15n abundance
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2020 ◽  
Vol 98 (6) ◽  
Author(s):  
Gonzalo Cantalapiedra-Hijar ◽  
Pablo Guarnido ◽  
Anne-Marie Schiphorst ◽  
Richard J Robins ◽  
Gilles Renand ◽  
...  

Abstract Improving the ability of animals to convert feed resources into food for humans is needed for more sustainable livestock systems. Genetic selection for animals eating less while maintaining their performance (i.e., low residual feed intake [RFI]) appears a smart strategy but its effectiveness relies on high-throughput animal phenotyping. Here, we explored plasma nitrogen (N) isotope ratios in an attempt to identify easily superior young bulls in terms of RFI. For this, 48 Charolais young bulls fed two contrasting diets (corn vs. grass silage diets) were selected from a larger population as extreme RFI animals (24 low-RFI vs. 24 high-RFI) and their plasma analyzed for natural 15N abundance (δ15N) in the whole protein (bulk protein) and in the individual protein-bound amino acids (PbAA). For the first time, we showed that the δ 15N in plasma bulk protein differed (P = 0.007) between efficient (low-RFI) and inefficient (high-RFI) cattle regardless of diet. Furthermore, most analyzed PbAA followed the same trend as the bulk protein, with lower (P < 0.05) δ 15N values in more efficient (low-RFI) compared with less efficient (high-RFI) cattle, again regardless of diet. The only three exceptions were Phe, Met, and Lys (P > 0.05) for which the first metabolic reaction before being catabolized does not involve transamination, a pathway known naturally to enrich AAs in 15N. The contrasted isotopic signatures across RFI groups only in those PbAA undergoing transamination are interpreted as differences in transamination rates and N-use efficiency between low- and high-RFI phenotypes. Natural isotopic N signatures in bulk proteins and specific PbAA can be proposed as biomarkers of RFI in growing beef cattle fed different diets. However, the current study cannot delineate whether this effect only occurs post-absorption or to some extent also in the rumen. Our data support the conclusion that most efficient cattle in terms of RFI upregulate N conservation mechanisms compared with less efficient cattle and justify future research on this topic.


2020 ◽  
Vol 494 (1) ◽  
pp. 1095-1113 ◽  
Author(s):  
Fei Li ◽  
Junzhi Wang ◽  
Min Fang ◽  
Shanghuo Li ◽  
Zhi-Yu Zhang ◽  
...  

ABSTRACT We present 1 and 3 mm observations of the 13C- and 15N-bearing isotopologues of dense gas tracers towards eight nearby infrared-bright galaxies. With the Institut de Radioastronomie Millimétrique 30-m telescope, we observed the J  = 1–0 transitions of H13CN, HC15N, H13CO+, HN13C, and H15NC towards M 82, NGC 3079, IC 694, Mrk 231, and NGC 6240. The J  = 3–2 transition of H13CN was obtained in M 82, NGC 3079, NGC 3504, NGC 4418, NGC 6240, and NGC 6946, using the 10-m Submillimeter Telescope (SMT). We report the first detections of HN13C J  = 1–0 and H13CN J  = 3–2 in M 82, and H13CN J  = 3–2 in NGC 6240 and NGC 3079. We find different line profiles between the J  = 1–0 and 3–2 transitions of H13CN in both M 82 and NGC 3079. The optical depths of HCN show significant variations among the sample, indicating that dense gas masses estimated from the line luminosities of HCN J  = 1–0 and 3–2 should be treated with caution for individual galaxies. Optical depth of HCN J  = 3–2 is found to be higher than that of HCN J  = 1–0 in M 82, NGC 3079, NGC 4418, and NGC 6240, which indicates that ground state transitions of dense gas tracers might better trace the star-forming gas than the high-J transitions. Based on the H13CN/HC15N line ratios, with the double-isotopic method, low 14N/15N abundance ratios of 120 and 140 are found in NGC 3079 and Mrk 231, respectively.


CATENA ◽  
2019 ◽  
Vol 180 ◽  
pp. 8-15 ◽  
Author(s):  
Yu-Ping Dong ◽  
Hao Huang ◽  
Wei Song ◽  
Xin-Chao Sun ◽  
Min Wang ◽  
...  

Toxins ◽  
2019 ◽  
Vol 11 (4) ◽  
pp. 211 ◽  
Author(s):  
Wancui Xie ◽  
Min Li ◽  
Lin Song ◽  
Rui Zhang ◽  
Xiaoqun Hu ◽  
...  

The dinoflagellate Alexandrium minutum (A. minutum) which can produce paralyticshellfish toxins (PSTs) is often used as a model to study the migration, biotransformation,accumulation, and removal of PSTs. However, the mechanism is still unclear. To provide a new toolfor related studies, we tried to label PSTs metabolically with 15N stable isotope to obtain 15N-PSTsinstead of original 14N, which could be treated as biomarker on PSTs metabolism. We then culturedthe A. minutum AGY-H46 which produces toxins GTX1-4 in f/2 medium of different 15N/Pconcentrations. The 15N-PSTs’ toxicity and toxin profile were detected. Meanwhile, the 15N labelingabundance and 15N atom number of 15N-PSTs were identified. The 14N of PSTs produced by A.minutum can be successfully replaced by 15N, and the f/2 medium of standard 15N/P concentrationwas the best choice in terms of the species’ growth, PST profile, 15N labeling result and experimentcost. After many (>15) generations, the 15N abundance in PSTs extract reached 82.36%, and the 15Natom number introduced into GTX1-4 might be 4–6. This paper innovatively provided the initialevidence that 15N isotope application of labeling PSTs in A. minutum is feasible. The 15N-PSTs asbiomarker can be applied and provide further information on PSTs metabolism.


2017 ◽  
Vol 89 (11) ◽  
pp. 6076-6081 ◽  
Author(s):  
Wolfram Eschenbach ◽  
Dominika Lewicka-Szczebak ◽  
Claus Florian Stange ◽  
Jens Dyckmans ◽  
Reinhard Well

2016 ◽  
Vol 568 ◽  
pp. 52-56 ◽  
Author(s):  
Junjun Wu ◽  
Qian Zhang ◽  
Fan Yang ◽  
Yao lei ◽  
Quanfa Zhang ◽  
...  

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