MolecularDevices Micro

Last modified by Harri Tapio Jäälinoja on 2025/06/23 14:59

Using Micro

Starting the system

  1. Power on the instrument.
  2. Start computer.
  3. Log on with your Windows account
  4. Mount L: disk
    1. Double-click "lmu_active1.bat" on the Desktop.
    2. In the command window, write your university username in the format ATKK\username, press Enter.
    3. In the command window, write your university password, press Enter.
  5. Start MetaXpress
    1. Double-click "20pa20ph10pa40wi IN Carta" icon on the Desktop.
    2. Select your data source (university username).

Known well-plates and calibration

Plate calibration is done in two steps:

  1. Measure variation of plate bottom thickness
    • requires an empty plate
  2. Measure required exposure time for autofocus laser
    • autofocus is based on the reflection of the laser from the plate and well bottom
    • reflection from the well bottom depends on the refractive index of the mounting media
    • requires a plate with relevant sample 
       

The system has now these calibrated settings:

Manufacturer

Plate model

Akita96-well

Greiner

Cellstar 655180 96-well F-bottom

GreinerCellstar 657160 6-well
GreinerCellstar 665180 12-well
GreinerCellstar 662160 24-well
GreinerCellstar 677180 48-well
Ibidi8-well slide (with slide holder)

Ibidi

uPlate 24-well
IbidiuPlate 96-well

Revvity

PhenoPlate 96-well

PerkinElmer

ViewPlate 96-well

Thermo Scientific

442404 MaxiSorp 96-well

If you use any other plates, you need to bring two plates for the training:

  1. empty plate
  2. a plate with sample (and media in the wells with no sample)

Troubleshooting network problems

  1. Check with LMU staff that you have correctly mounted the L-disk. 
    1. If L-disk is not available, use the local F disk (selector is in the "Run" tab).
  2. Check if you can connect to your usual data source
    1. You can also use the shared account MDCStore (see credentials), which uses the local database.  

Shutting down the system

The instrument power can be left always on. Here are the steps for the other components:

  1. Close the software.
  2. Check OpenIRIS for the next booking.
    • There is a booking within 2h: Log out.
    • There is no booking with 2h: Log out, shut down computer.
  3. Does the next user within 24h need the system warmed up?
    • Yes: Power on heating.
  4. If you used CO2, close CO2 bottle valve and regulator output valve.

Technical details

Nikon Objectives

ObjectiveNA

Resolution

0.61 x 509 nm / NA

Pixel sizeWorking distance
4X CFI Plan Apochromat Lambda D0.21.55 um 20.0 mm
10X Plan Apo Lambda

0.45

690 nm676 nm16 mm
20X Plan Apo Lambda0.8388 nm349 nm0.8 mm
20X Ph1 S Plan Fluor ELWD ADM0.45690 nm340 nm6.9-8.2 mm
40X Water Apo LambdaS LWD1.15270 nm170 nm 

The instrument only has room for four objectives at a time. There are two hardware configurations where either the 4x or 20x/0.45 objective is left out:

  • 20pa20ph10pa40wi
  • 20pa4pa10pa40wi

Light source (LED)

Lumencor AURA Light Engine

Filter specifications

LMU Micro on FPbase.

Excitation filters are built in the Lumencor light source (see manufacturer documentation).

FluorophoresWavelength (nm)Power (mW)

DAPI

377/54200
FITC475/28200
TRITC543/27300
TexasRed560/32200
Cy5

631/28

155

Filter specifications according to MolecularDevices documentation.

Filter

Wavelengths

DAPI

Excitation: 377/54 nm
Emission: 447/60 nm
Dichroic: 409 nm

FITC

Excitation: 475/28 nm
Emission: 536/40 nm
Dichroic: 506 nm
Cy3 (TRITC)Excitation: 543/27 nm
Emission: 593/40 nm
Dichroic: 562 nm

Texas Red

Excitation: 560/32 nm
Emission: 624/40 nm
Dichroic: 593 nm

Cy5

Excitation: 631/28 nm
Emission: 692/40 nm
Dichroic: 660 nm

Camera

4.2 Mpixel sCMOS camera.

  • 2160 x 2160 pixels
  • 16 bit
  • 82% QE
  • 40 fps
  • TIFF format