Materials and Reagents

15 ml screw cap glass vials (Kesell, catalog number: BLP025, package of 8)
200 µl gel pipette tips (Fisher Scientific, Basix^TM, catalog number: 13-611-116)
Thick black construction paper
Coumarin 540A dye (Exciton, catalog number: 05450)
LDS 798 dye (Exciton, catalog number: 07980)
Rhodamine 590 dye (Exciton, catalog number: 05901)
Fluorescein sodium salt, analytical standard (Sigma-Aldrich, catalog number: 30181-100MG)
Chloroform, CHCl₃ (Fisher Scientific, HPLC grade, catalog number: C607-1)
Deuterated chloroform, CDCl₃ (Sigma-Aldrich, catalog number: 151858-10x0.75ML)
Dimethyl sulfoxide, C₂H₆OS (Fisher Chemical, Certified ACS grade, catalog number: 151874-10x0.75)
Methanol, CH₃OH (Fisher Chemical, HPLC grade, catalog number: A452-4)
LDS 798 dye solution in CHCl₃:CDCl₃ (1:2) mixture (see Recipes)
Coumarin 540A dye solution in DMSO (see Recipes)
Rhodamine 590 dye solution in methanol (see Recipes)

Equipment

Optical Table: Sealed Hole Table Top with Tuned Damping (Newport, model: RS 2000^TM), set on High Performance Laminar Flow Isolators (4 pieces) (Newport, model: S 2000)
Femtosecond pulsed laser (InSight DeepSee Dual, Newport Spectra-Physics)
Photon Counting Spectrofluorimeter (ISS, model: PC1^TM)
Silver coated mirrors (Newport, model: New Focus 5103 (5 pcs.))
Stainless steel optical posts (Thorlabs, catalog numbers: TR3 (4pcs.) and TR4 (7 pcs.))
Standard ½” diameter, 3” long postholders (Thorlabs, catalog number: PH3 (11 pcs.))
Standard ½” diameter 1” long postholder (Thorlabs, catalog number: PH1 (1pc.))
Post holder bases (Thorlabs, catalog numbers: BA1 (11 pcs.) and BA1S (1pc.))
Bolts and nuts. ¼”–20 Hardware Kit (Thorlabs, catalog number: HW-KIT2)
New Focus mirror mount (Newport, catalog number: 9773 (5 pcs.))
Flipper Optic Mount (Newport, model: New Focus 9891)
Mounted achromatic half wave plate (690-1,200 nm) (Thorlabs, catalog number: AHWP10M-980)
Rotation Mount for Ø1" Optics (Thorlabs, catalog number: RSP1 (2 pcs.))
Unmounted Glan-Laser Polarizer, Ø10 mm CA, Uncoated (Thorlabs, catalog number: GL10P)
SM1 Lens Tube Mount for 8 mm and 10 mm Mounted Polarizing Prisms (Thorlabs, catalog number: SM1PM10)
Mounted Continuously Variable ND Filter, Ø50 mm, OD: 0.04-4.0, ARC: 650-1,050 nm (Thorlabs, catalog number: MDC-50C-4M-B)
Broadband Energy/Power Meter (Melles-Griot, Model 13PEM001)
25 mm Dia. x 45 mm FL, NIR II Coated, Achromatic Lens (Edmund Optics, model: ACH-NIR 25 x 45 NIR-II, Stock: 45-802)
22 mm-to-25 mm inner diameter lens tube adaptors, ISS Accessory, 2 pieces
ND New Focus reflective filters (Newport, catalog numbers: 5240 (OD 1), 5235 (OD 0.5), and 5233 (OD 0.3))
4-slot filter wheel with a stepper motor, ISS Accessory
Short pass filters, 633/SP (Semrock, catalog number: BSP01-633R-25), 680/SP (Semrock, catalog number: FF01-680/SP-25), 694/SP (Semrock, catalog number: FF02-694/SP-25), 745/SP (Semrock, catalog number: FF01-745/SP-25), 770/SP (Semrock, catalog number: FF01-770/SP-25)
Long pass filter 645/LP (Thorlabs, catalog number: FGL 645)
RS 232 Serial cable (15 ft)
Micro, square, stopper top special optical glass cuvettes, 3 x 3 mm (Starna Cells, catalog number: 23-3.45-SOG-3, quantity 6)
3-mm SOG cuvette adaptor holder (Starna Cells, catalog number: FCA3, quantity 4)
1 cm standard glass fluorometer rectangular cells (Starna Cells, catalog number: 23-G-10, quantity 4)
Micro spinbar magnetic stir bar, 5 x 1 mm (Thomas Scientific, catalog number: 1207Q08, quantity 6)
UV/Vis spectrophotometer (PerkinElmer, LAMBDA 950)
Luminescence Spectrometer (PerkinElmer, LS55)
200 µl pipette (Gilson, model: Pipetman Classic P200, catalog number: F123601)

Software

OriginPro 2017 (OriginLab, https://www.originlab.com)
Vinci 3 (ISS, http://www.iss.com/)
LabView2018 (National Instruments, https://www.ni.com)
Custom Labview program for scanning the laser wavelength could be obtained by sending an e-mail request to mikhail.drobijev@montana.edu

Procedure

Building optical setup for two-photon absorption measurements
1. On the optical table set up and fix a femtosecond laser and a spectrofluorimeter, approximately 2 m apart.
2. Remove the excitation lamp source (Figure 2), the mirror holder with two mirrors from the excitation monochromator (Figure 3), two lenses (in tubes) (Figures 4 and 5), optional beam splitter (Figure 6), and optional filter (Figure 7) from the excitation path of the PC1 spectrofluorimeter. The tube carrying the first lens and placed between the monochromator and optional beamsplitter must be removed as well (Figure 4). The second tube (empty), entering the sample compartment should be kept in place (Figure 5).
  
  Figure 2. Entrance aperture of the PC1 ISS spectrofluorimeter after the excitation lamp source was removed. A flip mirror is used for steering the laser beam into a powermeter head. Red dashed arrow shows the direction of laser beam propagation here and in Figures 3-7.
  
  Figure 3. Removing mirror holder with two mirrors from excitation monochromator compartment
  
  Figure 4. Removing tube holder with collimating lens (placed right after excitation monochromator) and setting an ISS filter wheel with four slots in place of it
  
  Figure 5. Changes in the sample compartment. A focusing lens is removed from the tube lens holder pointing toward the sample. 3-mm cuvette adaptors are inserted in the Sample and Reference cuvette holders. In the Left Emission Channel, an additional adaptor tube holder (25-mm) with a short-pass filter (770/SP) is slide onto a 22-mm tube lens holder.
  
