Best practice in CD Nicholas C. Price IBLS University of Glasgow Efraim Racker (1913-1991) “Don’t waste clean thoughts on dirty enzymes”. An example of poor CD data A glycoprotein – CD spectra recorded at progressively higher concentrations (e to a) At high protein concentrations, the spectra reflect the “HT voltage artefact”. An example of incorrect scaling Stated to be typical of a protein with significant -helix. However, the values of [] are about 5 times too small. Far UV CD of BSA at pH 7.0 (a) and 4.2 (b). A further example of incorrect scaling Vis-near UV CD spectrum of ETF (Electron Transferring Flavoprotein) (WT and mutant) ETF CD spectrum (continued) •According to the text, the molar concentrations are expressed in terms of the flavin. •In this case, we would need to use a protein concentration of about 250 mg/ml in a cell of pathlength 1 cm to obtain a maximum signal of 1 mdeg. •Much more likely is that the molar concentrations are expressed in terms of the peptide bond unit (some 550-fold higher). Main sections of talk Stages of CD analysis Preparation of sample Acquisition of data Presentation and analysis of data The stages of CD analysis •Preparation and characterisation of sample •Acquisition of data •Presentation and analysis of data Each of these must be carefully checked! Preparation and characterisation of sample (1) •Most protein samples are now produced by heterologous over-expression. •Is the protein pure and of the correct sequence; have any tags been removed and have any posttranslational modifications occurred? •Is the protein stable under the conditions studied? Preparation and characterisation of sample (2) How do we determine the concentration of the sample? Methods available include:•Coomassie Blue binding (Bradford assay) •Bicinchoninic acid (BCA) assay •UV absorption (280 nm or 205 and 280 nm) •Amino acid analysis Each has its merits but AAA is the gold standard. Preparation and characterisation of sample (3) •Make sure that the protein is stable in the solvent used and that solvent absorbance is not too high. •Avoid high concentrations of Cl- ions, carboxylate ions and imidazole, especially for far UV CD studies. •Always run a solvent blank and check the HT voltage over the wavelength range. •If necessary, adjust cell pathlength and protein concentration to optimise conditions. Effect of buffers on CD spectra (1) 1, 50 mM sodium phosphate, pH 7.4; 2, plus 150 mM NaCl; 3, plus 150 mM imidazole; 4, plus 50 mM acetate Effect of buffers on CD spectra (2) Acquisition of data (1) Is the spectropolarimeter regularly maintained and calibrated? Calibration of wavelength using (among others):•Holmium oxide (279.4, 361.0 and 453.7 nm) •Benzene vapour (241.7, 253.0 and 260.1 nm) •Neodymium glass (586.0 nm) Best to check calibration at a number of wavelengths. Acquisition of data (2) Amplitude calibration can be achieved using:•Camphor Sulphonic Acid (peaks at 290.5 nm and 192.5 nm) •Pantolactone (peak at 219 nm) •Tris(en)Co complex (peak at 490 nm) Acquisition of data (3) Is the cell properly cleaned and is its pathlength known accurately? Pathlengths can differ significantly from nominal values for short pathlength cells (<0.01 cm), and especially demountable cells. Acquisition of data (4) Are the machine settings optimised? •Bandwidth •Time constant (response time, dwell time) •Scan rate •Number of scans Useful guidelines are:SR x TC < bandwidth < W/10 (where W is width at ½ height of spectral feature). Effect of machine settings on CD spectra Solid line, 0.5 s, 50 nm/min; dotted line, 2 s, 50 nm/min; dashed line, 2 s, 100 nm/min. Presentation and analysis of CD data • CD data are presented in terms of either ellipticity (degrees) or absorbance. • In order to normalise data, they are referred to molar concentrations of chromophore or repeating unit. • For far UV CD, the repeating unit is the peptide bond. • The mean residue weight (MRW) is calculated from the molecular mass/(N – 1); N = number of amino acids. • For most proteins, MRW is around 110. Units for CD data (1) To calculate mean residue ellipticity ([]mrw ) []mrw = (MRW x obs) deg. cm2.dmol-1 10 x d x c Where obs d c = observed ellipticity in degrees = pathlength in cm = concentration in g/ml Units for CD data (2) If we know the molar concentration (m) of a solution:[]molar = (100 x obs) deg.cm2.dmol-1 (d x m) where d is the pathlength in cm. Units for CD data (3) For data in absorption units, it is usual to calculate the molar extinction coefficient = L– R in units of M-1.cm-1 If a solution of molar concentration m in a cell of pathlength d cm gives a difference in absorbance (AL - AR) of Aobs, the value of is given by:= Aobs M-1.cm-1 dxm Units for CD data (4) • Note the relationship []mrw = 3298 • There is some debate about the correct choice of molar units for near UV and visible CD – does it refer to the MRW or to the intact protein? The paper should state this clearly. Analysis of CD data (1) • There is a variety of algorithms for far UV CD analysis, e.g. SELCON, VARSLC, CDSSTR, CONTIN and K2d. • These can differ in terms of reference sets of proteins and wavelength ranges covered. • The online server DICHROWEB (hosted at Birkbeck College) allows easy data input and analysis. Analysis of CD data (2) Important criteria for assessing the reliability of analysis include:•Goodness of fit parameter NRMSD (should aim for <0.1, or ideally <0.05) •Difference (R) between X-ray and CD analysis (should aim for <0.1) •Comparison of calculated (reconstructed) and experimental spectrum (systematic differences?) •Consensus estimates of secondary structure using different algorithms References • Jones, C. et al. (2004) NPL Report, ISSN 17440602 • Kelly, S.M. et al. (2005) Biochim. Biophys. Acta 1751, 119-139 • Miles, A.J. et al. (2003) Spectroscopy 17, 653-661 • Miles, A.J. et al (2005) Spectroscopy 19, 43-51 • Whitmore, L. and Wallace, B.A. (2004) Nucl. Acids Res. 32, W668-W673