Looking through the same lens: Shear calibration for LSST, Euclid, and WFIRST with stage 4 CMB lensing

The next-generation weak lensing surveys (i.e., LSST, Euclid, and WFIRST) will require exquisite control over systematic effects. In this paper, we address shear calibration and present the most realistic forecast to date for LSST/Euclid/WFIRST and CMB lensing from a stage 4 CMB experiment (“CMB S4”). We use the cosmolike code to simulate a joint analysis of all the two-point functions of galaxy density, galaxy shear, and CMB lensing convergence. We include the full Gaussian and non-Gaussian covariances and explore the resulting joint likelihood with Monte Carlo Markov chains. We constrain shear calibration biases while simultaneously varying cosmological parameters, galaxy biases, and photometric redshift uncertainties. We find that CMB lensing from CMB S4 enables the calibration of the shear biases down to 0.2%–3% in ten tomographic bins for LSST (below the ∼ 0.5 % requirements in most tomographic bins), down to 0.4%–2.4% in ten bins for Euclid, and 0.6%–3.2% in ten bins for WFIRST. For a given lensing survey, the method works best at high redshift where shear calibration is otherwise most challenging. This self-calibration is robust to Gaussian photometric redshift uncertainties and to a reasonable level of intrinsic alignment. It is also robust to changes in the beam and the effectiveness of the component separation of the CMB experiment, and slowly dependent on its depth, making it possible with third-generation CMB experiments such as AdvACT and SPT-3G, as well as the Simons Observatory

High-Frequency Density Oscillations from a Plasma Source Used for Simulating Low-Earth Orbit Plasma Environment

We present data from ground-based, vacuum-chamber tests demonstrating the ability to modulate the output of a plasma source capable of producing a low-Earth orbit (LEO) type plasma. We obtained plasma oscillations up to 2.5 kHz impingent on stationary test equipment, which corresponds to meter-level ionospheric structures in LEO. This plasma source is, therefore, suitable for developing scientific instruments that measure the LEO plasma environment, in situ, with meter-level spatial resolution. Measurements were made using a fixed-bias collector and an electrometer sampling at 40 kHz. A mechanical aperture was established at the output of the plasma source via two concentric grids. The outer grid was free to rotate in the azimuthal direction with respect to the fixed inner grid. An identical, alternating hole pattern in the two grids resulted in a variable aperture that cycles through 90 open/close cycles per revolution. The frequency of the plasma oscillations is limited by the mechanism used to spin the grids and the bearing assembly on which the grids rotate. Higher frequencies are obtainable by upgrading the drive mechanism, allowing the possibility of centimeter-level spatial resolution

The Development of Test Facilities for Induced, High-Frequency Plasma Instabilities

We present results from modifications to test facilities equipped with a plasma source capable of producing a LEO-type environment. The modifications impose an oscillation to the output, thus simulating ionospheric disturbance. The frequency of the oscillations is adjustable as well as the base-line output of the source. Test results indicate that the density of the plasma can be varied with minimal impact on other plasma properties such as electron temperature. It is, therefore, possible to simulate realistic plasma environments such as day/night transitions or localized turbulence. The modified source is an effective tool for testing space instruments in a relevant environment increasing the instruments technology readiness level

The location of international practices: what is human rights practice?

This article opens up space to challenge state-centrism about human rights practice. To do so, it presents and critically assesses four methods that can be used to determine who and/or what counts as a part of any international practice: the agreement method, which locates a practice by referring to speech acts that define it; the contextual method, which locates a practice by referring to the actions, meanings, and intentions of practitioners; the value method, which locates a practice by identifying a value or principle that the practice reflects or instantiates; and the purpose method, which locates a practice by constructing an account of the sociopolitical reason(s) for a practice's existence. The purpose method, based on an interpretation of Rawls' constructivism, is developed, in a way that focuses on practitioners' judgement-based reasons to assign responsibility for human rights to any state or non-state actor

