The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
arXiv:2107.01633 · doi:10.1051/0004-6361/202140883
Abstract
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 cosmic HI and learn about cosmology. BINGO (Baryon Acoustic Oscillations [BAO] from Integrated Neutral Gas Observations) is a new unique radio telescope designed to be one of the first to probe BAO at radio frequencies. BINGO has two science goals: cosmology and astrophysics. Cosmology is the main science goal and the driver for BINGO's design and strategy. The key of BINGO is to detect the low redshift BAO to put strong constraints in the dark sector models. Given the versatility of the BINGO telescope, a secondary goal is astrophysics, where BINGO can help discover and study Fast Radio Bursts (FRB) and other transients, Galactic and extragalactic science. In this paper, we introduce the latest progress of the BINGO project, its science goals, describing the scientific potential of the project in each science and the new developments obtained by the collaboration. We introduce the BINGO project and its science goals and give a general summary of recent developments in construction, science potential and pipeline development obtained by the BINGO collaboration in the past few years. We show that BINGO will be able to obtain competitive constraints for the dark sector, and also that will allow for the discovery of several FRBs in the southern hemisphere. The capacity of BINGO in obtaining information from 21-cm is also tested in the pipeline introduced here. There is still no measurement of the BAO in radio, and studying cosmology in this new window of observations is one of the most promising advances in the field. The BINGO project is a radio telescope that has the goal to be one of the first to perform this measurement and it is currently being built in the northeast of Brazil. (Abridged)
arXiv comment23 pages. To appear in A&A
References in corpus (192)
- Array Programming with NumPy
- Dynamics of dark energy
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Evidence for oscillation of atmospheric neutrinos
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- The ATNF Pulsar Catalogue
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- Weak Gravitational Lensing
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- A bright millisecond radio burst of extragalactic origin
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
- Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
- Coupled Quintessence
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
- The Temperature of the Cosmic Microwave Background
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
- A Repeating Fast Radio Burst
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
- 21-cm Tomography of the Intergalactic Medium at High Redshift
- A bright millisecond-duration radio burst from a Galactic magnetar
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
- Transient radio bursts from rotating neutron stars
- Interacting Quintessence
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Fast Radio Bursts
- Interacting quintessence solution to the coincidence problem
- Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey
- Weak Gravitational Lensing by Large-Scale Structure
- A Living Theory Catalogue for Fast Radio Bursts
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
- CHIME/FRB Detection of Eight New Repeating Fast Radio Burst Sources
- Planck 2018 results. IV. Diffuse component separation
- Science with ASKAP - the Australian Square Kilometre Array Pathfinder
- The SDSS Damped Lya Survey: Data Release 3
- Dense magnetized plasma associated with a fast radio burst
- Periodic activity from a fast radio burst source
- The CHIME Fast Radio Burst Project: System Overview
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- The High Time Resolution Universe Pulsar Survey I: System configuration and initial discoveries
- The Fundamental Performance of FAST with 19-beam Receiver at L Band
- The Anglo-Australian Observatory's 2dF Facility
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- Highest-frequency detection of FRB 121102 at 4-8 GHz using the Breakthrough Listen Digital Backend at the Green Bank Telescope
- Models of Pulsar Glitches
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- Fast neutral outflows in powerful radio galaxies: a major source of feedback in massive galaxies
- A Second Source of Repeating Fast Radio Bursts
- Possible periodic activity in the repeating FRB 121102
- A possible connection between Fast Radio Bursts and Gamma-Ray Bursts
- Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlation
- Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
- An Anomalous Component of Galactic Emission
- Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter
- Planck Early Results: Thermal dust in Nearby Molecular Clouds
- HI intensity mapping : a single dish approach
- Towards a free-free template for CMB foregrounds
- Magnetic Dipole Microwave Emission from Dust Grains
- Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- All-Sky Interferometry with Spherical Harmonic Transit Telescopes
- A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
- Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- The MeerKAT Telescope as a Pulsar Facility: System verification and early science results from MeerTime
- Improving lognormal models for cosmological fields
- Testing General Relativity with 21 cm intensity mapping
- The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts
- The detection of an extremely bright fast radio burst in a phased array feed survey
- Fast radio bursts as a cosmic probe?
