output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2022 · astro-ph.GAShow all

111 papers · 2 filters

astro-ph.GA2022★ 54 cited

Overmassive black holes in dwarf galaxies out to z0.9 in the VIPERS survey

M. Mezcua, M. Siudek, H. Suh +3

Supermassive black holes (SMBHs) are thought to originate from early Universe seed black holes of mass -10 M and grown through cosmic time. S…

astro-ph.GA2022★ 43 cited

Seeking the growth of the first black hole seeds with JWST

Alessandro Trinca, Raffaella Schneider, Roberto Maiolino +3

In this paper we provide predictions for the BH population that would be observable with planned JWST surveys at . We base our study on the recently developed Cosmi…

astro-ph.GA2022★ 15 cited

New Lyman-alpha Emitters in EGS: Evidence of an Extended Ionized Structure at

Intae Jung, Steven L. Finkelstein, Rebecca L. Larson +21

We perform a ground-based near-infrared spectroscopic survey using the Keck/MOSFIRE spectrograph to target Ly emission at from 61 galaxies to trace the ionization st…

astro-ph.GA2022★ 5 cited

DDO68 C: the actual appearance of a ghost satellite dwarf through adaptive optics at the Large Binocular Telescope

Francesca Annibali, Enrico Pinna, Leslie K. Hunt +12

Through adaptive optics (AO) imaging with the SOUL+LUCI instrument at the Large Binocular Telescope we were able to resolve, for the first time, individual stars in the gas-rich ga…

astro-ph.GA2022★ 24 cited

The X-ray view of optically selected dual AGN

Alessandra De Rosa, Cristian Vignali, Paola Severgnini +12

We present a study of optically selected dual AGN with projected separations of 3--97~kpc. Using multi-wavelength (MWL) information (optical, X-rays, mid-IR), we characterized the…

astro-ph.GA2022★ 177 cited

The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques

Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher +52

The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy…