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Abstract:

BACKGROUND: Phenylalanine is converted to para- and ortho-tyrosine by hydroxyl free radical, or to para-tyrosine by the phenylalanine hydroxylase enzyme. The aim of this study was to measure para- and ortho-tyrosine in the urine and plasma of patients with chronic renal disease and/or diabetes, to obtain information on the renal handling of the different tyrosine isomers and, furthermore, to measure urinary levels of 8-epi-prostaglandin-F(2alpha), a marker of lipid peroxidation. METHODS: In our cross-sectional study we measured para-, ortho-tyrosine, and phenylalanine levels, using high performance liquid chromatography and 8-epi-prostaglandin-F(2alpha) with enzyme-linked immunosorbent assay (ELISA). We compared 4 groups: (1) controls (CONTR, N = 14), (2) patients with chronic kidney disease (CKD, N = 12), (3) patients with type 2 diabetes mellitus (DIAB, N = 17), (4) patients with chronic kidney disease and type 2 diabetes (DIAB-CKD, N = 19). RESULTS: We found a decreased plasma para-tyrosine level and decreased urinary para-tyrosine excretion in CKD patients, while the fractional excretion of para-tyrosine was similar in all 4 groups, approximately 1%. There was no difference in the plasma ortho-tyrosine levels between the groups. However, urinary ortho-tyrosine excretion was higher in all 3 groups of patients than in the CONTR group, and higher in DIAB and in DIAB-CKD patients than in CKD patients. The fractional excretion of ortho-tyrosine was significantly higher in DIAB and in DIAB-CKD patients than in the CONTR group. The fractional excretion of ortho-tyrosine exceeded 100% in the 2 diabetic groups. Urinary 8-epi-prostaglandin-F(2alpha)/creatinine ratio did not correlate with urinary ortho-tyrosine excretion. CONCLUSION: The difference between para-tyrosine levels of the groups is probably due to renal impairment, while there is indirect evidence for an increased tubular secretion or production of ortho-tyrosine in the kidney in diabetic patients with or without CKD.

Abstract:

We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandra/ACIS-I survey (Wang et al. 2002) towards the Galactic Centre (GC). These ~800 discrete sources, which contribute significantly to the GC X-ray emission, represent an important and previously unknown population within the Galaxy. From our VLT observations we will identify likely IR counterparts to a sample of the hardest sources, which are most likely X-ray binaries. With these data we can place constraints on the nature of the discrete weak X-ray source population of the GC.