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The article discusses the developments in excess insurance and reinsurance issues from October 1, 2015, through September 30, 2016 . Topics discussed include In re Viking Pump, Inc. on allocation and exhaustion on numerous insurance policies, equitable subrogation and unjust enrichment and discoverability of reinsurance information and arbitrator disclosures.

Current and prospective migration law and policy in Chile does not adequately incorporate the causes, content, and consequences of international migration to and from Chile. We describe and examine migration in-flows, out-flows, migration-related policies, and how those policies drive, and are driven by, notions of development in Chile. We explore contradictions in Chilean nascent migration policy currently under legislative review. We argue that it is imperative that migration, migration policy, and their relationship to development be discussed inclusively and transparently and be explicitly incorporated into the Chilean government's nascent migration and development legal policies and frameworks. [ABSTRACT FROM AUTHOR]

An introduction is presented in which the editor discusses various reports within the issue on topics including human trafficking, refugee resettlement in Tanzania, and migration and development of South Korean and Korean Chinese migrants.

A major debate continues about whether immigrants receive benefits by virtue of their attachment to ethnic communities and ethnic organizations. On one side of the controversy, a large body of literature suggests that the ethnic community, which often contains resources that promote immigrants' adaptation and assimilation, actually hinders adaptation because the resources of mainstream institutions are less accessible to immigrants (often because they are also minorities). On the opposite side of the argument, critics contend that the ethnic solidarity school emphasizes the positive effects of ethnic communities and ethnic organizations on immigrant populations, while ignoring many of the negative consequences of migrants' involvement in ethnic groups and ethnic institutions. The purpose of this article is to reconsider whether ethnic communities and ethnic institutions facilitate immigrants' socio-economic adaptation. Specifically, the study analyses the impact of ethnic organizations on public assistance utilization among South-East Asian and Eastern European refugees in the Chicago metropolitan area in the late 1980s. The paper proceeds in five stages. As a background to the overall study, the literature on ethnic communities and ethnic organizations is reviewed. This is followed by a discussion of the development of mutual assistance associations (MAAs) in the US. Third is a concise description of the data and methods. Fourth is a presentation of the results. The article concludes with an assessment of the implications of the findings and suggestions for future research. [ABSTRACT FROM AUTHOR]

This article examines the impact of various sociodemographic variables on refugees' employment propensities in the greater metropolitan Chicago area. It extends existing research and knowledge of forced migrants' labor force activities by exploring the impact of region of origin and refugees' access to support systems and organizations on employment retention and job maintenance. The analysis shows that refugees' labor force participation patterns and experiences are influenced differentially both by their background characteristics and by their exposure to U.S. assistance systems. Southeast Asian asylees are less successful in maintaining stable job placements when compared to their more socially advantaged and often more suitably placed Eastern European counterparts. Refugee self-help initiatives require greater empowerment and increased acceptance and status to assist other refugees in adjusting to the host society. [ABSTRACT FROM AUTHOR]

We present results of a Hubble Space Telescope (HST) UBVI -band study of star clusters in tidal tails, using new WFC3 and ACS imaging to complement existing WFPC2 data. We survey 12 tidal tails across seven merging systems, deriving ages and masses for 425 star cluster candidates (SCCs). The stacked mass distribution across all systems follows a power law of the form d N /d M  ∝  M β, with β = −2.02 ± 0.15, consistent with what is seen in other star-forming environments. GALEX and Swift UV imaging provide star formation rates (SFRs) for our tidal tails, which when compared with ages and masses of our SCCs, allows for a determination of the cluster formation efficiency (CFE). We find the CFE increases with increasing SFR surface density, matching the theoretical model. We confirm this fit down at SFR densities lower than previously measured (log ΣSFR (M⊙ yr−1 kpc−2) ≈ −4.2), as related to the CFE. We determine the half-light radii for a refined sample of 57 SCCs with our HST WFC3 and ACS imaging, and calculate their dynamical age, finding the majority of them to be gravitationally bound. We also provide evidence of only low-mass (<104 M⊙) cluster formation in our nearest galaxy, NGC 1487, consistent with the theory that this system is a dwarf merger. [ABSTRACT FROM AUTHOR]

