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Lipid Extraction from HeLa Cells, Quantification of Lipids, Formation of Large Unilamellar Vesicles (LUVs) by Extrusion and in vitro Protein-lipid Binding Assays, Analysis of the I...
Published 2016-10-01“…This article describes the protocols for 1) extraction of total lipids from eukaryotic cells using the method developed by Bligh and Dyer (1959), 2) the quantification of glycerophospholipids by gas chromatography after methanolysis, followed by 3) the formation of LUVs by extrusion, 4) protein-lipid binding assay, 5) analysis of the incubation product by transmission electron microscopy (TEM) and by flotation across a discontinuous sucrose gradient and finally, 6) analysis of the proteins by immunoblot and revelation of the glycerophospholipids by iodin fumigation.…”
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Scleral Buckling for Primary Retinal Detachment: Outcomes of Scleral Tunnels versus Scleral Sutures
Published 2021-07-01Get full text
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A Watershed-Segmentation-Based Improved Algorithm for Extracting Cultivated Land Boundaries
Published 2021-03-01“…The extraction accuracy was compared to the RGB color space using the <i>δ<sub>A</sub></i>, <i>δ<sub>P</sub></i>, and <i>K<sub>hat</sub></i>, that were improved by 76.92%, 62.01%, and 16.83%, respectively, in the Lab color space, while they were 55.79%, 49.67%, and 13.42% in the Luv color space. (4) Through the visual comparison, time efficiency, and segmentation accuracy, the comprehensive extraction effect using the proposed algorithm was obviously better than that of RGB color-based space algorithm. …”
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Measures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
Published 2010Journal article -
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Star forming galaxies at z ≈ 6 and reionization
Published 2006“…This declining comoving star formation rate (0.005 h70 M⊙ yr-1 Mpc-3 at z ≈ 6 at LUV > 0.1L* for a Salpeter IMF) poses an interesting challenge for models which suggest that LUV > 0.1L* star forming galaxies at z ≃ 6 reionized the universe. …”
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Further observational evidence for a critical ionizing luminosity in active galaxies
Published 2017“…Based upon the detection rate for z ≥ 0.1 associated absorption, we would expect approximately four detections. Of the 11 which have previously not been searched, there is sufficient source-frame optical/ultraviolet photometry to determine the ionizing photon rate for four. …”
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Atomic and molecular absorption in redshifted radio sources
Published 2017“…We report on a survey for associated H I 21-cm and OH 18-cm absorption with the Giant Metrewave Radio Telescope at redshifts z ≈ 0.2–0.4. Although the low-redshift selection ensures that our targets are below the critical ultraviolet luminosity (LUV ∼ 1023 W Hz−1), which is hypothesized to ionize all of the neutral gas in the host galaxy, we do not obtain any detection in the six sources searched. …”
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Precision diagnosis of burn injuries using imaging and predictive modeling for clinical applications
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Proteoliposomes for Studying Lipid-protein Interactions in Membranes in vitro
Published 2021-10-01“…This protocol describes the isolation of LHCII from leaves and details a four-step procedure to incorporate the detergent-solubilized membrane protein in large unilamellar vesicles (LUV). …”
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Neutrino nonstandard interactions and lepton flavor universality violation at SND@LHC via charm production
Published 2024-12-01“…Finally, we also study the effects of lepton universality violation (LUV) assuming that the new physics coupling is not lepton universal.…”
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The strong gravitationally lensed Herschel galaxy HLock01: Optical spectroscopy reveals a close galaxy merger with evidence of inflowing gas
Published 2018“…While the SMG appears very massive (M∗≃ 5 ×1011Mo), with a highly extinguished stellar component (AV≃ 4.3), the LBG is a young, lower-mass (M∗≃ 1 ×1010Mo), but still luminous (10 × LUV∗) satellite galaxy. …”
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Adduction of cholesterol 5,6-secosterol aldehyde to membrane-bound myelin basic protein exposes an immunodominant epitope.
Published 2011Journal article -
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Hubble Space Telescope imaging and keck spectroscopy of z approximate to 6 i-band dropout galaxies in the Advanced Camera for Surveys GOODS fields
Published 2004“…Using the rest-frame UV continuum from our six candidate z ∼ 6 galaxies from the GOODS-N field, we determine a lower limit to the unobscured volume-averaged global star formation rate at z ∼ 6 of (5.4 ± 2.2) × 10 -4 h70 M⊙ yr-1 Mpc-3. We find that the cosmic star formation density in Lyman break galaxies (LBGs) with unobscured star formation rates greater than 15 M⊙ yr-1 falls by a factor of 8 between z ∼ 3 and z ∼ 6. …”
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