- Foreground component separation with generalised ILC
- The Tianlai project: a 21cm cosmology experiment
- Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters
- On the FRB luminosity function -- II. Event rate density
- Observations of HI Absorbing Gas in Compact Radio Sources at Cosmological Redshifts
- The first interferometric detections of Fast Radio Bursts
- Testing the interaction between dark energy and dark matter via latest observations
- Observational constraints on the dark energy and dark matter mutual coupling
- Probing radio source environments via HI and OH absorption
- Testing Einstein's Equivalence Principle with Fast Radio Bursts
- On the normalised FRB luminosity function
- Faint Repetitions from a Bright Fast Radio Burst Source
- Algorithms for bispectra: forecasting, optimal analysis, and simulation
- Strongly lensed repeating Fast Radio Bursts as precision probes of the universe
- The miniJPAS survey: a preview of the Universe in 56 colours
- The State-of-Play of Anomalous Microwave Emission (AME) Research
- Redshifted Neutral Hydrogen 21cm Absorption toward Red Quasars
- Photon Mass Limits from Fast Radio Bursts
- Future Cosmological Constraints from Fast Radio Bursts
- NGC 4244: A Low Mass Galaxy with a Falling Rotation Curve and a Flaring Gas Layer
- Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
- The Presence and Distribution of HI Absorbing Gas in Sub-galactic Sized Radio Sources
- Neutral Hydrogen (21 cm) Absorption in Seyfert Galaxies: Evidence for Free-free Absorption and Sub-kiloparsec Gaseous Disks
- The HI absorption "Zoo"
- Towards a fully consistent parameterization of modified gravity
- Non-Gaussian statistics of critical sets in 2 and 3D: Peaks, voids, saddles, genus and skeleton
- The interstellar and circumnuclear medium of active nuclei traced by HI 21-cm absorption
- Optimal filter systems for photometric redshift estimation
- Detection of Repeating FRB 180916.J0158+65 Down to Frequencies of 300 MHz
- Radio and X-ray observations of the intermittent pulsar J1832+0029
- 1/f noise and other systematic effects in the Planck-LFI radiometers
- Kinematics and physical conditions of HI in nearby radio sources. The last survey of the old Westerbork Synthesis Radio Telescope
- Fast Radio Bursts as Probes of Magnetic Fields in the Intergalactic Medium
- New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
- Constraints on the Photon Mass with Fast Radio Bursts
- Non Gaussianity and Minkowski Functionals: forecasts for Planck
- The Planck-LFI instrument: analysis of the 1/f noise and implications for the scanning strategy
- A search for HI absorption in nearby radio galaxies using HIPASS
- Probing dark energy with baryonic oscillations and future radio surveys of neutral Hydrogen
- Fast Radio Transient searches with UTMOST at 843 MHz
- Cosmology with the Square Kilometre Array
- Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
- Simulations for single-dish intensity mapping experiments
- The Impact of Atmospheric Fluctuations on Degree-scale Imaging of the Cosmic Microwave Background
- Pulsar Timing Array Based Search for Supermassive Black Hole Binaries in the Square Kilometer Array Era
- Cosmological Parameter Estimation with Large Scale Structure Observations
- FRB 121102 Casts New Light on the Photon Mass
- The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects
- Extracting HI cosmological signal with Generalized Needlet Internal Linear Combination
- Extracting host galaxy dispersion measure and constraining cosmological parameters using fast radio burst data
- The Exploration of the Unknown
- Fast Radio Bursts
- HI Signal from Reionization Epoch
- On the detectability of extragalactic fast radio transients
- The imprint of the interaction between dark sectors in galaxy clusters
- Gravitational wave research using pulsar timing arrays
- Minkowski Functionals and Cluster Analysis for CMB Maps
- Interpreting the distributions of FRB observables
- HI absorption towards nearby compact radio sources
- Measuring the circum- and inter-galactic baryon contents with fast radio bursts
- The Tianlai Dish Pathfinder Array: design, operation and performance of a prototype transit radio interferometer
- A search for Fast Radio Bursts at low frequencies with Murchison Widefield Array high time resolution imaging
- A Bayesian Framework to Constrain the Photon Mass with a Catalog of Fast Radio Bursts
- A search for 21 cm HI absorption in AT20G compact radio galaxies
- Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
- Cosmological constraints from 21cm surveys after reionization
- Measuring the cosmic proper distance from fast radio bursts
- Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
- Forecast for FAST: from Galaxies Survey to Intensity Mapping
- Non-linear Redshift-Space Power Spectra
- A bright, high rotation-measure FRB that skewers the M33 halo
- Lensing of Fast Radio Bursts by Binaries to Probe Compact Dark Matter
- The Dispersion of Fast Radio Bursts from a Structured Intergalactic Medium at Redshifts z < 1.5
- A Giant Metrewave Radio Telescope search for associated H{\sc i} 21\,cm absorption in GHz-peaked-spectrum sources
- Practical solutions for perturbed f(R) gravity
