At least 50 total cell comets from 2 independent experiments were measured for the percentage of DNA in comet tails per condition. This was calculated by determining the background-corrected fluoresce
This dataset consists of X-ray absorption fine structure (XAFS) spectra at Cu K-edge of Copper(I) oxide measured at SPring-8 BL14B2, and is a part of XAFS database (MDR XAFS DB, https://doi.org/10.485
This dataset consists of X-ray absorption fine structure (XAFS) spectra at W L21-edge of Tungsten(VI) oxide measured at SPring-8 BL14B2, and is a part of XAFS database (MDR XAFS DB, https://doi.org/10
Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/ 20140321.114421.copied-20160212010847935PST.zip <a class="btn btn-xs piwik_download" type="applicat
