Results 41 to 50 of about 261,811 (317)
Error Assumptions on Generalized STAR Model
Journal of Mathematical and Fundamental Sciences, 2017 For GSTAR models, the least squares estimation method is commonly used since errors are assumed be uncorrelated. However, this method is not appropriate when errors are correlated, either in time or spatially.
Yundari +2 more
doaj +1 more source
Psychosocial Outcomes in Patients With Endocrine Tumor Syndromes: A Systematic Review
Pediatric Blood &Cancer, EarlyView.ABSTRACT Introduction The combination of disease manifestations, the familial burden, and varying penetrance of endocrine tumor syndromes (ETSs) is unique. This review aimed to portray and summarize available data on psychosocial outcomes in patients with ETSs and explore gaps and opportunities for future research and care.
Daniël Zwerus +6 more
wiley +1 more source
Extended relativistic hyperon star model [PDF]
Physical Review C, 2003 In this paper an equation of state of neutron star matter which includes strange baryons in the framework of Zimanyi and Moszkowski (ZM) model has been obtained. We concentrate on the effects of the isospin dependence of the equation of state constructing for the appropriate choices of parameters the hyperons star model.
Bednarek, I., Keska, M., Manka, R.
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Pediatric Blood &Cancer, EarlyView.ABSTRACT Purpose Metabolic syndrome (MetS) is a common complication in survivors of childhood acute lymphoblastic and myeloid leukemia (AL), and a major risk factor for premature cardiovascular disease, type‐2‐diabetes, and metabolic dysfunction‐associated steatotic liver disease (MASLD).
Visentin Sandrine +10 more
wiley +1 more source
Ground Testing Strategies for Verifying the Slew Rate Tolerance of Star Trackers
Sensors, 2014 The performance of a star tracker is largely based on the availability of its attitude solution. Several methods exist to assess star tracker availability under both static and dynamic imaging conditions.
Tom Dzamba, John Enright
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Model Atmospheres of Be Stars [PDF]
Symposium - International Astronomical Union, 1982 The basic concept of what a Be star is we owe to Struve (1931). His proposal that these stars are rapidly rotating and have an extended, disc-like, circumstellar envelope is still the basis for all models of Be stars. Unfortunately, progress in understanding the dynamics of Be stars has been painfully slow, a consequence of the very complex nature of ...
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Modelling neutron star mountains [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT As the era of gravitational-wave astronomy has well and truly begun, gravitational radiation from rotating neutron stars remains elusive. Rapidly spinning neutron stars are the main targets for continuous-wave searches since, according to general relativity, provided they are asymmetrically deformed, they will emit gravitational
F Gittins, N Andersson, D I Jones
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Pediatric Blood &Cancer, EarlyView.ABSTRACT Anaplastic sarcoma of the kidney (ASK) is a DICER1‐associated malignant tumor presumed to arise in a benign precursor, pediatric cystic nephroma (PCN). However, the initial oncogenic alteration(s) associated with malignant transformation are unknown.
Nahir Cortes‐Santiago +6 more
wiley +1 more source
Predictive modeling of treatment resistant depression using data from STAR*D and an independent clinical study. [PDF]
PLoS ONE, 2018 Identification of risk factors of treatment resistance may be useful to guide treatment selection, avoid inefficient trial-and-error, and improve major depressive disorder (MDD) care.
Zhi Nie +4 more
doaj +1 more source
Hydrodynamic model atmospheres for WR stars [PDF]
Astronomy & Astrophysics, 2005 accepted by A& ...
Gräfener, Götz +1 more
openaire +3 more sources