270 research outputs found
Utilidade da PET/CT, (18F-FDG), no estudo do linfoma Hodgkin e linfoma nĂŁo Hodgkin
Os linfomas sĂŁo tumores estabelecidos a nĂvel do sistema linfĂĄtico. Devido Ă sua heterogeneidade classificam-se como Linfoma Hodgkin (LH) e Linfoma nĂŁo Hodgkin (LNH), apresentando diferente prognĂłstico e seguimento quimioterapĂȘutico. Actualmente,
a Photon Emission Tomography/Computed Tomography (PET/CT, do acrĂłnimo inglĂȘs) Ă©
considerada âimagemâ de excelĂȘncia no estudo desta patologia. Neste contexto, Ă© objectivo
deste artigo verificar a utilidade da tĂ©cnica PET/CT e correlacionar o valor de Standard Uptake Value (SUV), obtido pela PET, com o estadio histolĂłgico do linfoma e com a resposta ao tratamento quimioterapĂȘutico. Metodologia - Analisaram-se retrospectivamente 356 estudos respeitantes a 231 pacientes, aos quais se realizou uma PET/CT para estadiamento, estudo de massa ou avaliação da resposta ao tratamento. ApĂłs a administração de uma
actividade média de 18F-FDG de 288,6 MBq, foram adquiridas imagens numa PET/CT GE
Discovery ST. Os resultados obtidos foram comparados com os dados clĂnicos dos pacientes. Resultados - Foram encontradas diferenças significativas entre a idade Vs tipo de linfoma. NĂŁo foram encontradas diferenças significativas entre: valor de SUVmĂĄx ganglionar, lesĂ”es extra-ganglionares e seu valor de SUV relativamente ao tipo de linfoma. Comprovou-se a influĂȘncia da PET/CT na alteração do estadio do linfoma e atitude terapĂȘutica. Em Ășltima anĂĄlise, obtiveram-se respectivamente os seguintes valores de sensibilidade, especificidade e exactidĂŁo: 98%, 79% e 88%. ConclusĂ”es - Os resultados obtidos permitem verificar a importĂąncia da imagem PET/CT no estadiamento, monitorização e alteração da atitude terapĂȘutica dos LH e LNH
New remarks on the Cosmological Argument
We present a formal analysis of the Cosmological Argument in its two main
forms: that due to Aquinas, and the revised version of the Kalam Cosmological
Argument more recently advocated by William Lane Craig. We formulate these two
arguments in such a way that each conclusion follows in first-order logic from
the corresponding assumptions. Our analysis shows that the conclusion which
follows for Aquinas is considerably weaker than what his aims demand. With
formalizations that are logically valid in hand, we reinterpret the natural
language versions of the premises and conclusions in terms of concepts of
causality consistent with (and used in) recent work in cosmology done by
physicists. In brief: the Kalam argument commits the fallacy of equivocation in
a way that seems beyond repair; two of the premises adopted by Aquinas seem
dubious when the terms `cause' and `causality' are interpreted in the context
of contemporary empirical science. Thus, while there are no problems with
whether the conclusions follow logically from their assumptions, the Kalam
argument is not viable, and the Aquinas argument does not imply a caused
origination of the universe. The assumptions of the latter are at best less
than obvious relative to recent work in the sciences. We conclude with mention
of a new argument that makes some positive modifications to an alternative
variation on Aquinas by Le Poidevin, which nonetheless seems rather weak.Comment: 12 pages, accepted for publication in International Journal for
Philosophy of Religio
Abundance determination in HII regions from spectra without the [OII]3727+3729 line
We suggest an empirical calibration for determination of oxygen and nitrogen
abundances and electron temperature in HII regions where the [OII]3727+3729
line (R_2) is not available. The calibration is based on the strong emission
lines of OIII, NII, and SII (NS calibration) and derived using the spectra of
HII regions with measured electron temperatures as calibration datapoints. The
NS calibration makes it possible to derive abundances for HII regions in nearby
galaxies from the SDSS spectra where R_2 line is out of the measured wavelength
range, but can also be used for the oxygen and nitrogen abundances
determinations in any HII region independently whether the nebular oxygen line
[OII]3727+3729 is available or not. The NS calibration provides reliable oxygen
and nitrogen abundances for HII regions over the whole range of metallicities.Comment: 6 pages, 4 figures, accepted for publication in the MNRA
2,2âČ-Dimethoxy-4,4âČ-[rel-(2R,3S)-2,3-diÂmethylbutane-1,4-diyl]diphenol
The title molÂecule, C20H26O4, commonly known as meso-dihydroÂguaiaretic acid, is a naturally occurring lignan extracted from Larrea tridentata and other plants. The molÂecule has a noncrystallographic inversion center situated at the midpoint of the central CâC bond, generating the meso stereoisomer. The central CâCâCâC alkyl chain displays an all-trans conformation, allowing an almost parallel arrangement of the benzene rings, which make a dihedral angle of 5.0â
(3)°. Both hydrÂoxy groups form weak OâHâŻOâH chains of hydrogen bonds along [100]. The resulting supraÂmolecular structure is an undulating plane parallel to (010)
The utility of PET/CT with 18F-FDG in the study of Hodgkin's lymphoma and non-Hodgkin's lymphoma
The lymphomas are tumors established in the lymphatic system. Due to their heterogeneity they can be classified as Hodgkin's lymphoma (HL) or non-Hodgkin's lymphoma (NHL), presenting each type of lymphoma, different prognosis and chemotherapeutic response. Currently Photon Emission Tomography/Computed Tomography (PET/CT) is considered as the "image" of excellence in the study of this pathology. In this context, it is of interest in this article to verify the usefulness of the PET/CT technique and to correlate the value of Standard Uptake Value (SUV) obtained by PET with the histological stage of lymphoma and the response to chemotherapeutic treatment. Methodology - We studied retrospectively 356 studies for 231 patients that did a PET/CT for staging, or evaluation of a mass or of the response to treatment. After administration of an average activity of 18F-FDG of 288.6 MBq, images were acquired on a PET/CT GE Discovery ST. These results were compared with clinical data of patients. Results - Significant differences were found between age vs type of lymphoma. No significant differences were found between: value of SUVmaxim nodes, extra-nodal lesions and their value of SUV for the type of lymphoma. It was verified the influence of PET/CT in the alteration of the stage of lymphoma as well as the therapeutic decision. Finally were found respectively the following values of sensitivity, specificity and accuracy: 98%, 79% and 88%. Conclusions - The results show the importance of imagingPET/CT in the evaluating the stage of the tumor and its role in monitoring and change of therapeutic decision
