora B kinase activity. Lastly, we demonstrate that Ku and Aurora B interact following ionizing radiation treatment and that Aurora B inhibition in response to DNA damage is dependent upon Ku70 S155 phosphorylation. This uncovers a new pathway where Ku may relay signaling to Aurora B to enforce cell cycle arrest in response to DNA damage

CREBBP mutations in individuals without Rubinstein-Taybi syndrome phenotype

Item does not contain fulltextMutations in CREBBP cause Rubinstein-Taybi syndrome. By using exome sequencing, and by using Sanger in one patient, CREBBP mutations were detected in 11 patients who did not, or only in a very limited manner, resemble Rubinstein-Taybi syndrome. The combined facial signs typical for Rubinstein-Taybi syndrome were absent, none had broad thumbs, and three had only somewhat broad halluces. All had apparent developmental delay (being the reason for molecular analysis); five had short stature and seven had microcephaly. The facial characteristics were variable; main characteristics were short palpebral fissures, telecanthi, depressed nasal ridge, short nose, anteverted nares, short columella, and long philtrum. Six patients had autistic behavior, and two had self-injurious behavior. Other symptoms were recurrent upper airway infections (n = 5), feeding problems (n = 7) and impaired hearing (n = 7). Major malformations occurred infrequently. All patients had a de novo missense mutation in the last part of exon 30 or beginning of exon 31 of CREBBP, between base pairs 5,128 and 5,614 (codons 1,710 and 1,872). No missense or truncating mutations in this region have been described to be associated with the classical Rubinstein-Taybi syndrome phenotype. No functional studies have (yet) been performed, but we hypothesize that the mutations disturb protein-protein interactions by altering zinc finger function. We conclude that patients with missense mutations in this specific CREBBP region show a phenotype that differs substantially from that in patients with Rubinstein-Taybi syndrome, and may prove to constitute one (or more) separate entities. (c) 2016 Wiley Periodicals, Inc

Political Radicalization as a Communication Process

Based on data taken from 412 adult education students in Montreal, Quebec, Canada, this research attempts to show that attitudes toward French Canadian Separatism by the sample members can be accounted for by differentiaf communication processes. Results show that attitudes held by sample members are well explained (R2 = .64) by a weighted average of the information they received from interpersonal and media sources. The resultant attitude shows substantial effects on behaviors related to separatism for the same respondents.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/67215/2/10.1177_009365027400100301.pd

Dust Devil Tracks

Dust devils that leave dark- or light-toned tracks are common on Mars and they can also be found on the Earth’s surface. Dust devil tracks (hereinafter DDTs) are ephemeral surface features with mostly sub-annual lifetimes. Regarding their size, DDT widths can range between ∼1 m and ∼1 km, depending on the diameter of dust devil that created the track, and DDT lengths range from a few tens of meters to several kilometers, limited by the duration and horizontal ground speed of dust devils. DDTs can be classified into three main types based on their morphology and albedo in contrast to their surroundings; all are found on both planets: (a) dark continuous DDTs, (b) dark cycloidal DDTs, and (c) bright DDTs. Dark continuous DDTs are the most common type on Mars. They are characterized by their relatively homogenous and continuous low albedo surface tracks. Based on terrestrial and martian in situ studies, these DDTs most likely form when surficial dust layers are removed to expose larger-grained substrate material (coarse sands of ≥500 μm in diameter). The exposure of larger-grained materials changes the photometric properties of the surface; hence leading to lower albedo tracks because grain size is photometrically inversely proportional to the surface reflectance. However, although not observed so far, compositional differences (i.e., color differences) might also lead to albedo contrasts when dust is removed to expose substrate materials with mineralogical differences. For dark continuous DDTs, albedo drop measurements are around 2.5 % in the wavelength range of 550–850 nm on Mars and around 0.5 % in the wavelength range from 300–1100 nm on Earth. The removal of an equivalent layer thickness around 1 μm is sufficient for the formation of visible dark continuous DDTs on Mars and Earth. The next type of DDTs, dark cycloidal DDTs, are characterized by their low albedo pattern of overlapping scallops. Terrestrial in situ studies imply that they are formed when sand-sized material that is eroded from the outer vortex area of a dust devil is redeposited in annular patterns in the central vortex region. This type of DDT can also be found in on Mars in orbital image data, and although in situ studies are lacking, terrestrial analog studies, laboratory work, and numerical modeling suggest they have the same formation mechanism as those on Earth. Finally, bright DDTs are characterized by their continuous track pattern and high albedo compared to their undisturbed surroundings. They are found on both planets, but to date they have only been analyzed in situ on Earth. Here, the destruction of aggregates of dust, silt and sand by dust devils leads to smooth surfaces in contrast to the undisturbed rough surfaces surrounding the track. The resulting change in photometric properties occurs because the smoother surfaces have a higher reflectance compared to the surrounding rough surface, leading to bright DDTs. On Mars, the destruction of surficial dust-aggregates may also lead to bright DDTs. However, higher reflective surfaces may be produced by other formation mechanisms, such as dust compaction by passing dust devils, as this may also cause changes in photometric properties. On Mars, DDTs in general are found at all elevations and on a global scale, except on the permanent polar caps. DDT maximum areal densities occur during spring and summer in both hemispheres produced by an increase in dust devil activity caused by maximum insolation. Regionally, dust devil densities vary spatially likely controlled by changes in dust cover thicknesses and substrate materials. This variability makes it difficult to infer dust devil activity from DDT frequencies. Furthermore, only a fraction of dust devils leave tracks. However, DDTs can be used as proxies for dust devil lifetimes and wind directions and speeds, and they can also be used to predict lander or rover solar panel clearing events. Overall, the high DDT frequency in many areas on Mars leads to drastic albedo changes that affect large-scale weather patterns

