<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Hofmann, F.</style></author><author><style face="normal" font="default" size="100%">Pietsch, W.</style></author><author><style face="normal" font="default" size="100%">Henze, M.</style></author><author><style face="normal" font="default" size="100%">Haberl, F.</style></author><author><style face="normal" font="default" size="100%">Strum, R.</style></author><author><style face="normal" font="default" size="100%">Della Valle, M.</style></author><author><style face="normal" font="default" size="100%">Hartmann, D. H.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">VizieR Online Data Catalog: X-ray variability of M31 central field (Hofmann+, 2013)</style></title><short-title><style face="normal" font="default" size="100%">VizieR Online Data Catalog</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">Binaries: X-ray</style></keyword><keyword><style  face="normal" font="default" size="100%">X-ray sources</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2013</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2013/05/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2013yCat..35550065H</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">J/A+A/555/A65</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">For all Chandra HRC-I observations a source catalogue was created and the energy flux of each source in each observation was derived. Fluxes were calculated assuming a generic power law spectrum and Galactic foreground absorption for each source. &lt;P /&gt;(5 data files).</style></abstract></record></records></xml>