*Corresponding author: Department of Aquatic Animal Health, Faculty of Fishery Sciences, West Bengal University of Animal and Fishery Sciences, 5-Budherhat Road, Chakgaria, Panchasayar, P. O., Kolkata-700 094, West Bengal, India. Tel: +91 94333 68328 E-mail: [email protected] Foundation Project: Supported by the Indian Council of Agricultural Research, Government of India, New Delhi under th...

Virginia Cooperative Extension programs and employment are open to all, regardless of race, color, national origin, sex, religion, age, disability, political beliefs, sexual orientation, or marital or family status. An equal opportunity/affirmative action employer. Issued in furtherance of Cooperative Extension work, Virginia Polytechnic Institute and State University, Virginia State University...

Address for correspondence: Ewa Łoś-Rycharska MD, PhD, Department of Pediatrics, Allergology and Gastroenterology, Collegium Medicum in Bydgoszcz, Nicolaus Copernicus University, 9 Skłodowskiej-Curie St, 85-094 Bydgoszcz, Poland, phone: +48 52 585 48 50, e-mail: [email protected] Received: 23.01.2016, accepted: 20.03.2016. Comparison of results and clinical value of skin prick tests with syntheti...

1 This work has been supported in part by Found of Fundamental Investigations (Republic of Belarus), Grant ‹M96-094. Abstract A design of multiple-valued circuits based on the multiple-valued programmable logic arrays (MV PLA’s) by generalized disjunctive decomposition is presented. Main subjects are 1) Generalized disjunctive decomposition of multiple-valued functions using multiple-terminal m...

NuSTAR observed the black hole candidate XTE J1908+094 during its 2013 and 2019 outbursts. We use relativistic reflection to measure spin of through 19 different assumptions relxill flavors parameter combinations. The most favored model in terms Deviance Information Criterion (DIC) measures be , inclination degrees (1σ statistical errors). look at effects coronal geometry density accretion disk...

XTE J1908+094 is an X-ray transient that went into outburst in February 2002. After two months it reached a 2-250 keV peak flux of 1 to 2 × 10 erg cms. Circumstantial evidence points to an accreting galactic black hole as the origin of the the X-radiation: pulsations nor thermonuclear flashes were detected that would identify a neutron star and the spectrum was unusually hard for a neutron star...