activity
20122021
most citedThe ASKAP-EMU Early Science Project:Radio Continuum Survey of the Small Magellanic Cloud

29 citations · 83 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2021★ 8 cited

Radio Continuum Sources behind the Large Magellanic Cloud

M. D. Filipović, I. S. Bojičić, K. R. Grieve +38

We present a comprehensive multi-frequency catalogue of radio sources behind the Large Magellanic Cloud between 0.2 and 20 GHz, gathered from a combination of new and legacy radio…

astro-ph.HE2020★ 29 cited

New Optically Identified Supernova Remnants in the Large Magellanic Cloud

Miranda Yew, Miroslav D. Filipović, Milorad Stupar +20

We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC). These objects were originally selected usi…

astro-ph.GA2019★ 29 cited

The ASKAP-EMU Early Science Project:Radio Continuum Survey of the Small Magellanic Cloud

T. D. Joseph, M. D. Filipović, E. J. Crawford +53

We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images ar…

astro-ph.GA2017★ 8 cited

Radio Planetary Nebulae in the Large Magellanic Cloud

Howard Leverenz, Miroslav D. Filipovic, B. Vukotic +2

We present 21 new radio-continuum detections at catalogued planetary nebula (PN) positions in the Large Magellanic Cloud (LMC) using all presently available data from the Australia…

astro-ph.SR2016★ 4 cited

Radio Planetary Nebulae in the Small Magellanic Cloud

Howard Leverenz, Miroslav D. Filipović, Ivan S. Bojičić +5

We present ten new radio continuum (RC) detections at catalogued planetary nebula (PN) positions in the Small Magellanic Cloud (SMC): SMPS6, LIN 41, LIN 142, SMP S13, SMP S14, SMP…

astro-ph.GA2012★ 5 cited

An analysis of the FIR/RADIO Continuum Correlation in the Small Magellanic Cloud

Howard Leverenz, Miroslav D. Filipović

The local correlation between far-infrared (FIR) emission and radio-continuum (RC) emission for the Small Magellanic Cloud (SMC) is investigated over scales from 3 kpc to 0.01 kpc.…