How unbiased statistical methods lead to biased scientific discoveries: A case study of the Efron-Petrosian statistic applied to the luminosity-redshift evolution of Gamma-Ray Bursts
arXiv:2010.02935 · doi:10.1093/mnras/stab1098
Abstract
Statistical methods are frequently built upon assumptions that limit their applicability to certain problems and conditions. Failure to recognize these limitations can lead to conclusions that may be inaccurate or biased. An example of such methods is the non-parametric Efron-Petrosian test statistic used in the studies of truncated data. We argue and show how the inappropriate use of this statistical method can lead to biased conclusions when the assumptions under which the method is valid do not hold. We do so by reinvestigating the evidence recently provided by multiple independent reports on the evolution of the luminosity/energetics distribution of cosmological Long-duration Gamma-Ray Bursts (LGRBs) with redshift. We show that the effects of detection threshold has been likely significantly underestimated in the majority of previous studies. This underestimation of detection threshold leads to severely-incomplete LGRB samples that exhibit strong apparent luminosity-redshift or energetics-redshift correlations. We further confirm our findings by performing extensive Monte Carlo simulations of the cosmic rates and the luminosity/energy distributions of LGRBs and their detection process.
References in corpus (39)
- Gamma-Ray Bursts
- Gamma-Ray Bursts in the Swift Era
- The Fourth BATSE Gamma-Ray Burst Catalog (Revised)
- Gamma-Ray Bursts in the Swift Era
- A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution
- The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold
- The Cosmic Rate, Luminosity Function and Intrinsic Correlations of Long GRBs
- Testing the Gamma-Ray Burst Energy Relationships
- Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs. I: Stellar mass at z<1
- The Konus-Wind catalog of gamma-ray bursts with known redshifts. I. Bursts detected in the triggered mode
- The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution
- Determination of the intrinsic Luminosity Time Correlation in the X-ray Afterglows of GRBs
- The BATSE 5B Gamma-Ray Burst Spectral Catalog
- GRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6
- The rate and luminosity function of long Gamma Ray Bursts
- Cosmological Evolution of Long Gamma-ray Bursts and Star Formation Rate
- An unexpectedly low-redshift excess of Swift gamma-ray burst rate
- The Optically Unbiased Gamma-Ray Burst Host (TOUGH) Survey. VII. The Host Galaxy Luminosity Function: Probing the Relationship Between GRBs and Star Formation to Redshift
- On the Radio and Optical Luminosity Evolution of Quasars
- Short vs. Long Gamma-Ray Bursts: A Comprehensive Study of Energetics and Prompt Gamma-Ray Correlations
- On the Cosmological Evolution of Long Gamma-ray Burst Properties
- Connecting GRBs and ULIRGs: A Sensitive, Unbiased Survey for Radio Emission from Gamma-Ray Burst Host Galaxies at 0<z<2.5
- The Possible Impact of GRB Detector Thresholds on Cosmological Standard Candles
- The Swift Gamma-Ray Burst redshift distribution: selection biases and optical brightness evolution at high-z?
- Quantifying the Luminosity Evolution in Gamma-ray Bursts
- A comprehensive statistical study on gamma-ray bursts
- The Luminosity Function and Formation Rate of A Complete Sample of Long Gamma-Ray Bursts
- Analytical Approach for the Determination of the Luminosity Distance in a Flat Universe with Dark Energy
- Cosmic Evolution of Long Gamma-Ray Burst Luminosity
- A Multivariate Fit Luminosity Function and World Model for Long GRBs
- Hardness as a Spectral Peak Estimator for Gamma-Ray Bursts
- A Multilevel Empirical Bayesian Approach to Estimating the Unknown Redshifts of 1366 BATSE Catalog Long-Duration Gamma-Ray Bursts
- Resolving the Excess of Long GRBs at low redshift in the Swift Era
- Fast fully-reproducible serial/parallel Monte Carlo and MCMC simulations and visualizations via ParaMonte::Python library
- ParaDRAM: A Cross-Language Toolbox for Parallel High-Performance Delayed-Rejection Adaptive Metropolis Markov Chain Monte Carlo Simulations
- A Catalog of Redshift Estimates for 1366 BATSE Long-Duration Gamma-Ray Bursts: Evidence for Strong Selection Effects on the Phenomenological Prompt Gamma-Ray Correlations
- Multilevel Bayesian Parameter Estimation in the Presence of Model Inadequacy and Data Uncertainty
- Gamma-Ray bursts: Energetics and Prompt Correlations
- ParaMonte: A high-performance serial/parallel Monte Carlo simulation library for C, C++, Fortran
Cited by in corpus (14)
- The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
- Quasar standardization: Overcoming Selection Biases and Redshift Evolution
- Revisiting the luminosity and redshift distributions of long gamma-ray bursts
- A Comparative Study of Luminosity Functions and Event Rate Densities of Long GRBs with Non-parametric Method
- Accounting for Selection Bias and Redshift Evolution in GRB Radio Afterglow Data
- The short gamma-ray burst population in a quasi-universal jet scenario
- Does the Redshift Distribution of Swift Long GRBs Trace the Star-Formation Rate?
- Are quasars reliable standard candles?
- Energetic requirements of the gamma-ray emission from pulsars: A nonparametric analysis of the data in the Fermi-LAT 12-Year Catalog
- Probing Evolution of Long Gamma-Ray Burst Properties through Their Cosmic Formation History
- Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts
- Application of Efron-Petrosian method to radio pulsar fluxes
- An alternative interpretation of magnetars' traits deduced from the observational data on their outburst fluxes and spectra
- An alternative statistical interpretation for the apparent plateaus in the duration distributions of GRBs