The article discusses several decisions issued by U.S. federal and state courts between October 1, 2016, and September 30, 2017 concerning reinsurance industry. Topics discussed include reinsurer's liability in excess of the "Reinsurance Accepted" amount in a facultative certificate; interpretation of the facultative certificate; and the First Circuit's decision in the case "Mountain Valley Property, Inc. v. Applied Risk Services Inc." related to powers of arbitration panels.

Pediatric and adult high-grade gliomas (HGGs) frequently harbor PDGFRA alterations. We hypothesized that cotreatment with everolimus may improve the efficacy of dasatinib in PDGFRα-driven glioma through combinatorial synergism and increased tumor accumulation of dasatinib. We performed dose-response, synergism, P-glycoprotein inhibition, and pharmacokinetic studies in in vitro and in vivo human and mouse models of HGG. Six patients with recurrent PDGFRα-driven glioma were treated with dasatinib and everolimus. We found that dasatinib effectively inhibited the proliferation of mouse and human primary HGG cells with a variety of PDGFRA alterations. Dasatinib exhibited synergy with everolimus in the treatment of HGG cells at low nanomolar concentrations of both agents, with a reduction in mTOR signaling that persisted after dasatinib treatment alone. Prolonged exposure to everolimus significantly improved the CNS retention of dasatinib and extended the survival of PPK tumor-bearing mice (mutant TP53, mutant PDGFRA, H3K27M). Six pediatric patients with glioma tolerated this combination without significant adverse events, and 4 patients with recurrent disease (n = 4) had a median overall survival of 8.5 months. Our results show that the efficacy of dasatinib treatment of PDGFRα-driven HGG was enhanced with everolimus and suggest a promising route for improving targeted therapy for this patient population. [ABSTRACT FROM AUTHOR]

Purpose: Brain tumors have become the leading cause of cancer-related mortality in young patients. Novel effective therapies on the basis of the unique biology of each tumor are urgently needed. The goal of this study was to evaluate the feasibility, utility, and clinical impact of integrative clinical sequencing and genetic counseling in children and young adults with high-risk brain tumors. Patients and Methods: Fifty-two children and young adults with brain tumors designated by the treating neuro-oncologist to be high risk (> 25% chance for treatment failure; mean age, 10.2 years; range, 0 to 39 years) were enrolled in a prospective, observational, consecutive case series, in which participants underwent integrative clinical exome (tumor and germline DNA) and transcriptome (tumor RNA) sequencing and genetic counseling. Results were discussed in a multi-institutional brain tumor precision medicine teleconference. Results: Sequencing revealed a potentially actionable germline or tumor alteration in 25 (63%) of 40 tumors with adequate tissue, of which 21 (53%) resulted in an impact on treatment or change of diagnosis. Platelet-derived growth factor receptor or fibroblast growth factor receptor pathway alterations were seen in nine of 20 (45%) glial tumors. Eight (20%) sequenced tumors harbored an oncogenic fusion isolated on RNA sequencing. Seventeen of 20 patients (85%) with glial tumors were found to have a potentially actionable result, which resulted in change of therapy in 14 (70%) patients. Patients with recurrent brain tumors receiving targeted therapy had a median progression-free survival (from time on therapy) of 4 months. Conclusion: Selection of personalized agents for children and young adults with high-risk brain tumors on the basis of integrative clinical sequencing is feasible and resulted in a change in therapy in more than two thirds of children and young adults with high-risk glial tumors. [ABSTRACT FROM AUTHOR]

