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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 …
The SRG/eROSITA all-sky survey-First X-ray catalogues and data release of the western Galactic hemisphere
A Merloni, G Lamer, T Liu, ME Ramos-Ceja… - Astronomy & …, 2024 - aanda.org
The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite
began surveying the sky in December 2019, with the aim of producing all-sky X-ray source …
began surveying the sky in December 2019, with the aim of producing all-sky X-ray source …
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging
CT Donnan, DJ McLeod, JS Dunlop… - Monthly Notices of …, 2023 - academic.oup.com
We reduce and analyse the available JWST ERO and ERS NIRCam imaging (SMACS0723,
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
A CEERS discovery of an accreting supermassive black hole 570 Myr after the Big Bang: identifying a progenitor of massive z> 6 quasars
We report the discovery of an accreting supermassive black hole at z= 8.679. This galaxy,
denoted here as CEERS_1019, was previously discovered as a Lyα-break galaxy by …
denoted here as CEERS_1019, was previously discovered as a Lyα-break galaxy by …
A census of photometrically selected little red dots at 4< z< 9 in JWST blank fields
Abstract Observations with the James Webb Space Telescope (JWST) have uncovered
numerous faint active galactic nuclei (AGN) at z∼ 5 and beyond. These objects are key to …
numerous faint active galactic nuclei (AGN) at z∼ 5 and beyond. These objects are key to …
EPOCHS. II. The ultraviolet luminosity function from 7.5< z< 13.5 using 180 arcmin2 of deep, blank fields from the PEARLS survey and public JWST data
We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate
density of distant galaxies (7.5< z< 13.5) in the" blank" fields of the Prime Extragalactic Areas …
density of distant galaxies (7.5< z< 13.5) in the" blank" fields of the Prime Extragalactic Areas …
JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z ≃ 9 – 15
CT Donnan, RJ McLure, JS Dunlop… - Monthly Notices of …, 2024 - academic.oup.com
We present a new determination of the evolving galaxy ultraviolet (UV) luminosity function
(LF) over the redshift range using a combination of several major Cycle-1 JWST imaging …
(LF) over the redshift range using a combination of several major Cycle-1 JWST imaging …
The SRG/eROSITA all-sky survey-Cosmology constraints from cluster abundances in the western Galactic hemisphere
The evolution of the cluster mass function traces the growth of linear density perturbations,
providing valuable insights into the growth of structures, the nature of dark matter, and the …
providing valuable insights into the growth of structures, the nature of dark matter, and the …
The bolometric quasar luminosity function at z = 0–7
In this paper, we provide updated constraints on the bolometric quasar luminosity function
(QLF) from z= 0 to z= 7. The constraints are based on an observational compilation that …
(QLF) from z= 0 to z= 7. The constraints are based on an observational compilation that …