83
Introduction to FCS

Introduction to FCS · 2018. 4. 12. · Introduction to Fluorescence Correlation Spectroscopy (FCS) Fluctuation analysis goes back to the beginning of the century •Brownian motion

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  • Introduction to FCS

  • What is diffusion? Diffusion of molecules Diffusion of light Generalization of the concept of diffusion Translational diffusion Rotational diffusion Some general rules about diffusion Diffusion in restricted spaces Diffusion in presence of flow Anomalous diffusion How to measure diffusion? Macroscopic methods Molecular level methods Fluctuation based methods Single particle tracking methods

  • Original observation by Brown: the Brownian motion (From A Fowler lectures) In 1827 the English botanist Robert Brown noticed that pollen grains suspended in water jiggled about under the lens of the microscope, following a zigzag path. Even more remarkable was the fact that pollen grains that had been stored for a century moved in the same way. In 1889 G.L. Gouy found that the "Brownian" movement was more rapid for smaller particles (we do not notice Brownian movement of cars, bricks, or people). In 1900 F.M. Exner undertook the first quantitative studies, measuring how the motion depended on temperature and particle size. The first good explanation of Brownian movement was advanced by Desaulx in 1877: "In my way of thinking the phenomenon is a result of thermal molecular motion in the liquid environment (of the particles)." This is indeed the case. A suspended particle is constantly and randomly bombarded from all sides by molecules of the liquid. If the particle is very small, the hits it takes from one side will be stronger than the bumps from other side, causing it to jump. These small random jumps are what make up Brownian motion.

  • In 1905 A. Einstein explained Brownian motion using energy equipartition: the kinetic theory of gases developed by Boltzmann and Gibbs could explain the randomness of the motion of large particles without contradicting the Second Principle of Thermodynamics. This was the first “convincing” proof of the particle nature of matter as declared by the adversaries of atomism. The role of fluctuations Explanation in terms of fluctuations

    Why measure diffusion with optical methods? Diffusion in microscopic spaces Diffusion in biological materials

    Difference between diffusion, “hopping” and binding

  • Introduction to Fluorescence Correlation Spectroscopy (FCS) Fluctuation analysis goes back to the beginning of the century

    •Brownian motion (1827). Einstein explanation of Brownian motion (1905) Noise in resistors (Johnson, Nyquist), white noise {Johnson, J.B., Phys. Rev. 32 pp. 97 (1928), Nyquist, H., Phys. Rev. 32 pp. 110 (1928)}

    •Noise in telephone-telegraph lines. Mathematics of the noise. Spectral analysis

    •I/f noise

    •Noise in lasers (1960)

    •Dynamic light scattering

    •Noise in chemical reactions (Eigen)

    •FCS (fluorescence correlation spectroscopy, 1972) Elson, Magde, Webb

    •FCS in cells, 2-photon FCS (Berland et al, 1994)

    •First commercial instrument (Zeiss 1998)

    Manfred Eigen

    Elliot Elson

    Keith Berland

  • Why we need FCS to measure the internal dynamics in cell??

    Methods based on perturbation Typically FRAP (fluorescence recovery after photobleaching) Methods based on fluctuations Typically FCS and dynamic ICS methods

    There is a fundamental difference between the two approaches, although they are related as to the physical phenomena they report.

    Dan Axelrod

  • Introduction to “number” fluctuations

    In any open volume, the number of molecules or particles fluctuate according to a Poisson statistics (if the particles are not-interacting) The average number depends on the concentration of the particles and the size of the volume The variance is equal to the number of particles in the volume This principle does not tell us anything about the time of the fluctuations

  • The fluctuation-dissipation principle (systems at equilibrium)

    If we perturb a system from equilibrium, it returns to the average value with a characteristic time that depends on the process responsible for returning the system to equilibrium Spontaneous energy fluctuations in a part of the system, can cause the system to locally go out of equilibrium. These spontaneous fluctuations dissipate with the same time constant as if we had externally perturbed the equilibrium of the system.

    External perturbation

    time

    ampl

    itude

    Equilibrium value

    Spontaneous fluctuation

    time

    ampl

    itude

    Equilibrium value

    Synchronized Non-synchronized

  • First Application of Correlation Spectroscopy (Svedberg & Inouye, 1911) Occupancy Fluctuation

    Collected data by counting (by visual inspection) the number of particles in the observation volume as a function of time using a “ultra microscope”

    120002001324123102111131125111023313332211122422122612214 2345241141311423100100421123123201111000111_2110013200000 10011000100023221002110000201001_333122000231221024011102_ 1222112231000110331110210110010103011312121010121111211_10 003221012302012121321110110023312242110001203010100221734 410101002112211444421211440132123314313011222123310121111 222412231113322132110000410432012120011322231200_253212033 233111100210022013011321113120010131432211221122323442230 321421532200202142123232043112312003314223452134110412322 220221

    Experimental data on colloidal gold particles:

  • 1

    2

    3

    456

    10

    2

    3

    456

    100

    Fre

    qu

    en

    cy

    86420

    Number of Particles

    7

    6

    5

    4

    3

    2

    1

    0

    Parti

    cle

    Num

    ber

    5004003002001000

    time (s)

    *Histogram of particle counts *Poisson behavior *Autocorrelation not

    available in the original paper. It can be easily calculated today.

    Particle Correlation and spectrum of the fluctuations

    Comments to this paper conclude that scattering will not be suitable to observe single molecules, but fluorescence could

  • • Number of fluorescent molecules in the volume of observation, diffusion or binding

    • Conformational Dynamics • Rotational Motion if polarizers are used either in emission

    or excitation • Protein Folding • Blinking • And many more

    Example of processes that could generate fluctuations

    What can cause a fluctuation in the fluorescence signal???

    Each of the above processes has its own dynamics. FCS can recover that dynamics

  • Generating Fluctuations By Motion

    Sample Space

    Observation Volume

    1. The rate of motion 2. The concentration of particles 3. Changes in the particle fluorescence while under observation, for example conformational transitions

    What is Observed? We need a small volume!!

    Note that the spectrum of the fluctuations responsible for the motion is “flat” but the spectrum of the fluorescence fluctuations is not

  • Defining Our Observation Volume under the microscope: One- & Two-Photon Excitation.

    1 - Photon 2 - Photon

    Approximately 1 um3

    Defined by the wavelength and numerical aperture of the

    objective

    Defined by the pinhole size, wavelength, magnification and

    numerical aperture of the objective

  • Why confocal detection? Molecules are small, why to observe a large volume? • Enhance signal to background ratio • Define a well-defined and reproducible volume Methods to produce a confocal or small volume (limited by the wavelength of light to about 0.1 fL) • Confocal pinhole • Multiphoton effects 2-photon excitation (TPE) Second-harmonic generation (SGH) Stimulated emission Four-way mixing (CARS) (not limited by light, not applicable to cells) • Nanofabrication • Local field enhancement • Near-field effects

  • Brad Amos MRC, Cambridge, UK

    1-photon

    2-photon Need a pinhole to define a small volume

  • 22

    )(λ

    πτ fhc

    Apdna ≈

    na Photon pairs absorbed per laser pulse p Average power τ pulse duration f laser repetition frequency A Numerical aperture λ Laser wavelength d cross-section

