2005
DOI: 10.1097/01.mpg.0000181888.19974.6e
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Utilization of Esophageal Ph Monitoring and Adherence to Naspghan Guidelines at Children's Healthcare of Atlanata (Choa)

Abstract: Background: Although IgA endomysial antibodies (EMA) and tissue transglutaminase (TG) are sensitive and specific serologic tests for the diagnosis of celiac disease, there is limited information on the association of the magnitude of antibody level with the severity of the histological abnormalities of the intestine. Purpose: To determine if EMA and TG titers correlate with the severity of histological changes in patients with celiac disease. Methods: We identified 148 children from our laboratory database tha… Show more

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Cited by 6 publications
(9 citation statements)
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“…Baryons create a distinct oscillatory signature in the power spectrum of the large-scale structure of the universe (Peebles & Yu 1970;Bond & Efstathiou 1984;Holtzman 1989;Hu & Sugiyama 1996;Eisenstein & Hu 1998a). These baryonic acoustic oscillations have been seen in the anisotropies of cosmic microwave background (Miller et al 1999;de Bernardis et al 2000;Hanany et al 2000;Halverson et al 2002;Lee et al 2001;Netterfield et al 2002;Benoît et al 2003;Bennett et al 2003;Pearson et al 2003) and recently in large galaxy redshift surveys (Eisenstein et al 2005;Cole et al 2005). Because the density of baryons is less than that of cold dark matter, the oscillations in the matter power spectrum are weaker in amplitude than those in the cosmic microwave background (hereafter CMB).…”
Section: Introductionmentioning
confidence: 95%
“…Baryons create a distinct oscillatory signature in the power spectrum of the large-scale structure of the universe (Peebles & Yu 1970;Bond & Efstathiou 1984;Holtzman 1989;Hu & Sugiyama 1996;Eisenstein & Hu 1998a). These baryonic acoustic oscillations have been seen in the anisotropies of cosmic microwave background (Miller et al 1999;de Bernardis et al 2000;Hanany et al 2000;Halverson et al 2002;Lee et al 2001;Netterfield et al 2002;Benoît et al 2003;Bennett et al 2003;Pearson et al 2003) and recently in large galaxy redshift surveys (Eisenstein et al 2005;Cole et al 2005). Because the density of baryons is less than that of cold dark matter, the oscillations in the matter power spectrum are weaker in amplitude than those in the cosmic microwave background (hereafter CMB).…”
Section: Introductionmentioning
confidence: 95%
“…For example, we have not incorporated the SDSS results on luminous red galaxies (Eisenstein et al 2005). The recent final power spectrum and window functions of the 2dFGRS survey Cole et al (2005) is not yet available.…”
Section: The Lss Datamentioning
confidence: 99%
“…The features in the galaxy power spectrum (the broadband shape and baryon acoustic oscillations) (Peebles & Yu 1970;Bond & Efstathiou 1984;Holtzman 1989;Hu & Sugiyama 1996;Cole et al 2005;Eisenstein et al 2005;Huetsi 2005) can be used as CMB-calibrated standard rulers for determining the angular-diameter distance D(z) and constraining dark energy (Eisenstein, Hu, & Tegmark 1998;Blake & Glazebrook 2003;Hu & Haiman 2003;Linder 2003;SE03;Angulo et al 2005).…”
Section: Introductionmentioning
confidence: 99%