Accretion history of AGN: Estimating the host galaxy properties in X-ray luminous AGN from z=0-3

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dc.contributor.authorColeman, Brandon
dc.contributor.authorKirkpatrick, Allison
dc.contributor.authorCooke, Kevin C.
dc.contributor.authorGlikman, Eilat
dc.contributor.authorLa Massa, Stephanie
dc.contributor.authorMarchesi, Stefano
dc.contributor.authorPeca, Alessandro
dc.contributor.authorTreister, Ezequiel
dc.contributor.authorAuge, Connor
dc.contributor.authorUrry, C. Megan
dc.contributor.authorSanders, Dave
dc.contributor.authorTurner, Tracey Jane
dc.contributor.authorAnanna, Tonima Tasnim
dc.date.accessioned2025-01-20T21:04:09Z
dc.date.available2025-01-20T21:04:09Z
dc.date.issued2022
dc.description.abstractWe aim to determine the intrinsic far-Infrared (far-IR) emission of X-ray-luminous quasars over cosmic time. Using a 16 deg(2) region of the Stripe 82 field surveyed by XMM-Newton and Herschel Space Observatory, we identify 2905 X-ray luminous (L-X > 10(42) erg/s) active galactic nuclei (AGN) in the range z approximate to 0-3. The IR is necessary to constrain host galaxy properties such as star formation rate (SFR) and gas mass. However, only 10 per cent of our AGN are detected both in the X-ray and IR. Because 90 per cent of the sample is undetected in the far-IR by Herschel, we explore the mean IR emission of these undetected sources by stacking their Herschel/SPIRE images in bins of X-ray luminosity and redshift. We create stacked spectral energy distributions from the optical to the far-IR, and estimate the median SFR, dust mass, stellar mass, and infrared luminosity using a fitting routine. We find that the stacked sources on average have similar SFR/L-bol ratios as IR detected sources. The majority of our sources fall on or above the main sequence line suggesting that X-ray selection alone does not predict the location of a galaxy on the main sequence. We also find that the gas depletion time scales of our AGN are similar to those of dusty star forming galaxies. This suggests that X-ray selected AGN host high star formation and that there are no signs of declining star formation.
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stac1679
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stac1679
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/93216
dc.identifier.wosidWOS:000824929000006
dc.issue.numero1
dc.language.isoen
dc.pagina.final98
dc.pagina.inicio82
dc.revistaMonthly notices of the royal astronomical society
dc.rightsacceso restringido
dc.subjectgalaxies: active
dc.subjectgalaxies: evolution
dc.subjectgalaxies: nuclei
dc.subjectquasars: general
dc.subjectgalaxies: star formation
dc.titleAccretion history of AGN: Estimating the host galaxy properties in X-ray luminous AGN from z=0-3
dc.typeartículo
dc.volumen515
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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