    From Webb, Denk and Strickler, 1990

  • Laser technology needed for two-photon excitation Ti:Sapphire lasers have pulse duration of about 100 fs Average power is about 1 W at 80 MHz repetition rate About 12.5 nJ per pulse (about 125 kW peak-power) Two-photon cross sections are typically about

    δ=10-50 cm4 sec photon-1 molecule-1 Enough power to saturate absorption in a diffraction limited spot

  • Orders of magnitude (for 1 μM solution, small molecule, water) Volume Device Size(μm) Molecules Time milliliter cuvette 10000 6x1014 104 microliter plate well 1000 6x1011 102 nanoliter microfabrication 100 6x108 1 picoliter typical cell 10 6x105 10-2 femtoliter confocal volume 1 6x102 10-4 attoliter nanofabrication 0.1 6x10-1 10-6

  • Determination of diffusion by fluctuation spectroscopy

  • Time (in us)600,000400,000200,0000

    Cou

    nts

    (in k

    Hz)

    550500450400350300250200150100

    500

    The time series

    Time (in us)1,380,0001,375,0001,370,0001,365,000

    Cou

    nts

    (in k

    Hz)

    80

    70

    60

    50

    40

    30

    20

    10

    0

    Detail of one time region

    Correlation plot (log averaged)

    Tau (s)1E-5 0.0001 0.001 0.01 0.1 1 10

    G(t)

    6

    5

    4

    3

    2

    1

    0

    The autocorrelation function N and relaxation time of the fluctuation

    PCH average

    counts1614121086420

    0.1

    1

    10

    100

    1,000

    10,000

    100,000

    1,000,000

    The histogram of the counts in a given time bin (PCH). N and brightness

    Data presentation and Analysis

    Duration

  • How to extract the information about the fluctuations and their characteristic time?

    Distribution of the amplitude of the fluctuations Distribution of the duration of the fluctuations

    To extract the distribution of the duration of the fluctuations we use a math based on calculation of the correlation function To extract the distribution of the amplitude of the fluctuations, we use a math based on the PCH distribution

  • The definition of the Autocorrelation Function

    )()()( tFtFtF −=δ G(τ) =δF(t)δF(t + τ)

    F(t) 2

    Phot

    on C

    ount

    s

    t

    τ

    t + τ

    time

    Average Fluorescence

  • ),()()( tCWdQtF rrr∫= κ

    kQ = quantum yield and detector sensitivity (how bright is our

    probe). This term could contain the fluctuation of the

    fluorescence intensity due to internal processes

    W(r) describes the profile of illumination

    C(r,t) is a function of the fluorophore concentration over time. This is the term that contains the “physics” of the diffusion processes

    What determines the intensity of the fluorescence signal??

    The value of F(t) depends on the profile of illumination!

    This is the fundamental equation in FCS

  • What about the excitation (or observation) volume shape?

    ( ) 2022 )(2

    0 )(,,w

    yx

    ezIIzyxF+

    =

    −= 2

    0

    22)(zw

    zExpzI

    2)(1

    1)(

    ozwzzI

    +=

    Gaussian z

    Lorentzian z

    More on the PSF in Jay’s lecture

    For the 2-photon case, these expression must be squared

  • The Autocorrelation Function

    10-9 10-7 10-5 10-3 10-1

    0.0

    0.1

    0.2

    0.3

    0.4

    Time(s)

    G(τ)

    G(0) ∝ 1/N As time (tau) approaches 0

    Diffusion

    In the simplest case, two parameters define the autocorrelation function: the amplitude of the fluctuation (G(0)) and the characteristic relaxation time of the fluctuation

  • The Effects of Particle Concentration on the Autocorrelation Curve

    = 4

    = 2

    0.5

    0.4

    0.3

    0.2

    0.1

    0.0

    G(t)

    10 -7 10 -6 10 -5 10 -4 10 -3

    Time (s)

    Observation volume

  • Why Is G(0) Proportional to 1/Particle Number?

    NNN

    NVarianceG 1)0( 22 ===10-9 10-7 10-5 10-3 10-1

    0.0

    0.1

    0.2

    0.3

    0.4

    Time(s)

    G(τ

    )

    A Poisson distribution describes the statistics of particle occupancy fluctuations. For a Poisson distribution the variance is proportional to the average:

    VarianceNumberParticleN =>=< _

    ( )2

    2

    2

    2

    )(

    )()(

    )(

    )()0(

    tF

    tFtF

    tF

    tFG

    −==

    δ

    2)()()(

    )(tF

    tFtFG

    τδδτ

    += Definition

  • G(0), Particle Brightness and Poisson Statistics

    1 0 0 0 0 0 0 0 0 2 0 1 1 1 0 0 0 0 0 0 1 0 0 0 0 0 0 0 1 0 1 0 0 0 1 0 0 1 0 0

    Average = 0.275 Variance = 0.256

    Variance = 4.09

    4 0 0 0 0 0 0 0 0 8 0 4 4 4 0 0 0 0 0 0 4 0 0 0 0 0 0 0 4 0 4 0 0 0 4 0 0 4 0 0

    Average = 1.1 0.296

    296.0256.0275.0 22 ==∝ VarianceAverageN

    Lets increase the particle brightness by 4x:

    Time

    ∝N

  • Effect of Shape on the (Two-Photon) Autocorrelation Functions:

    For a 2-dimensional Gaussian excitation volume: 1

    22

    41)(−

    +=

    DGwD

    NG τγτ

    For a 3-dimensional Gaussian excitation volume:

    21

    23

    1

    23

    4141)(−−

    +

    +=

    DGDG zD

    wD

    NG ττγτ

    2-photon equation contains a 8, instead of 4

    21

    21

    11)(−−

    ⋅+⋅

    +=

    DD

    SN

    Gττ

    ττγτ

    3D Gaussian “time” analysis: with τD=w2/4D and S=w/z

  • Blinking and binding processes

    Until now, we assumed that the particle is not moving. If we assume that the blinking of the particle is independent on its movement, we can use a general principle that states that the correlation function splits in the product of the two independent processes.

    )()()( τττ DiffusionBlinkingTotal GGG ⋅=

    −+= −λττ e

    KffKG BABinding

    2

    1)(

    K = kf / kb is the equilibrium coefficient; λ = kf + kb is the apparent reaction rate coefficient; and fj is the fractional intensity contribution of species j

  • How different is G(binding) from G(diffusion)?

    With good S/N it is possible to distinguish between the two processes. Most of the time diffusion and exponential processes are combined

    DataDiffusionExponential

    Difference betw een ACF for diffusion and binding

    tau1e-5 1e-4 1e-3 1e-2 1e-1 1e0 1e1

    G(t)

    5.5

    5

    4.5

    4

    3.5

    3

    2.5

    2

    1.5

    1

    0.5

    0

  • The Effects of Particle Size on the Autocorrelation Curve

    300 um2/s 90 um2/s 71 um2/s

    Diffusion Constants

    Fast Diffusion

    Slow Diffusion

    0.25

    0.20

    0.15

    0.10

    0.05

    0.00

    G(t)

    10 -7 10 -6 10 -5 10 -4 10 -3

    Time (s)

    D = k ⋅T6 ⋅π ⋅ η ⋅ r

    Stokes-Einstein Equation:

    3rVolumeMW ∝∝

    and

    Monomer --> Dimer Only a change in D by a factor of 21/3, or 1.26

  • Autocorrelation Adenylate Kinase -EGFP Chimeric Protein in HeLa Cells

    Qiao Qiao Ruan, Y. Chen, M. Glaser & W. Mantulin Dept. Biochem & Dept Physics- LFD Univ Il, USA

    Examples of different Hela cells transfected with AK1-EGFP

    Examples of different Hela cells transfected with AK1β -EGFP

    Fluorescence Intensity

  • Time (s)

    EGFPsolution

    EGFPcell

    EGFP-AKβ in the cytosol

    EGFP-AK in the cytosol

    Normalized autocorrelation curve of EGFP in solution (•), EGFP in the cell (• ), AK1-EGFP in the cell(•), AK1β-EGFP in the cytoplasm of the cell(•).