  Figure 6. Removing optional beam splitter
  
  Figure 7. Removing optional excitation filter
3. Disconnect the ‘Left Emission Wavelength’ stepper motor cable from its stepper motor jack inside PC1 (Figure 8).
  
  Figure 8. Electrically disconnecting Left Emission Wavelength filter wheel from its stepper motor and connecting an additional filter wheel in excitation path with the stepper motor of the Left Emission Wavelength filter wheel
4. In a spare motorized filter wheel with 4 slots (ISS accessories) insert New Focus ND reflective filters with OD = 1, OD = 0.5, and OD = 0.3 in the slots # 1, 2, and 3, respectively. Leave the slot # 4 empty.
5. Set a motorized filter wheel with these ND filters in the excitation optical path of PC1 right after the excitation monochromator and bolt it to the PC1 base (Figures 4 and 8).
6. Connect the stepper motor of this filter wheel to the stepper motor jack of the ‘Left Emission Wavelength’ wheel (Figure 8).
7. Put the excitation polarizer inside the optical path of the PC1.
8. Turn on the PC1 and the computer controlling it.
9. Create a file template in Vinci to measure the excitation power dependence of fluorescence in the left or right emission channels (Power Dependence file), Figure 9. For that, go to Experiment in Vinci software, then click on Single Point, and in the drug menu select Intensity. Right-click on the block called Fixed Parameter, click on Remove tab, and select Left Emission Wavelength box, then click OK. Right click on the block called Variable Parameters, click on Add tab and select Left Emission Wavelength function then click OK. In the Variable Parameters, Left Emission Wavelength box, click on the Edit List and call filter #1–0.1T, #2–0.3T, #3–0.5T, and #4–empty. In the Time Base window, select 10 s, and in Number of Iterations, select 1. Save this file as “Power Dependence”.
  
  Figure 9. Upper left part of the screenshot showing a Vinci 3 template file for the power dependence measurement in the Sample position in both left and right emission channels
10. Create a file template in Vinci to measure the two-photon excitation spectra of the two samples–one set in the Sample and another–in Reference position of the PC1 in one laser scan using left emission channel (Spectral Scan file), Figure 10. For that, go to Experiment in Vinci software, then click on Slow Kinetics, and in the drug menu select Intensity. Right-click on the block called Variable Parameters and add a Sample function. In the Time Base window, select 1.0 s, and in Time window in Variable parameters select 0 s for Start, 6,500 s for Stop, and 6.00 for Step. Select 200 min for ‘Measure Dark every __ minutes’. In the block Fixed Parameters under Left Emission Wavelength select empty in the Value box. Save the file as “Spectral Scan”.
  
  Figure 10. Upper left part of the screenshot showing a Vinci 3 template file for the spectral scan of two samples at once (set in the Sample and Reference positions)
11. Turn on the laser in the alignment mode (200 mW) at 720 nm. Use safety goggles.
12. Set the first mirror M1 assembled in the holder right after the laser output (main beam) to turn the beam 90° in horizontal plane, parallel to the table, see Figure 1.
13. Set first a half-wave plate and second a Glan Laser polarizer assembled in their rotation mounts after the M1 in the laser beam. Make sure the beam passing through both of them freely at its original height (as it came out of the laser).
14. Turn the half-wave plate fast axis approximately to 45° (turning laser polarization from horizontal to vertical).
15. Turn the Glan polarizer polarization axis close to vertical position.
16. Use 3 mirrors (M2-M4) in their holder assemblies to direct the laser beam to the entrance aperture of the spectrofluorimeter (see Figure 1). Use mirrors M2 and M3 to make the beam height close to the height of the entrance aperture of PC1 and parallel to the table. Use M3 and M4 to direct the beam to the center of the entrance aperture of PC1 in the horizontal plane.
17. Put the continuously variable neutral density filter in the beam after the M3 mirror.
18. Put the flip mirror FM after M4 and flip it up.
19. Put the power meter in the laser path after the flip mirror.
20. Turn the continuously variable neutral density (ND) filter wheel to the maximum transmission position.
21. Check that the laser power measured with the power meter is ~200 mW.
22. Turn the continuously variable ND filter to attenuate the power to ~20 mW.
23. In the VINCI Experiment software (ISS), go to Instrument Control tab and open the excitation shutter.
24. In the same tab set the Left Emission Wavelength to position 4 (corresponding to empty slot of the excitation ND filter wheel.
25. With mirrors M3 and M4 align the beam along the axis connecting the center of the entrance aperture of PC1 and the center of the window in the sample holder.
26. Insert the 45-mm achromatic lens into a 22 mm-to-25 mm diameter adaptor tube (ISS accessory) and slip that adaptor with the lens over a 22-mm ISS tube, with the lens facing toward the sample position (Figure 11).
  
  Figure 11. Placing a 45-mm achromatic lens into an excitation optical pathway inside the sample compartment. Left: An f = 45 mm achromatic lens is inserted and fixed in a 22-to-25 mm diameter adaptor tube. Right: Achromatic lens in the adaptor tube is slide over the 22-mm empty adaptor tube inside the sample compartment.
27. Make sure that the laser beam is still pointing at the center of the opening of the sample holder (now with the 45-mm lens in). If necessary slightly re-align the beam with mirrors M3 and M4.
28. Turn off the laser.
29. In the right emission channel, insert the Semrock 745/SP filter into a filter slot.
30. Disconnect the Laser from the computer with InSight GUI software and connect it through an RS 232 Serial port to a PC computer with the custom LabView program for tuning laser wavelength.
31. Turn on the laser using the LabView program (Figure 12, Supplemental file 1 Laser Scan).
  
  Figure 12. Front view of the custom-made LabView program to scan the laser from the initial to the final wavelength with a particular step and dwell time
32. Tune the laser to 850 nm.
33. Flip the flip mirror up.
34. Open the laser shutter with the LabView program.
35. Adjust the laser power to 200 mW. First make sure that continuously variable ND filter is turned to a fully transmitting position. Then, slowly rotate the half-wave plate (sitting immediately after the laser) until the laser power reads 200 mW. Use this position of the half-wave plate always, unless higher power is needed in experiment.
36. Move the head of the power meter into the sample compartment and fix it (with the 1” post holder and short post holder base BA1S), such that its sensor is centered inside the round opening of the excitation path and facing the laser beam. Set the excitation polarizer to horizontal (90°) position with the Instrument Control of PC1 software. Adjust the angle of the external Glan Laser polarizer by turning its rotation mount, to a position where the power is minimum. Lock this position with a screw on its rotation mount.
37. Slide the excitation polarizer out of the excitation optical path.
38. Calibrate the ND filters at several laser wavelengths in the whole tuning range. Set a first laser wavelength at 680 nm. By using the Instrument Control function in Vinci, change the position of the Left Emission Wavelength filter from 1 to 4 and record the power for all 4 positions. Calculate the ratio of power measured for positions 1-3 to that measured for position 4.
39. Repeat Step A38 for a set of wavelengths (680, 690, 710, 730, 780, 800, 810, 840, 900, 940, 960, 1,000, 1,050, 1,060, 1,100, 1,200, 1,300 nm) in the laser tuning range.
40. Summarize the data in the Origin Workbook, see Figure 13.
  
