activity
20152026
most citedJ-PLUS: The Javalambre Photometric Local Universe Survey

248 citations · 1.1k across the 40 of their papers we have counts for

collaborators

43 papers

gr-qc2026

Non-Stationary Wormholes and Matter Source Reconstruction in General Relativity

Geová Alencar, Tiago Crispim, Roberta Dárlla +1

We investigate non-stationary wormhole geometries in General Relativity embedded in evolving cosmological backgrounds. We employ a Simpson-Visser-like regularization of the tempora…

astro-ph.CO2024★ 2 cited

The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey

Xue Zhang, Yu Sang, Gabriel A. Hoerning +15

There are various surveys that will provide excellent data to search for and localize Fast Radio Bursts (FRBs). The BINGO project will be one such survey, and this collaboration ha…

astro-ph.CO2024★ 10 cited

Testing screened modified gravity with SDSS-IV-MaNGA

Ricardo G. Landim, Harry Desmond, Kazuya Koyama +1

Fifth forces are ubiquitous in modified gravity theories, and must be screened to evade stringent local tests. This can introduce unusual behaviour in galaxy phenomenology by affec…

astro-ph.CO2023

BINGO-ABDUS: a radiotelescope to unveil the dark sector of the Universe

Elcio Abdalla, Alessandro Marins, Filipe Abdalla +13

we review the Baryon Acoustic Oscillations from Integrated Neutral Gas Observations (BINGO) telescope, an international collaboration, led by Brazil and China, aiming to explore th…

astro-ph.IM2023★ 8 cited

The BINGO Project IX: Search for Fast Radio Bursts -- A Forecast for the BINGO Interferometry System

Marcelo V. dos Santos, Ricardo G. Landim, Gabriel A. Hoerning +19

The Baryon Acoustic Oscillations (BAO) from Integrated Neutral Gas Observations (BINGO) radio telescope will use the neutral Hydrogen emission line to map the Universe in the redsh…

astro-ph.CO2023★ 14 cited

Constraints on interacting dark energy revisited: implications for the Hubble tension

Gabriel A. Hoerning, Ricardo G. Landim, Luiza O. Ponte +3

We revisit a class of coupled dark energy models where dark energy interacts with dark matter via phenomenological energy exchange terms. We include the perturbation of the Hubble…

astro-ph.CO2022

Foreground removal and 21 cm signal estimates: comparing different blind methods for the BINGO Telescope

Alessandro Marins, Filipe B. Abdalla, Elcio Abdalla +17

The BINGO radiotelescope will observe hydrogen distribution using Intensity Mapping (IM) to analyze the Dark Energy paradigm through Baryon Acoustic Oscillations. The target signal…

astro-ph.CO2022★ 7 cited

The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations

Camila Paiva Novaes, Jiajun Zhang, Eduardo J. de Mericia +17

A new and promising technique for observing the Universe and study the dark sector is the intensity mapping of the redshifted 21cm line of neutral hydrogen (HI). The BINGO radio te…

astro-ph.CO2022★ 22 cited

A note on interacting holographic dark energy with a Hubble-scale cutoff

Ricardo G. Landim

Holographic dark energy with the Hubble radius as infrared cutoff has been considered as a candidate to explain the late-time cosmic acceleration and it can solve the coincidence p…

astro-ph.CO2022★ 6 cited

Testing synchrotron models and frequency resolution in BINGO 21 cm simulated maps using GNILC

