Atomic Force Microscopy Investigations of DNA Lesion Recognition in Nucleotide Excision Repair

Summary

Here, the study of different DNA lesion recognition approaches via single molecule AFM imaging is demonstrated with the nucleotide excision repair system as an example. The procedures of DNA and protein sample preparations and experimental as well as analytical details for the AFM experiments are described.

Abstract

AFM imaging is a powerful technique for the study of protein-DNA interactions. This single molecule method allows the simultaneous resolution of different molecules and molecular assemblies in a heterogeneous sample. In the particular context of DNA interacting protein systems, different protein complex forms and their corresponding binding positions on target sites containing DNA fragments can thus be distinguished. Here, an application of AFM to the study of DNA lesion recognition in the prokaryotic and eukaryotic nucleotide excision DNA repair (NER) systems is presented. The procedures of DNA and protein sample preparations are described and experimental as well as analytical details of the experiments are provided. The data allow important conclusions on the strategies by which target site verification may be achieved by the NER proteins. Interestingly, they indicate different approaches of lesion recognition and identification for the eukaryotic NER system, depending on the type of lesion. Furthermore, distinct structural properties of the two different helicases involved in prokaryotic and eukaryotic NER result in and explain the different strategies observed for these two systems. Importantly, these experimental and analytical approaches can be applied not only to the study of DNA repair but also very similarly to other DNA interacting protein systems such as those involved in replication or transcription processes.

Introduction

Atomic force microscopy (AFM) is a powerful technique for the analysis of protein-DNA interactions^{1,2,3,4,5,6,7,8,9}. It requires only low amounts of sample material to directly visualize heterogeneous samples with a resolution at the single molecule level. Heterogeneity can result from different conformational or oligomeric states of a protein. In particular, in the context of protein-DNA samples, protein complexes can display different stoichiometries and/or conformations induced by DNA binding in general or binding to a specific target site within DNA. Heterogeneous samples may also contain two (or more) different kinds of proteins, and different protein complex forms (e.g., consisting of only one type of protein versus heteromeric complexes) may interact differently with DNA. The studies discussed here exploit AFM imaging in air on static, dried samples of DNA repair proteins bound to long (~900 base pairs, bp) DNA fragments that contain a lesion, which represents a target of these proteins. The high, molecular resolution of AFM allows the distinction between different types of protein complexes and to determine the binding positions of the proteins on the DNA fragments. Importantly, the lesions are introduced into the DNA substrates at well-defined positions. Because the position of the lesion site in the DNA is known, the distributions of proteins bound on DNA provide insight into (different) lesion recognition properties of the (different) protein complexes, e.g., how well they recognize a particular type of lesion (compared to non-damaged DNA)^2,3,4,5,6. Their positions on the DNA also allow the distinction between protein complexes bound specifically at the lesions and complexes bound nonspecifically elsewhere on the DNA. Separate characterization of these different complex types (complexes bound specifically at the lesion versus nonspecific complexes) can reveal potential conformational changes in the complexes induced upon target site identification.

The DNA repair proteins focused on here are helicases that are responsible for lesion recognition in the nucleotide excision repair (NER) pathway. In bacteria, NER is achieved by the proteins UvrA, UvrB, and UvrC. UvrA is responsible for initial lesion sensing in a UvaA₂/UvrB₂ DNA-scanning complex. Upon lesion verification by UvrB this complex converts to monomeric UvrB bound at the lesion site and this specific complex can then recruit the prokaryotic NER endonuclease UvrC. UvrC excises a short (12-13 nt) stretch of single stranded DNA (ssDNA) containing the lesion. The missing stretch is then refilled by DNA polymerase. Finally, DNA ligase seals the newly synthesized stretch with the original DNA^9,10. In eukaryotes, most proteins of the NER cascade are part of the large, multimeric transcription factor II H (TFIIH) complex. After initial lesion sensing via the trimeric CEN2-XPC-HR23B complex, TFIIH is recruited to the DNA target site. When XPD within the complex verifies the presence of an NER target lesion, the eukaryotic NER endonucleases XPG and XPF are recruited to excise a short (24-32 nt) stretch of ssDNA containing the lesion^9,10. Here, specifically, the helicases UvrB and XPD from prokaryotic and eukaryotic NER, respectively, were studied. These helicases require an unpaired region in the DNA (a DNA bubble) to thread onto one of the two DNA single strands and subsequently translocate along this strand fueled by ATP hydrolysis. In addition to the DNA lesions, a DNA bubble was hence introduced in the substrates that functions as loading site for the proteins.