  Figure 13. Origin workbook containing a look up calibration table for the transmission properties of ND filters in the filter wheel set in the excitation path at several laser wavelengths
41. Turn off the laser.
42. Remove the power meter head from the sample compartment and place it back to its holder after the flip mirror.
43. Insert the 770/SP filter into a 22 mm-to-25 mm diameter adaptor tube (ISS accessory) and slip that adaptor with the filter over a 22-mm ISS tube (with the PC1 collecting lens in it) used for emission collection through the left emission channel.
44. In the Left Emission Filter Wheel with 4 slots (disconnected from its electric jack) insert the Semrock 633/SP, 694/SP, and 680/SP filters in slots 1, 2, and 3, respectively. Leave slot 4 empty.
45. Dismount two adaptor holders for 3 x 3 mm cuvettes (unscrew 4 miniature screws holding one side of the holder) and insert a rectangular band of black paper (0.9 x 4 cm) on the side containing 4 screws such that only a narrow slit of ~0.7 mm remains open into each of the holders, see Figure 1B, right, bottom. The slit is supposed to be on the left side of the facet, when looking at the holder.
46. Mount the holders back, fixing the pieces of paper inside them with 4 screws.
Measuring two-photon excitation spectral shapes using Left Emission Channel
1. Preparation of samples for two-photon spectral measurements.
  1. Prepare the stock solutions of samples (up to two new samples) and references (LDS798 and Coumarin 540A), see Recipes for preparation of reference solutions, and add 150 μl of them into the 3 x 3 mm optical cuvettes.
  2. Using Lambda 950 Spectrophotometer, measure absorption spectra of all the samples. The optical density in the spectral maximum of all solutions should be in the range of 0.2-1.5 when measured in 3 x 3 mm cuvettes placed in 3-mm adaptor holder.
  3. Put micro stir bars in solutions with reference.
2. Initial instrument setup preparation. Coumarin 540A solution in Sample holder. Filters 770/SP and 633/SP in the Left Emission Channel.
  1. Turn on the laser in the full power mode.
  2. Start the laser control LabView program (Supplemental file 3 LaserTestVI3.vi) from a PC computer.
  3. Turn on the PC1 spectrofluorimeter.
  4. Insert the adaptor holders for 3 x 3 cuvettes into the sample and reference holders of PC1 such that the masked side of either adaptor holder is directed to the left emission channel when it is set to the measurement (the reference holder can be set to measurement by selecting Reference position of the turret in the Instrument Control of Vinci). Keep the adaptor holders in place during all the measurements.
  5. Set the Sample position to measurement.
  6. In the Instrument Control start stirring both Sample and Reference.
  7. Insert the 3 x 3 mm cuvette with Coumarin 540A solution into the sample holder of PC1.
  8. Turn manually the left emission wavelength filter wheel to position 1 (corresponding to 633/SP filter).
  9. Slide the left emission polarizer in the emission path and set it to Magic Angle position (with Instrument Control function).
  10. Set the laser wavelength to 800 nm.
  11. Adjust the laser power with the continuous ND filter to ~20 mW.
  12. Send the laser beam to PC1 by flipping the flip mirror down.
  13. Make sure that the excitation polarizer in PC1 is moved out of the excitation optical path.
  14. Make sure with the Instrument Control of Vinci that the ND filter wheel in the excitation channel (Left Emission Wavelength) is set to empty position (slot 4).
  15. Open the excitation shutter with Instrument Control.
  16. In a dark room with the sample compartment lid removed, adjust the distance from the 45-mm lens to the sample by sliding the adaptor with the lens in it over the 22-mm tube (fixed) and maximizing the intensity of fluorescence at the left emission channel PMT.
  17. Fix the position of the adaptor (with respect to a 22-mm tube) with a small screw.
3. Adjusting power range for the samples #1 and #2. First, sample #1 and then sample #2 in Sample holder. Filters 770/SP and 633/SP (or 680/SP, 694/SP or empty) in the Left Emission Channel. Select the second short pass filter such that its cutoff wavelength is larger than fluorescence peak wavelength of samples #1 and #2.
  1. Put the cuvette with the sample #1 solution into the Sample position instead of Coumarin 540A solution.
  2. Cover the sample compartment with the lid.
  3. Measure the maximum signal at several wavelengths across the 2PA spectrum, e.g., 700, 800, 900, 1,000, 1,100, 1,200 nm (using left PMT).
  4. Repeat the same for the sample #2.
  5. Adjust the laser power with the continuous ND filter such that the maximum signal across the 2PA spectrum of both samples amounts ~1 x 10⁶ counts. Typically, this power will be in the range 10-100 mW, depending on sample concentration and two-photon brightness.
4. Checking the power dependence of fluorescence at different wavelengths for samples #1 and #2. First, sample #1 and then sample #2 in Sample holder. Filters 770/SP and 633/SP (or 680/SP, 694/SP or empty) in the Left Emission Channel.
  1. Using the Power Dependence file, check that the power dependence of sample #1 fluorescence is quadratic (power exponent between 1.95 and 2.05) at wavelengths in the short wavelength region of spectrum, where the one-photon excitation can contribute. Find the shortest wavelength by using discrete steps of 20 nm (i.e., 680, 700, 720 nm, etc.), at which the signal is quadratic.
  2. Repeat the Step B4a for sample #2.
5. Scanning 2PA spectra of samples #1 and #2. Sample #1–in Sample position and sample #2–in Reference position. Filters 770/SP and 633/SP (or 680/SP, 694/SP or empty) in the Left Emission Channel.
  1. Put cuvettes with sample #1 in the Sample position and with sample #2 in the Reference position of the sample compartment turret.
  2. In the scanning part of the LabView file controlling the laser, set the start wavelength of the scan equal to the largest number found in Steps B4a and B4b.
  3. Calculate the stop wavelength (λ_stop) by taking the longest possible wavelength observed as a long-wavelength edge of one-photon absorption spectrum multiplied by 2 and taking the closest number to it in a sequence of numbers starting at 680 with. Set this number as a stop wavelength.
  4. Set the step equal to 4 nm and the time per step equal to 42 s.
  5. Open the Spectral Scan file, make the notes about the experiment (samples names and positions, filters used, etc.) and start the scan.
  6. Start the laser scan.
  7. Once the scan is finished, remove the cuvettes with the samples from adaptor holders.
6. Scanning 2PA spectra of Coumarin 540A solution. One cuvette with Coumarin 540A solution–in Sample position and another cuvette with Coumarin 540A solution–in Reference position. Filters 770/SP and 633/SP in the Left Emission Channel.
  1. Put two cuvettes with the same solution of Coumarin 540A in DMSO into the Sample and Reference positions of the turret.
  2. Repeat Steps B5b-B5g with the stop wavelength equal to 980 nm in Step B5c and all other settings kept the same in Steps B5b-B5f and making the notes about the reference in Step B5e.
7. Scanning 2PA spectra of LDS 798 solution. One cuvette with LDS 798 solution–in Sample position and another cuvette with LDS 798 solution–in Reference position. Filter 770/SP in the Left Emission Channel.
  1. Put two cuvettes with the same solution of LDS 798 in chloroform/deuterated chloroform, 1:2, into the Sample and Reference positions of the turret.
  2. Turn manually the left emission wavelength filter wheel to position 4 (empty).
  3. Repeat Steps B5b-B5f with the start wavelength equal to 940 nm in Step B5b and all other settings kept the same in Steps B5b-B5f and making the notes about the reference in Step B5e.
8. Calculating corrected two-photon excitation spectra of samples #1 and #2 with the programs written in OriginLab.
  1. For a file that contains the two-photon raw spectral data (.ifx) in which two samples were measured simultaneously in the 'Sample' and 'Reference' holders:
    1. In OriginLab, create and save an Import Wizard (File > Import > Import Wizard) that will open the file into a workbook so that it looks similar to the example workbook displayed in Figure 14. The data columns that the Vinci program saves are 'Time', 'Sample', 'Intensity', 'IntensityStdError', and 'Real time'.
    2. Name this Import Wizard filter "2PA_sample_and_reference".
      
