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Csu w1 scan head

Manufactured by Oxford Instruments
Sourced in Japan

The CSU-W1 scan head is a component of Oxford Instruments' microscopy systems. It is designed to perform rapid, high-resolution scanning of samples. The CSU-W1 utilizes spinning disk confocal technology to enable fast, simultaneous multi-point illumination and detection. Its core function is to facilitate high-speed, high-sensitivity imaging of live samples.

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2 protocols using csu w1 scan head

1

Protrusion Dynamics in Transfected HFFs

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Time-lapse images of transfected HFFs in media at 10% CO2 and 37°C were captured using a spinning disk confocal microscope (Olympus iX83 base with a Yokagawa CSU-W1 scan head and an iXon Life 888 EM-CCD camera) with a 60×, 1.3 NA silicon oil objective. Lasers, 488 nm and 561 nm, excited GFP- and RFP-tagged proteins, respectively. One-hour treatments with 25 µM blebbistatin and/or 100 µM CK-666 were used to inhibit NMII and Arp2/3, respectively, in these live-cell imaging studies. Image stacks were imported into ImageJ 1.52s (NIH) to generate the kymographs for subsequent analysis. Three equally spaced measurements of protrusion dynamics were made for each kymograph analyzed using the KymographBuilder (v1.2.2) plugin in ImageJ.
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2

High-Resolution Live-Cell Imaging with FluidFM

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The FluidFM setup is composed of a FlexAFM 5-NIR scan head controlled by a C3000 controller (Nanosurf, Switzerland), a digital pressure controller (ranging from −800 mbar to +1,000 mbar) and Microfluidic Probes (Cytosurge). The scan head is mounted on an inverted AxioObserver microscope equipped with a temperature-controlled incubation chamber (Zeiss). The microscope is coupled to a spinning disk confocal microscope (Visitron, Germany) with a Yokogawa (Japan) CSU-W1 scan head and an EMCCD camera system (Andor, UK). For all images and videos, a 63× oil objective with 1.4 numerical aperture and a 2× lens switcher was used (without lens switcher: 4.85 pixel/micron and 9.69 pixel per micron with lens switcher); images are in 16 bit format. Image acquisition was controlled using the VisiView software (Visitron); linear adjustments and video editing were made with Fiji [67 (link)]; additionally, images and videos were noise-filtered using the wiener noise filtering function (wiener2; 3 by 3 neighborhood size) in MATLAB R2018a (MathWorks, USA). Movies were created using a self-written MATLAB script in order to visualize several sections or channels within the same movie. Colormaps originate from Thyng and colleagues [68 ]. Images of cantilevers containing extracts (Fig 2) were created summing up the slices of a Z-stack via Fiji and reconverting the image to 16 bit format.
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