4 resultados para Dual energy X-ray absorptiometry
em AMS Tesi di Dottorato - Alm@DL - Università di Bologna
Resumo:
Introduction:Persistent Hyperparathyroidism after transplantation (HPT),bone disease and vertebral fractures are an important clinical problem in renal transplant patients. Several factors such as renal osteodystrophy, immunosuppressive therapy, deficit/insufficiency Vitamin D may contribute to that.In literature are described different percentages of HPT, vertebral fractures and Osteoporosis/Osteopenia that may be due to the different therapy and to the different employ of steroid. We analyzed 90 patients who received a renal graft between 2005 e 2010. Patients and Methods: 44 male and 46 female. Average age 52,2± 10,1 years, follow-up 31,3±16,6 months, time on dialysis 37±29,6 months. Patients who had creatinine level greater than 2,5 mg/dl were excluded. Immunosuppressive therapy was based on basiliximab, steroids (1.6 to 2 mg/kg/day progressively reduced to 5 mg/day after 45 days from the transplantation) in all patients + calcineurin inhibitor+ mycophenolate mophetil/mycophenolic acid in 88,8% of patients or Everolimus± calcineurin inhibitor in the others. Patients were studied with X-ray of the spine, dual-energy-X-ray, PTH, 25(OH)VitD. Results: 41,1% had HPT; 41,1% had osteopenia at femoral neck and 36,7% at vertebral column; 16,7% had osteoporosis at femoral neck and 15,6% at vertebral column. 10 patients (11%) had vertebral fractures. Patients with normal bone mineral density, compared to those with osteoporosis/osteopenia, are more younger (average age 46,4±11,7 years vs 54.3±8,6); they have spent less time on dialysis (26,5±14,8 months vs 40,7±32,6) and they have values of 25(OH)VitD higher (22,1±7,6 ng/ml vs 17,8±8,5). Patients with vertebral fractures have values of 25(OH)VitD lowest (14,1±6,4 ng/ml vs 19,7±8,5) and they had transplant since more time (29,1±16,2 vs 48,1±8,7 months). There is a significant correlation between HPT and PTH pre transplantation; HPT and levels of VitD (p<0,05) Conclusion: Prevention of Bone disease and vertebral fractures after renal transplant includes: a)treatment before transplantation b)supplementation of vitamin D with cholecalciferol or calcidiol c)shorten the dialysis time.
Resumo:
Seyfert galaxies are the closest active galactic nuclei. As such, we can use
them to test the physical properties of the entire class of objects. To investigate
their general properties, I took advantage of different methods of data analysis. In
particular I used three different samples of objects, that, despite frequent overlaps,
have been chosen to best tackle different topics: the heterogeneous BeppoS AX
sample was thought to be optimized to test the average hard X-ray (E above 10 keV)
properties of nearby Seyfert galaxies; the X-CfA was thought the be optimized to
compare the properties of low-luminosity sources to the ones of higher luminosity
and, thus, it was also used to test the emission mechanism models; finally, the
XMM–Newton sample was extracted from the X-CfA sample so as to ensure a
truly unbiased and well defined sample of objects to define the average properties
of Seyfert galaxies.
Taking advantage of the broad-band coverage of the BeppoS AX MECS and
PDS instruments (between ~2-100 keV), I infer the average X-ray spectral propertiesof nearby Seyfert galaxies and in particular the photon index (
The gaseous environment of radio galaxies: a new perspective from high-resolution x-ray spectroscopy
Resumo:
It is known that massive black holes have a profound effect on the evolution of galaxies, and possibly on their formation by regulating the amount of gas available for the star formation. However, how black hole and galaxies communicate is still an open problem, depending on how much of the energy released interacts with the circumnuclear matter. In the last years, most studies of feedback have primarily focused on AGN jet/cavity systems in the most massive galaxy clusters. This thesis intends to investigate the feedback phenomena in radio--loud AGNs from a different perspective studying isolated radio galaxies, through high-resolution spectroscopy. In particular one NLRG and three BLRG are studied, searching for warm gas, both in emission and absorption, in the soft X-ray band. I show that the soft spectrum of 3C33 originates from gas photoionized by the central engine. I found for the first time WA in 3C382 and 3C390.3. I show that the observed warm emitter/absorbers is not uniform and probably located in the NLR. The detected WA is slow implying a mass outflow rate and kinetic luminosity always well below 1% the L(acc) as well as the P(jet). Finally the radio--loud properties are compared with those of type 1 RQ AGNs. A positive correlation is found between the mass outflow rate/kinetic luminosity, and the radio loudness. This seems to suggest that the presence of a radio source (the jet?) affects the distribution of the absorbing gas. Alternatively, if the gas distribution is similar in Seyferts and radio galaxies, the M(out) vs rl relation could simply indicate a major ejection of matter in the form of wind in powerful radio AGNs.
Resumo:
The hard X-ray band (10 - 100 keV) has been only observed so far by collimated and coded aperture mask instruments, with a sensitivity and an angular resolution lower than two orders of magnitude as respects the current X-ray focusing telescopes operating below 10 - 15 keV. The technological advance in X-ray mirrors and detection systems is now able to extend the X-ray focusing technique to the hard X-ray domain, filling the gap in terms of observational performances and providing a totally new deep view on some of the most energetic phenomena of the Universe. In order to reach a sensitivity of 1 muCrab in the 10 - 40 keV energy range, a great care in the background minimization is required, a common issue for all the hard X-ray focusing telescopes. In the present PhD thesis, a comprehensive analysis of the space radiation environment, the payload design and the resulting prompt X-ray background level is presented, with the aim of driving the feasibility study of the shielding system and assessing the scientific requirements of the future hard X-ray missions. A Geant4 based multi-mission background simulator, BoGEMMS, is developed to be applied to any high energy mission for which the shielding and instruments performances are required. It allows to interactively create a virtual model of the telescope and expose it to the space radiation environment, tracking the particles along their path and filtering the simulated background counts as a real observation in space. Its flexibility is exploited to evaluate the background spectra of the Simbol-X and NHXM mission, as well as the soft proton scattering by the X-ray optics and the selection of the best shielding configuration. Altough the Simbol-X and NHXM missions are the case studies of the background analysis, the obtained results can be generalized to any future hard X-ray telescope. For this reason, a simplified, ideal payload model is also used to select the major sources of background in LEO. All the results are original contributions to the assessment studies of the cited missions, as part of the background groups activities.