Science Impacts of the SPHEREx All-Sky Optical to Near-Infrared Spectral Survey: Report of a Community Workshop Examining Extragalactic, Galactic, Stellar and Planetary Science

SPHEREx is a proposed SMEX mission selected for Phase A. SPHEREx will carry out the first all-sky spectral survey and provide for every 6.2" pixel a spectra between 0.75 and 4.18 $\mu$m [with R$\sim$41.4] and 4.18 and 5.00 $\mu$m [with R$\sim$135]. The SPHEREx team has proposed three specific science investigations to be carried out with this unique data set: cosmic inflation, interstellar and circumstellar ices, and the extra-galactic background light. It is readily apparent, however, that many other questions in astrophysics and planetary sciences could be addressed with the SPHEREx data. The SPHEREx team convened a community workshop in February 2016, with the intent of enlisting the aid of a larger group of scientists in defining these questions. This paper summarizes the rich and varied menu of investigations that was laid out. It includes studies of the composition of main belt and Trojan/Greek asteroids; mapping the zodiacal light with unprecedented spatial and spectral resolution; identifying and studying very low-metallicity stars; improving stellar parameters in order to better characterize transiting exoplanets; studying aliphatic and aromatic carbon-bearing molecules in the interstellar medium; mapping star formation rates in nearby galaxies; determining the redshift of clusters of galaxies; identifying high redshift quasars over the full sky; and providing a NIR spectrum for most eROSITA X-ray sources. All of these investigations, and others not listed here, can be carried out with the nominal all-sky spectra to be produced by SPHEREx. In addition, the workshop defined enhanced data products and user tools which would facilitate some of these scientific studies. Finally, the workshop noted the high degrees of synergy between SPHEREx and a number of other current or forthcoming programs, including JWST, WFIRST, Euclid, GAIA, K2/Kepler, TESS, eROSITA and LSST.Comment: Report of the First SPHEREx Community Workshop, http://spherex.caltech.edu/Workshop.html , 84 pages, 28 figure

Isolation, purification and partial characterisation of cancer procoagulant from placental amnion-chorion membranes and its role in angiogenesis inflammation and metastasis

Cancer procoagulant (EC 3.4.22.26) is an enzyme that is derived from tumour and foetal tissue, but not normal tissue. It is a direct activator of factor X and has been isolated from amnion-chorion membranes as well as from extracts and cells from human melanoma. The presence of cancer procoagulant has been associated with the malignant phenotype, as well as having a particularly high activity in metastatic cells. Cancer procoagulant activity is elevated in the serum of early stage breast cancer patients and decreased to normal in the advanced stages of the disease. In this study, cancer procoagulant was successfully isolated from amnion-chorion membranes and purified to homogeneity. The molecular weight of cancer procoagulant was determined using SDS-PAGE and was found to be 68 kDa. Cancer procoagulant was delipidated and it was shown that its activity was increased by the presence of lipids in a dose-dependent manner. Recovery of cancer procoagulant after delipidation is poor, consequently, a larger mass of sample is required to obtain sufficient amounts of delipidated material for N-terminal amino acid analysis. The optimum pH of cancer procoagulant was determined to be pH 8 and its optimal temperature was found to be 50°C. Novel synthetic substrates were designed to assay for cancer procoagulant activity. Currently, 2 potential candidates have been identified, namely, PQVR-AMC and AVSQSKP-AMC. Cancer procoagulant-induced expression of cytokines is differently modulated in the less aggressive MCF-7 cell line as compared to the metastatic and more aggressive MDA-MB-231 cell line. There are marked similarities in the inflammatory response produced by cancer procoagulant in hTERT-HDLEC and MDA-MB-231 cells, which are both associated with migratory capacity. Furthermore, cancer procoagulant-induced PDGF-β expression in hTERT-HDLEC and MDA-MB-231 cells could point to involvement of cancer procoagulant in wound healing and metastatic spread, respectively. Cancer procoagulant induced the motility of MDA-MB-231, MCF-7 and hTERT- cells in vitro in a time- and dose-dependent manner. Together, these results suggest that cancer procoagulant plays a role in the migration of breast cancer cells as well as the migration of endothelial cells