    Autocorrelation of EGFP & Adenylate Kinase -EGFP

  • Autocorrelation of Adenylate Kinase –EGFP on the Membrane

    A mixture of AK1b-EGFP in the cytoplasm and membrane of the cell.

    Clearly more than one diffusion time

  • Diffusion constants (um2/s) of AK EGFP-AKβ in the cytosol -EGFP in the cell (HeLa). At the membrane, a dual diffusion rate is calculated from FCS data. Away from the plasma membrane, single diffusion constants are found.

    10 & 0.1816.69.619.68

    10.137.1

    11.589.549.12

    Plasma Membrane Cytosol

    Autocorrelation Adenylate Kinaseβ -EGFP

    13/0.127.97.98.88.2

    11.414.4

    1212.311.2

    D D

    egfp

    countswG(0)NBright

    akb1093egfp1000600000.360.0055.790.21

    akb1097egfp1001160000.270.0122.20.16

    akb1098egfp1002180000.330.0132.260.16

    akb1099egfp1003220000.330.0142.40.19

    akb1100egfp1004140000.390.0111.850.16

    akb1101egfp1005220000.330.0152.410.18

    average is 0,33

    Sheet2

    w=0.33

    countsDG(0)Nbrightness

    akb1000b100016000section4.280.19

    akb1006b100620000head10/0.233.780.23akb1on the border 50mV

    akb1007b100716000tail10/0.174.50.19akb1on the border 50mV

    akb1026b102614000section10/0.264.260.17akb3 on the border, 50mV

    akb1027b102711000perfect10/0.133.480.16akb3 on the border, 50mV

    akb1028b102810000head10/0.293.160.15akb3 on the border, 50mV

    akb1029b102912000tail10/0.163.830.16akb3 on the border, 50mV

    akb1030b103010000head10/0.223.490.16akb3 on the border, 50mV

    akb1031b103110000perfect10/0.163.510.16akb3 on the border, 50mV

    akb1032b103210000perfect remove a little head10/0.133.430.14akb3 on the border, 50mV

    akb1033b103310000section10/0.163.460.15akb3 on the border, 50mV

    akb1034b103410000perfect10/0.123.320.14akb3 on the border, 50mV

    akb1035b103510000good remove little10/0.23.880.14akb3 on the border, 50mV

    akb1036b103610000head10/0.173.370.14akb3 on the border, 50mV

    akb1037b10378000good14.90.0162.680.13akb3, near the border, 300mV

    akb1038b10387000head19.50.0192.820.13akb3, near the border, 300mV

    akb1039b10397000head110.0182.740.12akb3, near the border, 300mV

    akb1040b10405600good remove a peak6.610.0162.380.11akb3, very close to the border, 300mV

    akb1041b10415600good5.170.172.170.12akb3, very close to the border, 300mV

    akb1042b10425600good remove head10/0.362.290.12akb3, very close to the border, 300mV

    akb1043b10435600good10/0.092.380.12akb3, very close to the border, 300mV

    akb1044b10445000good remove a little5.140.172.160.12akb3, very close to the border, 300mV

    akb1046b10465600cut head10/0.122.260.12akb3, 10mW from the border to the center , see image 300mV

    akb1047b10475000ok3.120.0192.030.11akb3, 10mW from the border to the center , see image 300mV

    akb1048b10485000ok4.360.0231.960.12akb3, 10mW from the border to the center , see image 300mV

    akb1049b10494000good4.780.0261.460.14akb3, 10mW from the border to the center , see image 300mV

    akb1050b10502800good4.090.0311.290.11akb3, 10mW from the border to the center , see image 300mV

    akb1051b10513200good6.10.0341.250.13akb3, 10mW from the border to the center , see image 300mV

    akb1052b10523600good6.050.0321.410.13akb3, 10mW from the border to the center , see image 300mV

    akb1053b10534000good3.990.0251.60.12akb3, 10mW from the border to the center , see image 300mV

    akb1054b10543600good6.360.0281.680.11akb3, 10mW from the border to the center , see image 300mV

    akb1055b10553600good5.160.0251.40.13akb3, 10mW from the border to the center , see image 300mV

    akb1057b105714000section10 & 0.182.980.23akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1058b10589000head16.60.0192.320.18akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1059b10598000section9.610.022.030.19akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1061b10616400good9.680.0242.080.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1062b10626400good10.130.0222.120.15akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1063b10636400good7.10.021.940.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1064b10646400good11.580.021.910.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1065b10656400good9.540.01920.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1066b10666400ok9.120.172.340.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1067b106770002.540.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1068b10687000ok2.560.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1083b10838000good10/0.211.980.2akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1084b10843200ok150.0291.260.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1085b10853200ok12.90.0341.240.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1086b10862800ok190.0341.060.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1087b10872800ok16.60.031.420.09akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    Sheet3

    egfp

    countswG(0)NBright

    akb1093egfp1000600000.360.0055.790.21

    akb1097egfp1001160000.270.0122.20.16

    akb1098egfp1002180000.330.0132.260.16

    akb1099egfp1003220000.330.0142.40.19

    akb1100egfp1004140000.390.0111.850.16

    akb1101egfp1005220000.330.0152.410.18

    average is 0,33

    Sheet2

    w=0.33

    countsDG(0)Nbrightness

    akb1000b100016000section4.280.19

    akb1006b100620000head10/0.233.780.23akb1on the border 50mV

    akb1007b100716000tail10/0.174.50.19akb1on the border 50mV

    akb1026b102614000section10/0.264.260.17akb3 on the border, 50mV

    akb1027b102711000perfect10/0.133.480.16akb3 on the border, 50mV

    akb1028b102810000head10/0.293.160.15akb3 on the border, 50mV

    akb1029b102912000tail10/0.163.830.16akb3 on the border, 50mV

    akb1030b103010000head10/0.223.490.16akb3 on the border, 50mV

    akb1031b103110000perfect10/0.163.510.16akb3 on the border, 50mV

    akb1032b103210000perfect remove a little head10/0.133.430.14akb3 on the border, 50mV

    akb1033b103310000section10/0.163.460.15akb3 on the border, 50mV

    akb1034b103410000perfect10/0.123.320.14akb3 on the border, 50mV

    akb1035b103510000good remove little10/0.23.880.14akb3 on the border, 50mV

    akb1036b103610000head10/0.173.370.14akb3 on the border, 50mV

    akb1037b10378000good14.90.0162.680.13akb3, near the border, 300mV

    akb1038b10387000head19.50.0192.820.13akb3, near the border, 300mV

    akb1039b10397000head110.0182.740.12akb3, near the border, 300mV

    akb1040b10405600good remove a peak6.610.0162.380.11akb3, very close to the border, 300mV

