activity
19972007
most citedConfirmation of Errors in Hipparcos Parallaxes from HST/FGS Astrometry of the Pleiades

147 citations · 600 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph2007★ 10 cited

Oxygen abundance of open cluster dwarfs

Z. -X. Shen, X. -W. Liu, H. -W. Zhang +2

We present oxygen abundances of dwarfs in the young open cluster IC 4665 deduced from the OI 7774 triplet lines and of dwarfs in the open cluster Pleiades derived from the [OI]…

astro-ph2004★ 147 cited

Confirmation of Errors in Hipparcos Parallaxes from HST/FGS Astrometry of the Pleiades

David R. Soderblom, Ed Nelan, G. Fritz Benedict +4

We present absolute trigonometric parallaxes and relative proper motions for three members of the Pleiades star cluster, obtained with HST's Fine Guidance Sensor 1r, a white-light…

astro-ph2004★ 39 cited

Lick Northern Proper Motion Program. III. Lick NPM2 Catalog

Robert B. Hanson, Arnold R. Klemola, Burton F. Jones +1

The Lick Northern Proper Motion (NPM) program, a two-epoch (1947-1988) photographic survey of the northern two-thirds of the sky (Dec. > -23 deg), has measured absolute proper moti…

astro-ph2004★ 32 cited

Chandra X-ray observations of Young Clusters II. Orion Flanking Fields Data

Solange V. Ramirez, Luisa Rebull, John Stauffer +7

We present results of Chandra observations of two flanking fields (FF) in Orion, outside the Orion Nebula Cluster (ONC). The observations were taken with the ACIS-I camera with an…

astro-ph2004★ 50 cited

Chandra X-ray observations of Young Clusters I. NGC2264 Data

Solange V. Ramirez, Luisa Rebull, John Stauffer +7

We present results of a Chandra observation of a field in NGC 2264. The observations were taken with the ACIS-I camera with an exposure time of 48.1 ks. We present a catalog of 263…

astro-ph2003★ 111 cited

Why are the K dwarfs in the Pleiades so Blue?

John R. Stauffer, Burton F. Jones, Dana Backman +5

The K dwarfs in the Pleiades fall nearly one half magnitude below a main sequence isochrone when plotted in a color-magnitude diagram utilizing V magnitude as the luminosity index…