activity
19982023
most citedNo planet for HD 166435

764 citations · 2.2k across the 16 of their papers we have counts for

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7 papers · 1 filter

astro-ph2007★ 229 cited

Patterns of photometric and chromospheric variation among Sun-like stars: A 20-year perspective

G. W. Lockwood, B. A. Skiff, Gregory W. Henry +5

We examine patterns of variation of 32 primarily main sequence stars, extending our previous 7-12 year time series to 13-20 years by combining b, y data from Lowell Observatory wit…

astro-ph2006★ 189 cited

The Extrasolar Planet epsilon Eridani b - Orbit and Mass

G. Fritz Benedict, Barbara E. McArthur, George Gatewood +11

Hubble Space Telescope observations of the nearby (3.22 pc), K2 V star epsilon Eridani have been combined with ground-based astrometric and radial velocity data to determine the ma…

astro-ph2006★ 65 cited

A Survey of Chromospheric Activity in the Solar-Type Stars in the Open Cluster M67

Mark S. Giampapa, Jeffrey C. Hall, Richard R. Radick +1

We present the results of a spectroscopic survey of the Ca II H & K core strengths in a sample of 60 solar-type stars that are members of the solar-age and solar-metallicity open c…

astro-ph2004★ 49 cited

High-amplitude, long-term X-ray variability in the solar-type star HD 81809: the beginning of an X-ray activity cycle?

F. Favata, G. Micela, S. L. Baliunas

We present the initial results from our XMM program aimed at searching for X-ray activity cycles in solar-type stars. HD 81809 is a G2-type star (somewhat more evolved than the Sun…

astro-ph2001★ 764 cited

No planet for HD 166435

D. Queloz, G. W. Henry, J. P. Sivan +6

The G0V star HD166435 has been observed by the fiber-fed spectrograph ELODIE as one of the targets in the large extra-solar planet survey that we are conducting at the Observatory…

astro-ph2000★ 270 cited

Evidence for a Long-period Planet Orbiting Epsilon Eridani

Artie P. Hatzes, William D. Cochran, Barbara McArthur +10

High precision radial velocity (RV) measurements spanning the years 1980.8--2000.0 are presented for the nearby (3.22 pc) K2 V star Eri. These data, which represent a combinati…