Selection and characterization of conditionally active promotors in Lactobacillus plantarum, using alanine racemase as a promotor probe

This paper describes the use of the alr gene, encoding alanine racemase, as a promoter-screening tool for the identification of conditional promoters in Lactobacillus plantarum. Random fragments of the L. plantarum WCFS1 genome were cloned upstream of the promoterless alr gene of Lactococcus lactis in a low-copy-number plasmid vector. The resulting plasmid library was introduced into an L. plantarum Deltaalr strain (MD007), and 40,000 clones were selected. The genome coverage of the library was estimated to be 98%, based on nucleotide insert sequence and restriction analyses of the inserts of randomly selected clones. The library was screened for clones that were capable of complementing the D-alanine auxotroph phenotype of MD007 in media containing up to 10, 100, or 300 mug of the competitive Air inhibitor D-cycloserine per ml. Western blot analysis with polyclonal antibodies raised against lactococcal Air revealed that the Air production level required for growth increased in the presence of increasing concentrations Of D-cycloserine, adding a quantitative factor to the primarily qualitative nature of the alr complementation screen. Screening of the alr complementation library for clones that could grow only in the presence of 0.8 M NaCl resulted in the identification of eight clones that upon Western blot analysis showed significantly higher Air production under high-salt conditions than under low-salt conditions. These results established the effectiveness of the alanine racemase complementation screening method for the identification of promoters on their conditional or constitutive activity

Sequence, chromophore extraction and 3-D model of the photoactive yellow protein from Rhodobacter sphaeroides

The photoactive yellow protein (pyp) gene has been isolated from Rhodobacter sphaeroides by probing with a homologous PCR-product. A sequence analysis shows that this pyp gene encodes a 124 AA protein with 48% identity to the three known PYPs. Downstream from pyp, a number of adjacent open reading frames were identified, including a gene encoding a CoA-ligase homologue (pCL). This latter protein is proposed to be involved in PYP chromophore activation, required for attachment to the apoprotein. We have demonstrated the presence of the chromophoric group, previously identified in PYP from Ectothiorhodospira halophila as trans 4-hydroxy cinnamic acid, in phototrophically cultured R. sphaeroides cells by capillary zone electrophoresis. The basic structure of the chromophore binding pocket in PYP has been conserved, as shown by a 3D model of R. sphaeroides PYP, constructed by homology-based molecular modelling. In addition, this model shows that R. sphaeroides PYP contains a characteristic, positively charged patch

Maarten Prak, Catharina Lis, Jan Lucassen en Hugo Soly, Craft guilds in the early modern Low Countries. Work, power, and representation

Photoactive yellow protein (PYP) is a photoreceptor that has been isolated from three halophilic phototrophic purple bacteria. The PYP from Ectothiorhodospira halophila BN9626 is the only member for which the sequence has been reported at the DNA level. Here we describe the cloning and sequencing of the genes encoding the PYPs from E.halophila SL-1 (type strain) and Rhodospirillum salexigens. The latter protein contains, like the E.halophila PYP, the chromophore trans p-coumaric acid, as we show here with high performance capillary zone electrophoresis. Additionally, we present evidence for the presence of a gene encoding a PYP homolog in Rhodobacter sphaeroides, the first genetically well-characterized bacterium in which this photoreceptor has been identified. An ORF downstream of the pyp gene from E.halophila encodes an enzyme, which is proposed to be involved in the biosynthesis of the chromophore of PYP. The pyp gene from E.halophila was used for heterologous overexpression in both Escherichia coli and R.sphaeroides, aimed at the development of a holoPYP overexpression system (an intact PYP, containing the p-coumaric acid chromophore and displaying the 446 nm absorbance band). In both organisms the protein could be detected immunologically, but its yellow color was not observed. Molecular genetic construction of a histidine-tagged version of PYP led to its 2500-fold overproduction in E.coli and simplified purification of the heterologously produced apoprotein. HoloPYP could be reconstituted by the addition of p-coumaric anhydride to the histidine-tagged apoPYP (PYP lacking its chromophore). We propose to call the family of photoactive yellow proteins the xanthopsins, in analogy with the rhodopsins