by the same objective and transmitted through the multichroic mirror
onto a standard Olympus tube lens to create an intermediate image
at the exit of the microscope frame. This image was passed through
a multiband emission filter (FF01–440/521/607/694/809–25,
Semrock, USA) and was then directed into a magnifying telescope (Apo-Rodagon-N
105 mm, Qioptiq GmbH, Germany and Olympus’ wide field tube
lens with 180 mm focal length, #36–401, Edmund Optics, USA),
with two commercial direct vision prisms (117,240, Equascience, France)
placed within the infinity space between the lenses and mounted on
two motorized rotators (8MR190–2–28, Altechna UAB, Lithuania)
controlling the prisms’ angles around the optical axis. The
final image was acquired on a back illuminated sCMOS camera (Prime
BSI, Teledyne Photometrics, USA).
Image acquisition was coordinated
using micromanager software,43 (link) controlling
camera acquisition, laser excitation, XY stage location, and prism
rotator angles. The camera and laser excitation were synchronized
using an in-house-built TTL controller based on an Arduino Uno board
(Arduino AG, Italy).