activity
20142025
most citedBIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal

137 citations · 427 across the 20 of their papers we have counts for

collaborators

20 papers

eess.SP2025★ 1 cited

General Framework for Array Noise Analysis and Noise Performance of a Two-Element Interferometer With a Mutual-Coupling Canceler

Leonid Belostotski, Adrian T. Sutinjo, Ravi Subrahmanyan +2

This article investigates the noise performance of a two-element phased array and interferometer containing a recently introduced self-interference canceler, which in the context o…

astro-ph.IM2023★ 1 cited

A new technique to measure noise parameters for global 21-cm experiments

Danny C. Price, Cheuk-Yu Edward Tong, Adrian T. Sutinjo +2

Radiometer experiments to detect 21-cm Hydrogen line emission from the Cosmic Dawn and Epoch of Reionization rely upon precise absolute calibration. During calibration, noise gener…

astro-ph.HE2023

Calculation and Uncertainty of Fast Radio Burst Structure Based on Smoothed Data

Adrian T. Sutinjo, Danica R. Scott, Clancy W. James +7

Studies of the time-domain structure of fast radio bursts (FRBs) require an accurate estimate of the FRB dispersion measure in order to recover the intrinsic burst shape. Furthermo…

astro-ph.IM2022★ 6 cited

Measuring Noise Parameters Using an Open, Short, Load, and 1/8-wavelength Cable as Source Impedances

Danny C. Price, Cheuk-Yu Edward Tong, Adrian T. Sutinjo +2

Noise parameters are a set of four measurable quantities which determine the noise performance of a radio-frequency device under test. The noise parameters of a 2-port device can b…

astro-ph.IM2022★ 2 cited

System equivalent flux density of Stokes I, Q, U, V of a polarimetric interferometer

A. T. Sutinjo, D. C. X. Ung, M. Sokolowski

We present the system equivalent flux density (SEFD) expressions for all four Stokes parameters: I, Q, U, V. The expressions were derived based on our derivation of SEFD I (for Sto…

astro-ph.IM2022★ 18 cited

What is the SKA-Low Sensitivity for Your Favourite Radio Source ?

M. Sokolowski, S. J. Tingay, D. B. Davidson +8

The SKA will be the largest radio astronomy observatory ever built, providing unprecedented sensitivity over a very broad frequency (50 MHz to 15.3 GHz). The SKA-Low (50 - 350 MHz)…