Cross-calibration of Suzaku XIS and XMM-Newton EPIC using clusters of galaxies

We extend a previous cross-calibration study by the International Astronomical Consortium for High Energy Calibration (IACHEC) on XMM-Newton/EPIC, Chandra/ACIS and BeppoSAX/MECS X-ray instruments with clusters of galaxies to Suzaku/XIS instruments. Our aim is to study the accuracy of the energy-dependent effective area calibration of the XIS instruments by comparison of spectroscopic temperatures, fluxes and fit residuals obtained with Suzaku/XIS and XMM-Newton/EPIC-pn for the same cluster. The temperatures measured in the hard 2.0-7.0 keV energy band with all instruments are consistent within 5 %. However, temperatures obtained with the XIS instruments in the soft 0.5-2.0 keV band disagree by 9-29 %. We investigated residuals in the XIS soft band, which showed that if XIS0 effective area shape is accurately calibrated, the effective areas of XIS1 and XIS3 are overestimated below 1.0 keV (or vice versa). Adjustments to the modelling of the column density of the XIS contaminant in the 3-6 arcmin extraction region while forcing consistent emission models in each instrument for a given cluster significantly improved the fits. The oxygen column density in XIS1 and XIS3 contaminant must be increased by 1-2E17 cm^-2 in comparison to the values implemented in the current calibration, while the column density of the XIS0 contaminant given by the analysis is consistent with the public calibration. XIS soft band temperatures obtained with the modification to the column density of the contaminant agree better with temperatures obtained with the EPIC-pn instrument of XMM-Newton, than with those derived using the Chandra-ACIS instrument. However, comparison of hard band fluxes obtained using Suzaku-XIS to fluxes obtained using the Chandra-ACIS and EPIC-pn instruments proved inconclusive.Comment: 24 pages, 27 figures, accepted for publication in Astronomy & Astrophysic

Modified Tapvei OÜ Stairs Induce an Anxiolytic Effect in Female C57BL/6 Mice in the Elevated Plus-Maze Test

We evaluated the effect of modified Tapvei OÜ stairs (stairs) on the behaviour of female C57BL/6 and BALB/c mice in the elevated plus-maze (EPM) test. The mice were kept under standard conditions for 4 weeks (control) or exposed to stairs for 3 or 4 weeks, and were assessed thereafter with the EPM. The C57BL/6 mice displayed less anxiety, when compared with the BALB/c mice. Exposure to stairs had an anxiolytic effect in C57BL/6 mice, but not in BALB/c. The strain-dependent effects of stairs should be considered in the design of housing refinements and behavioural experiments

Purification and characterization of a serine protease and chitinases from Paecilomyces lilacinus and detection of chitinase activity on 2D gels

The filamentous fungus Paecilomyces lilacinus is currently developed as a biocontrol agent against plant parasitic nematodes. Nematode eggs and cuticles are the infection sites for biocontrol agents that penetrate by the production of lytic enzymes. P. lilacinus was cultured in liquid media and proteases and chitinases were induced by the introduction of egg yolk and chitin, respectively. A serine protease was purified from a culture medium using Sepharose-bacitracin affinity column. The protease occurred in three forms, two of which were C-terminally truncated. Chitinase activity was also observed in the culture supernatant, and after separation by isoelectric focusing six proteins were detected that showed activity. Chitinase activity was further confirmed on non-denaturing one-dimensional (1D) and two-dimensional (2D) gels using a sandwich assay with glycol chitin as a substrate. Two of the proteins had similarities with endochitinases as shown by their N-terminal amino acid sequences. © 2003 Elsevier Inc. All rights reserved

