An upper limit calculator (UL-CALC) for undetected extended sources with radio interferometers: radio halo upper limits
Lijo T. George, Ruta Kale, Yogesh Wadadekar

TL;DR
This paper introduces UL-CALC, a Python tool that automates the estimation of upper limits for undetected radio halos in galaxy clusters using radio interferometer data, aiding in astrophysical model constraints.
Contribution
The paper presents a novel automated Python tool for estimating radio halo upper limits, streamlining a previously manual and model-dependent process.
Findings
The tool successfully automates upper limit estimation for radio halos.
It is applicable to large sky surveys like LOFAR and SKA.
The tool is publicly available for community use.
Abstract
Radio halos are diffuse, extended sources of radio emission detected primarily in massive, merging galaxy clusters. In smaller and/or relaxed clusters, where no halos are detected, one can instead place upper limits to a possible radio emission. Detections and upper limits are both crucial to constrain theoretical models for the generation of radio halos. The upper limits are model dependent for radio interferometers and thus the process of obtaining these is tedious to perform manually. In this paper, we present a Python based tool to automate this process of estimating the upper limits. The tool allows users to create radio halos with defined parameters like physical size, redshift and brightness model. A family of radio halo models with a range of flux densities, decided based on the rms noise of the image, is then injected into the parent visibility file and imaged. The halo…
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