      Figure 14. An example of what the Origin workbook will look like after creating the "2PA_sample_and_reference" Import Wizard filter
  2. Add the auto-analysis script to that Import Wizard filter. To do this, first import the file used for the above step, select the filter you just created, and click "Next" through to the last window. Check "Save the filter" as well as "Specify advanced filter options". Save this as a new filter, "2PA_sample_and_reference_autocalculation". Click "Next", which brings you to a window to copy and paste Script 1 (see Supplemental file 2 Origin Script) in the window "Script after each file imported:".
  3. After filling in the appropriate values in the window that pops up (first wavelength, last wavelength, wavelength step, seconds per step), the resulting workbook should look like the following (Figure 15). Additionally, a graph (Figure 16) will pop up that shows what the raw data looks like after the script auto-deletes the points when the laser is stabilizing. It should look like data points clustered into two distinct spectra. If there are points that are randomly much lower in intensity than the others, that usually means the script did not work for some reason and the data should be manually sorted. This graph (Figure 16) is an important visual check that the script worked as it is meant to.
    
    Figure 15. An example of what the final workbook should look like after opening a file with the "2PA_sample_and_reference_autocalculation" Import Wizard filter
    
    Figure 16. An example of the graph showing what the raw data looks like after the script auto-deletes the points when the laser is stabilizing. This graph pops up after opening a file with the "2PA_sample_and_reference_autocalculation" Import Wizard filter. It is a visual check that the script worked as intended.
  4. If the samples measured are reference dyes to measure the correction function of the setup, then copy and paste the "correct" reference dye spectra into their corresponding columns (column D for the 'Sample holder', column E for the 'Reference holder). Make sure that the wavelength range you copied matches the wavelength range you measured. Columns F and G are now the correction functions for the 'Sample holder' and the 'Reference holder', respectively. They are set to divide the raw spectra by the correct spectra.
  5. Merge the short range correction functions separately measured with the reference dyes Coumarin 540A in DMSO (λ_start-980 nm) and LDS798 in 2:1 CDCl₃:CHCl₃ (940 nm-λ_stop) into full range correction function (λ_start-λ_stop). (Correction function data from the 'Sample holder' and the 'Reference holder' should be treated separately.)
    1. First, normalize the short range correction functions by dividing each of them by the mean of the column values in the 940-980 nm range.
    2. Now, find the mean of the row values of the two short range correction functions in the 940-980 nm range and accept it as a part of correction function for this range.
    3. Create the merged correction function. For the λ_start-936 nm range, paste the normalized correction function measured with Coumarin 540A in DMSO. For the 940 nm-980 nm range, paste the average correction function from the previous step. For the 980 nm-λ_stop range, paste the normalized correction function measured with LDS798 in 2:1 CDCl₃:CHCl₃.
  6. If the samples measured have unknown 2PA spectra, then copy and paste the correction functions that you measured previously for the sample holder and the reference holder (column D for the 'Sample holder', column E for the 'Reference holder'). Make sure that the wavelength range you copied matches the wavelength range you measured. Columns F and G are now the corrected 2PA spectral shapes for the samples measured in the 'Sample holder' and the 'Reference holder', respectively. They are set to divide the raw spectra by the correction functions.
Measurement of two-photon absorption cross sections of a red fluorescent protein (for example, RGECO1, described in Zhao et al., 2011) relatively to Rhodamine 590 in methanol at 1,060 nm using Right Emission Channel with registration of fluorescence at 600 nm.
1. Prepare the stock solution of Rhodamine 6G in methanol. Adjust the optical density at 528 nm in 3 x 3 mm cuvette to a number between 0.2 and 0.3. Record the exact number for OD.
2. Adjust the optical density of the sample in 3 x 3 mm cuvettes to 0.2-0.3. Record the exact number for OD.
3. Set the laser wavelength at 1,060 nm.
4. In the right emission channel, slide the polarizer in and set it to the magic angle using Instrument Control function.
5. Set the right emission monochromator to 600 nm and manually insert the two 2-mm slits into the monochromator.
6. Put the cuvette with reference Rhodamine 590 solution in the Sample holder of the turret
7. Adjust the laser power with the ND continuous filter such that the right emission intensity will be on the order of 50,000-100,000 when the excitation filter wheel is set to empty position (#4).
8. Record this power.
9. Repeat Steps C7 and C8 for the sample solution.
10. Run the Power Dependence file with registration in the Right Emission Channel for Rhodamine 590.
11. Repeat Step C10 for the sample without changing condition.
12. Using the OriginLab, plot the power dependencies of fluorescence signals as function of power squared and obtain the ratio F_{2, S} (λ_ex, λ_reg)/F_{2, R} (λ_ex, λ_reg) values as ratio of the slopes of linear fits of the sample and reference standard, respectively.
13. Using known extinction coefficients, calculate the ratio of concentrations:
14. To measure the φ numbers, dilute the sample and reference solutions to have optical densities, similar to each other at a selected wavelength (530 nm) and falling in the range of 0.05-0.07 in 1-cm optical cuvettes. Record their respective OD values at 530 nm: OD_S (530) and OD_R (530).
15. Using LS55 spectrofluorimeter, record fluorescence spectra of the sample and reference upon excitation at 530 nm with excitation slit equal to 5 nm and emission slit–16 nm.
16. Record the one-photon signals at 600 nm F_{1, S}(600) and F_{1, R} (600) and calculate the ratio:
17. Using eq. (2), all the ratio values obtained in Steps C12-C16, and Rhodamine 590 cross section σ₂(1060) = 10 GM, calculate the 2PA cross section of the sample.

