Active galactic nuclei: what's in a name?
Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …
supermassive black holes in galaxies, and present unique observational signatures that …
Obscured active galactic nuclei
RC Hickox, DM Alexander - Annual Review of Astronomy and …, 2018 - annualreviews.org
Active galactic nuclei (AGN) are powered by the accretion of material onto a supermassive
black hole (SMBH) and are among the most luminous objects in the Universe. However, the …
black hole (SMBH) and are among the most luminous objects in the Universe. However, the …
JWST UNCOVER: extremely Red and Compact Object at z phot≃ 7.6 triply imaged by A2744
Recent JWST/NIRCam imaging taken for the ultra-deep UNCOVER program reveals a very
red dropout object at z phot≃ 7.6, triply imaged by the galaxy cluster A2744 (zd= 0.308). All …
red dropout object at z phot≃ 7.6, triply imaged by the galaxy cluster A2744 (zd= 0.308). All …
Fitting AGN/Galaxy X-Ray-to-radio SEDs with CIGALE and Improvement of the Code
Modern and future surveys effectively provide a panchromatic view for large numbers of
extragalactic objects. Consistently modeling these multiwavelength survey data is a critical …
extragalactic objects. Consistently modeling these multiwavelength survey data is a critical …
The LOFAR Two-metre Sky Survey: Deep Fields data release 1. V. Survey description, source classifications, and host galaxy properties
PN Best, R Kondapally, WL Williams… - Monthly Notices of …, 2023 - academic.oup.com
Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
Universal bolometric corrections for active galactic nuclei over seven luminosity decades
Context. The AGN bolometric correction is a key element for understanding black hole (BH)
demographics and computing accurate BH accretion histories from AGN luminosities …
demographics and computing accurate BH accretion histories from AGN luminosities …
x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared
ABSTRACT Code Investigating GALaxy Emission (cigale) is a powerful multiwavelength
spectral energy distribution (SED) fitting code for extragalactic studies. However, the current …
spectral energy distribution (SED) fitting code for extragalactic studies. However, the current …
EPOCHS VII: discovery of high-redshift (6.5 < z < 12) AGN candidates in JWST ERO and PEARLS data
I Juodžbalis, CJ Conselice, M Singh… - Monthly Notices of …, 2023 - academic.oup.com
We present an analysis of a sample of robust high-redshift galaxies selected from the
'blank'fields of the Prime Extragalactic Areas for Reionization Science (PEARLS) survey and …
'blank'fields of the Prime Extragalactic Areas for Reionization Science (PEARLS) survey and …
Nuclear obscuration in active galactic nuclei
The material surrounding accreting supermassive black holes connects the active galactic
nucleus with its host galaxy and, besides being responsible for feeding the black hole …
nucleus with its host galaxy and, besides being responsible for feeding the black hole …
The close environments of accreting massive black holes are shaped by radiative feedback
The majority of the accreting supermassive black holes in the Universe are obscured by
large columns of gas and dust,,. The location and evolution of this obscuring material have …
large columns of gas and dust,,. The location and evolution of this obscuring material have …