The procedure for preparation of specific lesion DNA substrates has been described previously¹¹. It requires a circular DNA construct (plasmid) with two closely spaced restriction sites for a nickase. In the context of this study, the plasmid pUC19N (2729 bp) was used (created by S. Wilson's laboratory, NIEHS). This plasmid contains three closely spaced restriction sites for the nickase Nt.BstNBI that frame a 48 nucleotide (nt) stretch. After incubation with the nickase, the stretch of ssDNA between these sites can be removed and replaced by an oligonucleotide containing any target feature. After each step, complete enzymatic digestion is tested via agarose gel electrophoresis. Nicked circular DNA can be distinguished due to its lower electrophoretic mobility compared to the original supercoiled plasmid. Gapping of the DNA and replacement of the removed stretch by the specific substrate oligonucleotide can be evaluated via digestion with a restriction enzyme which incises the substrate exclusively within the region between the nicks. Linearization of the circular plasmid by the enzyme will hence be suppressed for the gapped DNA and restored after insertion of the specific oligonucleotide. Finally, two endonuclease restriction sites (ideally single cutters) allow for the generation of a linear DNA substrate, with length as desired and with the specific target site at a defined position as well as a DNA bubble at a distance from the lesion either in 5' or 3' direction.

Recognition of the lesions by the NER helicases can be investigated via AFM imaging. Stalled DNA translocation of the helicases at the lesion site is visible as a peak in the protein position distribution on the DNA and indicates lesion recognition. Because DNA translocation of these helicases is furthermore directional, with 5'-to-3' polarity, the dependence of lesion recognition on the position of the loading site (DNA bubble upstream or downstream from the lesion) also indicates whether the lesion is preferentially recognized on the translocated or on the opposite, non-translocated ssDNA strand^5,9. In the following sections, the methods used will be introduced and major findings from these experiments will be briefly discussed. Importantly, analogous to the exemplary work on DNA repair shown here, AFM imaging can be applied to the study of different DNA interacting systems, such as DNA replication or transcription^8,12,13,14.

