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  • Biochemistry and Biotechnology  (1)
  • Space Communications, Spacecraft Communications, Command and Tracking  (1)
  • 1
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Electrophoresis 14 (1993), S. 759-763 
    ISSN: 0173-0835
    Keywords: Chemistry ; Biochemistry and Biotechnology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology , Chemistry and Pharmacology
    Notes: Obtaining accurate molecular weight estimates for glycoproteins by sodium dodecyl sulfate-polyacrylamide gel electrophoresis (SDS-PAGE) has been difficult due to the lack of SDS binding by the carbohydrate moieties of the proteins. This leads to lower charge-to-mass ratios for SDS-glycoprotein complexes, resulting in over-estimation of molecular weights by SDS-PAGE. In order to minimize these inaccuracies for proteins with abnormal charge-to-mass ratios, a Ferguson plot may be employed. This application requires the determination of relative mobilities for standard proteins in addition to unknowns at several different gel concentrations. Historically, this technique has not been popular because it requires time-consuming preparation of gels with varying matrix concentrations, electrophoresis, and staining/destaining of gels. In this paper a procedure is demonstrated which automatically generates all of the data required for a Ferguson plot using a replaceable sieving matrix (thereby eliminating gel polymerization) in a capillary format. In addition, this technique possesses the advantages inherent to capillary electrophoresis, namely, very fast separation times, and on-line monitoring which allows quantitation and precludes post-separation staining and destaining of gels.
    Additional Material: 5 Ill.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-07-13
    Description: Millisecond pulsars (MSPs) are rapidly rotating neutron stars that appear to pulsate across the electromagnetic spectrum. Some MSPs have long-term timing stability that rivals that of atomic clocks. Pulse arrival phase can be predicted with great accuracy at any reference point in the Solar System through use of a pulsar timing model on a spacecraft. Comparing observed phase to predictions gives information that may be used in a navigation process. Why X-rays? Some stable MSPs have conveniently detectable X-ray emissions. X-rays are immune to interstellar dispersion effects thought to limit radio pulsar timing models. Highly directional compact detectors possible.
    Keywords: Space Communications, Spacecraft Communications, Command and Tracking
    Type: GSFC-E-DAA-TN51848 , Annual American Astronautical Society (AAS) Guidance and Control Conference 2018; Feb 02, 2018 - Feb 07, 2018; Breckenridge, CO; United States
    Format: application/pdf
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