Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator III: Foreground removal
arXiv:2308.08284 · doi:10.1093/mnras/stad2495
Abstract
Neutral hydrogen (HI) -cm intensity mapping (IM) is a promising probe of the large-scale structures in the Universe. However, a few orders of magnitude brighter foregrounds obscure the IM signal. Here we use the Tapered Gridded Estimator (TGE) to estimate the multi-frequency angular power spectrum (MAPS) from a bandwidth uGMRT Band data at . In foregrounds remain correlated across the entire range, whereas the -cm signal is localized within (typically ). Assuming the range to have minimal -cm signal, we use in this range to model the foregrounds. This foreground model is extrapolated to , and subtracted from the measured . The residual in the range is used to constrain the -cm signal, compensating for the signal loss from foreground subtraction. is found to be noise-dominated without any trace of foregrounds. Using we constrain the -cm brightness temperature fluctuations , and obtain the upper limit at . We further obtain the upper limit where and are the comoving HI density and bias parameters respectively. Although the upper limit is nearly times larger than the expected -cm signal, it is times tighter over previous works using foreground avoidance on the same data.
Accepted for publication in MNRAS. 16 pages (including Appendix), 8 figures (plus 8 in Appendix), 5 Tables. In version 2, the HI symbol is changed in the arxiv abstract; there are no changes in the manuscript
References in corpus (50)
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- Late-time cosmology with 21cm intensity mapping experiments
- Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR
- Post-correlation radio frequency interference classification methods
- The Epoch of Reionization Window: I. Mathematical Formalism
- The Epoch of Reionization Window: II. Statistical Methods for Foreground Wedge Reduction
- First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
- Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
- On using visibility correlations to probe the HI distribution from the dark ages to the present epoch I: Formalism and the expected signal
- Foregrounds for redshifted 21 cm studies of reionization: GMRT 153 MHz observations
- Characterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT observations
- The multi-frequency angular power spectrum of the epoch of reionization 21 cm signal
- HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies
- HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
- Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
- HI 21-centimetre emission from an ensemble of galaxies at an average redshift of one
- Neutral hydrogen (HI) gas content of galaxies at
- Theoretical and observational constraints on the HI intensity power spectrum
- Visibility based angular power spectrum estimation in low frequency radio interferometric observations
- Towards simulating and quantifying the light-cone EoR 21-cm signal
- Gaussian Process Foreground Subtraction and Power Spectrum Estimation for 21 cm Cosmology
- GMRT observation towards detecting the Post-reionization 21-cm signal
- Estimation of Cosmological Parameters from HI Observations of Post-reionization Epoch
- Cosmological constraints from 21cm surveys after reionization
- DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra
- Detailed study of ELAIS N1 field with the uGMRT -- II. Source Properties and Spectral Variation Of Foreground Power Spectrum from 300-500 MHz Observations
- The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
- Damped Lyman-alpha Absorbers from Sloan Digital Sky Survey DR16Q with Gaussian processes
- Demonstrating the Tapered Gridded Estimator (TGE) for the Cosmological HI 21-cm Power Spectrum using GMRT observations
- The Ooty Wide Field Array
- The angular power spectrum measurement of the Galactic synchrotron emission in two fields of the TGSS survey
- A direct detection of neutral hydrogen intensity mapping on Mpc scales at and
- A Tapered Gridded Estimator (TGE) for the Multi-Frequency Angular Power Spectrum (MAPS) and the Cosmological HI 21-cm Power Spectrum
- First multi-redshift limits on post-Epoch of Reionization (post-EoR) 21 cm signal from z = 1.96 - 3.58 using uGMRT
- All sky angular power spectrum: I. Estimating brightness temperature fluctuations using TGSS 150 MHz survey
- Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling
- Statistical analysis of the causes of excess variance in the 21 cm signal power spectra obtained with the Low-Frequency Array
- Characterizing EoR foregrounds: A study of the Lockman Hole Region at 325 MHz
- Statistical recovery of the BAO scale from multipoles of the beam-convolved 21cm correlation function
- Primordial Non-Gaussianity in the Forest: 3D Bispectrum of Ly-alpha Flux Spectra Along Multiple Lines of Sight
- Calibration Requirements for Epoch of Reionization 21-cm signal observations -- I. Effect of time-correlated gains
- A study of Kepler supernova remnant: angular power spectrum estimation from radio frequency data
- Towards 21-cm Intensity Mapping at with uGMRT using the Tapered Gridded Estimator I: Foreground Avoidance
- Multi-frequency angular power spectrum of the 21~cm signal from the Epoch of Reionisation using the Murchison Widefield Array
- The auto and cross angular power spectrum of the Cas A supernova remnant in radio and X-ray
- Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator II: Cross-polarization power spectrum
- Calibration requirements for Epoch of Reionization 21-cm signal observations -- II. Analytical estimation of the bias and variance with time-correlated residual gains
- Why and When to Expect Gaussian Error Distributions in Epoch of Reionization 21-cm Power Spectrum Measurements
- The Tracking Tapered Gridded Estimator (TTGE) for the power spectrum from drift scan observations
- Impact of inhomogeneous reionization on post-reionization 21 cm intensity mapping measurement of cosmological parameters
Cited by in corpus (5)
- The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from MWA drift scan observations I: Validation and preliminary results
- Post-reionization HI 21-cm signal: A probe of negative cosmological constant
- Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator -- IV. Wideband analysis
- Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum
- Bayes-SCF: A Bayesian filter to mitigate foreground leakage in the 21-cm power spectrum