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most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations · 28.5k across the 331 of their papers we have counts for

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astro-ph2000★ 47 cited

The Stellar Content and Distance of UGC 4483

A. E. Dolphin, L. Makarova, I. D. Karachentsev +7

We present HST/WFPC2 observations of UGC 4483, an irregular galaxy in the M81/NGC 2403 complex. Stellar photometry was carried out with HSTphot, and is complete to V ~ 26.0 and I ~…

astro-ph2000★ 1 cited

A Lack of Planets in 47 Tucanae from an HST Search

Ronald L. Gilliland, T. M. Brown, P. Guhathakurta +21

We report results from a large Hubble Space Telescope project to observe a significant (~34,000) ensemble of main sequence stars in the globular cluster 47 Tucanae with a goal of d…

astro-ph2000★ 1 cited

Dwarf Spheroidal Galaxies in the M81 Group Imaged with WFPC2

I. D. Karachentsev, V. E. Karachentseva, A. E. Dolphin +7

We obtained HST/WFPC2 images of the dwarf spheroidal (dSph) galaxies K61, K63, K64, DDO78, BK6N, and kk77 in the M81 group. Our color-magnitude diagrams show red giant branches wit…

astro-ph2000★ 94 cited

Dynamical Mass Estimates for the Halo of M31 from Keck Spectroscopy

N. W. Evans, M. I. Wilkinson, P. Guhathakurta +2

The last few months have seen the measurements of the radial velocities of all of the dwarf spheroidal companions to the Andromeda galaxy (M31) using the spectrographs (HIRES and L…

astro-ph2000★ 29 cited

Hubble Space Telescope Photometry of the Dwarf Spheroidal Galaxy ESO 410-G005

Igor D. Karachentsev, Margarita E. Sharina, Eva K. Grebel +7

We present HST WFPC2 imaging of the nearby low-surface-brightness dwarf spheroidal galaxy ESO 410-G005, which has been resolved into stars for the first time. The resulting color-m…

astro-ph2000★ 2 cited

A Dwarf Galaxy Survey in the Local Volume

E. K. Grebel, P. Seitzer, A. E. Dolphin +6

We are carrying out a comprehensive multi-wavelength study of dwarf galaxies in the Local Volume (< 5 Mpc). After our all-sky survey more than doubled the dwarf census we are now m…