Protocol

1. Sample Preparation

1. Preparation of DNA substrates¹¹
   1. Generating a ssDNA gap in the plasmid
      1. Completely digest a sample of the plasmid (here: modified pUC19, pUC19N) in a reaction tube with an appropriate nickase (here: Nt.BstNBI) followed by enzyme heat inactivation, using conditions according to the manufacturer's protocol (see Figure 1 for a schematic presentation). Start with ~50 µL and ~500 nM plasmid for a sufficient yield.
      2. Verify plasmid nicking by agarose gel electrophoresis on diluted samples (~20 nM)¹⁵. Wear gloves for protection against the DNA binding dye used for DNA visualization.
         NOTE: Different electrophoretic mobilities allow distinction between nicked (relaxed) and supercoiled circular plasmid DNA (Figure 1).
      3. Remove the incised ssDNA stretch (between the nick sites) from the plasmid by incubation with a ~10-fold excess of the complementary oligonucleotide (oligonucleotide 1 in Table 1), shaking at 300 rpm for 30 min near the melting temperature of the oligonucleotide (here: 68 °C for pUC19N) in a heat block (Figure 1).
      4. Separate the gapped plasmid from the smaller DNA fragments using a 50 kDa molecular weight cut off (MWCO) filter by centrifugation for 10 min at 10,000 x g in a table centrifuge (Figure 1). To extract the concentrated DNA from the filter, invert the filter and insert into a new 1.5 mL reaction tube. Centrifuge for 3 min at 1,000 x g.
      5. Refill the resulting concentrated DNA sample to 500 µL with deionized, filtered water, add an additional ~5-fold excess of complementary oligonucleotide and repeat steps 1.1.1.3 and 1.1.1.4 at least 3 times.
      6. Test for complete gapping of the DNA by incubation with a suitable restriction enzyme (here: XhoI or BglII) using conditions according to the manufacturer's description. Use diluted (nicked versus gapped) DNA samples (~20 nM). Run an agarose gel electrophoresis to distinguish between linearized plasmid (containing no ssDNA gap) and non-incised DNA (gapped DNA) using the nicked DNA as positive control (include a DNA ladder for reference, Figure 1). Wear gloves.
   2. Refilling the gap with modified ssDNA oligonucleotides
      1. Anneal the gapped plasmid via incubation with a ~25-fold excess of a 5' phosphorylated oligonucleotide that contains the specific target site(s) of choice, incubating at ~45 °C for 4 h (Figure 1). Here, use 48 nt ssDNA containing a lesion, either a fluorescein adducted thymine or a cyclobutane pyrimidine dimer (CPD), and in addition a short (8 nt) non-complementary sequence to produce DNA bubbles (see Table 1).
      2. Covalently link the annealed insert to the plasmid by incubation with T4 DNA ligase overnight at room temperature according to the manufacturer's protocol (Figure 1). For this reaction, add ATP containing concentrated buffer stock solution to produce suitable buffer conditions for the ligase (e.g., use UvrB reaction buffer: 50 mM Tris-HCl pH 7.5, 10 mM MgCl₂, 50 mM KCl, 5 mM DTT, 1 mM ATP).
      3. Test for the insertion of the specific oligonucleotide into the gapped plasmid by digestion of diluted samples with a suitable restriction enzyme (same as in 1.1.1.6) according to the manufacturer's protocol followed by an agarose gel electrophoresis (as in 1.1.1.6, Figure 1).
   3. Preparation of linear DNA substrate
      1. Digest the modified plasmid DNA with restriction enzymes (ideally with a single restriction site in the plasmid) using conditions as recommended by the manufacturer (Figure 1). This step produces linear fragments containing the inserted modification at a defined position. Here, use SspI and BspQI cutting at positions 613 and 255 bp upstream and downstream of the insert, respectively, resulting in a 916 bp DNA fragment containing the specific lesion site at ~30% of the DNA length.
         NOTE: For AFM imaging experiments as described here, DNA fragments with lengths between ~200 bp and ~2,000 bp are suitable substrates.
      2. Isolate the target fragment via agarose gel electrophoresis and gel extraction using a commercial kit. Wear gloves for protection.
      3. Optionally, cut agarose gel with a scalpel to separate the DNA ladder and diluted sample lanes (first two lanes) from the lanes containing the concentrated DNA to be purified. Only expose the gel part with the first two lanes to UV irradiation by placing only this part of the gel on a UV table.
         1. Cut out the band corresponding to the fragment of choice with a scalpel. Re-unite the two gel parts (off the UV table). Use the position of the excised band from the dilute sample as orientation for the position of the band of the desired DNA substrate. Account for the higher concentration by cutting out slightly broader slices than for the dilute control.
            NOTE: Because here, recognition of UV-lesions was investigated, introduction of additional UV lesions via UV irradiation was carefully avoided in the DNA substrate by this approach.
      4. Calculate the DNA concentration c from the absorption at 260 nm measured by a UV-Vis spectrophotometer using Lambert-Beer's law with a double stranded DNA (dsDNA) average molar extinction coefficient of ϵ_260nm ~6,700 M⁻¹ cm⁻¹ per bp:
         
         where L is the path length (measurement chamber length, typically 1 cm).
2. Expression and purification of proteins
   1. Recombinantly express UvrB in E. coli and purify the protein via standard chitin bead affinity¹⁵ and size exclusion chromatography¹⁵ as previously described¹⁶.
      NOTE: The uvrB gene from Bacillus caldotenax had been cloned into the pTYB1 vector.
   2. Express XPD in E. coli and purify the protein via standard nickel IDA affinity¹⁵ and size exclusion chromatography¹⁵ followed by anion exchange chromatography¹⁵, as previously described¹⁷.
      NOTE: The gene for Chaetomium thermophilum Xeroderma pigmentosum group D protein (XPD) had been cloned into the pBADM11 vector. C. thermophilum p44 was a kind gift from Caroline Kisker's laboratory, expressed and purified as described¹⁷.

2. AFM Experiment

1. Sample preparation
   1. Optionally, pre-incubate the DNA substrate at 65 °C for 10 min in a heat block to remove potential micro-salt crystals that may have formed during storage in the fridge.
   2. Prepare reaction buffer(s) at a 10-fold concentration (10x buffers).
      NOTE: XPD reaction buffer at 1x concentration contained 20 mM Tris-HCl pH 7.5, 10 mM KCl, 5 mM MgCl₂, 1 mM TCEP, 2 mM ATP; 1x UvrB reaction buffer contained 50 mM Tris-HCl pH 7.5, 50 mM KCl, 10 mM MgCl₂, 5 mM DTT, and 1 mM ATP.
   3. Pre-incubate proteins at a higher concentration in suitable incubation conditions to enhance complex formation. Pre-dilute a small volume (e.g., 1 µL) of the individual proteins in 1x protein reaction buffer to the desired concentration and mix small volumes (e.g., 1 µL) of the individual protein solutions in a 0.5 mL reaction tube.
      1. Place the tube in a heat block for incubation temperatures higher than room temperature. Choose a concentration ratio depending on the expected complex stoichiometry, either equimolar or corresponding concentrations. Here, incubate 1 µL XPD (20 µM in 1 x XPD reaction buffer) and 1 µL p44 (20 µM in 1x XPD reaction buffer) at 10 µM each for 10 min at 37 °C.
   4. Incubate samples at suitable protein and DNA concentrations in protein reaction buffer in a 0.5 mL reaction tube. Here, use 500 nM UvrB or 1 µM XPD + 1 µM p44 and 100 nM DNA. Pipette small volumes to save material, e.g., 0.25-0.5 µL protein (pre-diluted to a 10-fold incubation concentration) and DNA in a total volume of 2.5-5 µL of 1x protein reaction buffer. Here, incubate for 30 min at 37 °C in a heat block. Spin down in a reaction tube briefly (~1 s) in a table centrifuge to ensure mixing of small volumes.
2. Sample deposition
   1. Prepare a mica substrate: cut an approximately 1 x 1 cm² piece of mica from larger strips using a scalpel. Strip off top layers of the multi-layered mica mineral piece using adhesive tape to reveal a clean, flat, and atomically smooth substrate surface.
      NOTE: The mica piece can be re-used for multiple experiments by stripping off further layer(s).
   2. Prepare the AFM deposition buffer with deionized, filtered water, e.g., 25 mM HEPES pH 7.5, 25 mM Na-acetate, 10 mM Mg-acetate. Filter through a 0.02 µm syringe filter.
      NOTE: Divalent cations in the deposition buffer serve to chelate the negatively charged DNA molecules to the mica surface, which also is negatively charged at neutral pH. If the relatively high Mg²⁺ ion concentration in the deposition buffer poses a problem for a particular protein-DNA system, alternatively, the mica surface can be pre-loaded with amino groups using silatrane-based chemistry to provide positive surface charges for anchoring¹⁸. Sample deposition can then be carried out in a buffer that contains no or only low amounts of divalent cations.
   3. Dilute the sample (see 2.1) for immediate deposition onto mica in deposition buffer. Deposit a small volume (here: 20 µL).
      NOTE: Dilution factors depend on the sample concentration. Here, dilute samples 50-100x. As a rule of thumb, ~1 nM DNA results in a good surface coverage for ~1,000 bp.
   4. Immediately rinse sample three to four times with a few milliliters of filtered, deionized water, blot off excess liquid, and blow dry in a gentle stream of nitrogen. The entire process from sample deposition to dried samples can be carried out within less than 30 s.
   5. Fix the piece of mica on a microscope slide using adhesive tape at its edges.
      NOTE: Different AFM systems have different requirements for fixing the sample to the stage. Other AFMs possess magnetic stages, and the mica pieces are fixed onto magnetic disks, e.g., using thermal glue. Details of the AFM system used here can be found in the Table of Materials.
3. AFM imaging
   1. Place the sample (see 2.2.5) centrally on the AFM stage and fix the microscope slide on the stage with magnetic pads.
   2. Insert the AFM tip into the tip holder. Use cantilevers with a sharp (<10 nm) AFM probe suitable for oscillating, intermittent contact mode imaging in air. Use AFM probes, for example, as listed in the Table of Materials. Here (depends on AFM), fix the tip in the holder under a clamp by tightening the clamp screw (finger tight). Insert the tip holder into the AFM measurement head. Rest the head on its back for this step.
   3. Place the AFM measurement head on top of the sample. Details depend on the AFM model. Here, make sure the head stands stably with its legs inside the stage indentations. Make sure the mica is located on the stage where the AFM tip will hover directly above it. Micrometer screws on the right of the stage allow for fine positioning of the sample.
   4. Align the AFM laser on the back of the cantilever for optimal signal strength from the position sensitive photodetector onto which the laser is reflected. Details depend on the AFM model.
      1. Here, turn the wheels at the right side and back of the AFM measurement head to adjust the x- and y-positions of the AFM laser to direct it centrally onto the end of the cantilever. Watch the reflection signal in the AFM video window (if available, here: press the camera icon and chose input: Svideo).
      2. Once crudely positioned, optimize the detector sum signal (Sum in Sum and Deflection Meter window in AFM software) by fine tuning the laser position with the two wheels (stay at the end of the cantilever, the sum signal depends on the AFM and cantilever type, here: aim for sum >5).
   5. Zero the difference signal from the top and bottom diodes of the detector array (here: Deflection signal in Sum and Deflection Meter window) by directing the AFM laser reflection onto the detector center (here: turn the wheel at the left side of the AFM measurement head).
      NOTE: Deviations from zero then indicate the deflection of the cantilever due to surface interactions, which are translated into height information by the AFM.
   6. Determine the cantilever resonance frequency by a frequency tune implemented into the AFM software (here: command auto tune in Master Panel/Tune window). Choose an amplitude corresponding to 1 V input for the piezo that drives the cantilever oscillation. Set the oscillation frequency to slightly (5%) lower than the resonance frequency and zero the phase of the oscillation.
   7. Approach the tip to the sample surface using the crude engage mode (here: command Engage in Master Panel window) until the protective setting (set-point) is reached. Use ~2% cutting of the free level oscillation amplitude as the set-point (here, enter Set Point 980 mV in the Master Panel).
   8. Fine-engage the AFM tip with the sample surface by lowering the set point using the AFM software. Aim for repulsive mode imaging with the cantilever oscillation phase (Phase in Sum and Deflection Meter window) just below the free level phase (before engage, here typically ~70). Here, use typical final set points on the order of 70-80% of the free level amplitude (1 V).
   9. Before scanning, choose the signals for recording in the Master Channel Panel. Choose height (Ht) and amplitude (Am).
   10. Begin sample scanning (here: command Do Scan in Master Panel window). Use a scan speed of e.g., 2.5 µm/s (command Scan Speed in Master Panel) to image surface areas of 4 µm x 4 µm or 8 µm x 8 µm (enter Scan Size in Master Panel) with pixel resolutions of 2,048 or 4,096 (Scan Points and Scan Lines in Master Panel), respectively.
   11. Save the image file (command Save Image in Master Panel) with no fitting modifications (choose None in Master Channel Panel/Save Plane Fit).
   12. For further analysis, process the saved image. Load the image (command Browse Saved Data in the AFM Analysis menu). Open the Modify Panel (press M in the top section of the image). Apply a planefit in x and y dimensions to the height image (extension HtR) (command XY in Planefit window in Modify Panel, choose Planefit Order 3). Then flatten the image (command Flatten in Flatten window in Modify Panel) choosing Flatten Order 3.
   13. Export the image as a TIFF file (press Commands in top section of image, choose TIFF Export 2x corresponding to 2,048 pixel resolution) for further analysis.

