Combining Information from Crosslinks and Monolinks in the Modeling of Protein Structures

Monolinks are produced in a chemical crosslinking mass spectrometry experiment and are more abundant than crosslinks. They convey residue exposure information, but so far have not been used in the modeling of protein structures. Here, we present the Monolink Depth Score (MoDS), for assessing structural models based on the depth of monolinked residues, corresponding to their distance to the nearest bulk water. Using simulated and reprocessed experimental data from the Proteomic Identification Database, we compare the performance of MoDS to MNXL, our previously developed score for assessing models based on crosslinking data. Our results show that MoDS can be used to effectively score models based on monolinks, and that a crosslink/monolink combined score (XLMO) leads to overall higher performance. The work strongly supports the use of monolink data in the context of integrative structure determination. We also present XLM-Tools, a program to assist in this effort, available at: https://github.com/Topf-Lab/XLM-Tools

Pituitary apoplexy following shoulder arthroplasty: a case report

<p>Abstract</p> <p>Introduction</p> <p>Pituitary apoplexy following a major surgical procedure is a catastrophic event and the diagnosis can be delayed in a previously asymptomatic patient. The decision on thromboprophylaxis in shoulder replacements in the absence of definite guidelines, rests on a careful clinical judgment.</p> <p>Case presentation</p> <p>A previously healthy 62-year-old Caucasian male patient who underwent shoulder arthroplasty developed hyponatremia resistant to correction with saline replacement. The patient had a positive family history of deep vein thrombosis and pulmonary embolism and heparin thromboprophylaxis was considered on clinical grounds. The patient developed hyponatremia resistant to conventional treatment and later developed ocular localizing signs with oculomotor nerve palsy. The diagnosis was delayed due to other confounding factors in the immediate post-operative period. Subsequent workup confirmed a pituitary adenoma with features of pituitary insufficiency. The patient was managed successfully on conservative lines with a multidisciplinary approach.</p> <p>Conclusions</p> <p>A high index of suspicion is required in the presence of isolated post-operative hyponatremia resistant to medical correction. A central cause, in particular pituitary adenoma, should be suspected early. Thromboprophylaxis in shoulder replacements needs careful consideration as it may be a contributory factor in precipitating this life-threatening condition.</p

Methods for Molecular Modelling of Protein Complexes.

Biological processes are often mediated by complexes formed between proteins and various biomolecules. The 3D structures of such protein-biomolecule complexes provide insights into the molecular mechanism of their action. The structure of these complexes can be predicted by various computational methods. Choosing an appropriate method for modelling depends on the category of biomolecule that a protein interacts with and the availability of structural information about the protein and its interacting partner. We intend for the contents of this chapter to serve as a guide as to what software would be the most appropriate for the type of data at hand and the kind of 3D complex structure required. Particularly, we have dealt with protein-small molecule ligand, protein-peptide, protein-protein, and protein-nucleic acid interactions.Most, if not all, model building protocols perform some sampling and scoring. Typically, several alternate conformations and configurations of the interactors are sampled. Each such sample is then scored for optimization. To boost the confidence in these predicted models, their assessment using other independent scoring schemes besides the inbuilt/default ones would prove to be helpful. This chapter also lists such software and serves as a guide to gauge the fidelity of modelled structures of biomolecular complexes

Adaptive Tracking of Angular Velocity for a Planar Rigid Body With Unknown Models for Inertia and Input Nonlinearity

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/57795/1/AdaptiveTrackingTACTTCST1D.pd

Triplet repeats in human genome: distribution and their association with genes and other genomic regions

Motivation: Simple sequence repeats (SSRs) or microsatellite repeats are found abundantly in many prokaryotic and eukaryotic genomes. Among SSRs, triplet repeats are of special significance because some of them have been linked to various genetic disorders. The objective of the study is to analyze the triplet repeats of complete human genome and to identify the genes that contain the triplet repeats in their coding region. The analysis will help us to identify the candidate genes that have potential for repeat expansion. Results: We have analyzed triplet repeats in the complete human genome from the publicly available sequences. Our analysis revealed that AGC and CCG repeat were predominantly present in the coding regions of the genome while UTRs and the upstream sequences contained CCG repeats in relative abundance. Analysis of density of triplet repeats (bp/Mb) revealed that AAT and AAC were the abundant repeats whereas ACT and ACG were the rare repeats found in human genome. We could identify about 2135 known or predicted genes that were associated with at least one of the triplet repeat types. A large proportion of putative transcripts that were identified by gene finding programs were found to be associated with triplet repeats. These transcripts will be the candidate genes for analysis of triplet repeat expansion and a possible association with disease phenotypes. Identification of 171 genes which contain a minimum of ten repeat units will be of particular interest in future in correlating their association with any disease phenotype due to the expansion potential of repeats present in them. The list of genes and other details of analysis are given in the online supplementary data (http://www.ingenovis.com/tripletrepeats)

Effect of inducers against tobamovirus infection in tomato and bell Pepper

Tomato and bell pepper seeds were treated with salicylic acid (50 mM), neem oil (5%) and Pseudomonas fluorescens (slurry). The seedlings were sprayed with salicylic acid (50 mM) and neem oil (5%). The concentration of Tomato mosaic tobamovirus (ToMV) and Tobacco mosaic tobamovirus (TMV) was assessed based on the number of local lesions on Nicotiana glutinosa. The results showed that the seed/seedling treatment with inducers reduced the number of local lesions when compared to untreated ones. Salicylic acid was an effective inducer

