Spatially and spectrally resolved HCN/HCO+ ratios in 18 nearby ULIRGs show outflow or AGN signatures in 16 galaxies, classified into spherical-shell, spectrally-distinct-compact, and filled geometries.
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XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.
citing papers explorer
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Spectrally and spatially resolved (sub)millimeter HCN-to-HCO$^{+}$ flux ratios in nearby ultraluminous infrared galaxies
Spatially and spectrally resolved HCN/HCO+ ratios in 18 nearby ULIRGs show outflow or AGN signatures in 16 galaxies, classified into spherical-shell, spectrally-distinct-compact, and filled geometries.
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A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN
XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.