x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared

G Yang, M Boquien, V Buat, D Burgarella… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT Code Investigating GALaxy Emission (cigale) is a powerful multiwavelength
spectral energy distribution (SED) fitting code for extragalactic studies. However, the current …

Euclid. I. Overview of the Euclid mission

Y Mellier, A Abdurroúf, JAA Barroso… - Astronomy & …, 2024 - aanda.org
The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …

MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey

N Maddox, BS Frank, AA Ponomareva… - Astronomy & …, 2021 - aanda.org
We present the HI emission project within the MIGHTEE survey, currently being carried out
with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind …

MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei

CL Hale, IH Whittam, MJ Jarvis, PN Best… - Monthly Notices of …, 2023 - academic.oup.com
We present deep 1.4 GHz source counts from∼ 5 deg2 of the continuum Early Science data
release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration survey …

Deep Extragalactic VIsible Legacy Survey (DEVILS): motivation, design, and target catalogue

LJM Davies, ASG Robotham, SP Driver… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a large
spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near …

Active galactic nuclei as seen by the Spitzer Space Telescope

M Lacy, A Sa**a - Nature Astronomy, 2020 - nature.com
Abstract The Spitzer Space Telescope revolutionized studies of active galactic nuclei
(AGNs). Its combined sensitivity and map** speed at mid-infrared wavelengths revealed a …

On the Observational Difference between the Accretion Disk–Corona Connections among Super-and Sub-Eddington Accreting Active Galactic Nuclei

H Liu, B Luo, WN Brandt, MS Brotherton… - The Astrophysical …, 2021 - iopscience.iop.org
We present a systematic X-ray and multiwavelength study of a sample of 47 active galactic
nuclei (AGNs) with reverberation map** measurements. This sample includes 21 super …

Heavily obscured AGN detection: A radio versus X-ray challenge

G Mazzolari, R Gilli, M Brusa, M Mignoli, F Vito… - Astronomy & …, 2024 - aanda.org
Context. In the supermassive black hole (SMBH)-galaxy coevolution scenario, heavily
obscured active galactic nuclei (AGN) represent a fundamental phase of SMBH growth …

Investigating the Star Formation Rates of Active Galactic Nucleus Hosts Relative to the Star-forming Main Sequence

N Cristello, F Zou, WN Brandt, CTJ Chen… - The Astrophysical …, 2024 - iopscience.iop.org
A fundamental question in galaxy and black hole evolution remains how galaxies and their
supermassive black holes have evolved together over cosmic time. Specifically, it is still …

The host-galaxy properties of type 1 versus type 2 active galactic nuclei

F Zou, G Yang, WN Brandt, Y Xue - The Astrophysical Journal, 2019 - iopscience.iop.org
The unified model of active galactic nuclei (AGNs) proposes that different AGN optical
spectral types are caused by different viewing angles with respect to an obscuring" torus." …