Figure 3. Existence of mutual trust and commitment as facilitating factor of cooperation between company and HE institutions, by size of the company (in per cent)
Figure 3. 4: Total fraction of the ini- tial mass of an SSP ejected by AGB stars at time t = ∞ as a func- tion of initial stellar metal mass frac- tion, assuming the yields of van den Hoek & Groenewegen (1997) (black, thick lines), Marigo (2001) (red, medium thick lines), or Xxxxxx et al. (2004) (blue, thin lines). The calculations assume a Chabrier IMF and integrate the yields over a stel- lar initial mass range [0.8, 6] M⊙, but the fractions are normalized to the mass range [0.1, 100] M⊙. Differ- ent yield sets predict similar ejected mass fractions. The ejected mass fraction is insensitive to metallicity. puffs up and is eventually shed, causing the star to lose up to 60 % of its mass. Prior to the AGB phase, material in the core (where most of the heavy elements reside) is dredged up into the envelope via convection. As a result, the ejecta are particularly rich in carbon and nitrogen. Building on pioneering work by Xxxx & Xxxxxx (1978) and Xxxxxxx & Xxxx (1981), various groups have published AGB yields (x.x. Xxxxxxxxx & Xxxxxxxxxx 1997; xxx xxx Xxxx & Xxxxxxxxxxx 1997; Xxxxxx 2001; Xxxxxxx et al. 2001; Xxxxxxx et al. 2002; Xxxxxx et al. 2004). Table 3.3 outlines the extent of the resolution (in mass and metallicity) of the AGB yields of van den Hoek & Groenewegen (1997), Xxxxxx (2001) and Xxxxxx et al. (2004), which are some of the most complete sets for our purposes. These yields are compared in Fig. 3.3, which shows the abundance relative to hydrogen, in solar units6, of various elements in the ejecta as a function of stellar metallicity. These calculations are for an SSP with a Chabrier IMF and the mass range [0.8, 6] M⊙ at time t = ∞. The yields agree very well at solar metallicity, and for the case of helium, this agreement extends to lower metallicities. However, for nitrogen, oxygen, and particularly carbon, different yields sets give very different results at low metallicities. We show in Fig. 3.4, for each yield set, the integrated fraction of the initial SSP mass ejected by stars in the mass range [0.8, 6] M⊙ at time t = ∞, normalized to the total initial stellar mass over the range [0.1, 100] M⊙. The ejected mass fractions are very similar for the different yield sets. In this work we use the yields of Marigo (2001). Although these only go up to 5 M⊙, they form a complete set with the SN Type II yields of Portinari et al. (1998) since they are both based on the Padova evolutionary tracks. Indeed, there are very few yield pairings that form a consiste...
Figure 3. Author Manuscript Author Manuscript Author Manuscript Inter-rater agreement and intra-rater agreement for normative parameters at 60 ml balloon fill volume. All values showed good-to-excellent agreement. Inter- and intra-rater agreement data are presented as ICC and PCC (95% CI). ICC and PCC agreement: <0.40 (poor); 0.40–0.59 (fair); 0.6–0.74 (good); and 0.75–1.00 (excellent). Upper and lower limits of error bars represent the 95% CI. CI, confidence intervals; ICC, Intraclass correlation coefficient; PCC, Xxxxxxx’x correlation coefficient. Author Manuscript Author Manuscript Author Manuscript Author Manuscript Xxxxxxxxx et al.
Figure 3. All Databases Database Devices Archive Database in a Folder. File Viewer window only
Figure 3. 1: A graph of online resource allocation between SDs and the MEC servers. Per time-slot t, the mth SD receives the arriving workload bm and stores them in the queue qm. Then, the workload in the queue qm will be allocated to locally process dm and offload to the MEC servers amn, ∀n ∈ N . The nth MEC server receives the amount of workload ΣM amn and stores them in the queue qM+n. Finally, the nth MEC server executes the amount of zn out of the workload in its queue qM+n, which are recorded by local controller (LC).
Figure 3. 2.2.1.1 Some actors speak in favour of the creation of a platform grouping all of the calls for tenders related to PPAs The standard agreement prepared by FEE provides that the PPA may be entered into with or without a support mechanism. However, in practice, as explained below, companies would rather choose a PPA related to an installation that does not benefit from a support mechanism, so that they can benefit from GOs. The conditions precedent will naturally depend on the project maturity. The model chosen by FEE is that of a physical PPA, which relates to the selling of electricity, guarantees of origin, and xxxxx- xxx capacity certificates. Both the FEE standard agree- ment and the guide published by La Plateforme Verte are about bilateral GC PPAs only, i.e. GC PPAs entered into between a sole buyer and a sole producer. These standard agreements would have to be adapted in the event there are several customers and/or several producers.
2.2.2 The main contractual provisions and points of attention
Figure 3. N-Terminal protein sequencing of bovine neutrophil gelatinase-associated lipocalin (bNGAL). N-Terminal protein sequencing of bNGAL (20 µg) was performed by the automatic Xxxxx degradation procedure using an Applied Biosystems gas-phase sequencer, model 473A (Applied Biosystems, Foster City, CA). The sequencing result of bNGAL, presented by the standard one-letter code for AA, is aligned to the predicted sequence of bNGAL (National Center for Biotechnology Information: XP_605012) and published sequences of human neutrophil gelatinase-associated lipocalin (hNGAL), mouse 24p3/uterocalin (24p3), and rat α2-microglobulin-related protein (A2UMRP; Xxxxxxxx et al., 2000). The shaded box represents motif 1, a highly conserved sequence among lipocalins (Flower et al., 1991). bNGAL was N-linked glycosylated. Based on the aver- age Mr of 2,200 for a complex glycan (Xxxx et al., 1988), the difference in Mr of 2,000 observed on SDS-PAGE before and after deglycosylation suggests that mono- meric bNGAL (Mr 25,000) bears one N-linked glycan. Monosaccharide analysis of bNGAL showed the pres- ence of mannose, N-acetylgalactosamine, N-acetylglu- cosamine, and N-acetylneuraminic acid (Table 1). Fu- cose and galactose were hardly detected, which sug- gested that, in the event of N-linked glycosylation of bNGAL, galactose was substituted with N-acetylgalac- tosamine. This has previously been observed for other N-linked glycoproteins produced in bovine milk and has been ascribed to the presence of an N-acetylgalactosam- inyl transferase in mammary gland epithelium (Xxx xxx Xxxxxxxxxx et al., 1999). The MALDI-TOF analysis of desialylated bNGAL glycans showed 7 significant peaks (Figure 5, peaks A–G). The proposed glycan com- positions and structures, deduced from the mass-to- charge (m/z) values of 6 of these peaks, are shown in Table 2 and Figure 6, respectively. The observed m/z value of each proposed structure differs maximally by
Figure 3. 2 Xxx Xxxxx Fountain
Figure 3. Mindfulness as a buffer of the prospective relation between emotional distress and reported somatic symptoms: a SEModel
Figure 3. . a) Rolling mill components to be considered in the thermal crown model, b) Circular ring of roll
