We present a quantitative analysis of the star formation history (SFH) of the Local Group dSph galaxy Leo I, from the information in its Hubble Space Telescope...
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PublicationThe Star Formation History of the Local Group Dwarf Galaxy Leo I
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PublicationThe star formation history of the Magellanic Clouds
The star formation history of the Magellanic Clouds, including the old and intermediate-age star formation events, can be studied reliably and in detail through...
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PublicationThe Star Formation History of the Pegasus Dwarf Irregular Galaxy
The star formation history (SFH) of the Pegasus dIr, a likely Local Group member at 0.95 Mpc from the Milky Way, is investigated. We characterize the SFH by two...
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PublicationThe star formation history of the Sculptor dwarf spheroidal galaxy
We present the star formation history (SFH) of the Sculptor dwarf spheroidal galaxy based on deep g, r photometry taken with Dark Energy Camera at the Blanco...
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PublicationThe star formation history of the Sextans dwarf spheroidal galaxy: a true fossil of the pre-reionization era
We present the star formation history (SFH) of the Sextans dwarf spheroidal galaxy based on deep archive B, I photometry taken with Suprime-Cam at Subaru...
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PublicationThe star formation rates of QSOs
We 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)]...
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PublicationThe star formation timescale of elliptical galaxies. Fitting [Mg/Fe] and total metallicity simultaneously
The alpha element to iron peak element ratio, for example [Mg/Fe], is a commonly applied indicator of the galaxy star formation timescale (SFT) since the two...
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PublicationThe star-formation rates of 1.5 < z < 2.5 massive galaxies
The star formation rate (SFR) is a key parameter in the study of galaxy evolution. The accuracy of SFR measurements at z ~ 2 has been questioned following a...
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PublicationThe starburst galaxy NGC 6089: an ISO view
We present ISOCAM and ISOPHOT observations of the galaxy pair NGC 6090. The SED derived from all ISO measurements is typical for strong starbursts which were...