A Note on Small Business Survival Rates in Rural Areas: The Case of Washington State

Using Washington State Department of Revenue and Employment Security Department data, this article uses non-parametric duration analysis to examine the nine-year time path of rural firm survival and hazard rates. The focus is on a cohort of rural firms that started operations in 1992; the cohort is followed up to the year 2000. Survival rates are estimated by using standard non-parametric (life-table) duration analysis. Using straightforward statistical tests, the study finds evidence that survival rates are statistically higher for firms that start as employers and for firms in the natural resource and service-based sectors. Copyright 2005 Blackwell Publishing Ltd..

Efficiency, Ownership and Market Structure, Corporate Control and Governance in the Turkish Banking Industry

Turkish banks are quite heterogeneous in terms of organizational form, ownership structure, size, age, portfolio concentration, growth prospects and attitude toward risk. They also exhibit strong variations in performance as measured by several efficiency indices. In the light of theoretical advances in corporate finance and financial institutions, this paper is an in-depth cross-sectional analysis of the Turkish banking sector, which explores the various bank, market and regulatory characteristics that may explain the efficiency variations across banks. Consistent with the related hypotheses investigated, the results indicate that a number of independent bank characteristics are significantly correlated with various efficiency measures. Copyright Blackwell Publishers Ltd, 2003.

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta