Sökning: "IDL"
Visar resultat 1 - 5 av 10 uppsatser innehållade ordet IDL.
1. Validation of anti-cytokeratin antibodies used in rapid cancer diagnostics by isoelectric focusing and QCM technology
Uppsats för yrkesexamina på avancerad nivå, Uppsala universitet/BiokemiSammanfattning : Antibodies are Y-shaped proteins. In the human body, antibodies areproduced by plasma cells, mainly T and B cells which are included inthe adaptive immune system. The production of antibodies is stimulatedby antigens. The binding between an antigen-specific antibody and itsantigen can be like the interconnect between a lock and a key. LÄS MER
2. Measuring the Characteristic Sizes of Convection Structures in AGB Stars with Fourier Decomposition Analyses : the Stellar Intensity Analyzer (SIA) Pipeline.
Master-uppsats, Uppsala universitet/Teoretisk astrofysikSammanfattning : Context. Theoretical studies predict that the length scale of convection in stellar atmospheres isproportional to the pressure scale height, which implies that giant and supergiant stars should have convection granules of sizes comparable to their radii. LÄS MER
3. Analytical Method Development of Fluorinated Silanes using Mass Spectrometry
Kandidat-uppsats, Örebro universitet/Institutionen för naturvetenskap och teknikSammanfattning : The aim of this study was to develop an analytical method for fluorinated silanes. Furthermore, as a secondary aim, to explore if there would be possible to detect 1H,1H,2H,2H-perfluorooctyl triethoxysilane (6:2 PTrEtSi) and 1H,1H,2H,2H-perfluorodecyl triethoxysilane (8:2 PTrEtSi) in two different matrices, sludge and cosmetic extract. LÄS MER
4. Identification of elements and molecules in the spectra of an M dwarf star using high resolution infrared spectroscopy.
Kandidat-uppsats, Uppsala universitet/Institutionen för fysik och astronomiSammanfattning : M dwarfs are abundant and long-lived stellar objects. The formation of planets around stars in stellar systems is believed to be metallicity dependent. To determine the metallicity with synthetic spectrum analysis, the elements producing the absorption lines ofthe spectra first have to be identified. LÄS MER
5. Determining the effective temperature of cool stars from near-infrared spectra
Master-uppsats, Lunds universitet/Astronomi - Genomgår omorganisation; Lunds universitet/Institutionen för astronomi och teoretisk fysik - Genomgår omorganisationSammanfattning : Context. Effective temperature is one of the fundamental stellar parameters. A traditional spectroscopic way to determine it is from optical spectra using excitation balance of Fe-lines. LÄS MER