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@@ -6,10 +6,11 @@ This folder contains X-ray total scattering data described in the paper | |
Polymorphism in magic sized Au144(SR)60 clusters, | ||
Kirsten M. Ø. Jensen, Pavol Juhás, Marcus A. Tofanelli, | ||
Christine L. Heinecke, Gavin Vaughan, Christopher J. Ackerson, | ||
and Simon J. L. Billinge | ||
and Simon J. L. Billinge, *Nature Communications*, 2016, | ||
http://dx.doi.org/10.1038/ncomms11859. | ||
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to be published in Nature Communications, 2016. The samples, data | ||
acquisition and data reduction processes are described in detail therein. | ||
The samples, data acquisition and data reduction processes are described | ||
in detail therein. | ||
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This folder contains the following data files: | ||
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@@ -29,13 +30,13 @@ These datasets were measured from 5 different samples Au144(PET)60, | |
Au144(SC4)60, Au144(SC6)60, Au144(SC12)60 and Au144(pMBA)60, as stated in the | ||
file names. All scattering data were measured at 100 K. The first 4 datasets | ||
were obtained at the 11-ID-B beamline of the Advanced Photon Source (APS), | ||
with a wavelength of 0.143 Å. The data are provided as integrated total | ||
scattering intensities versus Q [1/nm] in .chi files and as reduced pair | ||
distribution functions (PDF-s) in .gr files. The data in Kapton_APS.chi are | ||
background scattering intensities to be used with the APS data. The last | ||
dataset, Au144pMBA_100K_ESRF, was obtained at the European Synchrotron | ||
Radiation Facility (ESRF) beamline ID11 using X-ray wavelength of 0.177 Å. | ||
Here, the background has already been subtracted. | ||
with a wavelength of 0.143 Å. The data are provided in plain text format | ||
as integrated total scattering intensities versus Q [1/nm] in .chi files and | ||
as reduced pair distribution functions (PDF-s) in .gr files. The data in | ||
Kapton_APS.chi are background scattering intensities to be used with the APS | ||
data. The last dataset, Au144pMBA_100K_ESRF, was obtained at the European | ||
Synchrotron Radiation Facility (ESRF) beamline ID11 using X-ray wavelength of | ||
0.177 Å. Here, the background has already been subtracted. | ||
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Please contact Prof. Simon J. L. Billinge [email protected] from | ||
Columbia University for any questions regarding the data and their use. |