Eduardo J. de Mericia, Larissa Santos, Carlos Alexandre Wuensche +16

To recover the 21 cm hydrogen line, it is essential to separate the cosmological signal from the much stronger foreground contributions at radio frequencies. The BINGO radio telesc…

astro-ph.CO2021★ 23 cited

The BINGO Project VI: HI Halo Occupation Distribution and Mock Building

Jiajun Zhang, Pablo Motta, Camila P. Novaes +19

BINGO (Baryon Acoustic Oscillations from Integrated Neutral Gas Observations.) is a radio telescope designed to survey from 980 MHz to 1260 MHz, observe the neutral Hydrogen (HI) 2…

astro-ph.CO2021★ 26 cited

The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping

Andre A. Costa, Ricardo G. Landim, Camila P. Novaes +17

The 21cm line of neutral hydrogen (HI) opens a new avenue in our exploration of the structure and evolution of the Universe. It provides complementary data to the current large-sca…

astro-ph.CO2021★ 22 cited

The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis

Karin S. F. Fornazier, Filipe B. Abdalla, Mathieu Remazeilles +20

Observing the neutral hydrogen distribution across the Universe via redshifted 21cm line intensity mapping constitutes a powerful probe for cosmology. However, the redshifted 21cm…

astro-ph.CO2021★ 20 cited

The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps

Vincenzo Liccardo, Eduardo J. de Mericia, Carlos A. Wuensche +21

The large-scale distribution of neutral hydrogen (HI) in the Universe is luminous through its 21 cm emission. The goal of the Baryon Acoustic Oscillations from Integrated Neutral G…

astro-ph.IM2021★ 1 cited

The BINGO Project III: Optical design and optimisation of the focal plane

Filipe B. Abdalla, Alessandro Marins, Pablo Motta +26

The BINGO telescope was designed to measure the fluctuations of the 21-cm radiation arising from the hyperfine transition of neutral hydrogen and aims to measure the Baryon Acousti…

astro-ph.IM2021★ 32 cited

The BINGO Project II: Instrument Description

Carlos A. Wuensche, Thyrso Villela, Elcio Abdalla +41

The measurement of diffuse 21-cm radiation from the hyperfine transition of neutral hydrogen (HI signal) in different redshifts is an important tool for modern cosmology. However,…

astro-ph.CO2021★ 61 cited

The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations

Elcio Abdalla, Elisa G. M. Ferreira, Ricardo G. Landim +43

Observations of the redshifted 21-cm line of neutral hydrogen (HI) are a new and powerful window of observation that offers us the possibility to map the spatial distribution of co…

astro-ph.CO2021★ 3 cited

Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 z 0.45 -- status update

Carlos A. Wuensche, Elcio Abdalla, Filipe Batoni Abdalla +48

BINGO (BAO from Integrated Neutral Gas Observations) is a unique radio telescope designed to map the intensity of neutral hydrogen distribution at cosmological distances, making th…

gr-qc2021

Fractional dark energy: phantom behavior and negative absolute temperature

Ricardo G. Landim

The fractional dark energy (FDE) model describes the accelerated expansion of the Universe through a nonrelativistic gas of particles with a noncanonical kinetic term. This term is…

astro-ph.CO2021★ 26 cited

Fractional dark energy

Ricardo G. Landim

In this paper we introduce the fractional dark energy model, in which the accelerated expansion of the Universe is driven by a nonrelativistic gas (composed by either fermions or b…

astro-ph.CO2020★ 119 cited

The miniJPAS survey: a preview of the Universe in 56 colours

S. Bonoli, A. Marín-Franch, J. Varela +166

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique…

hep-ph2020★ 3 cited

Fat brane and seesaw mechanism in extra dimensions

Bjorn Garbrecht, Ricardo G. Landim

In this paper we present a higher-dimensional seesaw mechanism. We consider a single, flat extra dimension, where a fat brane is localized and contains the standard model (SM) fiel…

astro-ph.CO2020★ 8 cited

Dark photon dark matter and fast radio bursts

Ricardo G. Landim

The nature of dark matter (DM) is still a mystery that may indicate the necessity for extensions of the Standard Model (SM). Light dark photons (DP) may comprise partially or entir…

hep-ph2019★ 4 cited

Fat brane, dark matter and localized kinetic terms in six dimensions

Ricardo G. Landim

Extra dimensions (ED) have been used as attempts to explain several phenomena in particle physics over the years. In this paper we investigate the role of an abelian gauge field as…