We have developed an observing programme using deep, multiband imaging to probe the chaotic regions of tidal tails in search of an underlying stellar population, using NGC 3256's 400 Myr twin tidal tails as a case study. These tails have different colours of u - g = 1.05 ± 0.07 and r - i = 0.13 ± 0.07 for NGC 3256W, and u - g = 1.26 ± 0.07 and r - i = 0.26 ± 0.07 for NGC 3256E, indicating different stellar populations. These colours correspond to simple stellar population ages of 288+11-54 and 841+125-157 Myr for NGC 3256W and NGC 3256E, respectively, suggesting that NGC 3256W's diffuse light is dominated by stars formed after the interaction, while light in NGC 3256E is primarily from stars that originated in the host galaxy. Using a mixed stellar population model, we break our diffuse light into two populations: one at 10 Gyr, representing stars pulled from the host galaxies, and a younger component, whose age is determined by fitting the model to the data. We find similar ages for the young populations of both tails (195-13+0 and 170-70+44 Myr for NGC 3256W and NGC 3256E, respectively), but a larger percentage of mass in the 10 Gyr population for NGC 3256E (98+1-3 per cent versus 90+5-6 per cent). Additionally, we detect 31 star cluster candidates in NGC 3256W and 19 in NGC 2356E, with median ages of 141 and 91 Myr, respectively. NGC 3256E contains several young (<10 Myr), low-mass objects with strong nebular emission, indicating a small, recent burst of star formation. [ABSTRACT FROM AUTHOR]

The peculiar spiral NGC 2782 is the result of a minor merger with a mass ratio ~4:1 occurring ~200 Myr ago. This merger produced a molecular and Hi-rich, optically bright eastern tail and an Hi-rich, optically faint western tail. Non-detection of CO in the western tail by Braine et al. suggested that star formation had not yet begun. However, deep UBVR and Hα narrowband images show evidence of recent star formation in the western tail, though it lacks massive star clusters and cluster complexes. Using Herschel PACS spectroscopy, we discover 158μm [Cii] emission at the location of the three most luminous Hα sources in the eastern tail, but not at the location of the even brighter Hα source in the western tail. The western tail is found to have a normal star formation efficiency (SFE), but the eastern tail has a low SFE. The lack of CO and [C ii] emission suggests that the western tail Hii region may have a low carbon abundance and be undergoing its first star formation. The western tail is more efficient at forming stars, but lacks massive clusters. We propose that the low SFE in the eastern tail may be due to its formation as a splash region where gas heating is important even though it has sufficient molecular and neutral gas to make massive star clusters. The western tail, which has lower gas surface density and does not form high-mass star clusters, is a tidally formed region where gravitational compression likely enhances star formation. [ABSTRACT FROM AUTHOR]

We present a spectroscopic survey of 21 young massive clusters and complexes and one tidal dwarf galaxy (TDG) candidate in Stephan's Quintet, an interacting compact group of galaxies. All of the selected targets lie outside the main galaxies of the system and are associated with tidal debris. We find clusters with ages between a few and 125 Myr and confirm the ages estimated through Hubble Space Telescope photometry by Fedotov et al., as well as their modeled interaction history of the Quintet. Many of the clusters are found to be relatively long-lived, given their spectrosopically derived ages, while their high masses suggest that they will likely evolve to eventually become intergalactic clusters. One cluster, T118, is particularly interesting, given its age (~125 Myr), high mass (~2 x 106 M☉), and position in the extreme outer end of the young tidal tail. This cluster appears to be quite extended (Reff ~ 12-15 pc) compared to clusters observed in galaxy disks (Reff ~ 3-4 pc), which confirms an effect we previously found in the tidal tails of NGC 3256, where clusters are similarly extended. We find that star and cluster formation can proceed at a continuous pace for at least ~150 Myr within the tidal debris of interacting galaxies. The spectrum of the TDG candidate is dominated by a young population (~7 Myr), and, assuming a single age for the entire region, has a mass of at least 106 M☉. [ABSTRACT FROM AUTHOR]