منابع مشابه
The growth assessment of very low birth weight infant at corrected two years old
Background: The aim of this study was to determine the growth status of very low birth infant at corrected age of two years. Methods: This cross-sectional study was performed on all babies with birth weight ≤1500 gr without any congenital anomalies, genetic disturbance and chronic disease (e.g. cardiopulmonary insufficiency, cholestasis, malabsorption). They were called at corrected age 2 year...
متن کاملVery-Low-Birthweight Infants at
To determine whether history of chronic lung disease (CLD) in children born at very low birthweight (VLBW) confers additional risk for impaired health, growth, and neurodevelopment, 17 VLBW children born in 1984 who had CLD (requiring supplemental oxygen more than 30 days after birth) in infancy and 28 VLBW children who did not have CLD were assessed at age 7 years. Assessments included a medic...
متن کاملGrowth and very low birth weight.
Information on the likelihood of catch up growth in poorly grown very low birthweight children is sparse. The centiles for weight, height, and head circumference were recorded at both 2 and 5 years of age for 135 very low birthweight children and 42 normal birthweight children. At both ages significantly more children of very low birth weight were under the 10th centile for weight and height. C...
متن کاملFacial Texture Coding at Very Low Bit
| This paper treats the topic of how to eeciently represent facial textures, for model based coding of human face images. The scheme is based on the Karhunen-Lo eve transform and involves an elaborate normalization process that enhances PSNR with around 0.5 dB compared to normalization with scaling, translation and rotation. It also seems to augment the perceived visual quality. Furthermore , a...
متن کاملEvolution at Very Low and Zero Z
Rotation deeply affects the evolution of very metal poor massive stars. Indeed, even moderately rotating stars reach the break–up limit during the Main–Sequence (MS) phase, they evolve rapidly to the red after the core H–burning phase and important surface enrichment in CNO elements occurs at the supergiant stage. High rotation and the self enrichment in heavy elements Z tend to enhance the qua...
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ژورنال
عنوان ژورنال: Europhysics Letters (EPL)
سال: 1995
ISSN: 0295-5075,1286-4854
DOI: 10.1209/0295-5075/32/1/011