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LHAASO-WCDA Observation of the BL LAC 1ES 1218+304

22 Oct 2026, 17:05
5m
Tianfu Cosmic Ray Research Center

Tianfu Cosmic Ray Research Center

No. 1500 Kezhi Road, Tianfu New Area, Chengdu, China
Poster poster-b

Speaker

博仁 刘

Description

This is a preliminary LHAASO-WCDA analysis of the high-synchrotron-peaked BL Lac object 1ES 1218+304. Using data collected from March 2021 to July 2025, we construct an eight-day light curve, significance maps, and a time-averaged spectral energy distribution (SED), while considering possible source confusion from the nearby 1ES 1215+303 and NGC 4278. The signal is strongest in the low-$N_{\rm hit}$ bins. A Bayesian Blocks analysis of the current weighted light curve finds no clear, statistically significant change point. We describe the observed spectrum with a power law with an exponential cutoff fixed at 10 TeV. And we get the intrinsic spectrum with Saldana-Lopez's EBL model.

Primary authors

Min Zha(高能所) 会财 李(高能所) 博仁 刘

Presentation materials

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