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CONGENITAL DISORDER OF GLYCOSYLATION, TYPE IIp

Known as: CDG IIp, CDG2P, CDGIIp 
 
National Institutes of Health

Related topics

Related topics

4 relations
Autosomal recessive inheritanceHypercholesterolemiaLiver DysfunctionSteatohepatitis

Papers overview

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2017
2017
Magnetar Powered Ordinary Type IIP Supernovae
We investigate the properties of Type IIP supernovae that are dominantly powered by the rotational kinetic energy of the newly… Expand
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2016
2016
A novel voltammetric sensor for sensitive detection of mercury(II) ions using glassy carbon electrode modified with graphene-based ion imprinted polymer.
In this paper, a novel strategy was proposed to prepare ion-imprinted polymer (IIP) on the surface of reduced graphene oxide (RGO… Expand
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2014
2014
A semianalytical light curve model and its application to type IIP supernovae
The aim of this work is to present a semianalytical light curve model code that can be used for estimating physical properties of… Expand
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2013
2013
Type IIP supernova 2008in: the explosion of a normal red supergiant
Context. The explosion energy and the ejecta mass of a type IIP supernova make up the basis for the theory of explosion mechanism… Expand
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2012
2012
DNA- and RNA-binding and enhanced DNA-photocleavage properties of a ferrocenyl-containing ruthenium(II) complex.
The interaction of [Ru(bpy)(2)(fip)](PF(6))(2) {bpy=2,2'-bipyridine, fip=2-ferrocenyl-1H-imidazo[4,5-f][1,10]-phenanthroline… Expand
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2011
2011
Dimethylglyoxime based ion-imprinted polymer for the determination of Ni(II) ions from aqueous samples
A Ni(II)-dimethylglyoxime ion-imprinted polymer {Ni(II)-DMG IIP} was synthesised by the bulk polymerisation method. The… Expand
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2009
2009
Do the Photometric Colors of Type II-P Supernovae Allow Accurate Determination of Host Galaxy Extinction?
We present infrared photometry of supernova (SN) 1999em, plus optical photometry, infrared photometry, and optical spectroscopy… Expand
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Highly Cited
2006
Highly Cited
2006
Radio and X-Ray Emission as Probes of Type IIP Supernovae and Red Supergiant Mass Loss
Type IIP (plateau) supernovae are thought to come from stars with initial mass ~8-25 M☉ that end their lives as red supergiants… Expand
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Highly Cited
2006
Highly Cited
2006
Optical and infrared observations of the Type IIP SN2002hh from day 3 to 397
We present optical and infrared (IR) observations of the type IIP SN2002hh from 3 to 397 days after explosion. The optical… Expand
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2003
2003
Determination of primordial metallicity and mixing in the Type IIP supernova 1993W
We present the results of a large grid of synthetic spectra and compare them to early spectroscopic observations of SN 1993W… Expand
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