Sensitive Chandra coverage of a representative sample of weak-line quasars: revealing the full range of X-ray properties

Abstract

We present deeper Chandra observations for weak-line quasars (WLQs) in a representative sample that previously had limited X-ray constraints, and perform X-ray photometric analyses to reveal the full range of X-ray properties of WLQs. Only 5 of the 32 WLQs included in this representative sample remain X-ray undetected after these observations, and a stacking analysis shows that these 5 have an average X-ray weakness factor of > 85. One of the WLQs in the sample that was known to have extreme X-ray variability, SDSS J1539+3954, exhibited dramatic X-ray variability again: it changed from an X-ray normal state to an X-ray weak state within ~ 3 months in the rest frame. This short timescale for an X-ray flux variation by a factor of $\gtrsim$ 9 further supports the thick disk and outflow (TDO) model proposed to explain the X-ray and multiwavelength properties of WLQs. The overall distribution of the X-ray-to-optical properties of WLQs suggests that the TDO has an average covering factor of the X-ray emitting region of ~ 0.5, and the column density of the TDO can range from $N_{\mathrm{H}}$ $\sim 10^{23-24}{\mathrm{cm}}^{-2}$ to $N_{\mathrm{H}}$ $\gtrsim 10^{24}{\mathrm{cm}}^{-2}$, which leads to different levels of absorption and Compton reflection (and/or scattering) among WLQs.

arXiv comment16 pages, 10 figures. Accepted for publication in MNRAS

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