All Tables

• Table 1: XCOUNT predicted X-ray counts using different stellar birthrates, compared with the observations.
• Table 4: Unabsorbed X-ray luminosity and emission measure for the stars in the sample with known parallax.
• Table 2: Infrared counterparts identified for the stellar sample, with colour information from 2MASS.
• Table 3: Best-fit parameters derived from the spectral analysis of the 58 stellar sources in the XMM-Newton Bright Serendipitous survey, with errors measured as the 90% confidence range.