2017ApJ...846...80S

We undertook coordinated campaigns with the Green Bank, Effelsberg, and Arecibo radio telescopes during Chandra X-ray Observatory and XMM-Newton observations of the repeating fast radio burst FRB 121102 to search for simultaneous radio and X-ray bursts. We find 12 radio bursts from FRB 121102 during 70 ks total of X-ray observations. We detect no X-ray photons at the times of radio bursts from FRB 121102 and further detect no X-ray bursts above the measured background at any time. We place a 5σ upper limit of 3 x 10^–11 erg cm^–2 on the 0.5-10 keV fluence for X-ray bursts at the time of radio bursts for durations 700 ms, which corresponds to a burst energy of 4 x 10⁴⁵ erg at the measured distance of FRB 121102. We also place limits on the 0.5-10 keV fluence of 5 x 10^–10 and 1 x 10^–9 erg cm^–2 for bursts emitted at any time during the XMM-Newton and Chandra observations, respectively, assuming a typical X-ray burst duration of 5 ms. We analyze data from the Fermi Gamma-ray Space Telescope Gamma-ray Burst Monitor and place a 5σ upper limit on the 10-100 keV fluence of 4 x 10^–9 erg cm^–2 (5 x 10⁴⁷ erg at the distance of FRB 121102) for gamma-ray bursts at the time of radio bursts. We also present a deep search for a persistent X-ray source using all of the X-ray observations taken to date and place a 5σ upper limit on the 0.5-10 keV flux of 4 x 10^–15 erg s^–1 cm^–2 (3 x 10⁴¹ erg s^–1 at the distance of FRB 121102). We discuss these non-detections in the context of the host environment of FRB 121102 and of possible sources of fast radio bursts in general.