How does Green Pea the X-ray luminosity evolve with star-formation rate

Green Peas, compact starforming galaxies at zvirgul0.2 have become the best locallaboratories for highredshift galaxies. While relatively large amounts ofoptical data are available for Green Peas, their Xray properties remain largelyunknown. We have recently requested XMMNewton observations of three Green Peasto remedy this situation. We have discovered an intriguingly large Xrayemission in two of the targets, while the third observation was damaged withhigh background. We request here a reobservation of the third target which willallow us to complete the project goals and verify the Xray luminositydependence on starformation rate and other galaxy parameters. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]