Data analysis

The variations of spectral profiles, i.e., deviations of relative values at one wavelength when the spectra are normalized at another wavelength (e.g., peak) contain the random and systematic contributions. The random contribution comes from reproducibility of the laser parameters in consecutive scans of the same sample. We have observed that the deviations across the spectra were not larger than 4% in 2-3 consecutive scans. Since two scans (sample and reference standard) are used to calculate the corrected 2PA spectrum, this results in a random error of 6%. The systematic spectral deviations come from the accuracy of the measurement of 2PA spectra of references standards. Those can be estimated to be about 5% for Coumarin 540A (de Reguardati et al., 2016) and ~10% for LDS 798 (Makarov et al., 2011). This results in the total spectral shape errors of 8% in the short wavelength range (680-980 nm) and 12% in the long wavelength range (980-1,300 nm).
The error of the 2PA cross section measurement is a combination of the errors of individual parameters entering eq. (2). The errors of F₂ numbers are estimated from linear fits of the fluorescence intensity vs. power squared plots (usually 1% for both F_2,S and F_2,R). The errors in differential quantum yields, φ for both sample and reference were determined from 12 independent measurements of one protein and found to be 7%. The errors in concentrations come mostly from the errors in measurements of extinction coefficients of the sample, equal to 5% (Molina et al., 2019). The systematic error, coming from the uncertainty in the 2PA cross section of reference standard is 10% for Rhodamine 590 (see Notes section). Therefore, the total error calculated in quadrature for the σ₂ of the sample measured at one wavelength (1,060 nm) amounts to 15%. This translates to the error of absolute σ₂ value, determined at different wavelengths of ~18% (Molina et al., 2019).

Notes

We use the mixture of chloroform/deuterated chloroform (1:2) as solvent for LDS 798 to get rid of chloroform absorption at 1,150 nm. We observed virtually no changes in 1PA spectra of the dyes when going from pure chloroform to the mixture.

The shapes of the one-photon and two-photon absorption spectra of Coumarin 540A in DMSO closely match each other in the region of 745-1,000 nm, if the 1PA is plotted versus one-photon wavelength doubled (de Reguardati et al., 2016; Figure 17). In the shorter wavelength range, 680-745 nm the relative 2PA values presented in (de Reguardati et al., 2016) systematically exceed the 1PA values. We have measured independently the 2PA spectrum of Coumarin 540A in DMSO, using Prodan in DMSO as a reference standard (de Reguardati et al., 2016) in the region of 680-800 nm, and obtained much better correlation between the 2PA and 1PA spectral shapes of Coumarin 540A, cf. red and black lines in Figure 17.

Figure 17. Spectral shapes on 1PA and 2PA spectra of Coumarin 540A in DMSO. The 1PA spectrum measured in this work, black line, and 2PA spectrum (de Reguardati et al., 2016), blue line, are normalized at their peak values. The short wavelength part of the 2PA spectrum (680-800 nm), red line, was measured in this work, using Prodan in DMSO (de Reguardati et al., 2016) as a standard.

To double check the spectral shape of Coumarin 540A (A_2PA,R(λ) function) in a broad range from 680 to 1,000 nm, we measured the 2PA spectrum of Rhodamine 590 (= Rhodamine 6G) in methanol versus Coumarin 540A in DMSO and compared it to the known literature data (Figure 18). The data from Hermann and Ducuing (1972), Makarov et al. (2008), de Reguardati et al. (2016) were presented as measured, in absolute cross section values (see Footnote a and b to the Table 5 below for the Hermann and Ducuing data). The data from Albota et al. (1998), Rodriguez et al. (2009), Rodriguez and Chiesa (2011), Rodriguez and Chiesa (2012) were scaled to a value of 74 GM at 820 nm that matches the measurements of Makarov et al. (2008), de Reguardati et al. (2016). The spectrum from Wakebe and Van Keuren (1999), originally presented as relative spectrum for Rhodamine 6G in ethanol, is shifted 17 nm to the red (in 2PA wavelengths) and scaled to a value of 34 GM at 844, matching the measurements of Makarov et al. (2008), de Reguardati et al. (2016). In almost the whole region of Coumarin 540A absorption, from 690 to 960 nm, there is a good correlation between the spectral shapes measured in Albota et al. (1998) and de Reguardati et al. (2016), therefore we conclude that these spectra present the best approximation to the 2PA spectrum of Rhodamine 6G. This conclusion is supported by good matches of other data to these spectra in different spectral regions or at separate wavelengths: Hermann and Ducuing data at 694 and 1,060 nm; Wakebe and Van Keuren data–in the 806-1,106 nm region; Makarov et al. (2008) data–in the 720-900 and 1,060-1,100 nm regions; Rodriguez et al. (2007) data–in the 720-860 nm region.