3. AFM Analysis

1. Protein complex volume
   1. Pre-select relevant protein-DNA complexes by direct visual inspection of the images in the AFM software, using a suitable color scheme to maximize different appearances of different size complexes (see different colors and sizes of different complexes in Figure 2; here: color scheme SeaLandAndFire in the AFMsoftware). For XPD samples, possible complexes included XPD/p44-DNA as well as XPD-DNA and p44-DNA, with distinctly different sizes due to the relatively large, different molecular masses of XPD (~95 kDa) and p44 (~40 kDa).
   2. Measure volumes of individual protein peaks on the DNA to verify the complex type. This can be achieved with different image software (here: the section tool of the AFM software).
      1. Measure the height (h) and diameter (d) of the protein peak sections with the section window cursors. Measure the diameter close to the base of the particle section.
      2. Determine the volume (V) of the peaks using simple mathematical models, e.g., using the following formula, which is based on a spherical cap model:
         
   3. Translate measured volumes into an approximate protein molecular mass.
      1. Initially, calibrate the AFM system for volume to molecular weight (MW) conversion using a range of proteins with known molecular weight (here: a total of 12 experiments with between 25 and 851 data points each were conducted on 5 different proteins in monomeric, dimeric, trimeric, or tetrameric states) ^4,19,20. Deposit and image proteins (as described above, in 2.2 and 2.3) and measure their volumes as described above (3.1.2). Plot the volumes over their known molecular weights. The resulting graph will show a linear relationship between V and MW, the equation for which can be obtained by a line fit to the data. For the AFM system used here, the following relationship was obtained¹⁹:
         
