activity
20122026
most citedThe influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 m wavelengths

70 citations · 228 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

Optical Variability as a Probe of Hidden Nuclear Activity in Type 2 AGNs

Maša Lakićević

Optical variability in Type 2 active galactic nuclei (AGNs) is rarely explored because the direct accretion-disk continuum is obscured by circumnuclear dust. Nevertheless, detectab…

astro-ph.IM2022★ 29 cited

The LSST era of supermassive black holes accretion-disk reverberation mapping

Andjelka B. Kovacevic, Viktor Radovic, Dragana Ilic +22

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will detect an unprecedentedly large sample of actively accreting supermassive black holes with typical accreti…

astro-ph.GA2021★ 22 cited

Tracing the outflow kinematics in Type 2 Active Galactic Nuclei

Jelena Kovacevic-Dojcinovic, Ivan Dojcinovic, Masa Lakicevic +1

We have used the sample of 577 active galactic nuclei Type 1.8-2 spectra (z < 0.25), taken from Sloan Digital Sky Survey, to trace the influence of the outflow kinematics to the pr…

astro-ph.GA2018

Kinematic differences between NLS1 and BLAGN sources

M. Lakićević, L. Č. Popović, J. Kovačević-Dojčinović

It is well-known that the higher policyclic aromatic hydrocarbon (PAH) abundance, lower black hole mass, higher accretion rate and lower luminosities are among the major characteri…

astro-ph.HE2018★ 17 cited

ALMA observations of supernova remnant N49 in the LMC: I. Discovery of CO clumps associated with X-ray and radio continuum shells

Y. Yamane, H. Sano, J. Th. van Loon +24

N49 (LHA 120-N49) is a bright X-ray supernova remnant (SNR) in the Large Magellanic Cloud. We present new CO( = 1-0, 3-2), HI, and 1.4 GHz radio-continuum observations of…

astro-ph.IM2016★ 5 cited

Study of the atmospheric conditions at Cerro Armazones using astronomical data

Masha Lakicevic, Stefan Kimeswenger, Stefan Noll +3

Aims: We studied the precipitable water vapour (PWV) content near Cerro Armazones and discuss the potential use of our technique of modelling the telluric absorbtion lines for the…

astro-ph.GA2014★ 70 cited

The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 m wavelengths

Maša Lakićević, Jacco Th. van Loon, Margaret Meixner +20

We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and submillimeter wavelengths.…

astro-ph.HE2014★ 63 cited

Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA & ATCA

Giovanna Zanardo, Lister Staveley-Smith, Remy Indebetouw +18

We present a comprehensive spectral and morphological analysis of the remnant of Supernova (SN) 1987A with the Australia Telescope Compact Array (ATCA) and the Atacama Large Millim…

astro-ph.HE2012★ 22 cited

The remnant of Supernova 1987A resolved at 3 mm wavelength

Masha Lakicevic, Giovanna Zanardo, Jacco Th. van Loon +4

The proximity of core-collapse Supernova 1987A (SN1987A) in the Large Magellanic Cloud (LMC) and its rapid evolution make it a unique case study of the development of a young super…