Publication
Modeling the Continuum and Line Spectra of the Seyfert 2 Galaxy NGC 5252
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PublicationModeling the ionizing spectra of H II regions: individual stars versus stellar ensemblesAims: We study how IMF sampling affects the ionizing flux and emission line spectra of low mass stellar clusters. Methods: We performed 2 × 106 Monte Carlo...
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PublicationModeling the Stellar Populations in the Canis Major Overdensity: The Relation between the Old and Young PopulationsWe analyze the stellar populations of the Canis Major stellar overdensity using quantitative color-magnitude diagram (CMD) fitting techniques. The analysis is...
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PublicationModeling Tidal Streams in Evolving Dark Matter HalosWe explore whether stellar tidal streams can provide information on the secular, cosmological evolution of the Milky Way's gravitational potential and on the...
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PublicationModelling gaseous and stellar kinematics in the disc galaxies NGC 772, 3898 and 7782We present V-band surface photometry and major-axis kinematics of stars and ionized gas of three early-type spiral galaxies, namely NGC 772, 3898 and 7782. For...
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PublicationModelling neutral hydrogen in galaxies using cosmological hydrodynamical simulationsThe characterization of the atomic and molecular hydrogen content of high-redshift galaxies is a major observational challenge that will be addressed over the...
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PublicationModelling of surface brightness fluctuation measurements. Methodology, uncertainty, and recommendationsAims: The goal of this work is to scrutinise the surface brightness fluctuation (SBF) calculation methodology. We analysed the SBF derivation procedure...
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PublicationModelling simple stellar populations in the near-ultraviolet to near-infrared with the X-shooter Spectral Library (XSL)We present simple stellar population models based on the empirical X-shooter Spectral Library (XSL) from near-ultraviolet (NUV) to near-infrared (NIR)...
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PublicationModelling the emission of passive galaxy candidates at z∼3Early-type galaxies (ETGs) are of crucial importance to trace back the galaxy mass assembly across cosmic time, yet their formation and quenching remain...