activity
20102023
most citedAn absorption profile centred at 78 megahertz in the sky-averaged spectrum

1.2k citations · 2.8k across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2023★ 4 cited

Low-Frequency Radio Recombination Lines Away From the Inner Galactic Plane

Akshatha K. Vydula, Judd D. Bowman, David Lewis +8

Diffuse radio recombination lines (RRLs) in the Galaxy are possible foregrounds for redshifted 21~cm experiments. We use EDGES drift scans centered at ~declination to char…

astro-ph.IM2022★ 13 cited

Analytic approximations of scattering effects on beam chromaticity in 21-cm global experiments

Alan E. E. Rogers, John P. Barrett, Judd D. Bowman +6

Scattering from objects near an antenna produce correlated signals from strong compact radio sources in a manner similar to those used by the Sea Interferometer to measure the radi…

astro-ph.CO2022★ 24 cited

A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors -- I. Mathematical formalism

Peter H. Sims, Judd D. Bowman, Nivedita Mahesh +7

Accurately accounting for spectral structure in spectrometer data induced by instrumental chromaticity on scales relevant for detection of the 21-cm signal is among the most signif…

astro-ph.CO2022★ 31 cited

The Second Radio Synchrotron Background Workshop: Conference Summary and Report

J. Singal, N. Fornengo, M. Regis +24

We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the d…

astro-ph.CO2022★ 27 cited

A Bayesian Calibration Framework for EDGES

Steven G. Murray, Judd D. Bowman, Peter H. Sims +5

We develop a Bayesian model that jointly constrains receiver calibration, foregrounds and cosmic 21cm signal for the EDGES global 21\,cm experiment. This model simultaneously descr…

astro-ph.CO2021★ 9 cited

Effects of model incompleteness on the drift-scan calibration of radio telescopes

Bharat K. Gehlot, Daniel C. Jacobs, Judd D. Bowman +76

Precision calibration poses challenges to experiments probing the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn and Epoch of Reionization (z~30-6). In both inter…

astro-ph.IM2021★ 43 cited

Validation of EDGES Low-Band Antenna Beam Model

Nivedita Mahesh, Judd D. Bowman, Thomas J. Mozdzen +4

The response of the antenna is a source of uncertainty in measurements with the Experiment to Detect the Global EoR Signature (EDGES). We aim to validate the beam model of the low-…

astro-ph.GA2020★ 26 cited

Absolute Calibration of Diffuse Radio Surveys at 45 and 150 MHz

Raul A. Monsalve, Alan E. E. Rogers, Judd D. Bowman +7

We use EDGES measurements to determine scale and zero-level corrections to the diffuse radio surveys by Guzmán et al. at MHz and Landecker & Wielebinski at MHz. We find…

astro-ph.IM2020

Radio-Frequency Interference at the McGill Arctic Research Station

T. Dyson, H. C. Chiang, E. Egan +7

The frequencies of interest for redshifted 21 cm observations are heavily affected by terrestrial radio-frequency interference (RFI). We identify the McGill Arctic Research Station…

astro-ph.IM2019★ 1 cited

Canada and the SKA from 2020-2030

Kristine Spekkens, Cynthia Chiang, Roland Kothes +57

This white paper submitted for the 2020 Canadian Long-Range Planning process (LRP2020) presents the prospects for Canada and the Square Kilometre Array (SKA) from 2020-2030, focuss…

astro-ph.CO2019★ 72 cited

Emulating the Global 21-cm Signal from Cosmic Dawn and Reionization

Aviad Cohen, Anastasia Fialkov, Rennan Barkana +1

The 21-cm signal of neutral hydrogen is a sensitive probe of the Epoch of Reionization (EoR) and Cosmic Dawn. Currently operating radio telescopes have ushered in a data-driven era…

astro-ph.IM2019★ 18 cited

Discovering the Sky at the Longest Wavelengths with Small Satellite Constellations

Xuelei Chen, Jack Burns, Leon Koopmans +29

Due to ionosphere absorption and the interference by natural and artificial radio emissions, ground observation of the sky at the decameter or longer is very difficult. This unexpl…

astro-ph.CO2019★ 64 cited

Results from EDGES High-Band: III. New Constraints on Parameters of the Early Universe

