Astrophysics with the laser interferometer space antenna

P Amaro-Seoane, J Andrews, M Arca Sedda… - Living Reviews in …, 2023 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

Active galactic nuclei: what's in a name?

P Padovani, DM Alexander, RJ Assef… - The Astronomy and …, 2017 - Springer
Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …

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 …

The eROSITA X-ray telescope on SRG

P Predehl, R Andritschke, V Arefiev… - Astronomy & …, 2021 - aanda.org
eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary
instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully …

A challenge to the standard cosmological model

NJ Secrest, S von Hausegger, M Rameez… - The Astrophysical …, 2022 - iopscience.iop.org
We present the first joint analysis of catalogs of radio galaxies and quasars to determine
whether their sky distribution is consistent with the standard ΛCDM model of cosmology …

On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback

JM Piotrowska, AFL Bluck, R Maiolino… - Monthly Notices of the …, 2022 - academic.oup.com
In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …

The Redshift Evolution of the M•–M⋆ Relation for JWST's Supermassive Black Holes at z> 4

F Pacucci, A Loeb - The Astrophysical Journal, 2024 - iopscience.iop.org
JWST has detected many overmassive galactic systems at z> 4, where the mass of the black
hole, M•, is 10–100 times larger than expected from local relations, given the host's stellar …

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 …

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 …

The COSMOS2015 galaxy stellar mass function-Thirteen billion years of stellar mass assembly in ten snapshots

I Davidzon, O Ilbert, C Laigle, J Coupon… - Astronomy & …, 2017 - aanda.org
We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …