activity
19962023
most citedThe Habitable Exoplanet Observatory (HabEx) Mission Concept Study Final Report

146 citations · 601 across the 13 of their papers we have counts for

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7 papers · 1 filter

astro-ph2006★ 24 cited

Interplanetary Lyman line profiles: variations with solar activity cycle

Eric Quémerais, Rosine Lallement, Jean-Loup Bertaux +4

Interplanetary Lyman alpha line profiles are derived from the SWAN H cell data measurements. The measurements cover a 6-year period from solar minimum (1996) to after the solar max…

astro-ph1999★ 82 cited

Stellar Populations at the Center of IC 1613

Andrew A. Cole, Eline Tolstoy, John S. Gallagher +18

We have observed the center of the Local Group dwarf irregular galaxy IC 1613 with WFPC2 aboard the Hubble Space Telescope in the F439W, F555W, and F814W filters. We find a dominan…

astro-ph1999★ 80 cited

WFPC2 Observations of Compact Star Cluster Nuclei in Low Luminosity Spiral Galaxies

Lynn D. Matthews, John S. Gallagher, III +16

We have used the Wide Field Planetary Camera 2 aboard the Hubble Space Telescope to image the compact star cluster nuclei of the nearby, late-type, low-luminosity spiral galaxies N…

astro-ph1998★ 26 cited

Detection of Surface Brightness Fluctuations in NGC 4373 Using the Hubble Space Telescope

M. A. Pahre, J. R. Mould, A. Dressler +1

Surface brightness fluctuations (SBF) have been detected for three elliptical galaxies-NGC 3379 in the Leo group, NGC 4406 in the Virgo cluster, and NGC 4373 in the Hydra-Centaurus…

astro-ph1998★ 13 cited

Far-Ultraviolet and Visible Imaging of the Nucleus of M32

A. A. Cole, J. S. Gallagher, J. R. Mould +1

We have imaged the nucleus of M32 at 1600 Angstroms (FUV) and 5500 Angstroms (V) using the Wide-Field/Planetary Camera 2 (WFPC2) aboard HST. We detected the nucleus at 1600 Angstro…

astro-ph1997★ 103 cited

Stellar Populations in Three Outer Fields of the LMC

Marla C. Geha, Jon A. Holtzman, Jeremy R. Mould +16

We present HST photometry for three fields in the outer disk of the LMC extending approximately four magnitudes below the faintest main sequence turnoff. We cannot detect any stron…