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Low-frequency radio selection finds radio-bright galaxies regardless of the amount of obscuration by gas and dust. We report chandra observations of a complete 178~MHz-selected, and so orientation unbiased, sample of 44 $0.5<z<1$ 3CRR sources. The sample is comprised of quasars and narrow-line radio galaxies (NLRGs) with similar radio luminosities, and the radio structure serves as both an age and an orientation indicator. Consistent with Unification, intrinsic obscuration (measured by h, X-ray hardness ratio, and X-ray luminosity) generally increases with inclination. However, the sample includes a population not seen in high-$z$ 3CRR sources: NLRGs viewed at intermediate inclination angles with h~$<10^{22}$~cm$^{-2}$. Multiwavelength analysis suggests these objects have lower $L/L_{rm Edd}$ than typical NLRGs at similar orientation. Thus both orientation and $L/L_{rm Edd}$ are important, and a radiation-regulated Unification provides a better explanation of the samples observed properties. In comparison with the 3CRR sample at $1<z<2$, our lower-redshift sample shows a higher fraction of Compton-thin NLRGs (45% vs. 29%) but similar Compton-thick fraction (20%), implying a larger covering factor of Compton-thin material at intermediate viewing angles and so a more puffed-up torus atmosphere. We posit that this is due to a range of $L/L_{rm Edd}$ extending to lower values in this sample. In contrast, at high redshifts the narrower range and high $L/L_{rm Edd}$ values allowed orientation (and so simple Unification) to dominate the samples observed properties.
We present the spatial analysis of five Compton thick (CT) active galactic nuclei (AGNs), including MKN 573, NGC 1386, NGC 3393, NGC 5643, and NGC 7212, for which high resolution Chandra observations are available. For each source, we find hard X-ray
We present the joint Chandra, XMM-Newton and NuSTAR analysis of two nearby Seyfert galaxies, NGC 3081 and ESO 565-G019. These are the only two having Chandra data in a larger sample of ten low redshift ($z le 0.05$), candidates Compton-thick Active G
The motivation of the unified model is to explain the main properties of the large zoo of active galactic nuclei with a single physical object. The discovery of broad permitted lines in the polarized spectrum of type 2 Seyfert galaxies in the mid 80s
We study the statistical properties of faint X-ray sources detected in the Chandra Bulge Field. The unprecedented sensitivity of the Chandra observations allows us to probe the population of faint Galactic X-ray sources down to luminosities L(2-10 ke
We use time-domain optical spectroscopy to distinguish between broad emission lines powered by accreting black holes (BHs) or stellar processes (i.e., supernovae) for 16 galaxies identified as AGN candidates by Reines etal (2013). Our study is primar