Low redshift calibration of the Amati relation using galaxy clusters

Abstract

In this work, we use angular diameter distances of 38 galaxy clusters with joint X-ray/SZE observation to circumvent the circularity problem in the Amati relation for Gamma-ray Bursts (GRBs). Assuming the validity of cosmic-distance duality relation, we obtain the luminosity distance from the cluster angular diameter distance and use that to calculate the isotropic equivalent energy of two different GRB datasets, after restricting the GRB redshift range to $z<0.9$. We then check the validity of the Amati relation for both these datasets. The best-fit Amati relation parameters using galaxy cluster distances as low-redshift anchors are consistent with a previous estimate for the same dataset. The intrinsic scatter which we obtain for the two datasets is about 45% and 15%, and is comparable with that found by other distance anchors used to vet the Amati relation.

arXiv comment8 pages, 4 figures. Accepted for publication in JCAP

References in corpus (61)

• emcee: The MCMC Hammer
• The Supernova -- Gamma-Ray Burst Connection
• The Simons Observatory: Science goals and forecasts
• Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
• Cosmological Parameters from Observations of Galaxy Clusters
• The Physics of Gamma-Ray Bursts and Relativistic Jets
• Formation of Galaxy Clusters
• Short-Hard Gamma-Ray Bursts
• Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters
• A Photometric Redshift of z ~ 9.4 for GRB 090429B
• The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications
• Reconstruction of dark energy and expansion dynamics using Gaussian processes
• The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
• Measuring the cosmological parameters with the Ep,i-Eiso correlation of Gamma-Ray Bursts
• Determination of the Cosmic Distance Scale from Sunyaev-Zel'dovich Effect and Chandra X-ray Measurements of High Redshift Galaxy Clusters
• A Possible Cepheid-Like Luminosity Estimator for the Long Gamma-Ray Bursts
• The THESEUS space mission concept: science case, design and expected performances
• The baryonic Tully-Fisher relation for different velocity definitions and implications for galaxy angular momentum
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
• Testing the Distance-Duality Relation with Galaxy Clusters and Type Ia Supernovae
• Addressing the circularity problem in the $E_{\text{p}}-E_{\text{iso}}$ correlation of Gamma-Ray Bursts
• Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
• Cosmic Distance Duality Relation and the Shape of Galaxy Clusters
• Gamma-Ray Bursts in $1.8<z<5.6$ Suggest that the Time Variation of the Dark Energy is Small
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Gamma-ray burst prompt correlations: selection and instrumental effects
• Two new tests to the distance duality relation with galaxy clusters
• Gamma Ray Burst afterglow and prompt-afterglow relations: an overview
• Model independent calibrations of gamma ray bursts using machine learning
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Classification of Gamma-Ray Burst durations using robust model-comparison techniques
• Limit on graviton mass from galaxy cluster Abell 1689
• A Consistent Test of the Distance-Duality Relation with Galaxy Clusters and Type Ia Supernave
• High efficiency photospheric emission entailed by formation of a collimation shock in gamma-ray bursts
• Statistical classification of gamma-ray bursts based on the Amati relation
• Markov Chain Monte Carlo joint analysis of Chandra X-ray imaging spectroscopy and Sunyaev-Zeldovich Effect data
• A Significant Problem With Using the Amati Relation for Cosmological Purposes
• Model Comparison of $\Lambda$CDM vs $R_h=ct$ using Cosmic Chronometers
• Constraints on variation of fine structure constant from joint SPT-SZ and XMM-Newton observations
• A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
• The improved Amati correlations from Gaussian copula
• Cosmological Tests Using the Angular Size of Galaxy Clusters
• Yet another test of Radial Acceleration Relation for galaxy clusters
• Improving sampling and calibration of GRBs as distance indicators
• Search for Lorentz Invariance Violation from stacked Gamma-Ray Burst spectral lag data
• A search for the variation of speed of light using galaxy cluster gas mass fraction measurements
• Galaxy cluster angular size data constraints on dark energy
• Redshift evolution of the Amati relation: calibrated results from the Hubble diagram of quasars at high redshifts
• Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
• Two Dimensional Clustering of Gamma-Ray Bursts using durations and hardness
• Measuring dark energy with expansion and growth
• A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
• The $E_{\mathrm{p}}$ - $E_{\mathrm{iso}}$ relation and the internal shock model
• Scaling relations for dark matter core density and radius from Chandra X-ray cluster sample
• Mass-Velocity Dispersion Relation in MaNGA Brightest Cluster Galaxies
• A model-independent test of the evolution of gas depletion factor for SPT-SZ and Planck ESZ clusters
• A test of the evolution of gas depletion factor in galaxy clusters using strong gravitational lensing systems
• Galaxy clusters, cosmic chronometers and the Einstein equivalence principle
• Characterization of the GRB prompt fundamental plane using Fermi-GBM data

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• Gamma Rays Bursts: A Viable Cosmological Probe?
• Astrophysical and Cosmological Searches for Lorentz Invariance Violation
• Testing the standardizability of, and deriving cosmological constraints from, a new Amati-correlated gamma-ray burst data compilation
• Testing the consistency of new Amati-correlated gamma-ray burst dataset cosmological constraints with those from better-established cosmological data
• Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample
• Calibration of luminosity correlations of gamma-ray bursts using quasars
• Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network
• A test of Amati relation using HII galaxy distances