Table 1. Correct 2PA spectral shape of Coumarin 540A in DMSO, with 680-760 nm data corrected by Prodan in DMSO (de Reguardati et al., 2016)

Wavelength	Relative value	Wavelength	Relative value	Wavelength	Relative value	Wavelength	Relative value
680	0.135	760	0.376	840	0.990	920	0.523
684	0.117	764	0.408	844	0.996	924	0.478
688	0.113	768	0.445	848	0.999	928	0.434
692	0.112	772	0.483	852	1.00	932	0.390
696	0.112	776	0.522	856	0.998	936	0.348
700	0.115	780	0.561	860	0.994	940	0.307
704	0.118	784	0.600	864	0.985	944	0.268
708	0.124	788	0.639	868	0.973	948	0.232
712	0.135	792	0.678	872	0.955	952	0.199
716	0.146	796	0.715	876	0.934	956	0.169
720	0.160	800	0.751	880	0.908	960	0.143
724	0.176	804	0.786	884	0.881	964	0.120
728	0.194	808	0.819	888	0.850	968	0.100
732	0.215	812	0.851	892	0.816	972	0.0832
736	0.234	816	0.881	896	0.780	976	0.0683
740	0.256	820	0.908	900	0.741	980	0.0556
744	0.279	824	0.931	904	0.700	984	0.0448
748	0.303	828	0.952	908	0.657	988	0.0355
752	0.325	832	0.968	912	0.613	992	0.0274
756	0.350	836	0.980	916	0.568	996	0.0203

When the 2PA spectral shape of Coumarin 540A in DMSO is taken as a reference, the 2PA spectrum of Rhodamine 6G in methanol shows strongly overestimated absorption in the region of 680-750 region (cf. open diamonds and light blue line in Figure 18). This can be due to overestimated values of 2PA of Coumarin 540A, as shown in Figure 17. However, when the 2PA spectrum of Coumarin 540A corrected in the 680-740 nm range with Prodan (see Table 1 for the values) is taken for the A_2PA,R(λ) function, the Rhodamine 6G spectrum (dark green line with triangles in Figure 18) matches quite well the literature spectra of Albota et al. (1998) and de Reguardati et al. (2016) in the region of 680-980 nm. Therefore we conclude that the corrected 2PA spectrum of Coumarin 540A in DMSO is a good approximation for the A_2PA,R(λ) function when the corrected spectrum of Coumarin 540A in DMSO is used as a reference in the range of 680-980 nm.

Table 2. Correct 2PA spectral shape of LDS 798 in chloroform from 936-1,300 nm; values are from fitting a Gaussian to the LDS 798 z-scan data from Makarov et al., 2011

Wavelength	Relative value	Wavelength	Relative value	Wavelength	Relative value	Wavelength	Relative value
936	0.116	1028	0.410	1120	0.847	1212	0.978
940	0.124	1032	0.428	1124	0.864	1216	0.970
944	0.132	1036	0.446	1128	0.879	1220	0.961
948	0.141	1040	0.465	1132	0.894	1224	0.950
952	0.150	1044	0.484	1136	0.907	1228	0.937
956	0.159	1048	0.503	1140	0.920	1232	0.923
960	0.169	1052	0.522	1144	0.933	1236	0.908
964	0.180	1056	0.542	1148	0.944	1240	0.892
968	0.191	1060	0.561	1152	0.954	1244	0.874
972	0.203	1064	0.581	1156	0.963	1248	0.855
976	0.215	1068	0.601	1160	0.972	1252	0.835
980	0.227	1072	0.621	1164	0.979	1256	0.813
984	0.240	1076	0.641	1168	0.985	1260	0.791
988	0.253	1080	0.661	1172	0.991	1264	0.767
992	0.267	1084	0.681	1176	0.994	1268	0.742
996	0.282	1088	0.701	1180	0.997	1272	0.717
1000	0.296	1092	0.720	1184	0.999	1276	0.692
1004	0.311	1096	0.740	1188	1.00	1280	0.665
1008	0.327	1100	0.759	1192	0.999	1284	0.638
1012	0.343	1104	0.777	1196	0.998	1288	0.611
1016	0.359	1108	0.795	1200	0.995	1292	0.584
1020	0.376	1112	0.813	1204	0.991	1296	0.556
1024	0.393	1116	0.831	1208	0.985	1300	0.529

Figure 18. Two-photon absorption spectra (logarithmic scale) of Rhodamine 6G in merthanol or ethanol. The data of Hermann and Ducuing (1972)–black stars, Makarov et al. (2008)–blue circles, de Reguardati et al. (2016)–light blue line, are presented in absolute σ₂ values (see footnotes a and b to Tables 3-5 after Table 5). The data of Albota et al. (1998)–red circles, Rodriguez et al. (2009)–ping right triangles; Rodriguez and Chiesa (2011)–pink left triangles, Rodriguez and Chiesa (2012)–pink up triangles are scaled (see text), and Wakebe and Van Keuren (1999)–orange circles are scaled and shifted (see text). The (scaled) spectrum obtained here using Coumarin 540A in DMSO 2PA spectrum (de Reguardati et al., 2016) as a standard, is shown by open diamonds. The spectrum measured in this work (scaled) relatively to Coumarin 540A in DMSO in 740-1,000 nm region and relatively to Prodan in DMSO in 680-740 nm region is shown by dark green down triangles connected with continuous line. The spectrum obtained in this work relatively to LDS 798 in chloroform/deuterated chloroform, is shown by purple diamonds connected with continuous line.

In Makarov et al. (2011), the 2PA spectra of the LDS 798 dye in chloroform were obtained using fluorescence (relatively to Styryl 9M [Makarov et al., 2008]) and z-scan (absolute measurement) techniques. The shapes of the one-photon and two-photon absorption spectra are very broad, structureless, and closely match each other in the region of 900-1,300 nm, if the 1PA is plotted versus one-photon wavelength doubled (Makarov et al., 2011; Figure 19).

Figure 19. Spectral shapes of 1PA (purple line) (measured here) and 2PA spectra of LDS 798 in chloroform, green open squares–using fluorescence technique relatively to Styryl 9M, and black squares–using z-scan and absolute method (Makarov et al., 2011). All spectra are normalized at their peak values. Black dashed line shows a Gaussian fit to the z-scan data in the region from 900 to 1,300 nm that is used as an A_2PA,R(λ) function here. This figure is adapted from Makarov et al. (2011).

