0000000000447570

AUTHOR

Georgios Dimitriadis

showing 2 related works from this author

The effects of insulin on transport and metabolism of glucose in skeletal muscle from hyperthyroid and hypothyroid rats.

1997

The effects of insulin on the rates of glucose disposal were studied in soleus muscles isolated from hyper- or hypothyroid rats. Treatment with triiodothyronine for 5 or 10 days decreased the sensitivity of glycogen synthesis but increased the sensitivity of lactate formation to insulin. The sensitivity of 3-O methylglucose to insulin was increased only after 10 days of treatment and was accompanied by an increase in the sensitivity of 2-deoxyglucose phosphorylation; however, 2-deoxyglucose and glucose 6-phosphate in response to insulin remained unaltered. In hypothyroidism, insulin-stimulated rates of 3-O-methylglucose transport and 2-deoxyglucose phosphorylation were decreased; however, a…

Malemedicine.medical_specialtymedicine.medical_treatmentClinical BiochemistryBiological Transport ActiveBiologyCarbohydrate metabolismIn Vitro TechniquesBiochemistryHyperthyroidismDinoprostonechemistry.chemical_compoundHypothyroidismInternal medicinemedicineAnimalsInsulinGlycolysisDrug InteractionsLactic AcidPhosphorylationRats WistarGlycogen synthaseMuscle SkeletalHexokinaseInsulinGlucose transporterGeneral MedicineMetabolismRatsCortisoneEndocrinologyGlucosechemistryBasal (medicine)Growth Hormonebiology.proteinTriiodothyronineGlycolysisGlycogenEuropean journal of clinical investigation
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Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations

2019

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints on its progenitor system (Dimitriadis et al. 2018, Shappee et al. 2018b). Here, we present extensive optical, ultraviolet, and near-infrared photometry, as well as dense sampling of optical spectra, for this object. SN 2018oh is relatively normal in its photometric evolution, with a rise time of 18.3$\pm$0.3 days and $\Delta$m$_{15}(B)=0.96\pm$0.03 mag, but it seems to have bluer $B - V$ colors. We construct the "uvoir" bolometric light curve hav…

DATA RELEASEULTRAVIOLETFACTORY OBSERVATIONSFOS: Physical sciencesAstrophysicsType (model theory)medicine.disease_causeSN 2011FE01 natural sciencesLuminosityPhotometry (optics)individual (SN 2018oh) [supernovae]supernovae: generalCIRCUMSTELLAR MATERIAL0103 physical sciencesmedicineSPECTRAAbsorption (logic)Ejecta010303 astronomy & astrophysicssupernovae: individualQCSolar and Stellar Astrophysics (astro-ph.SR)QBLIGHT CURVESHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHIGH-VELOCITY FEATURES010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceIMPROVED DISTANCESWHITE-DWARF MODELSAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [supernovae]Ultraviolet
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