activity
20212026
most citedA dusty compact object bridging galaxies and quasars at cosmic dawn

92 citations · 480 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026

A tidal disruption event in a quasar at redshift 7.19

S. Fujimoto, Q. Fei, G. B. Brammer +41

We report a long-lived nuclear transient in GNz7q, a red quasar at powered by a black hole and hosted by a compact, dusty starburst galaxy. Th…

astro-ph.GA2023

The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z~4.5

M. Béthermin, C. Accard, C. Guillaume +40

The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density (-) is essential to understand star formation proces…

astro-ph.GA2023★ 36 cited

Sub-Millimetre Galaxies with Webb: Near-Infrared Counterparts and Multi-wavelength Morphology

S. Gillman, B. Gullberg, G. Brammer +12

We utilise the unprecedented depth and resolution of recent early-release science (ERS) JWST observations to define the near-infrared counterparts of sub-millimetre selected galaxi…

astro-ph.GA2023★ 54 cited

The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5

F. Rizzo, F. Roman-Oliveira, F. Fraternali +13

Spatially-resolved studies of the kinematics of galaxies provide crucial insights into their assembly and evolution, enabling to infer the properties of the dark matter halos, deri…

astro-ph.GA2022★ 55 cited

The gas and stellar content of a metal-poor galaxy at as revealed by JWST and ALMA

K. E. Heintz, C. Giménez-Arteaga, S. Fujimoto +27

We present a joint analysis of the galaxy S04590 at based on NIRSpec, NIRCam, and NIRISS observations obtained through as part of Early Release Observations programme of…

astro-ph.GA2022★ 26 cited

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913

M. Ginolfi, E. Piconcelli, L. Zappacosta +18

The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation models predict these…

astro-ph.CO2022★ 28 cited

Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS

Maria Tsedrik, Chiara Moretti, Pedro Carrilho +2

Interacting dark energy models have been suggested as alternatives to the standard cosmological model, CDM. We focus on a phenomenologically interesting class of dark scattering…

astro-ph.GA2022★ 92 cited

A dusty compact object bridging galaxies and quasars at cosmic dawn

S. Fujimoto, G. B. Brammer, D. Watson +18

Understanding how super-massive black holes form and grow in the early Universe has become a major challenge since the discovery of luminous quasars only 700 million years after th…

astro-ph.GA2022★ 60 cited

Dynamical characterization of galaxies up to

F. Rizzo, M. Kohandel, A. Pallottini +4

The characterization of the dynamical state of galaxies up to z~7 is crucial for constraining the mechanisms driving the mass assembly in the early Universe. However, it is unclear…

astro-ph.CO2022★ 37 cited

The Halo Bispectrum Multipoles in Redshift Space

Federico Rizzo, Chiara Moretti, Kevin Pardede +5

We present the analysis of the halo bispectrum in redshift-space in terms of its multipoles, monopole, quadrupole and hexadecapole, measured from a large set of simulations. We fit…

astro-ph.CO2022★ 33 cited

Bispectrum-window convolution via Hankel transform

Kevin Pardede, Federico Rizzo, Matteo Biagetti +3

We present a method to perform the exact convolution of the model prediction for bispectrum multipoles in redshift space with the survey window function. We extend a widely applied…

astro-ph.CO2021★ 59 cited

Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space

Andrea Oddo, Federico Rizzo, Emiliano Sefusatti +2

We present a joint likelihood analysis of the halo power spectrum and bispectrum in real space. We take advantage of a large set of numerical simulations and of an even larger set…