    akb1041b10415600good5.170.172.170.12akb3, very close to the border, 300mV

    akb1042b10425600good remove head10/0.362.290.12akb3, very close to the border, 300mV

    akb1043b10435600good10/0.092.380.12akb3, very close to the border, 300mV

    akb1044b10445000good remove a little5.140.172.160.12akb3, very close to the border, 300mV

    akb1046b10465600cut head13/0.122.260.12akb3, 10mW from the border to the center , see image 300mV

    akb1047b10475000ok7.90.0192.030.11akb3, 10mW from the border to the center , see image 300mV

    akb1048b10485000ok7.90.0231.960.12akb3, 10mW from the border to the center , see image 300mV

    akb1049b10494000good8.80.0261.460.14akb3, 10mW from the border to the center , see image 300mV

    akb1050b10502800good8.20.0311.290.11akb3, 10mW from the border to the center , see image 300mV

    akb1051b10513200good11.40.0341.250.13akb3, 10mW from the border to the center , see image 300mV

    akb1052b10523600good14.40.0321.410.13akb3, 10mW from the border to the center , see image 300mV

    akb1053b10534000good120.0251.60.12akb3, 10mW from the border to the center , see image 300mV

    akb1054b10543600good12.30.0281.680.11akb3, 10mW from the border to the center , see image 300mV

    akb1055b10553600good11.20.0251.40.13akb3, 10mW from the border to the center , see image 300mV

    akb1057b105714000section10/0.182.980.23akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1058b10589000head16.60.0192.320.18akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1059b10598000section9.610.022.030.19akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1061b10616400good9.680.0242.080.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1062b10626400good10.130.0222.120.15akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1063b10636400good7.10.021.940.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1064b10646400good11.580.021.910.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1065b10656400good9.540.01920.16akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1066b10666400ok9.120.172.340.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1067b106770002.540.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1068b10687000ok2.560.14akb3, 10mW from the border to the center , see image 300mV another set 188, (77--245)

    akb1083b10838000good10/0.211.980.2akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1084b10843200ok150.0291.260.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1085b10853200ok12.90.0341.240.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1086b10862800ok190.0341.060.13akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    akb1087b10872800ok16.60.031.420.09akb3 @1000mV, the computer is rebooted.vertical (156-78),(30-195), 10 points

    Sheet3

  • Two Channel Detection: Cross-correlation

    Each detector observes the same particles

    Sample Excitation Volume

    Detector 1 Detector 2

    Beam Splitter 1. Increases signal to noise by isolating correlated signals.

    2. Corrects for PMT noise

    lfd

  • Removal of Detector Noise by Cross-correlation

    11.5 nM Fluorescein

    Detector 1

    Detector 2

    Cross-correlation

    Detector after-pulsing

    lfd

  • )()(

    )()()(

    tFtF

    tdFtdFG

    ji

    jiij ⋅

    +⋅=

    ττ

    Detector 1: Fi

    Detector 2: Fj

    t

    τ

    Calculating the Cross-correlation Function

    t + t

    time

    time

    lfd

  • Thus, for a 3-dimensional Gaussian excitation volume one uses:

    21

    212

    1

    212

    1212

    4141)(−−

    +

    +=

    zD

    wD

    NG ττγτ

    Cross-correlation calculations

    One uses the same fitting functions you would use for the standard autocorrelation curves.

    G12 is commonly used to denote the cross-correlation and G1 and G2 for the autocorrelation of the individual detectors. Sometimes you will see Gx(0) or C(0) used for the cross-correlation.

    lfd

  • Two-Channel Cross-correlation

    Each detector observes particles with a particular color

    The cross-correlation ONLY if particles are observed in both channels

    The cross-correlation signal:

    Sample

    Red filter Green filter

    Only the green-red molecules are observed!!

    lfd

  • Two-color Cross-correlation

    Gij(τ) =dFi (t) ⋅dFj (t + τ)

    Fi(t) ⋅ Fj (t)

    )(12 τG

    Equations are similar to those for the cross correlation using a simple beam splitter:

    Information Content Signal

    Correlated signal from particles having both colors.

    Autocorrelation from channel 1 on the green particles.

    Autocorrelation from channel 2 on the red particles.

    )(1 τG

    )(2 τG

    lfd

  • Experimental Concerns: Excitation Focusing & Emission Collection

    Excitation side: (1) Laser alignment (2) Chromatic aberration (3) Spherical aberration Emission side: (1) Chromatic aberrations (2) Spherical aberrations (3) Improper alignment of detectors or pinhole (cropping of the beam and focal point position)

    We assume exact match of the observation volumes in our calculations which is difficult to obtain experimentally.

    lfd

  • Uncorrelated

    Correlated

    Two-Color FCS

    1)()()()(

    )( −>>+<=

    tFtFtFtF

    Gji

    jiij

    ττ

    Interconverting

    2211111 )( NfNftF +=2221122 )( NfNftF +=

    Ch.2 Ch.1

    450 500 550 600 650 7000

    20

    40

    60

    80

    100

    Wavelength (nm)

    %T

    For two uncorrelated species, the amplitude of the cross-correlation is proportional to:

    +++

    +∝ 2

    2222121122122112

    11211

    222211121112

    )()0(

    NffNNffffNffNffNff

    G

    lfd

  • Simulation of cross-correlation Same diffusion =10 µm2/s

    Channel 1 Channel 2

    Molecules 100

    Molecules 50

    Molecules 20 20

    1/70

    1/120

    Correlation plot (log averaged)

    Tau (s)1E-5 0.0001 0.001 0.01 0.1 1

    G(t)

    7

    6

    5

    4

    3

    2

    1

    0

    fraction

    The fraction cannot be larger than the smallest of the G(0)’s

  • Discussion

    1. The PSF: how much it affects our estimation of the processes?

    2. Models for diffusion, anomalous? 3. Binding? 4. FRET (dynamic FRET)? 5. Bleaching?

    6. ……and many more questions

  • The Photon Counting Histogram: Statistical Analysis of Single Molecule

    Populations

    Laboratory for Fluorescence Dynamics University of California, Irvine

  • Transition from FCS

    • The Autocorrelation function only depends on fluctuation duration and fluctuation density (independent of excitation power)

    • PCH: distribution of intensities (independent of time)

  • Fluorescence Trajectories

    Intensity = 115,000 cps

    Intensity = 111,000 cps

    Fluorescent Monomer:

    Aggregate:

    0

    5

    10

    15

    20

    0 0.1 0.2 0.3 0.4 0.5Time (sec)

    k (c

    ount

    s)

    0

    5

    10

    15

    20

    0 0.1 0.2 0.3 0.4 0.5Time (sec)

    k (c

    ount

    s)

  • Photon Count Histogram (PCH)

    Can we quantitate this?

    What contributes to the distribution of intensities?

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 3 6 9 12 15 18 21 24k (counts)

    log(

    occu

    renc

    es)

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 3 6 9 12 15 18 21 24k (counts)

    log(

    occu

    renc

    es)

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 3 6 9 12 15 18 21 24k (counts)

    log(

    occu

    renc

    es)

  • Fixed Particle Noise (Shot Noise)

    0

    10

    20

    30

    40

    50

    60

    70

    0 2000 4000 6000 8000 10000

    Time

    Cou

    nts

    Noise is Poisson ( )kkk

    kkPoik

    −= exp!