Since the z-scan data are obtained with absolute method (LDS 798 is a primary standard), we use the corresponding 2PA shape (black squares in Figure 19) for the A_2PA,R(λ) function. To interpolate the A_2PA,R(λ) function to intermediate wavelengths, we use a Gaussian fit to the experimental data between 900 and 1,300 nm, shown by a dashed black line in Figure 19. This spectrum is presented in Table 2. To check the performance of this function, the 2PA spectrum of Rhodamine 590 in methanol was measured relatively to LDS 798 in CHCl₃/CDCl₃ (1:2) in the 940-1,140 mn region, see Figure 18. The data (purple line) match well the spectra of Albota et al. (1998); Wakebe and Van Keuren (1999), and de Reguardati et al. (2016) and overlaps well with the spectrum measured using Coumarin 540A (dark green line) in the region 940-980 nm. This corroborates our choice of LDS 798 as a reference standard for the spectral shape in the 940-1,300 nm region.
In the measurements of two-photon cross sections, we use optical densities OD < 0.05 at the fluorescence registration wavelength and OD < 0.3 in the absorption peak (in 3-mm cuvette). That is needed to exclude possible re-absorption and re-emission effects.

We suggest using Rhodamine 590 in methanol as a reference standard (see Tables 3 and 4 for literature data) for measuring 2PA cross sections at selected wavelengths. Most consistent literature data were collected near 1,060 nm (Table 3). For this wavelength we suggest using σ₂ = 10 ± 1 GM.

Table 3. Literature data for the two-photon cross section of Rhodamine 6G in methanol or ethanol in the 1,054-1,064 nm region. Most of the values (column no. 7) group around 10 GM. The average of all 11 measurements provides σ₂ = 12 ± 2 GM (average ± SE of mean). The underlined values are obtained either with mode-locked lasers or using the methods where the uncertainty in the second-order time correlation function of laser intensity g⁽²⁾ was removed. Out of these six measurements, the lowest (4.2 GM) (Kaatz and Shelton, 1999), was obtained by using Hyper Rayleigh scattering technique to calibrate the laser properties, including g⁽²⁾. The authors found that this method gave underestimated values of σ₂, compared to those obtained with standard calibration against one-photon fluorescence. Therefore, the suggested value of σ₂ is calculated by excluding this measurement and averaging the numbers selected in italic in column 7.

Wavelength (nm)	Solvent	Conc. (M)	Pulse	Original σ₂(GM)	Correction 1 σ₂(GM)	Correction 2 σ₂ (GM) (final)	Ref.
1060	C₂H₅OH	n/a	ns	12.9 ± 6	25.8 ± 12^a	10.1 ± 4.7^b	Hermann and Ducuing, 1972
1060	C₂H₅OH	10^-3	60 ns	5.5	11^a	5.5^c	Bradley et al., 1972
1060	C₂H₅OH	10^-4	30 ns	26	52^a	26^c	Vsevolodov et al., 1973
1060	C₂H₅OH	10^-3	ps	3.6	7.2^a	7.2	Bradley et al., 1972
1060	C₂H₅OH	10^-6	110 ns	11 ± 5	22 ± 10^a	11 ± 5^c	Li and She, 1982
1064	C₂H₅OH	10^-2	cw	12 ± 2	48 ± 8^d	24 ± 4^c	Catalano and Cingolani, 1982
1054	CH₃OH	0.2	5 ps	10 ± 1	-	10 ± 1	Penzkofer and Leupacher, 1987
1064	CH₃OD	2.2 10^-6	125 ns	4.2 ± 0.8	-	4.2 ± 0.8	Kaatz and Shelton, 1999
1064	C₂H₅OH	10^-4	10 ns	15 ± 1	30 ± 2^a	15 ± 1^c	Rodriguez, et al., 2007
1060	CH₃OH	8 10^-6	100 fs	10 ± 1	-	10 ± 2	Makarov et al., 2008
1060	CH₃OH	n/a	100 fs	11 ± 1	-	11 ± 1	de Reguardati et al., 2016
Suggested conditions and cross section value
1060	CH₃OH	10^-5	100 fs			*10 ± 1*

Table 4. Other σ₂ values of Rhodamine 6G at selected wavelengths. The σ₂ values showing satisfactory matching between two or more measurements are italicized in column 7. Recommended values of σ₂ are calculated as average of these numbers for each wavelength.

Wavelength (nm)	Solvent	Conc. (M)	Pulse	Original σ₂(GM)	Correction 1 σ₂(GM)	Correction 2 σ₂ (GM) (final)	Ref.
694	C₂H₅OH	n/a	ns	355 ± 170	710 ± 355^a	277 ± 138^b	Hermann and Ducuing, 1972
694	CH₃OH	0.04	30 ps	180 ± 20	^-	180 ± 20	Sperber and Penzkofer, 1986
690 700	CH₃OH	1.1 10^-4	100 fs	136 176	^-	156^e	Albota et al., 1999
694	CH₃OH	8 10^-6	100 fs	112 ± 22	-	112 ± 22	Makarov et al., 2008
692	CH₃OH	n/a	100 fs	202 ± 16	-	202 ± 16	de Reguardati et al., 2016
Suggested conditions and cross section value
694	CH₃OH	10^-5	100 fs			180 ± 23

730	CH₃OH	8 10^-6	100 fs	50 ± 10	-	50 ± 10	Makarov et al., 2008
730	CH₃OH	n/a	100 fs	50 ± 4	-	50 ± 4	de Reguardati et al., 2016
Suggested conditions and cross section value
730	CH₃OH	10^-5	100 fs			50

812	CH₃OH	8 10^-6	100 fs	71 ± 14	-	71 ± 14	Makarov et al., 2008
812	CH₃OH	n/a	100 fs	79 ± 6	-	79 ± 6	de Reguardati et al., 2016
Suggested conditions and cross section value
812	CH₃OH	10^-5	100 fs			75

940	CH₃OH	1.1 10^-4	100 fs	7.7	^-	7.7	Albota et al., 1999
940	CH₃OH	8 10^-6	100 fs	8.3 ± 1.7	-	8.3 ± 1.7	Makarov et al., 2008
940	CH₃OH	n/a	100 fs	11.1 ± 0.9	-	11.1 ± 0.9	de Reguardati et al., 2016
Suggested conditions and cross section value
940	CH₃OH	10^-5	100 fs			9.0 ± 1.0

960	CH₃OH	1.1 10^-4	100 fs	12.7	^-	12.7	Albota et al., 1999
960	CH₃OH	8 10^-6	100 fs	10.9 ± 2.2	-	10.9 ± 2.2	Makarov et al., 2008
960	CH₃OH	n/a	100 fs	17 ± 1.4	-	17.0 ± 1.4	de Reguardati et al., 2016
Suggested conditions and cross section value
960	CH₃OH	10^-5	100 fs			13 ± 2

We suggest using Fluorescein in water at pH 11 as a reference standard for molecules fluorescing in green part of the spectrum (500-550 nm). Part C of the protocol should be adjusted then to measuring fluorescence in the green region. Table 5 summarizes the literature data for Fluorescein with recommended wavelengths and σ₂ values.

