Publicación
The SAMI Galaxy Survey: the third and final data release
We have entered a new era where integral-field spectroscopic surveys of galaxies are sufficiently large to adequately sample large-scale structure over a...
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PublicaciónThe SAMI-Fornax Dwarfs Survey - IV. Star formation histories of dwarf and early-type galaxies: insights from full spectral fittingWe present a study on the star formation histories (SFHs) of galaxies covering the range 10 4 < M ⋆/M ⊙ < 10 12, leveraging full spectral fitting algorithms...
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CharlaThe Scutum-Crux Complex: Tying massive stellar formation with the overall structure of the Milky WayWith the discovery of several massive, young clusters in the last five years, the area around the base of the Scutum-Crux arm (around l=28) has become one of...
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PublicaciónThe second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environmentWe report the detection of the radio afterglow of a long gamma-ray burst (GRB) 111005A at 5-345 GHz, including very long baseline interferometry observations...
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CharlaThe Star Formation & Chemical Evolution timescales of two nearby dwarf spheroidal galaxiesWe present the detailed Star Formation History of the nearby Sculptor and Fornax dwarf spheroidal galaxies, from wide-field photometry of resolved stars, going...
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PublicaciónThe Star Formation History and Dust Production in Andromeda IXLocal Group (LG), the nearest and most complete galactic environment, provides valuable information on the formation and evolution of the Universe. Studying...
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CharlaThe star formation history of different types of dwarf galaxiesWe are going to present a new code to derive the SFH of a complex stellar population system, like a galaxy. This code has been used to obtain the SFH of six...
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PublicaciónThe star formation history of galaxies: the role of galaxy mass, morphology and environmentWe analyse the star formation history (SFH) of galaxies as a function of present-day environment, galaxy stellar mass and morphology. The SFH is derived by...
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PublicaciónThe star formation rates of QSOsWe examine the far-infrared (FIR) properties of a sample of 5391 optically selected QSOs in the 0.5 < z < 2.65 redshift range down to log [νL ν, 2500(erg s -1)]...