Raul A. Monsalve, Anastasia Fialkov, Judd D. Bowman +5

We present new constraints on parameters of cosmic dawn and the epoch of reionization derived from the EDGES High-Band spectrum ( MHz). The parameters are probed by evaluat…

astro-ph.IM2019★ 60 cited

Spectral Index of the Diffuse Radio Background Between 50 and 100 MHz

Thomas J. Mozdzen, Nivedita Mahesh, Raul A. Monsalve +2

We report the spectral index of diffuse radio emission between 50 and 100 MHz from data collected with two implementations of the Experiment to Detect the Global EoR Signature (EDG…

astro-ph.CO2018★ 1.2k cited

An absorption profile centred at 78 megahertz in the sky-averaged spectrum

Judd D. Bowman, Alan E. E. Rogers, Raul A. Monsalve +2

After stars formed in the early Universe, their ultraviolet light is expected, eventually, to have penetrated the primordial hydrogen gas and altered the excitation state of its 21…

astro-ph.CO2018★ 49 cited

Results from EDGES High-Band: II. Constraints on Parameters of Early Galaxies

Raul A. Monsalve, Bradley Greig, Judd D. Bowman +5

We use the sky-average spectrum measured by EDGES High-Band ( MHz) to constrain parameters of early galaxies independent of the absorption feature at ~MHz reported by B…

astro-ph.CO2018★ 236 cited

Concerns about Modelling of the EDGES Data

Richard Hills, Girish Kulkarni, P. Daniel Meerburg +1

It is predicted that the spectrum of radio emission from the whole sky should show a dip arising from the action of the light from the first stars on the hydrogen atoms in the surr…

astro-ph.CO2018★ 210 cited

Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude

A. Ewall-Wice, T. -C. Chang, J. Lazio +3

We estimate the 21 cm Radio Background from accretion onto the first intermediate-mass Black Holes between and . Combining potentially optimistic, but pl…

astro-ph.CO2017★ 118 cited

Results from EDGES High-Band: I. Constraints on Phenomenological Models for the Global cm Signal

Raul A. Monsalve, Alan E. E. Rogers, Judd D. Bowman +1

We report constraints on the global cm signal due to neutral hydrogen at redshifts . We derive our constraints from low foreground observations of the av…

astro-ph.IM2017★ 58 cited

A Space-Based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21-cm Global Spectrum

Jack O. Burns, Richard Bradley, Keith Tauscher +19

The redshifted 21-cm monopole is expected to be a powerful probe of the epoch of the first stars and galaxies (). The global 21-cm signal is sensitive to the thermal and i…

astro-ph.IM2016★ 77 cited

Improved Measurement of the Spectral Index of the Diffuse Radio Background Between 90 and 190 MHz

Thomas. J. Mozdzen, Judd. D. Bowman, Raul. A. Monsalve +1

We report absolutely calibrated measurements of diffuse radio emission between 90 and 190 MHz from the Experiment to Detect the Global EoR Signature (EDGES). EDGES employs a wide b…

astro-ph.IM2016★ 18 cited

One-Port Direct/Reverse Method for Characterizing VNA Calibration Standards

Raul A. Monsalve, Alan E. E. Rogers, Thomas J. Mozdzen +1

This paper introduces a one-port method for estimating model parameters of VNA calibration standards. The method involves measuring the standards through an asymmetrical passive ne…

astro-ph.IM2016★ 89 cited

Calibration of the EDGES High-Band Receiver to Observe the Global 21-cm Signature from the Epoch of Reionization

Raul A. Monsalve, Alan E. E. Rogers, Judd D. Bowman +1

The EDGES High-Band experiment aims to detect the sky-average brightness temperature of the -cm signal from the Epoch of Reionization (EoR) in the redshift range $14.8 \gtrsim…

astro-ph.IM2015★ 51 cited

Limits on Foreground Subtraction from Chromatic Beam Effects in Global Redshifted 21 cm Measurements

Thomas J. Mozdzen, Judd D. Bowman, Raul A. Monsalve +1

Foreground subtraction in global redshifted 21 cm measurements is limited by frequency-dependent (chromatic) structure in antenna beam patterns. Chromatic beams couple angular stru…