MRD: a microsatellite repeats database for prokaryotic and eukaryotic genomes

MRD is a database system to access the microsatellite repeats information of genomes such as archea, eubacteria, and other eukaryotic genomes whose sequence information is available in public domains. MRD stores information about simple tandemly repeated k-mer sequences where k= 1 to 6, i.e. monomer to hexamer. The web interface allows the users to search for the repeat of their interest and to know about the association of the repeat with genes and genomic regions in the specific organism. The data contains the abundance and distribution of microsatellites in the coding and non-coding regions of the genome. The exact location of repeats with respect to genomic regions of interest (such as UTR, exon, intron or intergenic regions) whichever is applicable to organism is highlighted. MRD is available on the World Wide Web at http://www.ccmb.res.in/mrd webcite and/or http://www.ingenovis.com/mrd webcite. The database is designed as an open-ended system to accommodate the microsatellite repeats information of other genomes whose complete sequences will be available in future through public domain

Retrieval Analysis of the Emission Spectrum of WASP-12b: Sensitivity of Outcomes to Prior Assumptions and Implications for Formation History

We analyze the emission spectrum of the hot Jupiter WASP-12b using our HELIOS-R retrieval code and HELIOS-K opacity calculator. When interpreting Hubble and Spitzer data, the retrieval outcomes are found to be prior-dominated. When the prior distributions of the molecular abundances are assumed to be log-uniform, the volume mixing ratio of HCN is found to be implausibly high. A VULCAN chemical kinetics model of WASP-12b suggests that chemical equilibrium is a reasonable assumption even when atmospheric mixing is implausibly rigorous. Guided by (exo)planet formation theory, we set Gaussian priors on the elemental abundances of carbon, oxygen, and nitrogen with the Gaussian peaks being centered on the measured C/H, O/H, and N/H values of the star. By enforcing chemical equilibrium, we find substellar O/H and stellar to slightly superstellar C/H for the dayside atmosphere of WASP-12b. The superstellar carbon-to-oxygen ratio is just above unity, regardless of whether clouds are included in the retrieval analysis, consistent with Madhusudhan et al. Furthermore, whether a temperature inversion exists in the atmosphere depends on one's assumption for the Gaussian width of the priors. Our retrieved posterior distributions are consistent with the formation of WASP-12b in a solar-composition protoplanetary disk, beyond the water iceline, via gravitational instability or pebble accretion (without core erosion) and migration inward to its present orbital location via a disk-free mechanism, and are inconsistent with both in situ formation and core accretion with disk migration, as predicted by Madhusudhan et al. We predict that the interpretation of James Webb Space Telescope WASP-12b data will not be prior-dominated

Methane in the atmosphere of the transiting hot Neptune GJ436b?

We present an analysis of seven primary transit observations of the hot Neptune GJ436b at 3.6, 4.5 and $8~\mu$m obtained with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. After correcting for systematic effects, we fitted the light curves using the Markov Chain Monte Carlo technique. Combining these new data with the EPOXI, HST and ground-based $V, I, H$ and $K_s$ published observations, the range $0.5-10~\mu$m can be covered. Due to the low level of activity of GJ436, the effect of starspots on the combination of transits at different epochs is negligible at the accuracy of the dataset. Representative climate models were calculated by using a three-dimensional, pseudo-spectral general circulation model with idealised thermal forcing. Simulated transit spectra of GJ436b were generated using line-by-line radiative transfer models including the opacities of the molecular species expected to be present in such a planetary atmosphere. A new, ab-initio calculated, linelist for hot ammonia has been used for the first time. The photometric data observed at multiple wavelengths can be interpreted with methane being the dominant absorption after molecular hydrogen, possibly with minor contributions from ammonia, water and other molecules. No clear evidence of carbon monoxide and dioxide is found from transit photometry. We discuss this result in the light of a recent paper where photochemical disequilibrium is hypothesised to interpret secondary transit photometric data. We show that the emission photometric data are not incompatible with the presence of abundant methane, but further spectroscopic data are desirable to confirm this scenario.Comment: 19 pages, 10 figures, 1 table, Astrophysical Journal in pres

Radiative Transfer for Exoplanet Atmospheres

Remote sensing of the atmospheres of distant worlds motivates a firm understanding of radiative transfer. In this review, we provide a pedagogical cookbook that describes the principal ingredients needed to perform a radiative transfer calculation and predict the spectrum of an exoplanet atmosphere, including solving the radiative transfer equation, calculating opacities (and chemistry), iterating for radiative equilibrium (or not), and adapting the output of the calculations to the astronomical observations. A review of the state of the art is performed, focusing on selected milestone papers. Outstanding issues, including the need to understand aerosols or clouds and elucidating the assumptions and caveats behind inversion methods, are discussed. A checklist is provided to assist referees/reviewers in their scrutiny of works involving radiative transfer. A table summarizing the methodology employed by past studies is provided.Comment: 7 pages, no figures, 1 table. Filled in missing information in references, main text unchange