Détail du document
Identifiant
oai:arXiv.org:2407.03597
Sujet
Astrophysics - Astrophysics of Gal...Auteur
Cai, Minxuan Wan, Zhen Cai, Zhenyi Fan, Lulu Wang, JunxianCatégorie
sciences : astrophysique
Année
2024
Date de référencement
10/07/2024
Mots clés
agn variation flux method fvg hostRésumé
In terms of the variable nature of normal active galaxy nuclei (AGN) and luminous quasars, a so-called flux variation gradient (FVG) method has been widely utilized to estimate the underlying non-variable host galaxy fluxes.
The FVG method assumes an invariable AGN color, but this assumption has been questioned by the intrinsic color variation of quasars and local Seyfert galaxies.
Here, using an up-to-date thermal fluctuation model to simulate multi-wavelength AGN variability, we theoretically demonstrate that the FVG method generally overestimates the host galaxy flux; that is, it is more significant for brighter AGN/quasars.
Furthermore, we observationally confirm that the FVG method indeed overestimates the host galaxy flux by comparing it to that estimated through other independent methods.
We thus caution that applying the FVG method should be performed carefully in the era of time-domain astronomy.
Cai, Minxuan,Wan, Zhen,Cai, Zhenyi,Fan, Lulu,Wang, Junxian, 2024, The Host Galaxy Fluxes of Active Galaxy Nuclei Are Generally Overestimated by the Flux Variation Gradient Method
