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Mapping the Extended Ly α Emission within the Circumgalactic Medium of Quasars Hosted by Dusty Starbursts with CubeCarve
Journal article   Open access   Peer reviewed

Mapping the Extended Ly α Emission within the Circumgalactic Medium of Quasars Hosted by Dusty Starbursts with CubeCarve

Kevin Hall and Hai Fu
The Astrophysical journal, Vol.1002(2), 216
05/10/2026
DOI: 10.3847/1538-4357/ae6065
url
https://doi.org/10.3847/1538-4357/ae6065View
Published (Version of record) Open Access

Abstract

We present a study of extended Ly α emission around four quasars hosted by dusty starbursts, which are composite systems thought to represent a transitional stage in quasar evolution. To extract faint circumgalactic medium (CGM) emission in the presence of bright point sources, we introduce CubeCarve , a dual-channel deconvolution algorithm that separates unresolved quasar emission from spatially extended structure. This approach enables reliable recovery of Ly α emission projected onto the quasar position without introducing subtraction artifacts. Using CubeCarve v1.0.0, we find that the Ly α surface brightness profiles of these systems are, on average, fainter and shallower than those of quasars of similar bolometric luminosities. We also find that the total integrated Ly α luminosities of the nebulae are lower in systems whose host galaxies exhibit brighter far-IR emission. These results suggest that the CGM conditions in composite systems differ from those in the broader quasar population. Our study highlights both the physical diversity of quasar CGM environments and the effectiveness of CubeCarve for recovering diffuse emission in modern integral-field unit datasets.

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