Table 5. Some suggested σ₂ values of Fluorescein in alkaline water solution at different wavelengths. The σ₂ values showing satisfactory matching between two or more measurements are italicized in column 7. Recommended values of σ₂ are calculated as average of these numbers for each wavelength.

Wavelength (nm)	Solvent	Conc. (M)	Pulse	Original σ₂(GM)	Correction 1 σ₂(GM)	Correction 2 σ₂ (GM) (final)	Ref.
710	H₂O pH11	8 10^-5	100 fs	17.3 ± 4.4		17.3 ± 4.4	Xu and Webb, 1996
710	H₂O pH11	3 10^-6	100 fs	16.5 ± 3.3	-	16.5 ± 3.3	Makarov et al., 2008
Suggested conditions and cross section value
710	H₂O pH11	10^-5	100 fs			16.9

730	H₂O pH11	8 10^-5	100 fs	25.0 ± 6.3		25.0 ± 6.3	Xu and Webb, 1996
730	H₂O pH11	3 10^-6	100 fs	24.2 ± 4.8	-	24.2 ± 4.8	Makarov et al., 2008
Suggested conditions and cross section value
730	H₂O pH11	10^-5	100 fs			24.6

782	H₂O pH11	n/a	100 fs	46 ± 10		46 ± 10	Xu et al., 1995
782	H₂O pH11	8 10^-5	cw (single mode)	38 ± 10		38.0 ± 10	Xu and Webb, 1996
782	H₂O pH11	3 10^-6	100 fs	46 ± 9	-	46 ± 9	Makarov et al., 2008
Suggested conditions and cross section value
782	H₂O pH11	10^-5	100 fs			43 ± 3

802	H₂O pH11	8 10^-5	cw (single mode)	36 ± 10		36 ± 10	Xu and Webb, 1996
802	H₂O pH11	3 10^-6	100 fs	38 ± 8	-	38 ± 8	Makarov et al., 2008
Suggested conditions and cross section value
802	H₂O pH11	10^-5	100 fs			37

842	H₂O pH11	8 10^-5	100 fs	12 ± 3		12 ± 3	Xu and Webb, 1996
842	H₂O pH11	3 10^-6	100 fs	13 ± 3	-	13 ± 3	Makarov et al., 2008
Suggested conditions and cross section value
842	H₂O pH11	10^-5	100 fs			12.5

900	H₂O pH11	8 10^-5	100 fs	16 ± 4		16 ± 4	Xu and Webb, 1996
900	H₂O pH11	3 10^-6	100 fs	15 ± 3	-	15 ± 3	Makarov et al., 2008
Suggested conditions and cross section value
900	H₂O pH11	10^-5	100 fs			15.5

1000	H₂O pH11	3 10^-6	100 fs	3.1 ± 0.6	-	3.1 ± 0.6	Makarov et al., 2008
1000	H₂O pH11	n/a	100 fs	3.3 ± 0.3	-	3.3 ± 0.3	de Reguardati et al., 2016
Suggested conditions and cross section value
1000	H₂O pH11	10^-5	100 fs			3.2

1060	C₂H₅OH	10^-5	60 ns	0.18	0.36^a	0.18^c	Bradley et al., 1972
1060	C₂H₅OH		ps	0.075	0.15^a	0.15	Bradley et al., 1972
1050	H₂O pH11	8 10^-5	100 fs	0.23 ± 0.07		0.23 ± 0.07	Xu and Webb, 1996
1050	H₂O pH11	3 10^-6	100 fs	0.17 ± 0.03	-	0.17 ± 0.03	Makarov et al., 2008
Suggested conditions and cross section value
1050	H₂O pH11	10^-5	100 fs			0.2

Footnotes for Tables 3-5:
^aMultiplied by factor 2 to conform with the more recent definition of σ₂ (two photons are needed to excite one molecule), cf. Xu and Webb (1996); Kaatz and Shelton (1999); Makarov et al. (2008).
^bMultiplied by factor 0.39 to conform with the current reference value of quartz, d₁₁ = 0.30 pm/V (versus 0.48 pm/V), see Kaatz and Shelton (1999).
^cRe-evaluated using the laser coherence function value g⁽²⁾ = 2, see Weber (1971); Bradley et al. (1972); Kaatz and Shelton (1999). That factor was not included in original analysis.
^dMultiplied by factor 4 to conform with the more recent definition of σ₂ (two photons are needed to excite one molecule), cf. Xu and Webb (1996); Kaatz and Shelton (1999); Makarov et al. (2008).
^eInterpolated between 690 and 700 nm measurements.

Recipes

LDS 798 dye solution in CHCl₃:CDCl₃ (1:2) mixture
1. Dissolve 0.1 mg of LDS 798 in 0.75 ml of CHCl₃ in a 15 ml screw cap glass vial
2. Add 1.5 ml of CDCl₃. Stir overnight on magnetic stirrer. The optical density of the final solution at 594 nm (spectral maximum) in 3 mm cuvette should be OD ~1.2. This corresponds to a concentration of ~10^-4 M
3. It can be stored in closed vial in the dark at room temperature for at least 2 months
Coumarin 540A dye solution in DMSO
1. Dissolve 0.15 mg of Coumarin 540A in 3.3 ml of DMSO in a 15 ml screw cap glass vial
2. The optical density of the final solution at 427 nm (spectral maximum) in 3 mm cuvette should be OD ~0.6. This corresponds to a concentration of ~10^-4 M
3. It can be stored in closed vial in the dark at room temperature for at least 2 months
Rhodamine 590 dye solution in methanol
1. Dissolve 0.05 mg of Rhodamine 6G in 10 ml of CH₃OH in a 15 ml screw cap glass vial
2. The optical density of the final solution at 528 nm (spectral maximum) in a 3 mm cuvette should be OD ~0.3. This corresponds to a concentration of ~10^-5 M
3. It can be stored in a closed vial in the dark at room temperature for at least 4 months

Acknowledgments

We thank Alexey Drobizhev for the custom LabView program. This work was supported by the NINDS grants U01 NS094246 and U24 NS109107 for MD, TEH, and RSM, and the Ruth L. Kirschtein National Research Service Award, number F31NS108593 for RSM.
This protocol was derived from Molina, R.S., Qian, Y., Wu, J., Shen, Y., Campbell, R. E., Drobizhev, M. and Hughes, T. E. (2019) Understanding the fluorescence change in red genetically encoded calcium ion indicators. Biophys. J. 116: 1873-1886.

Competing interests

The authors declare no financial and non-financial competing interests.

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