    ),(

    1

    10

    100

    1000

    0 20 40 60k (counts)

    log(

    occu

    ranc

    es)

    Contribution from the detector noise

  • The Point Spread Function (PSF)

    −−= 2

    0

    2

    20

    2

    322exp),(zzrzrI DG ω

    −=

    )(4exp

    )(4),( 2

    2

    42

    40

    2 zr

    zzrIGL ωωπ

    ω

    +=

    220

    2 1)(Rzzz ωω

    λπω20=Rz

    One Photon Confocal:

    Two Photon:

    Contribution from the profile of illumination

  • Single Particle PCH

    + +

    Have to sum up the poissonian distributions for all possible positions of the particle within the PSF

    Counts

    Log(

    Prob

    abili

    ty)

    Counts

    Log(

    Prob

    abili

    ty)

    Counts

    Log(

    Prob

    abili

    ty)

    ( ) rdrPSFkPoiV

    kpV

    ∫=

    0

    )(,1)(0

    )1( ε

    +…

    + +… +

  • • What if I have two particles in the PSF? • Have to calculate every possible position of

    the second particle for each possible position of the first!

  • 0

    10

    20

    30

    Time

    k8

    0

    10

    20

    30

    Time

    k

    8

    Combining Distributions

    + =

    Particle 1 Particle 2 Together

    0

    10

    20

    30

    Time

    k

    8

    0 10 20 30 40k (counts)

    log(

    occu

    renc

    es)

    0 10 20 30 40k (counts)

    log(

    occu

    renc

    es)

    0 10 20 30 40k (counts)

    log(

    occu

    renc

    es)

    Contribution from several particles of same brightness

    + =

  • 0 10 20 30 40k (counts)

    log(

    occu

    renc

    es)

    0

    10

    20

    30

    Time

    k8

    0

    10

    20

    30

    Time

    k

    8

    Combining Distributions

    + =

    Particle 1 Particle 2 Together

    0

    10

    20

    30

    Time

    k

    8

    = 0 10 20 30 40

    k (counts)

    log(

    occu

    renc

    es)

    0 10 20 30 40k (counts)

    log(

    occu

    renc

    es)

  • Convolution • Sum up all combinations of two probability distributions

    (joint probability distribution) • Distributions (particles) must be independent

    1

    10

    100

    1000

    10000

    0 20 40 60Intensity

    Log

    (Pro

    babi

    lity)

    1

    10

    100

    1000

    0 50 100Intensity

    Log

    (Pro

    babi

    lity)

    ∑=

    =

    + ⋅−=kr

    rrprkpkp

    0

    )2()1()21( )()()(

  • More Particles

    ∑=

    =

    −− ⋅−=⊗=kr

    r

    nnn rprkpkpkpkp0

    )1()1()1()1()( )()()()()(

    )()()( )1()1()2( kpkpkp ⊗=+ +…

    + +… )()()( )2()1()3( kpkpkp ⊗=

    Contribution from particles of different brightness

  • How Many Particles Do We Have in the PSF?

    ∑ ⋅=n

    n NnPkpNkPCH ),()(),( )(

    ),(),( NnPoiNnP =Particle occupation fluctuates around average, N with a poissonian distribution

    Calculate poisson weighted average of n particle distributions

    0 10 20 30 40particles in PSF

    log(

    occu

    ranc

    es)

  • Multiple Species

    • Species are independent so just convolute!

    0 10 20 30 40k (counts)

    log(

    occu

    ranc

    es)

    = 0 10 20 30 40

    k (counts)

    log(

    occu

    ranc

    es)

    0 10 20 30 40k (counts)

    log(

    occu

    ranc

    es)

    1 uM Fluorescein 1 uM R110 1 uM Fl & 1uM R110

    Chart1

    0

    1

    2

    3

    4

    5

    6

    7

    8

    9

    10

    11

    12

    13

    14

    15

    16

    17

    18

    19

    20

    21

    22

    k (counts)

    log(occurances)

    0

    0

    4

    3

    22

    47

    58

    100

    123

    142

    129

    96

    83

    64

    62

    35

    28

    12

    9

    3

    2

    1

    1

    hist1

    BinFrequency

    0240

    4247

    894

    1276

    1647

    2039

    2429

    2831

    3227

    3620

    4021

    4417

    4817

    5215

    5610

    6010

    6411

    688

    7210

    765

    808

    845

    882

    924

    962

    1000

    1044

    1081

    1120

    1160

    1201

    More0

    hist1

    Intensity

    Log (Probability)

    hist2

    BinFrequency

    013253

    4183430

    8241335

    12260336

    16157204

    2084123

    244372

    281546

    32431

    36121

    40021

    44017

    48017

    52015

    56010

    60010

    64011

    6808

    72010

    7605

    8008

    8405

    8802

    9204

    9602

    10000

    10404

    10801

    11200

    11600

    12001

    More0

    hist2

    Intensity

    Log (Probability)

    hist3

    Intensity

    Log (Probability)

    convolute

    BinFrequency

    09

    481

    8117

    12134

    16134

    2099

    2479

    2850

    3240

    3633

    4032

    4424

    4825

    5217

    5616

    6013

    6414

    6810

    7210

    7615

    807

    8411

    885

    924

    966

    1005

    1042

    1082

    1123

    1161

    1201

    More1

    convolute

    Intensity

    Log (Probability)

    traj

    BinFrequencydivider

    0240155.84415584420000000006500.02

    42472193.8061938062160.3896103896000000009150

    8942889.11088911092257.792207792261.038961039000000012050

    12763116.88311688312973.3766233766859.240759240849.350649350600000013000

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    2429515.48451548451036.3636363636737.1628371628987.012987013565.7842157842356.493506493518.83116883120002150

    2831179.8201798202530.5194805195394.4055944056596.003996004610.3896103896469.4805194805265.084915084920.129870129900750

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    4021012.337662337718.781218781256.9430569431100.9490509491163.6363636364227.4225774226402.5974025974325.024975025182.81718281720

    4417004.695304695315.184815184835.214785214883.7662337662121.6783216783243.1068931069350.6493506494240.75924075920

    48170003.79620379629.390609390629.220779220862.2877122877130.0699300699211.7382617383259.74025974030

    521500002.34765234777.792207792221.728271728366.5834165834113.2867132867156.84315684320

    5610000001.94805194815.794205794223.226773226857.99200799283.91608391610

    60100000001.44855144866.193806193820.229770229842.9570429570

    641100000001.54845154855.394605394614.9850149850

    688000000001.34865134873.9960039960

    72100000000000.9990009990

    76500000000000

    80800000000000

    84500000000000

    88200000000000

    92400000000000

    96200000000000

    100000000000000

    104400000000000

    108100000000000

    112000000000000

    116000000000000

    120100000000000

    12400000000000

    12800000000000

    13200000000000

    13600000000000

    14000000000000

    14400000000000

    14800000000000

    15200000000000

    15600000000000

    traj

    Intensity

    Log (Probability)