         NOTE: This step does not have to be repeated before each measurement, but is only done once. The volume to MW calibration can be applied to images obtained under similar imaging conditions using AFM probes with slightly varying diameters.
      2. Based on their measured volumes (3.1.2) and the V-to-MW calibration (3.1.3.1), determine the approximate MW of the protein complexes²⁰, which provides information on its molecular content. E.g., for XPD/p44 samples, ~50 kDa, ~100 kDa, and ~140 kDa were obtained, consistent with p44-DNA complexes (or peaks caused by mere DNA superstructure), XPD only peaks, and XPD/p44 peaks, respectively.
2. Protein complex positions on DNA
   1. Determine the DNA fragment lengths.
      1. Trace the DNA fragments in the AFM images, e.g., with the freehand line function of a suitable image analysis software (see for example Table of Materials) and measure the length of the line.
         NOTE: Exclude DNA aggregates as well as fragments cut off by the image margins.
      2. Bin and plot the DNA lengths from the entire experiment in a histogram, using suitable data analysis and graphing software (e.g., see Table of Materials).
      3. Fit the length distributions with a Gaussian curve in the data analysis and graphing software to determine the length of the DNA fragments. In order to know the position of the inserted DNA target site (see 1.1), only include DNA fragments with the correct length within two standard deviations from the center of the Gauss curve (y = y₀ + z exp(-2(x-x_c)²/w²), where z is a norm factor and x_c and w are the center and full maximum half width of the Gaussian) in further analyses.
         NOTE: The DNA length at the center of the Gauss curve must be close to the theoretical length of the DNA fragment (calculated using 0.34 nm/bp). Lengths of up to 10% shorter than the theoretical value are typical and are likely caused by AFM resolution limits.
   2. Determine positions of protein peaks on DNA substrates.
      1. Measure the distance of the protein peaks from the closer DNA fragment end, as described in 3.2.1.1 and divide by the total DNA length to obtain distances in units of fraction of DNA length.
      2. Bin and plot the measured distances in a histogram using a suitable data analysis and graphing software (see e.g., Figure 3). As a rule of thumb, choose a bin size that gives approximately √n bins for n data points.
         NOTE: Since DNA ends cannot be distinguished here, plot only to fraction of DNA length 0.5 (center of DNA fragment). Because DNA end binding is not the focus of the study, exclude DNA ends from the analyses by starting to bin the position data slightly after position 0 (e.g., here: binning from a DNA length fraction of 0.02).
   3. Determine the target site specificity from protein complex position distributions.
      1. Fit the maximum (enhanced binding occurrences) in the position distribution with a Gauss curve as in 3.2.1.3 but footed on the height of background binding (see Figure 3).
      2. Calculate the specificity S for the specific site versus the nonspecific DNA background (protein molecules bound to non-specific DNA sites) with the following formula²¹
         
         A_sp: Number of specific complexes (area under the Gaussian curve)
         A_nsp: Number of nonspecific complexes (area of the background, i.e. (fraction DNA length) x (average background height y₀); the fraction of DNA length covered here is 0.48 for a histogram starting at 0.02 DNA length)
         N: number of possible DNA binding sites (here: N = 914 excluding DNA ends)
3. DNA bend angles
   1. Using the angle tool in a suitable image analysis software, measure the angle β between two lines placed centrally along the DNA backbone and centering at the protein peak (see e.g., inset in Figure 4). Measure the angles for a statistically relevant number of protein-DNA complexes (>50, ideally >100)^2,3,5.
      NOTE: The DNA bend angle is defined as 180°-β^2,3,5.
   2. Using data analysis and graphing software (see Table of Materials) produce a bend angle distribution histogram by binning the DNA bend angles.
   3. Fit the bend angle distribution with a Gauss curve. If more than one maximum is apparent in the distribution, choose multiple peak Gauss fit. The center(s) of the Gaussian curve(s) give(s) the average bend angle state of the particular species.
   4. If a shift in the bend angle(s) (maxima of Gaussian fit(s)) is apparent for distributions, for instance, of different protein variants or different protein complex species, apply a student t -test to evaluate the significance level of the changes.