The bearable lightness of being
How are philosophical questions about what kinds of things there are to be understood and how are they to be answered? This paper defends broadly Fregean answers to these questions. Ontological categories-such as object, property, and relation-are explained in terms of a prior logical categorization of expressions, as singular terms, predicates of varying degree and level, etc. Questions about what kinds of object, property, etc., there are are, on this approach, reduce to questions about truth and logical form: for example, the question whether there are numbers is the question whether there are true atomic statements in which expressions function as singular terms which, if they have reference at all, stand for numbers, and the question whether there are properties of a given type is a question about whether there are meaningful predicates of an appropriate degree and level. This approach is defended against the objection that it must be wrong because makes what there depend on us or our language. Some problems confronting the Fregean approach-including Frege's notorious paradox of the concept horse-are addressed. It is argued that the approach results in a modest and sober deflationary understanding of ontological commitments
Multiple cycles of dose-intensive chemotherapy with repeated stem cell support as induction treatment in metastatic breast cancer: a feasibility study
The purpose of this trial was to study feasibility and tolerance of a dose-intensive multicyclic alternating induction chemotherapy with repeated stem cell support in a series of 43 metastatic breast cancer patients. Anthracycline-naive patients (n = 21) received cyclophosphamide 2.5 g/m2 plus doxorubicin 80 mg/m2 alternating every 14 days with paclitaxel 200-350 mg/m2 plus cisplatin 120 mg/m2. Patients who had previously received anthracyclines (n = 22) received cisplatin 120 mg/m2 plus etoposide 600 mg/m2 alternating with paclitaxel 200-350 mg/m2 plus ifosfamide 8 g/m2. Peripheral blood stem cells were infused after every course except the first, with a median CD34+ dose of 2.1 ÂŽ 106/kg per cycle. Positive selection of CD34+ cells was performed in good mobilizers. The median number of cycles administered was six (4-8), and the time interval between them was 17 days. Median summation dose intensities (SDI) actually administered for the CA-TP and PE-TI protocol were 4.95 and 4.69, respectively (87% of scheduled SDI). There were 15 complete (35%) and 21 partial responses (49%), for an overall response rate of 84% (95% CI, 73%-95%). Infection or neutropenic fever occurred in 50% of the cycles. There was one treatment-related death. After a median follow-up of 26 months, the median event-free-survival was 12 months (95% CI: 10-14) and overall survival was 31 months. These high dose-intensity induction treatments seem to be feasible with sequential stem cell support
The oxygen abundance distribution in M101
The well-observed spiral galaxy M101 was considered. The radial distributions
of oxygen abundances determined in three different ways (with the classic Te -
method, with the R23 - method, and with the P -- method) were compared. It was
found that the parameters (the central oxygen abundance and the gradient) of
the radial O/H(P) abundance distribution are close to those of the O/H(Te)
abundance distribution. The parameters of the O/H(R23) abundance distribution
differ significantly from those of the O/H(Te) abundance distribution: the
central O/H(R23) oxygen abundance is higher by around 0.4dex and the gradient
is steeper by a factor of around 1.5 as compared to those values in the O/H(Te)
abundance distribution.
The dispersion in O/H(P) abundance at fixed radius is rather small, around
0.08 dex, and is equal to that in O/H(Te) abundance. The dispersion in O/H(R23)
abundance at fixed radius is appreciably larger, around 0.16 dex, compared to
that in O/H(Te) abundance. It has been shown that the extra dispersion in
O/H(R23) abundances is an artifact and reflects scatter in excitation parameter
P at fixed radius.Comment: 7 pages, 5 figures, accepted for publication in Astronomy and
Astrophysic
"Counterpart" method for abundance determinations in HII regions
We suggest a new way of the determining abundances and electron temperatures
in HII regions from strong emission lines. Our approach is based on the
standard assumption that HII regions with similar intensities of strong
emission lines have similar physical properties and abundances. A "counterpart"
for a studied HII region may be chosen among HII regions with well-measured
abundances (reference HII regions) by comparison of carefully chosen
combinations of strong line intensities. Then the abundances in the
investigated HII region can be assumed to be the same as that in its
counterpart. In other words, we suggest to determine the abundances in HII
regions "by precedent". To get more reliable abundances for the considered HII
region, a number of reference HII regions is selected and then the abundances
in the target HII region is estimated through extra-/interpolation. We will
refer to this method of abundance determination as the counterpart method or,
for brevity, the C method. We define a sample of reference HII regions and
verify the validity of the C method. We find that this method produces reliable
abundances. Finally, the C method is used to obtain the radial abundance
distributions in the extended discs of the spiral galaxies M83, NGC4625 and NGC
628.Comment: 21 pages, 11 figures, accepted for publication in the MNRA
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