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20032009
most citedI Zw 18 revisited with HST/ACS and Cepheids: New Distance and Age

144 citations · 314 across the 8 of their papers we have counts for

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astro-ph200851 cited

A New Hubble Space Telescope Distance to NGC 1569: Starburst Properties and IC 342 Group Membership

Aaron J. Grocholski, Alessandra Aloisi, Roeland P. van der Marel +8

We present deep HST ACS/WFC photometry of the dwarf irregular galaxy NGC 1569, one of the closest and strongest nearby starburst galaxies. These data allow us, for the first time,…

astro-ph2007144 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

Very metal poor Classical Cepheids: variables in IZw18

G. Fiorentino, M. Marconi, G. Clementini +5

In the framework of an ongoing ACS@HST project (HST program #10586, PI: Aloisi) we have obtained deep multi-color imaging of the very metal-poor Blue Compact Dwarf galaxy IZw18. Th…

astro-ph20071 cited

Stellar Populations in Field Early-Type Galaxies

F. Annibali, A. Bressan, R. Rampazzo +2

We have acquired intermediate resolution spectra in the 3700-7000 A wavelength range for a sample of 65 early-type galaxies predominantly located in low density environments, a lar…

astro-ph20073 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-ph2006114 cited

The star formation history of early-type galaxies as a function of mass and environment

M. S. Clemens, A. Bressan, B. Nikolic +3

Using the third data release of the Sloan Digital Sky Survey (SDSS) we have rigorously defined a volume limited sample of early-type galaxies in the redshift range z < 0.1. We have…