151,216 research outputs found

    Male patients commencing FOLFOX / FOLFIRI chemotherapy in 2014, descriptive statistics

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    Background: Metastatic colorectal cancer is an incurable illness; however the advent of chemotherapy has significantly improved survival and symptom control. FOLFOX and FOLFIRI are used at SPBOH as the standard of care for patients with metastatic disease. No statistical data is available on that cohort of patients; this study aims to establish a population data-set for patients on FOLFOX/FOLFIRI. Methods: This retrospective cross-sectional study included all patients on FOLFOX and FOLFIRI in 2014. Only male patients were included, data was retrospectively extracted from the ward’s logbook and ISOFT clinical manager. Cycle 1, 6 and 12 dates were documented. Data was analysed using clinically reliable statistical tools, all reported p-values were statistically significant at <0.05. Results: From a total of 108 patients, 4 patients were excluded from the analysis. The average age of patients was 65.2 years. The average length of 12 cycles was 24.5 weeks. 19% of patients had cycles longer than 7 months whereas only 10% lasted more than 8 months on treatment. 41% of patients dropped out before completing the full course with a complication and mortality rate of 17%. Patients on FOLFIRI were more likely to have their chemotherapy changed and were also more likely to have received previous treatment. Conclusion: Although chemotherapy increases survival in metastatic colorectal cancer we have to appreciate that many patients do not proceed smoothly with their treatment. Many of those patients are middle aged independent individuals, after-all the physician must draw the line at the appropriate time and focus on palliative care rather than continuing ineffectively with chemotherapy.peer-reviewe

    The space density of Compton-thick AGN at z~0.8 in the zCOSMOS-Bright Survey

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    The obscured accretion phase in BH growth is a key ingredient in many models linking the AGN activity with the evolution of their host galaxy. At present, a complete census of obscured AGN is still missing. The purpose of this work is to assess the reliability of the [NeV] emission line at 3426 A to pick up obscured AGN up to z~1 by assuming that [NeV] is a reliable proxy of the intrinsic AGN luminosity and using moderately deep X-ray data to characterize the amount of obscuration. A sample of 69 narrow-line (Type 2) AGN at z=0.65-1.20 were selected from the 20k-zCOSMOS Bright galaxy sample on the basis of the presence of the [NeV] emission. The X-ray properties of these galaxies were then derived using the Chandra-COSMOS coverage of the field; the X-ray-to-[NeV] flux ratio, coupled with X-ray spectral and stacking analyses, was then used to infer whether Compton-thin or Compton-thick absorption were present in these sources. Then the [NeV] luminosity function was computed to estimate the space density of Compton-thick (CT) AGN at z~0.8. Twenty-three sources were detected by Chandra, and their properties are consistent with moderate obscuration (on average, ~a few 10^{22} cm^-2). The X-ray properties of the remaining 46 X-ray undetected Type 2 AGN were derived using X-ray stacking analysis. Current data indicate that a fraction as high as ~40% of the present sample is likely to be CT. The space density of CT AGN with logL_2-10keV>43.5 at z=0.83 is (9.1+/-2.1) 10^{-6} Mpc^{-3}, in good agreement with both XRB model expectations and the previously measured space density for objects in a similar redshift and luminosity range. We regard our selection technique for CT AGN as clean but not complete, since even a mild extinction in the NLR can suppress [NeV] emission. Therefore, our estimate of their space density should be considered as a lower limit.Comment: 10 pages, 7 figures, 2 tables, A&A, in pres
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