    Sheet9

    00018324180

    10001419614400.135335283200

    20001832418810.27067056650.27067056650.2706705665

    302415225171220.27067056651.08268226590.5413411329

    400013169131630.18044704431.62402339880.5413411329

    500074972040.09022352221.44357635450.3608940886

    600020400202450.03608940890.90223522160.1804470443

    700021441212860.0120298030.43307290640.0721788177

    800021441213270.00343708660.16841724140.0240596059

    900014196143680.00085927160.05499338490.0068741731

    1001112144134090.00019094930.01546688950.0017185433

    11011121441344100.00003818990.00381898510.0003818985

    120416141961848110.00000694360.00084017670.0000763797

    13000981952120.00000115730.00016664660.0000138872

    14011111211256130.0000001780.0000300890.0000023145

    150001936119605.99999412681.9999995853

    16000152251564

    170002248422681.9999957856

    18000214412172

    19024172891976

    20011121441380

    21000141961484

    220636214412788

    230981266763592

    24012144204003296

    2508641419622100

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    310247499

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    340391728920

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    288039

    289040

    290041

    291048

    292030

    293034

    294037

    295030

    296037

    297037

    298042

    299048

    300052

    301038

    302018

    303035

    304032

    305046

    306033

    307036

    308033

    309041

    310041

    311031

    312038

    313034

    314049

    315051

    316052

    317047

    318032

    319044

    320030

    321039

    322052

    323038

    324043

    325037

    326032

    327039

    328038

    329052

    330055

    331027

    332036

    333038

    334045

    335044

    336045

    337048

    338042

    339037

    340039

    341056

    342040

    343030

    344038

    345041

    346041

    347049

    348036

    349038

    350028

    351038

    352035

    353044

    354037

    355040

    356039

    357033

    358034

    359046

    360035

    361034

    362055

    363037

    364038

    365047

    366032

    367046

    368029

    369039

    370043

    371043

    372042

    373036

    374039

    375036

    376050

    377040

    378046

    379047

    380043

    381038

    382056

    383035

    384047

    385038

    386040

    387051

    388041

    389039

    390030

    391039

    392039

    393034

    394037

    395039

    396038

    397048

    398032

    399040

    400036

    401040

    402036

    403040

    404043

    405036

    406042

    407041

    408034

    409051

    410053

    411038

    412037

    413039

    414036

    415039

    416034

    417039

    418037

    419041

    420051

    421046

    422041

    423043

    424042

    425047

    426052

    427052

    428047

    429034

    430034

    431039

    432053

    433049

    434051

    435041

    436035

    437047

    438038

    439037

    440036

    441032

    442041

    443044

    444044

    445033

    446030

    447040

    448036

    449046

    450041

    451047

    452044

    453047

    454038

    455055

    456044

    457050

    458043

    459044

    460026

    461042

    462041

    463030

    464039

    465031

    466033

    467036

    468037

    469055

    470039

    471034

    472038

    473036

    474052

    475041

    476030

    477047

    478046

    479040

    480035

    481038

    482034

    483048

    484042

    485041

    486034

    487051

    488040

    489033

    490046

    491034

    492038

    493039

    494041

    495044

    496036

    497031

    498028

    499032

    500044

    501046

    502033

    503034

    504055

    505047

    506032

    507039

    508039

    509036

    510032

    511037

    512038

    513036

    514040

    515030

    516041

    517041

    518038

    519044

    520034

    521027

    522024

    523045

    524038

    525035

    526039

    527056

    528030

    529039

    530042

    531043

    532035

    533046

    534039

    535044

    536041

    537043

    538041

    539043

    540047

    541047

    542054

    543043

    544044

    545036

    546044

    547038

    548057

    549036

    550047

    551038

    552041

    553033

    554032

    555043

    556042

    557036

    558031

    559043

    560043

    561036

    562033

    563037

    564037

    565032

    566049

    567050

    568040

    569040

    570038

    571040

    572034

    573045

    574037

    575050

    576030

    577039

    578035

    579036

    580036

    581048

    582025

    583053

    584045

    585045

    586049

    587036

    588047

    589044

    590033

    591041

    592050

    593037

    594030

    595037

    596049

    597026

    598036

    599046

    600040

    601043

    602045

    603041

    604039

    605037

    606042

    607037

    608040

    609036

    610040

    611040

    612036

    613031

    614035

    615040

    616051

    617034

    618032

    619028

    620038

    621054

    622049

    623042

    624038

    625035

    626038

    627050

    628030

    629047

    630037

    631046

    632053

    633051

    634045

    635045

    636039

    637040

    638043

    639027

    640049

    641036

    642038

    643039

    644041

    645034

    646057

    647039

    648035

    649045

    650038

    651046

    652033

    653033

    654040

    655042

    656044

    657042

    658042

    659048

    660044

    661041

    662044

    663037

    664040

    665048

    666040

    667031

    668028

    669036

    670041

    671045

    672024

    673051

    674044

    675046

    676042

    677044

    678033

    679036

    680044

    681044

    682033

    683035

    684034

    685040

    686026

    687036

    688039

    689042

    690038

    691033

    692037

    693038

    694053

    695045

    696048

    697046

    698031

    699040

    700041

    701043

    702038

    703041

    704040

    705036

    706043

    707042

    708039

    709047

    710045

    711029

    712048

    713038

    714047

    715036

    716047

    717038

    718034

    719055

    720030

    721035

    722037

    723039

    724044

    725031

    726045

    727037

    728035

    729044

    730036

    731032

    732043

    733045

    734038

    735039

    736042

    737043

    738043

    739029

    740042

    741045

    742038

    743036

    744058

    745025

    746037

    747034

    748050

    749039

    750027

    751051

    752035

    753040

    754052

    755033

    756049

    757032

    758046

    759037

    760026

    761046

    762042

    763045

    764035

    765061

    766040

    767037

    768033

    769042

    770045

    771037

    772039

    773038

    774036

    775050

    776037

    777037

    778040

    779029

    780041

    781044

    782038

    783035

    784032

    785054

    786037

    787050

    788040

    789032

    790038

    791044

    792045

    793043

    794033

    795035

    796035

    797041

    798043

    799045

    800034

    801036

    802043

    803044

    804043

    805035

    806051

    807041

    808036

    809038

    810037

    811051

    812039

    813035

    814033

    815051

    816044

    817046

    818029

    819038

    820042

    821038

    822046

    823036

    824042

    825045

    826044

    827035

    828039

    829042

    830048

    831040

    832039

    833035

    834052

    835047

    836045

    837037

    838044

    839053

    840048

    841043

    842034

    843042

    844045

    845037

    846033

    847048

    848030

    849036

    850045

    851025

    852033

    853027

    854031

    855039

    856040

    857036

    858041

    859043

    860042

    861038

    862036

    863042

    864043

    865033

    866043

    867042

    868033

    869036

    870037

    871037

    872033

    873040

    874034

    875048

    876041

    877042

    878028

    879039

    880041

    881048

    882046

    883036

    884040

    885029

    886049

    887039

    888037

    889054

    890027

    891038

    892039

    893035

    894041

    895051

    896031

    897039

    898052

    899031

    900046

    901045

    902042

    903046

    904052

    905054

    906048

    907041

    908039

    909036

    910051

    911025

    912049

    913040

    914039

    915046

    916038

    917047

    918043

    919035

    920035

    921052

    922046

    923036

    924025

    925043

    926029

    927045

    928038

    929038

    930047

    931034

    932038

    933039

    934040

    935040

    936037

    937032

    938045

    939043

    940038

    941038

    942039

    943053

    944043

    945043

    946038

    947044

    948041

    949042

    950036

    951026

    952043

    953046

    954049

    955039

    956032

    957040

    958040

    959038

    960035

    961032

    962040

    963029

    964027

    965037

    966038

    967038

    968035

    969035

    970043

    971031

    972038

    973041

    974037

    975041

    976028

    977043

    978032

    979035

    980037

    981046

    982033

    983041

    984034

    985043

    986037

    987047

    988034

    989043

    990032

    991035

    992051

    993039

    994039

    995031

    996042

    997033

    998037

    999039

    39.98

    Time

    Counts

    0

    4

    8

    12

    16

    20

    24

    28

    32

    36

    40

    44

    48

    52

    56

    60

    64

    68

    k (counts)

    log(occurances)

