Detection of a gamma-ray flare from the high-redshift blazar DA 193
arXiv:1812.07350 · doi:10.3847/1538-4357/aafa10
Abstract
High-redshift () blazars are the most powerful members of the blazar family. Yet, only a handful of them have both X-ray and -ray detection, thereby making it difficult to characterize the energetics of the most luminous jets. Here, we report, for the first time, the Fermi-Large Area Telescope detection of the significant -ray emission from the high-redshift blazar DA 193 (). Its time-averaged -ray spectrum is soft (-ray photon index = ) and together with a relatively flat hard X-ray spectrum (14195 keV photon index = ), DA 193 presents a case to study a typical high-redshift blazar with inverse Compton peak being located at MeV energies. An intense GeV flare was observed from this object in the first week of 2018 January, a phenomenon rarely observed from high-redshift sources. What makes this event a rare one is the observation of an extremely hard -ray spectrum (photon index = ), which is somewhat unexpected since high-redshift blazars typically exhibit a steep falling spectrum at GeV energies. The results of our multi-frequency campaign, including both space- (Fermi, NuSTAR, and Swift) and ground-based (Steward and Nordic Optical Telescope) observatories, are presented and this peculiar -ray flare is studied within the framework of a single-zone leptonic emission scenario.
14 pages, 9 figures, 2 tables, to appear in the Astrophysical Journal
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