Results

Distinguishing between different complex types based on protein complex volumes

The helicase activity of the prokaryotic NER helicase UvrB is stimulated by DNA binding^22,23. UvrB requires an unpaired region in the DNA (a DNA bubble) in order to load correctly onto one of the two single ssDNA strands. In vivo, this DNA structure is provided by DNA interactions throu...

Discussion

AFM statistical analyses of binding positions of proteins on long DNA fragments that contain specific target sites can reveal interesting details on the particular strategies employed by the protein to recognize these sites^2,3,4,5,6. To interpret the resulting position distributions, the positions of the targets in the DNA need to be precisely known. This is a...

Materials

List of materials used in this article

Name	Company	Catalog Number	Comments
Molecular Force Probe (MFP) 3D	Asylum Research	N/A	atomic force microscope (AFM)
Precision 390	DELL	N/A	computer
ThermoMixer and 1.5 mL block	Eppendorf	5382000015	heat block for DNA preparation
Rotilabo Block-Heater H 250 & blocks for 0.5 mL tubes	Carl Roth GmbH	Y264.1 & Y267.1	heat block for protein-DNA incubations
Mini-Sub Cell GT	Bio-Rad Laboratories GmbH	1704467	electrophoresis chamber with gel caster and power supply
Power Pac Basic	Bio-Rad Laboratories GmbH	1645050	electrophoresis power supply
Centifuge 5415 D with rotor	Eppendorf	2262120-3	table centrifuge
Ultra-Lum electronic UV transillumonator MEB-15	Ultralum	900-1322-02	UV irradiation table
NanoDrop ND-1000	VWR International / PEQLAB Biotechnologie GmbH	N/A	UV spectrophotometer
TKAX-CAD with 0.2 μm capsule filter	Unity Lab Services	N/A	water deionization and filter unit
Name	Company	Catalog number	Comments
Software
MFP software on Igor Pro	Asylum Research	N/A	AFM software
ImageJ (open source Java image processing)	NIH Image	N/A	Image analysis software
Excel (Microsoft Office)	Microsoft Corporation	N/A	data analysis software
Origin9 / Origin2016	OriginLab Corporation	N/A	statistical data analysis and graphing software
Name	Company	Catalog number	Comments
Material
OMCL-AC240TS	Olympus	OMCL-AC240TS	AFM cantilevers
grade V-5 muscovite	SPI Supplies	1805	mica sheets
Amicon Ultra 0.5 mL 50k Ultracell	Millipore Ireland Ltd.	UFC505096	centrifuge filters
NucleoSpin Extract II	Macherey-Nagel GmbH	740 609.250	Agarose gel extraction kit
Rotilabo cellulose paper type 111A	Carl Roth GmbH	AP59.1	AFM deposition blotting paper
Anatop 25 (0.02 μm)	Whatman GmbH	6809-2102	syringe filter
SSpI, BspQI	New England Biolabs (NEB)	R0132, R0712	restriction enzymes for DNA substrate preparation
XhoI, BglII		R0146, R0144	restriction enzymes for DNA preparation controls
nicking restriction enzyme Nt.BstNBI	New England Biolabs (NEB)	R0607	nickase
T4 DNA ligase	New England Biolabs (NEB)	M0202S	Ligase
Tris, HEPES	Carl Roth GmbH	4855, 9105	buffer chemicals
NaCl, MgCl2, KCl, MgAcetate	Carl Roth GmbH	3957, HN03, HN02, P026	salt chemicals
NaAc	Sigma-Aldrich Chemie GmbH	32318	salt chemicals
DTT, TCEP, EDTA		6908, HN95, 8040	chemicals/reagents
agarose, acetic acid, HCl	Carl Roth GmbH	2267, 3738, K025	reagents
ATP	Carl Roth GmbH	K054	nucleotides
oligonucleotide #1 in Table 1	Biomers	custom	complementary DNA oligonucleotide
oligonucleotides #2, #3, and #6 in Table 1	Integrated DNA Technologies (IDT)	custom	fluorescein containing oligonucleotides
oligonucleotides #4  and #5 in Table 1	private (available from e.g. TriLink or GlenResearch)		CPD containing oligonucleotides
SafeSeal reaction tube 0.5 mL and 1.5 mL	Sarstedt	72.704 and 72.706	incubation tubes
GeneRuler 1 kb	Thermo Scientific	SM0311	DNA ladder
6x concentrate gel loading dye purple	New England Biolabs (NEB)	51406	DNA loading dye
Midori Green	Nippon Genetics Europe GmbH	999MG28055	DNA stain