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100 w highpressure mercury burner

Manufactured by Olympus
Sourced in United States, Japan

The 100 W High-Pressure Mercury Burner is a laboratory equipment designed for producing high-intensity ultraviolet (UV) light. It operates using a mercury-vapor lamp that generates a broad spectrum of UV radiation when powered. The device is capable of producing 100 watts of electrical power.

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3 protocols using 100 w highpressure mercury burner

1

Brightfield and Fluorescence Microscopy of Microbubbles

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Brightfield and Fluorescence Microscopy were performed using a BX50 Upright Microscope (ACH 60X/0.80 ∞/0.17 objective) or a IX70 Inverted Microscope (ACH 60X/0.80 ∞/0.17 objective) with a 100 W HighPressure Mercury Burner, Olympus (Waltham, MA). A diluted sample of bubbles at 1 × 107 MB/mL was placed in a small well created by using high vacuum silicone grease, Dow Corning (Midland, MI), on a 25 × 75 × 1 mm microscope slide covered with a glass slide cover Fisher Scientific (Waltham, MA). Type A immersion oil (η = 150 cSt) was used for upright microscopy, and type FF immersion oil (η = 170 cSt) was used for inverted microscopy, Cargille Laboratories (Ceder Grove, NJ). The appropriate filters were used to separate DiO and DiD fluorescence. Images were acquired using a Rolera Bolt CMOS QImaging Camera (Surrey, British Columbia, Canada). Confocal microscopy was performed for select experiments using the UT Dallas Imaging Core Facility (Olympus FV3000RS).
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2

Characterization of PDLCs by Microscopy

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The PDLCs were characterized by brightfield and fluorescence microscopy with either a BX50 Upright Microscope (ACH 60X/0.80 ∞/0.17 objective) or an IX70 Inverted Microscope (ACH 60X/0.80 ∞/0.17 objective) with a 100 W High-Pressure Mercury Burner, Olympus (Waltham, MA, USA). Diluted samples of PDLCs were pipetted onto 25 × 75 × 1 mm microscope slides and placed under a glass coverslip (Fisher Scientific, Waltham, MA, USA) in preparation for imaging. The appropriate filters were used to separate DiO and DiD fluorescence. Microscopy pictures were acquired by a Rolera Bolt CMOS QImaging Camera (Surrey, BC, Canada). Images for both the PDLCs and the DBCO blocked negative control groups were acquired from three independent samples (n = 3) using ten images per sample.
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3

Quantifying Angiogenic Tube Formation

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Vessel formation was assessed at the aforementioned time points. Fluorescent images were captured utilizing an Olympus IX81 equipped with Disc Spinning Unit and a 100 W high-pressure mercury burner (Olympus America, Center Valley, PA), a Hamamatsu Orca II CCD camera (Hamamatsu Photonics, K.K., Hamamatsu City, Japan), and Metamorph Premier software (Molecular Devices, Sunnyvale, CA). Imaged beads were chosen at random provided that vessels emanating from a given bead did not form anastomoses with vessels from adjacent beads. Images from at least 30 beads per condition were captured over three separate trials at low magnification (4×) for each independent experiment and processed using the Angiogenesis Tube Formation module in Metamorph Premier (Molecular Devices). Each image was segmented and analyzed based on any tube-like pattern that falls within a specified minimum and maximum width of each segment above a contrast threshold. The total network length, the number of branch points, and number of segments were quantified.
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