    0

    0

    0

    0

    1

    2

    3

    27

    79

    185

    266

    196

    145

    64

    28

    4

    1

    0

    00.9048374180.36787944120.0497870684

    10.09048374180.36787944120.1493612051

    20.00452418710.18393972060.2240418077

    30.00015080620.06131324020.2240418077

    40.00000377020.015328310.1680313557

    50.00000007540.0030656620.1008188134

    60.00000000130.00051094370.0504094067

    700.0000729920.0216040315

    800.0000091240.0081015118

    Counts

    Log(Probability)

    Counts

    Log(Probability)

    Counts

    Log(Probability)

  • Conv. with

    1 particle PCH … 3 Particle PCH

    Species 1 PCH

    Average weighted by number probability

    Species 2 PCH …

    Final PCH

    convolution

    total broadening

    initial distribution

    Recap: Factors that contribute to the final broadening of the PCH

    Convolve

    w/ Self

    1 Particle PCH

    2 Particle PCH

    Sum over PSF

    Fixed Particle Shot Noise

  • Method

    • Sum up Poisson distributions from all possible arrangements and number of fluorophores in excitation volume (PSF) – Intensity weighted sum of all possible single

    particle histograms (Poisson functions) – Convolution to get multiple particle histograms – Number probability weighted sum of multiple

    particle histograms – Convolution to get multi-species histograms

    Chen et al., Biophys. J., 1999, 77, 553.

  • Fitting

    dkkPCHkPCHM

    kPCHkPCHMk observedobserved

    observedmodel

    −⋅⋅−

    =∑

    max

    2

    2 ))(1()()()(

    χ

    M is number of observations

    d is number of fitting parameters

    Chen et al., Biophys. J., 1999, 77, 553.

  • Model Test

    1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 10 20 30k (counts)

    log(

    occu

    renc

    es)

    ε = 91,330 cpsm

    N = 0.12

    ε = 9,030 cpsm

    N = 1.28

    1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 10 20 30k (counts)

    log(

    occu

    renc

    es)

  • Hypothetical situation: Protein Interactions

    • 2 proteins are labeled with a fluorophore • Proteins are soluble • How do we assess interactions between these

    proteins?

  • Dimer has double the brightness

    + ε = εmonomer ε = 2 x εmonomer

    All three species are present in equilibrium mixture

    Typical one photon εmonomer = 10,000 cpsm

  • Photon Count Histogram (PCH)

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 2 4 6 8 10 12 14k (counts)

    log(

    occu

    ranc

    es)

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 2 4 6 8 10 12 14k (counts)

    log(

    occu

    ranc

    es)

    1.E+00

    1.E+01

    1.E+02

    1.E+03

    1.E+04

    1.E+05

    0 2 4 6 8 10 12 14k (counts)

    log(

    occu

    ranc

    es)

    + +

  • 1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

    1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

    Simulation Solution

    ε = 9,000 cpsm

    N = 1.3

    ε = 16,000 cpsm

    N = 0.73

    + +

  • 1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

    1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

    Global Fitting: Fit Data Sets Simultaneously

    ε = 9,000 cpsm N = 1.3

    ε1 = 9,000 cpsm N1 = 0.29 ε2 = 18,100 cpsm N2 = 0.50

    Link

    + +

    or

  • What we measure is the number of particles in the PSF. How Do We Get Concentrations?

    • N is defined relative to PSF volume • One photon:

    • Two photon:

    • Definition is same as for FCS • Can use FCS to determine w0 (and maybe z0)

    rdrPSFVPSF

    ∫= )(( ) 2/30203 2/πzwV DG =

    λπ 40

    2wVGL =

    w0 = 0.21 um, z0 = 1.1 um, VPSF = 0.091 um3, C = 23 nM

  • How to Improve Accuracy

    • Minimize sources of instrument noise – PSF heterogeneity – Shot noise

    • Maximize particle burst amplitudes

  • 1E-121E-11

    1E-101E-091E-08

    1E-071E-061E-05

    0.00010.0010.01

    0.11

    0 2 4 6 8 10

    Counts

    Prob

    abili

    ty

    0.0000001

    0.000001

    0.00001

    0.0001

    0.001

    0.01

    0.1

    1

    0 2 4 6 8 10

    Counts

    Prob

    abili

    ty

    Effect of Brightness

    ε = 10,000 cpsm ε = 100,000 cpsm

    Poisson PCH

    PCH

    Poisson

  • -200

    0

    200w

    eigh

    ted

    resi

    dual

    s-200

    0

    200

    wei

    ghte

    d re

    sidu

    als

    Saturation Effect Rhodamine 110 on the Zeiss Confocor 3

    10 uW laser

    Laser power is not an infinite source of brightness!

    0.00000010.000001

    0.000010.0001

    0.0010.01

    0.11

    0 2 4 6k (counts)

    log(

    occu

    renc

    es)

    60 uW laser

    0.000001

    0.00001

    0.0001

    0.001

    0.01

    0.1

    1

    0 2 4 6 8 10k (counts)

    log(

    occu

    renc

    es)

    Multi-Species Fit

  • 0.0000001

    0.000001

    0.00001

    0.0001

    0.001

    0.01

    0.1

    1

    0 2 4 6 8 10

    Counts

    Prob

    abili

    ty

    1E-121E-11

    1E-101E-091E-08

    1E-071E-061E-05

    0.00010.0010.01

    0.11

    0 2 4 6 8 10

    Counts

    Prob

    abili

    ty

    Concentration Effect

    N=1 N=10

    Poisson PCH PCH Poisson

    Brightness increases by 100%

    Brightness increases by 10%

    Note: if N is too low, experiment becomes photon limited

  • Sampling Time Effect

    Wu and Mueller, Biophys. J., 2005, 89, 2721.

