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TYC 8380-1953-1: Discovery of an RS CVn Binary Through the XMM-Newton Slew Survey

Stelzer, B.; López-Santiago, J.; Saxton, R.

In this article we report the discovery of the chromospherically active (RS CVn type) binary TYC 8380-1953-1 through the XMM-Newton slew survey and present results of our optical and X-ray follow-up. With a flux limit of 6 × 10^-13 ergs cm^-2 s^-1 in the soft band (0.2-2 keV), the XMM-Newton slew has a similar sensiti…

Using the XMM-Newton Optical Monitor to Study Cluster Galaxy Evolution

Kuntz, K. D.; Hammer, Derek; Miller, Neal A. +2 more

We explore the application of XMM-Newton Optical Monitor (XMM-OM) ultraviolet (UV) data to study galaxy evolution. Our sample is constructed as the intersection of all Abell clusters with z < 0.05 and having archival XMM-OM data in either the UVM2 or UVW1 filters, plus optical and UV photometry from the Sloan Digital Sky Survey and GALEX, respe…