分类: 天文学 >> 天文学 提交时间: 2023-02-19
摘要: We present the XMM-Newton X-ray analysis of 19 X-ray luminous galaxy clusters of low-to-mid redshift ($< 0.4$) selected from the MCXC cluster catalogue in the Hyper Supri%survey as the first work in our series paper. We derive the hydrostatic equilibrium mass and study scaling relations using i) the whole sample, ii) only relaxed clusters and iii) only disturbed clusters. When considering the whole sample, the $Y_{\rm X}$-$M_{\rm tot}$ and $M_{\rm gas}$-$M_{\rm tot}$ relations agree with self-similarity. In terms of morphology, relaxed clusters show a flatter relation in $L_{\rm X,ce}$-$M_{\rm tot}$, $L_{\rm X,bol}$-$M_{\rm tot}$, $L_{\rm X,ce}$-$T$, $L_{\rm bol,ce}$-$T$, $M_{\rm gas}$-$M_{\rm tot}$ and $Y_{\rm X}$-$M_{\rm tot}$. The $L_{\rm bol,ce}$-$M_{\rm tot}$, $L_{\rm X,ce}$-$M_{\rm tot}$ $L_{\rm bol,ce}$-$T$ and $L_{\rm X,ce}$-$T$ relations show a slope $\sim$3$\sigma$ steeper. The residuals in the $M_{\rm gas}$-$M_{\rm tot}$ and $T$-$M_{\rm tot}$ relations and the intrinsic covariance between $M_{\rm gas}$ and $T$ show hints of positive correlation, casting doubt on whether the $Y_{\rm X}$ parameter is a truly low scatter mass proxy. The $M_{\rm gas}$-$M_{\rm tot}$ and $T$-$M_{\rm tot}$ plots color-coded with the offset of the $L_{\rm X,ce}$-$M_{\rm tot}$ relation show these two relations to be brightness dependent but not the $L_{\rm X,ce}$-$T$ relation, suggesting relations involving $M_{\rm tot}$ are biased due to sample selection based on luminosity. Following the work which studied an optical sample and combining our result with literature studies, we find the $M_{\rm tot}$ derived not using mass proxies deviate from $L_{\rm X}$ $\propto$ $M_{\rm gas}^{2}M_{\rm tot}^{-1}$ and $M_{\rm tot}$ based on hydrostatic equilibrium are more massive than what is expected by their relation using caustic masses. This indicates mass bias plays an important role in scaling relations.
分类: 天文学 >> 天文学 提交时间: 2023-02-19
摘要: An incremental version of the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi-Large Area Telescope is presented. This version (4LAC-DR3) derives from the third data release of the 4FGL catalog based on 12 years of E>50 MeV gamma-ray data, where the spectral parameters, spectral energy distributions (SEDs), yearly light curves, and associations have been updated for all sources. The new reported AGNs include 587 blazar candidates and four radio galaxies. We describe the properties of the new sample and outline changes affecting the previously published one. We also introduce two new parameters in this release, namely the peak energy of the SED high-energy component and the corresponding flux. These parameters allow an assessment of the Compton dominance, the ratio of the Inverse-Compton to the synchrotron peak luminosities, without relying on X-ray data.