Purification and partial characterisation of cathepsin D from ostrich skeletal muscle, and its activity during meat maturation

Cathepsin D, a muscle proteinase, participates in lysosomally mediated protein degradation in vivo. This enzyme has been proposed to play a significant role in the postmortem proteolysis process apparently associated with tenderisation. The lack of data on the postmortem characteristics of ostrich meat, especially on the ageing process and its influence on meat tenderness, called for an investigation into this process. There is no data available for purified ostrich cathepsin D, and the aim of this study was, therefore, to isolate, purify and characterise cathepsin D from ostrich skeletal muscle and subsequently investigate the possible role that it may have in the tenderisation process of meat. Cathepsin D was successfully isolated and purified from ostrich skeletal muscle using pepstatin A-agarose chromatography. The purified enzyme was composed of two subunits (14 and 29kDa). The amino acid composition as well as the N-terminal amino acid sequence of both subunits were determined. Kinetic parameters (Km and Vm), thermodynamic parameters (Ea, ∆H, ∆S and ∆G) and functional characteristics (effect of pH, temperature and various inhibitors on cathepsin D activity) were determined and are reported in this study. Ostrich muscle cathepsin D showed a pH optimum of 4 and a temperature optimum of 45°C. The activity of cathepsin D was strongly inhibited by pepstatin A and DTT. Purified ostrich cathepsin D displayed kinetic and functional properties similar to previously reported values from various species. The effect of storage on the activity of cathepsin D was investigated over a 30 day period. It was established that substantial postmortem cathepsin D activity remained throughout the storage period, to implicate cathepsin D, fulfilling a possible role in meat maturation

The experiential salience of music in identity for singing teachers

Professional musicians with strong identities in music may also have a high degree of music in their identities. Accordingly, a rigid identification with work may be problematic for musicians, particularly when forces beyond their control change their work circumstances. In this study, we conducted semi-structured interviews with 10 singing teachers, representing a subset of professional musicians, and used interpretative phenomenological analysis (IPA) to explore the ways in which they enacted music in their identities. The framework of musical identities in action was used to interpret the findings, revealing the dynamic, embodied, and situated complexity of music in participants’ identities. Music had existential salience in the accounts of nine participants. Its salience resulted from the dynamic and situated presence of music across the lifespan, the literal embodiment of the singing voice, and the metaphorical embodiment of the presence of music in participants’ experiences. While a strong sense of music in people’s identities can promote lifelong engagement with music, if the emphasis on music is existential, the identity of a professional musician may be at risk when they are faced with an external threat to their livelihood. This is important knowledge for music educators and professional musicians’ career thinking

Becoming singular: Musical identity construction and maintenance through the lens of identity process theory

This study uses identity process theory to understand the social–psychological processes that motivate individuals to construct an identity in which music, singing, and singing teaching feature prominently. We conducted reflexive thematic analysis of semi-structured interviews with 10 Australian singing teachers (with an average age 60) to understand how they enacted identity principles that motivate identity construction and maintenance. Findings were captured in two themes: (1) ‘It has just been music’: Living a musical life is my destiny; (2) ‘I know my value’: Achieving goals in music and teaching is motivating. Participants’ consistent musical engagement across the lifespan satisfied the identity principles of continuity and positive distinctiveness. The identity principles of self-efficacy and self-esteem were satisfied through the social connections created with peers and through teaching singing; participants derived self-worth from celebrating and contributing to the success of others. Teaching singing was a way to become ‘singular’, that is, distinctive, and distinctively valued by the self and others. This article provides an example of how identity process theory can be applied in musical identities research to uncover new insights into the psychological processes of identity construction, with implications for understanding identity resilience and musical engagement across the lifespan