XMM-Newton and INTEGRAL analysis of the Ophiuchus cluster of galaxies

We investigated the non-thermal hard X-ray emission in the Ophiuchus cluster of galaxies. Our aim was to characterise the physical properties of the non-thermal component and its interaction with the cosmic microwave background. We performed spatially resolved spectroscopy and imaging using XMM-Newton data to model the thermal emission. Combining this with INTEGRAL ISGRI data, we modeled the 0.6-140 keV band total emission in the central 7 arcmin region. The models that best describe both PN and ISGRI data contain a power-law component with a photon index in a range 2.2-2.5. This component produces ~10% of the total flux in the 1-10 keV band. The pressure of the non-thermal electrons is ~1% of that of the thermal electrons. Our results support the scenario whereby a relativistic electron population, which produces the recently detected radio mini-halo in Ophiuchus, also produces the hard X-rays via inverse compton scattering of the CMB photons. The best-fit models imply a differential momentum spectrum of the relativistic electrons with a slope of 3.4-4.0 and a magnetic field strength B=0.05-0.15 microG. The lack of evidence for a recent major merger in the Ophiuchus center allows the possibility that the relativistic electrons are produced by turbulence or hadronic collisions.Comment: Accepted for publication in Astronomy and Astrophysics, v2 includes some text improvement

Summary of the 13th IACHEC Meeting

We summarize the outcome of the 13th meeting of the International Astronomical Consortium for High Energy Calibration (IACHEC), held at Tenuta dei Ciclamini (Avigliano Umbro, Italy) in April 2018. Fifty-one scientists directly involved in the calibration of operational and future high-energy missions gathered during 3.5 days to discuss the current status of the X-ray payload inter-calibration and possible approaches to improve it. This summary consists of reports from the various working groups with topics ranging from the identification and characterization of standard calibration sources, multi-observatory cross-calibration campaigns, appropriate and new statistical techniques, calibration of instruments and characterization of background, and communication and preservation of knowledge and results for the benefit of the astronomical community.Comment: 12 page

A Conscious Porcine Model for Sudden Cardiac Death

No abstract availabl

Biogeochemical cycling and ecological thresholds in a High Arctic lake (Svalbard)

Lakes are a dominant feature of the Arctic landscape and a focal point of regional and global biogeochemical cycling. We collected a sediment core from a High Arctic Lake in southwestern Svalbard for multiproxy paleolimnological analysis. The aim was to find linkages between the terrestrial and aquatic environments in the context of climate change to understand centennial-long Arctic biogeochemical cycling and environmental dynamics. Two significant thresholds in elemental cycling were found based on sediment physical and biogeochemical proxies that were associated with the end of the cold Little Ice Age and the recent warming. We found major shifts in diatom, chironomid and cladoceran communities and their functionality that coincided with increased summer temperatures since the 1950s. We also discovered paleoecological evidence that point toward expanded bird (Little Auk) colonies in the catchment alongside climate warming. Apparently, climate-driven increase in glacier melt water delivery as well as a prolonged snow- and ice-free period have increased the transport of mineral matter from the catchment, causing significant water turbidity and disappearance of several planktonic diatoms and clear-water chironomids. We also found sedimentary accumulation of microplastic particles following the increase in Little Auk populations suggesting that seabirds potentially act as biovectors for plastic contamination. Our study demonstrates the diverse nature of climate-driven changes in the Arctic lacustrine environment with increased inorganic input from the more exposed catchment, larger nutrient delivery from the increased bird colonies at the surrounding mountain summits and subsequent alterations in aquatic communities.Peer reviewe

XMM−NewtonXMM-Newton Ω\Omega project: III. Gas mass fraction shape in high redshift clusters

We study the gas mass fraction, $f\_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f\_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low redshift quite well. This result is consistent with the gravitational instability picture leading to self similar structures for both the dark and baryonic matter. However, the mean $f\_{\rm gas} in distant clusters shows some differences to local ones, indicating a departure from strict scaling. This result is consistent with the observed evolution in the luminosity-temperature relation. We quantitatively investigate this departure from scaling laws. Within the local sample we used, a moderate but clear variation of the amplitude of the gas mass fraction with temperature is found, a trend that weakens in the outer regions. These variations do not explain departure from scaling laws of our distant clusters. An important implication of our results is that the gas fraction evolution, a test of the cosmological parameters, can lead to biased values when applied at radii smaller than the virial radius. From our$XMM$ clusters, the apparent gas fraction at the virial radius is consistent with a non-evolving universal value in a high matter density model and not with a concordance.Comment: Accepted, A&A, in pres