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Emission peak

Figure 3 Composite plot of 2 K excitonic spectra from 11 GaAs/Alo,3Gao 7AS quantum wells with different thicknesses. The well width of each is given next to its emission peak. Figure 3 Composite plot of 2 K excitonic spectra from 11 GaAs/Alo,3Gao 7AS quantum wells with different thicknesses. The well width of each is given next to its emission peak.
A quick analysis of Equation (77) shows that if the melt layer is thin (kd 1), the emission spectrum corresponds to an absorption spectrum. This means that the emission peaks occur at the same wave numbers as the absorption bands. In case of thick melt layers (kd 1) Equation (77) becomes the following expression ... [Pg.170]

Another notable feature of the in vivo bacterial luminescence is seen in their emission spectra. Although the emission peak of in vitro bacterial luminescence is normally at about 490 nm, the in vivo emission peaks of various bacterial species and strains are significantly shifted from 490 nm, ranging from the shortest wavelength of 472 nm to over 500 nm. Some expanded notes concerning in vivo bacterial luminescence are given below. [Pg.42]

The spectra of the luminescence of coelenterazine catalyzed by recombinant Renilla luciferase in the presence and absence of Renilla GFP are shown in Fig. 4.6.3 (Lorenz et al., 1991). Note that the luminescence intensity at the emission peak is increased more than... [Pg.149]

According to the Kuwabara-Wassink paper, the purified luciferin in aqueous neutral buffer solution showed an absorption maximum at 320 nm, and a fluorescence emission peak at 490 nm. The luminescence emission maximum measured with Airth s fungal luciferase system was 524 nm at pH 6.5, whereas the chemiluminescence emission maximum of the luciferin with H2O2 plus a droplet of strong NaOH plus ferrous sulfate was 542 nm. No information was reported on the chemical nature of the luciferin. [Pg.294]

Davenport et al. (1952) were unsuccessful in their attempts to restore the luminescence of the filtered aqueous extract of Luminodesmus. Hastings and Davenport (1957) saw a weak luminescence in their filtered aqueous extracts made from the acetone powder of the millipedes. They found that the luminescence is dependent on pH, with an optimum at about pH 8.9, and that the light intensity could be increased by 10-30% by adding ATP. Hastings and Davenport also measured the luminescence spectrum of live animals, finding an emission peak at 495 nm. [Pg.308]

When a photoprotein solution (1.3 ml) was shaken with ethanol (0.7 ml) containing one drop of concentrated HC1 and then the mixture was extracted twice with 2 ml each of ethyl acetate, about 75% of the chromophore was extracted into the ethyl acetate extract. The chromophore isolated showed an absorption peak at 398 nm in neutral methanol (Fig. 10.2.5). The isolated chromophore was practically non-fluorescent, like the native photoprotein. However, the acidification of a methanolic solution with HC1 resulted in a sharpening and two-fold increase of the 398 nm absorption peak, accompanied by the appearance of fluorescence. In aqueous 0.1 M HC1, two fluorescence emission peaks (595 nm and 650 nm) were found, together with a corresponding excitation peak (400 nm). Treatment of the 398 nm absorbing chromophore with 0.1 M NaOH resulted in a rapid loss of the 398 nm absorption peak. Dithionite did not affect the 398 peak, suggesting that the chromophore does not contain Fe3+. [Pg.313]

Luminescence of Pyrosoma. All species of the genus Pyrosoma (about 10 species) are bioluminescent. Pyrosoma is one of the few organisms reported to luminesce in response to light (Bowlby et al., 1990). The luminescence emission spectrum of Pyrosoma atlantica is bimodal according to Kampa and Boden (1957), with the primary peak near 482 nm, and the secondary near 525 nm. Swift et al. (1977) reported the emission maxima of two Pyrosoma species at 485 and 493 nm, respectively, and Bowlby et al. (1990) found an emission peak at 475 nm with P. atlantica. A corrected bioluminescence spectrum of P. atlantica (A.max 485 nm) reported by Herring (1983) is shown in Fig. 10.5.2. [Pg.320]

Its fluorescence showed two emission peaks, 564 nm and 626 nm the excitation peaks for the former emission peak were at 305 nm and 374 nm, and those for the latter were at 332 nm and 392 nm, indicating the presence of two different components in the preparation. It appears that the characteristics of the fluorescent proteins were altered by isolation and purification. [Pg.330]

Currently no information is available on the chemical nature of the luminescence reaction that causes the 479 and 469 nm emission peaks from A. scintillans and M. niger. [Pg.330]

The presence of a critical St content in ASt-x can also be seen in fluorescence spectra [29], This copolymer in aqueous solution shows an excimer emission peaking at 325 nra. As shown in Fig. 8, the intensity of the excimer emission increases, while the monomer emission decreases, with increasing St content. Eventually the excimer dominates the monomer emission at an St content of 72 mol%. The excimer emission becomes apparent at an St content of about 50 mol%, which agrees with the critical St content estimated by viscometry and NMR spectroscopy. The existence of the critical St content suggests the hydro-phobic self-aggregation to be a cooperative process. [Pg.67]

A mode is defined by ifs polarization, a geometrical extent equal to A /4 and time-bandwidth equal to unity. The population of mode is wl% near the emission peak ... [Pg.370]

Figures 3a-f show the emission and excitation spectra for all six humic fractions. The excitation and emission maxima are listed in Table III along with the maxima of the phase-resolved emission spectra. In each case the emission spectrum was scanned with the excitation maximum wavelength held constant, and the excitation spectrum was scanned with the emission maximum wavelength held constant. Several interesting features are noted. The two humic samples ( Figures 3a,b) each have two excitation maxima and it appears that a double peak has been merged into the emission scan as evidenced by the shoulder on the high energy side of the emission peak. Similarly it seems evident that the exaggerated shoulders in the emission spectra of all the fractions point to the inclusion of two emission peaks in each spectrum. This evidence suggests the presence of two chromophores in each humic fraction. Figures 3a-f show the emission and excitation spectra for all six humic fractions. The excitation and emission maxima are listed in Table III along with the maxima of the phase-resolved emission spectra. In each case the emission spectrum was scanned with the excitation maximum wavelength held constant, and the excitation spectrum was scanned with the emission maximum wavelength held constant. Several interesting features are noted. The two humic samples ( Figures 3a,b) each have two excitation maxima and it appears that a double peak has been merged into the emission scan as evidenced by the shoulder on the high energy side of the emission peak. Similarly it seems evident that the exaggerated shoulders in the emission spectra of all the fractions point to the inclusion of two emission peaks in each spectrum. This evidence suggests the presence of two chromophores in each humic fraction.
Poly(2-methoxy, 5-(2 -ethylhexyloxy)-1,4-phenylene vinylene) MEH-PPV Emission peak = 605 nm p-type doping by sulfuric acid (H2SO4) -type doping by sodium (electron donor) Iodine (I2) = electron acceptor = > oxidizing agent... [Pg.195]

Fig. 4. PL spectra as a function of emission peak energy (i.e., wavelength) measured at room temperature. Fig. 4. PL spectra as a function of emission peak energy (i.e., wavelength) measured at room temperature.

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See also in sourсe #XX -- [ Pg.101 ]




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