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19942026
most citedLegacy ExtraGalactic UV Survey (LEGUS) with The Hubble Space Telescope. I. Survey Description

229 citations · 2.1k across the 58 of their papers we have counts for

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astro-ph2008★ 225 cited

Age Determination of Six Intermediate-age SMC Star Clusters with HST/ACS

Katharina Glatt, Eva K. Grebel, Elena Sabbi +9

We present a photometric analysis of the star clusters Lindsay 1, Kron 3, NGC339, NGC416, Lindsay 38, and NGC419 in the Small Magellanic Cloud (SMC), observed with the Hubble Space…

astro-ph2007

Progressive star formation in the young SMC cluster NGC 602

Lynn Redding Carlson, E. Sabbi, M. Sirianni +9

NGC 602 is a young stellar cluster located in a peripheral region of the Small Magellanic Cloud known as the wing. Far from the main body of the galaxy and abutting the Magellanic…

astro-ph2007★ 64 cited

Starbursts in the Local Universe: new HST/ACS observations of the irregular galaxy NGC 4449

F. Annibali, A. Aloisi, J. Mack +5

We present photometry with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST) of stars in the Magellanic starburst galaxy NGC 4449. The galaxy has been image…

astro-ph2007★ 144 cited

I Zw 18 revisited with HST/ACS and Cepheids: New Distance and Age

A. Aloisi, G. Clementini, M. Tosi +9

We present new V and I-band HST/ACS photometry of I Zw 18, the most metal-poor blue compact dwarf (BCD) galaxy in the nearby universe. It has been argued in the past that I Zw 18 i…

astro-ph2007★ 3 cited

A New Deep HST/ACS CMD of I Zw 18: Evidence for Red Giant Branch Stars

A. Aloisi, F. Annibali, J. Mack +8

We present results from new deep HST/ACS photometry of I Zw 18, the most metal-poor blue compact dwarf galaxy in the nearby universe. It has been previously argued that this is a v…

astro-ph2006★ 7 cited

IZw18, or the picture of Dorian Gray: the more you watch it, the older it gets

M. Tosi, A. Aloisi, J. Mack +1

IZw18 has been recurrently claimed to be a young galaxy, but stars of increasingly older ages are found every time deeper magnitude levels are reached with high-resolution photomet…