Cool Stars 14 - Submitted Abstract # 190 This version created on 05 October 2006 Sigma Orionis in X-rays, Chandra and XMM observations Nancy Adams-Wolk, Harvard-Smithsonian CfA Scott Wolk, Harvard-Smithsonian CfA Frederick Walter, University at Stony Brook Bradley Spitzbart, Harvard-Smithsonian CfA William Sherry, National Solar Observatory We present observations of Sigma Orionis from the Chandra and XMM observatories. Using tools from the ANCHORS pipeline production, we cross-correlate the X-ray data and present the spectra and X-ray luminosity function. We will discuss the data, the reduction methods, and the ANCHORS tools that were used. ANCHORS is a web based archive of point sources observed during Chandra observations of regions of star formation. It is designed to aid both the X-ray astronomer with a desire to compare X-ray datasets and the star formation astronomer wishing to compare stars across the spectrum. Automated pipeline processing ensures consistent analysis techniques for direct comparisons among clusters and observing epochs. This is the first attempt to use ANCHORS software on an HRC Chandra dataset, instead of ACIS. This work will lead to the use of HRC data being included in the ANCHORS archive. ----------------------------------