    00.05

    0.10.15

    0.20.25

    0.30.35

    1.E-05 1.E-03 1.E-01tau (s)

    G(ta

    u)

    02000400060008000

    1000012000

    1.E-05 1.E-03 1.E-01Bin Size (s)

    Brig

    htne

    ss (c

    psm

    )

    0

    510

    15

    2025

    30

    1.E-05 1.E-03 1.E-01Bin Size (s)

    Num

    ber

    Again, shorter sampling leads to photon limited acquisition

    In general sample as long as possible without diffusion averaging

  • PSF X,Y, and Z Dimensions Don’t Matter Z

    X

    VPSF = 0.08 fL

    VPSF = 0.08 fL 1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

  • 1.E-06

    1.E-05

    1.E-04

    1.E-03

    1.E-02

    1.E-01

    1.E+00

    0 5 10 15k (counts)

    log(

    occu

    renc

    es)

    Functional Form DOES Matter

    3DG

    GL2 poisson

  • Functional Form Matters for PCH

    PSF z-Profile

    1.E-101.E-091.E-081.E-071.E-061.E-051.E-041.E-031.E-021.E-011.E+00

    0 2 4 6

    z (um)

    Inte

    nsity

    (Log

    )

    3D Gaussian

    GL Squared

    0.E+00

    1.E-01

    2.E-01

    3.E-01

    4.E-01

    5.E-01

    6.E-01

    7.E-01

    8.E-01

    9.E-01

    1.E+00

    0 2 4 6

    z (um)

    Inte

    nsity

    3D GaussianGL Squared

    PCH

    0.000001

    0.00001

    0.0001

    0.001

    0.01

    0.1

    1

    0 2 4 6 8

    k (counts per time bin)

    Prob

    abili

    ty 3D Gaussian

    Gauss-Lorentz Squared

    Chart1

    00

    0.050.05

    0.10.1

    0.150.15

    0.20.2

    0.250.25

    0.30.3

    0.350.35

    0.40.4

    0.450.45

    0.50.5

    0.550.55

    0.60.6

    0.650.65

    0.70.7

    0.750.75

    0.80.8

    0.850.85

    0.90.9

    0.950.95

    11

    1.051.05

    1.11.1

    1.151.15

    1.21.2

    1.251.25

    1.31.3

    1.351.35

    1.41.4

    1.451.45

    1.51.5

    1.551.55

    1.61.6

    1.651.65

    1.71.7

    1.751.75

    1.81.8

    1.851.85

    1.91.9

    1.951.95

    22

    2.052.05

    2.12.1

    2.152.15

    2.22.2

    2.252.25

    2.32.3

    2.352.35

    2.42.4

    2.452.45

    2.52.5

    2.552.55

    2.62.6

    2.652.65

    2.72.7

    2.752.75

    2.82.8

    2.852.85

    2.92.9

    2.952.95

    33

    3.053.05

    3.13.1

    3.153.15

    3.23.2

    3.253.25

    3.33.3

    3.353.35

    3.43.4

    3.453.45

    3.53.5

    3.553.55

    3.63.6

    3.653.65

    3.73.7

    3.753.75

    3.83.8

    3.853.85

    3.93.9

    3.953.95

    44

    4.054.05

    4.14.1

    4.154.15

    4.24.2

    4.254.25

    4.34.3

    4.354.35

    4.44.4

    4.454.45

    4.54.5

    4.554.55

    4.64.6

    4.654.65

    4.74.7

    4.754.75

    4.84.8

    4.854.85

    4.94.9

    4.954.95

    55

    5.055.05

    5.15.1

    5.155.15

    5.25.2

    5.255.25

    5.35.3

    5.355.35

    5.45.4

    5.455.45

    5.55.5

    5.555.55

    5.65.6

    5.655.65

    5.75.7

    5.755.75

    5.85.8

    5.855.85

    5.95.9

    5.955.95

    66

    6.056.05

    6.16.1

    6.156.15

    6.26.2

    6.256.25

    6.36.3

    6.356.35

    6.46.4

    6.456.45

    6.56.5

    6.556.55

    6.66.6

    6.656.65

    6.76.7

    6.756.75

    6.86.8

    6.856.85

    6.96.9

    6.956.95

    77

    7.057.05

    7.17.1

    7.157.15

    7.27.2

    7.257.25

    7.37.3

    7.357.35

    7.47.4

    7.457.45

    7.57.5

    7.557.55

    7.67.6

    7.657.65

    7.77.7

    7.757.75

    7.87.8

    7.857.85

    7.97.9

    7.957.95

    88

    8.058.05

    8.18.1

    8.158.15

    8.28.2

    8.258.25

    8.38.3

    8.358.35

    8.48.4

    8.458.45

    8.58.5

    8.558.55

    8.68.6

    8.658.65

    8.78.7

    8.758.75

    8.88.8

    8.858.85

    8.98.9

    8.958.95

    99

    9.059.05

    9.19.1

    9.159.15

    9.29.2

    9.259.25

    9.39.3

    9.359.35

    9.49.4

    9.459.45

    9.59.5

    9.559.55

    9.69.6

    9.659.65

    9.79.7

    9.759.75

    9.89.8

    9.859.85

    9.99.9

    9.959.95

    1010

    3D Gaussian

    GL Squared

    3DG

    GL^2

    z (um)

    Intensity

    1

    1

    0.9992003199

    0.997423129

    0.9968051145

    0.9897519974

    0.9928258579

    0.9771620197

    0.9872815716

    0.9599357243

    0.9801986733

    0.9384489084

    0.9716107672

    0.9131529325

    0.9615583782

    0.8845545671

    0.9500886338

    0.8531948884

    0.9372548956

    0.8196286389

    0.9231163464

    0.7844052603

    0.9077375355

    0.748052508

    0.8911878885

    0.7110632203

    0.873541186

    0.6738854883

    0.8548750167

    0.636916185

    0.8352702114

    0.6004975874

    0.8148102622

    0.5649166752

    0.793580734

    0.5304066038

    0.7716686739

    0.49714983

    0.7491620228

    0.4652823867

    0.7261490371

    0.4348988611

    0.7027177229

    0.4060576977

    0.6789552903

    0.3787865283

    0.6549476305

    0.353087306

    0.6307788205

    0.3289410871

    0.6065306597

    0.3063123657

    0.5822822402

    0.285152911

    0.5581095554

    0.2654050949

    0.5340851478

    0.2470047214

    0.5102777978

    0.2298833902

    0.486752256

    0.2139704338

    0.4635690175

    0.1991944766

    0.4407841408

    0.1854846634

    0.4184491089

    0.1727716045

    0.3966107333

    0.1609880829

    0.3753110989

    0.1500695624

    0.3545875486

    0.1399545335

    0.3344727057

    0.1305847284

    0.3149945317

    0.1219052322

    0.2961764167

    0.1138645116

    0.2780373005

    0.1064143829

    0.260591821

    0.0995099316

    0.2438504869

    0.0931094

    0.2278198714

    0.0871740494

    0.2125028243

    0.0816680087

    0.1978986991

    0.0765581127

    0.184003592

    0.0718137378

    0.1708105895

    0.0674066365

    0.1583100226

    0.0633107759

    0.1464897235

    0.0595021803

    0.1353352832

    0.0559587801

    0.124830308

    0.052660269

    0.1149566705

    0.0495879676

    0.1056947559

    0.0467246969

    0.0970237

    0.0440546584

    0.0889216175

    0.0415633237

    0.0813658197

    0.0392373313

    0.0743330209

    0.0370643912

    0.0677995311

    0.0350331971

    0.0617414361

    0.0331333447

    0.0561347628

    0.0313552578

    0.0509556313

    0.0296901187

    0.0461803914

    0.0281298059

    0.0417857461

    0.0266668359

    0.0377488601

    0.0252943106

    0.0340474547

    0.0240058682

    0.0306598898

    0.0227956393

    0.0275652323

    0.0216582061

    0.0247433132

    0.0205885652

    0.0221747727

    0.0195820935

    0.0198410947

    0.0186345173

    0.0177246314

    0.0177418837

    0.0158086187

    0.0169005346

    0.0140771833

    0.0161070831

    0.0125153423

    0.0153583913

    0.0111089965

    0.0146515509

    0.009844917

    0.0