- The Tianlai Cylinder Pathfinder Array: System Functions and Basic Performance Analysis
- Forecasts for Dark Energy Measurements with Future HI Surveys
- Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
- Cosmology with Gravitational Wave/Fast Radio Burst Associations
- The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
- The detectability of HI 21-cm absorption in damped Lyman-alpha systems
- Associated 21-cm absorption towards the cores of radio galaxies
- Limits on the Weak Equivalence Principle and Photon Mass with FRB 121102 Sub-pulses
- Optimised angular power spectra for spectroscopic galaxy surveys
- Detecting Helium Reionization with Fast Radio Bursts
- A Giant Metrewave Radio Telescope survey for associated HI 21-cm absorption in the Caltech-Jodrell Flat-spectrum sample
- 21 cm intensity mapping with the Five hundred metre Aperture Spherical Telescope
- The BINGO Project II: Instrument Description
- Long-term Observations of Three Nulling Pulsars
- Potential Impact of Global Navigation Satellite Services on Total Power HI Intensity Mapping Surveys
- The ALFALFA HI Absorption Pilot Survey: A Wide-Area Blind Damped Lyman Alpha System Survey of the Local Universe
- Polarization of the Atmosphere as a Foreground for Cosmic Microwave Background Polarization Experiments
- Observing Cosmological Processes in Real Time with Repeating Fast Radio Bursts
- Robust Limits on Photon Mass from Statistical Samples of Extragalactic Radio Pulsars
- Radio Pulsars
- The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
- New Limits on the Photon Mass with Radio Pulsars in the Magellanic Clouds
- Flux density variability of 286 radio pulsars from a decade of monitoring
- The nature of fast radio bursts
- The Dark Sector Cosmology
- The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
- Noise Properties of the Planck-LFI Receivers
- The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
- Radio Properties of Rotating Radio Transients: Single Pulse Spectral and Wait Time Analyses
- The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
- A New Method to Test the Einstein's Weak Equivalence Principle
- Probing WHIM around Galaxy Clusters with Fast Radio Bursts and the Sunyaev-Zel'dovich effect
- HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4
- Baryon acoustic oscillations from Integrated Neutral Gas Observations: Broadband corrugated horn construction and testing
- Testing Weak Equivalence Principle with Strongly Lensed Cosmic Transients
- Tomographic local 2D analyses of the WISExSuperCOSMOS all-sky galaxy catalogue
- Baryon acoustic oscillations from Integrated Neutral Gas Observations: Radio frequency interference measurements and telescope site selection
- Cosmic Transients, Einstein's Equivalence Principle and Dark Matter Halos
- Dark photon dark matter and fast radio bursts
- A first quantification of the effects of absorption for HI Intensity Mapping experiments
Cited by in corpus (33)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids
- Wormhole solutions in gravity with a radial dependent B parameter
- The BINGO Project II: Instrument Description
- The Second Radio Synchrotron Background Workshop: Conference Summary and Report
- The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
- Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
- The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
- The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
- The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
- Wormhole Geometry and Three-Dimensional Embedding in Extended Symmetric Teleparallel Gravity
- The local PNG bias of neutral Hydrogen,
- Cosmography from well-localized Fast Radio Bursts
- Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble Constant
- Constraining Cosmic Inflation with Observations: Prospects for 2030
- Stable soliton dark matter wormhole in non-minimally coupled gravity
- 21-cm foreground removal using AI and frequency-difference technique
- Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
- Cosmological constraints from low redshift 21 cm intensity mapping with machine learning
- Testing the consistency of early and late cosmological parameters with BAO and CMB data
- The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
- Analyzing the 21cm forest with Wavelet Scattering Transform: Insight into non-Gaussian features of the 21cm forest
- Testing synchrotron models and frequency resolution in BINGO 21 cm simulated maps using GNILC
- Expanded Generalized Needlet Internal Linear Combination (eGNILC) Framework for the 21-cm Foreground Removal
- The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey
- Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
- Stability of the spacetime of a magnetized compact object
- Needlets and foreground removal for SKAO hydrogen intensity maps
- Cosmological Forecasts from the Baryon Acoustic Oscillations in 21cm Intensity Mapping
- Deep learning with hybrid frequency differencing and principal component analysis for 21-cm foreground and beam mitigation
- Universality in quasinormal modes of a magnetized black hole
- The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
- Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys