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2025ApJ...984....5L - Astrophys. J., 984, 5 (2025/May-1)

Detection of an Orphan X-Ray Flare from a Blazar Candidate EP240709a with the Einstein Probe.

LIU M., ZHANG Y., WANG Y., XUE R., BUCKLEY D., HOWELL D.A., JIN C., LI W., MONAGENG I., PAN H., SUN N.-C., TINYANONT S., WANG L., YUAN W., AN J., ANDREWS M., ANUTARAWIRAMKUL R., BUTPAN P., CHEN Y., CHENG H., CUI W., DAI C.-Y., DAI L., FARAH J., FENG H., FU S., GUO Z., JIA S., JIANG S., LI A., LI C., LI D., LIAN T., LIANG Y., LIU H., LIU X., LIU Y., MAO J., McCULLY C., NEWSOME M., PADILLA GONZALEZ E., PAN X., SUN X., TERRERAN G., WANG Z.-R., WU Q., XIAO H., XIONG D., XU D., XU X., XUE S., YANG H., YANG J., ZHANG J., ZHANG W., ZHANG W. and ZOU H.

Abstract (from CDS):

Blazars are often observed to flare across multiple wavelengths. Orphan flares from blazars have only been detected a few times, providing an opportunity to understand the structure of the jet in the accreting system. We report a remarkable orphan X-ray flare from a blazar candidate EP240709a, detected by the Einstein Probe (EP) in July 2024. The multiband spectral properties and variability support EP240709a as a high-energy peaked BL Lacertae-type object. The flux in 0.5-10 keV increased by at least 28 times to the value of low state in 2020, with no significant flaring detected in other bands during the same period. EP240709a exhibits the harder-when-brighter tendency in the X-ray band during the orphan flare, while its infrared-optical spectra are featureless. We employ one-zone and two-zone leptonic synchrotron self-Compton models to perform the spectral energy distribution fitting. Detecting this rare orphan flare shows the potential of EP in discovering peculiar activities from AGN in high-cadence X-ray sky surveys.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Active galactic nuclei - Blazars - Jets - High energy astrophysics

Simbad objects: 7

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