Showing 1,661 - 1,680 results of 3,030 for search '(((pinnau OR (pingna OR (pinn OR spine))) OR (fine OR line)) OR (pingk OR (pin OR ling)))', query time: 0.33s Refine Results
  1. 1661

    Orchestrations of the Malay habitus : Malay food consumption practices in cosmopolitan Singapore by Nurul Dina Amalina Abdulkahar

    Published 2015
    “…Singaporean Malays are frequently depicted as constituting a monolithic, insular and fiercely Muslim ethnic group due to the hard-line multicultural discourse perpetuated by the state prior to the national cosmopolitan project in 1999. …”
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    Final Year Project (FYP)
  2. 1662

    Performance of Singapore banking industry by Sin, Yang Fong, Tan, Siew Yean, Wong, Say Hui

    Published 2015
    “…This study attempts to determine whether Singapore is in a vantage position to exploit opportunities that arise by capitalising in the aforementioned strengths. The bottom line is : Singapore's financial sector must continue to push for greater innovation and professionalism, yet maintaining a safe and secure social structure.…”
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    Final Year Project (FYP)
  3. 1663

    Empowerment or Reinforcement of Gender Regime: Rethinking Social Enterprises’ Intentions and Impact through Gender Lens by Tymosiewicz, Natalia Elizabeth

    Published 2017
    “…Evidence presented also suggests selection of beneficiaries were often made in line with personal motivations, and entrepreneurs are moving beyond quantitative means of impact assessment. …”
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    Final Year Project (FYP)
  4. 1664

    A software system for business by Tan, Joel Jun Rong

    Published 2018
    “…This project is line with the national movement by the government to move towards a smart and cashless society. …”
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    Final Year Project (FYP)
  5. 1665

    Denoising ECG signals by Oh, Melissa Kai Zhen

    Published 2018
    “…ECG signal is known to have plenty of noise signal that corrupts its data, some of these noises are baseline wandering (BW), power-line interferences and electromyographic interferences (EMG). …”
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    Final Year Project (FYP)
  6. 1666

    Multipass steering protocols at Jefferson lab by Bodenstein, RM, Tiefenback, MG

    Published 2008
    “…We plan to characterize static and acceleration- dependent components of the beam line perturbations to allow systematic and rapid configuration of the accelerator at different linac energy gains.…”
    Conference item
  7. 1667

    Receiver design for the REACH global 21-cm signal experiment by Roque, ILV, Razavi-Ghods, N, Carey, SH, Ely, JA, Handley, W, Magro, A, Chiello, R, Huang, T, Alexander, P, Anstey, D, Bernardi, G, Bevins, HTJ, Cavillot, J, Croukamp, W, Cumner, J, de Lera Acedo, E, de Villiers, DIL, Fialkov, A, Gessey-Jones, T, Gueuning, Q, Josaitis, AT, Kulkarni, G, Leeney, SAK, Maiolino, R, Zarb-Adami, K

    Published 2025
    “…We detail the REACH radiometric system designed to enable measurements of the 21-cm neutral hydrogen line. Included is the radiometer architecture and end-to-end system simulations as well as a discussion of the challenges intrinsic to highly-calibratable system development. …”
    Journal article
  8. 1668

    Geometric grouping of repeated elements within images by Schaffalitzky, F, Zisserman, A

    Published 1999
    “…Also, information on the plane pose, such as its vanishing line, can be recovered from the grouping.…”
    Book section
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  17. 1677

    Characterization of nickel-titanium based thin films crystallized by fast and ultra-fast annealing methods by Motemani Sharabiani, Yahya

    Published 2012
    “…The decrease in transformation temperature is caused by the fine nano-scale structure in Ti-Ni-Hf thin samples. …”
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    Thesis
  18. 1678

    Nebular dominated galaxies: insights into the stellar initial mass function at high redshift by Cameron, AJ, Katz, H, Witten, C, Saxena, A, Laporte, N, Bunker, A

    Published 2024
    “…Modelling the UV turnover with a DLA requires extreme column densities (𝑁HI > 1023 cm−2 ), and simultaneously explaining the high 𝑓esc,Ly𝛼 requires a fine-tuned geometry. In contrast, modelling the spectrum as primarily nebular provides a good fit to both the continuum and emission lines, motivating scenarios in which (a) we are observing only nebular emission or (b) the ionizing source is powering extreme nebular emission that outshines the stellar emission. …”
    Journal article
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