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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

Semantic Scholar uses AI to extract papers important to this topic.
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… 
Highly Cited
2016
Highly Cited
2016
A novel voltammetric sensor for sensitive detection of mercury(II) ions using glassy carbon electrode modified with graphene-based ion imprinted polymer.
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… 
2013
2013
Borderline personality features and emotional reactivity: the mediating role of interpersonal vulnerabilities.
2012
2012
DNA- and RNA-binding and enhanced DNA-photocleavage properties of a ferrocenyl-containing ruthenium(II) complex.
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… 
Review
2010
Review
2010
SUPERNOVA 2009kf: AN ULTRAVIOLET BRIGHT TYPE IIP SUPERNOVA DISCOVERED WITH PAN-STARRS 1 AND GALEX
We present photometric and spectroscopic observations of a luminous Type IIP Supernova (SN) 2009kf discovered by the Pan-STARRS 1… 
2008
2008
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… 
Highly Cited
2005
Highly Cited
2005
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… 
2002
2002
Determination of Primordial Metallicity and Mixing in the Type II-P Supernova 1993W
We present the results of a large grid of synthetic spectra and compare them to early spectroscopic observations of SN 1993W… 
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