Table 1.

Summary of metrics and troubleshooting

Monitoring points (measuring frequency)MetricsLimit valuesPossible reasons for out of limit values: Proposed solutions
Point spread function (once per mo) FWHM XY exp/theory <1.5 Dirty or damaged objective: Meticulous front lens cleaning.
Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Pinhole and collimator lens misalignment (LSCM): Check the alignment.
Optical aberrations: Check the manufacturer correction specifications (APO, PlanAPO…); remove DIC or additional lens from the light path; clean optical elements in the light path; regulate correction collar for NA, temperature, or cover slip thickness.
Sample: Adjust stage and sample flatness; choose #1.5 (0.17 mm thick) cover slip; image beads near cover slip; use appropriate mounting or immersion medium at the right temperature; make sure there are no bubbles in the immersion oil.
Vibrations-drifts: Use an anti-vibration optical table and regulate air pressure properly; do a short time-lapse of a single bead.
Galvanometric scanners (LSCM): Calibrate bidirectional mode; check at mono-directional mode.
Excitation light alignment and polarization: Check sources coalignment and inspect light guide (polarization, bends). 
FWHM Z exp/theory <1.5 
LAR Case-dependent illumination source 
Field illumination (twice per yr) Uniformity (U) >50% Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Large camera sensor chip size (WF, SDCM): Crop the central field of view of the camera sensor chip.
Incorrect position of the field diaphragm (WF): Centering of the field diaphragm.
Sources and system alignment: Adjusting the collector lens or liquid light guide position; checking possible bending of the optical fibers; coalignment of the light sources; pinhole alignment; beam size at the back focal plane of the objective.
UV misalignment: Check the manufacturers’ correction specifications of the optical path components. 
Centering (C) >20% 
Co-registration (twice per yr) Ratio rexp/rref Chromatic aberrations: Check the constructor correction specifications of the considered lens (APO, PlanAPO…).
Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Sources and system alignment: Dichroic mirror and filter positions; additional lenses and light sources alignment.
Micro-lenses disk (SDCM): Check the constructor correction specifications of the optical path components. 
Illumination power stability (once per yr) Stability STABpower >97% Laser dying: Thorough check by the constructor.
Electrical instabilities: AC-powered light source; check the power grid stability of the room.
Environmental variations (thermal, air flow, humidity...): General verification of environmental and vibration conditions.
Fiber polarization: Check the bends of the optical fibers; proper alignment of laser in fiber.
Defective optical components (AOTF, AOM, fiber): Thorough check by the constructor. 

SDnormalized intensity 
<0.2 
Stage drift (once per yr) Va: Mean velocity after stabilization [0–50] nm/min Environmental variations (thermal, air flow, humidity...): General verification of environmental conditions; protect the stage from thermal shifts (cover, temperature-controlled chamber, or incubator); let the stage stabilize before starting experiments.
Stage control components not properly working: Check joystick at “no move” position, check controller status.
Mechanical instability: Tighten the mechanical elements; thorough check by the constructor. 
Vb: Mean velocity before stabilization [0–100] nm/min 
τstab <120 min 
Stage positioning repeatability (once per yr) σpositioning deviation Stage specifications Environmental variations (thermal, air flow, humidity...): General verification of environmental conditions.
Mechanical instability: Clean pieces of broken cover slip; tighten mechanical elements; thorough check by the constructor.
Objective touches sample insert if position far from center: Change insert or limit movements to central positions.
Not enough oil on the objective: Add enough oil beneath the whole sample before starting an experiment.
Stage drift: Let the stage stabilize before starting a multiposition experiment. 
Camera read noise (once per yr) VAR
STABnoise 
>90%
>97% 
Electronics issue; detector temperature; detector aging; cosmic rays: Thorough check by the constructor. 
Monitoring points (measuring frequency)MetricsLimit valuesPossible reasons for out of limit values: Proposed solutions
Point spread function (once per mo) FWHM XY exp/theory <1.5 Dirty or damaged objective: Meticulous front lens cleaning.
Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Pinhole and collimator lens misalignment (LSCM): Check the alignment.
Optical aberrations: Check the manufacturer correction specifications (APO, PlanAPO…); remove DIC or additional lens from the light path; clean optical elements in the light path; regulate correction collar for NA, temperature, or cover slip thickness.
Sample: Adjust stage and sample flatness; choose #1.5 (0.17 mm thick) cover slip; image beads near cover slip; use appropriate mounting or immersion medium at the right temperature; make sure there are no bubbles in the immersion oil.
Vibrations-drifts: Use an anti-vibration optical table and regulate air pressure properly; do a short time-lapse of a single bead.
Galvanometric scanners (LSCM): Calibrate bidirectional mode; check at mono-directional mode.
Excitation light alignment and polarization: Check sources coalignment and inspect light guide (polarization, bends). 
FWHM Z exp/theory <1.5 
LAR Case-dependent illumination source 
Field illumination (twice per yr) Uniformity (U) >50% Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Large camera sensor chip size (WF, SDCM): Crop the central field of view of the camera sensor chip.
Incorrect position of the field diaphragm (WF): Centering of the field diaphragm.
Sources and system alignment: Adjusting the collector lens or liquid light guide position; checking possible bending of the optical fibers; coalignment of the light sources; pinhole alignment; beam size at the back focal plane of the objective.
UV misalignment: Check the manufacturers’ correction specifications of the optical path components. 
Centering (C) >20% 
Co-registration (twice per yr) Ratio rexp/rref Chromatic aberrations: Check the constructor correction specifications of the considered lens (APO, PlanAPO…).
Damaged objective: Close examination of the front lens (scratches, lens detachment); send to repair.
Sources and system alignment: Dichroic mirror and filter positions; additional lenses and light sources alignment.
Micro-lenses disk (SDCM): Check the constructor correction specifications of the optical path components. 
Illumination power stability (once per yr) Stability STABpower >97% Laser dying: Thorough check by the constructor.
Electrical instabilities: AC-powered light source; check the power grid stability of the room.
Environmental variations (thermal, air flow, humidity...): General verification of environmental and vibration conditions.
Fiber polarization: Check the bends of the optical fibers; proper alignment of laser in fiber.
Defective optical components (AOTF, AOM, fiber): Thorough check by the constructor. 

SDnormalized intensity 
<0.2 
Stage drift (once per yr) Va: Mean velocity after stabilization [0–50] nm/min Environmental variations (thermal, air flow, humidity...): General verification of environmental conditions; protect the stage from thermal shifts (cover, temperature-controlled chamber, or incubator); let the stage stabilize before starting experiments.
Stage control components not properly working: Check joystick at “no move” position, check controller status.
Mechanical instability: Tighten the mechanical elements; thorough check by the constructor. 
Vb: Mean velocity before stabilization [0–100] nm/min 
τstab <120 min 
Stage positioning repeatability (once per yr) σpositioning deviation Stage specifications Environmental variations (thermal, air flow, humidity...): General verification of environmental conditions.
Mechanical instability: Clean pieces of broken cover slip; tighten mechanical elements; thorough check by the constructor.
Objective touches sample insert if position far from center: Change insert or limit movements to central positions.
Not enough oil on the objective: Add enough oil beneath the whole sample before starting an experiment.
Stage drift: Let the stage stabilize before starting a multiposition experiment. 
Camera read noise (once per yr) VAR
STABnoise 
>90%
>97% 
Electronics issue; detector temperature; detector aging; cosmic rays: Thorough check by the constructor. 

Summary of the basic metrics, the recommended measuring frequency, the experimental limit values, the possible reasons associated with their exceeding values, and troubleshooting advice.

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