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20032009
most citedCats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions

810 citations

Showing 2007Show all

9 papers · 1 filter

astro-ph20073 cited

Oscillations in Procyon A: First results from a multi-site campaign

S. Hekker, T. Arentoft, H. Kjeldsen +45

Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…

astro-ph2007

3D Spectroscopy and the Virtual Observatory

Bryan W. Miller

Integral field, or 3D, spectroscopy is the technique of obtaining spectral information over a two-dimensional, hopefully contiguous, field of view. While there is some form of astr…

astro-ph20075 cited

Millimagnitude Photometry for Transiting Extrasolar Planetary Candidates IV: The Puzzle of the Extremely Red OGLE-TR-82 Primary Solved

Sergio Hoyer, Sebastian Ramirez Alegria, Valentin D. Ivanov +12

We present precise new V, I, and K-band photometry for the planetary transit candidate star OGLE-TR-82. Good seeing V-band images acquired with VIMOS instrument at ESO VLT allowed…

astro-ph200759 cited

Gemini Spectroscopic Survey of Young Star Clusters in Merging/Interacting Galaxies. II. NGC 3256 Clusters

Gelys Trancho, Nate Bastian, Bryan W. Miller +1

We present Gemini optical spectroscopy of 23 young star clusters in NGC3256. We find that the cluster ages range are from few Myr to ~150 Myr. All these clusters are relatively mas…

astro-ph200713 cited

Witnessing the formation of a galaxy cluster at z=0.485: optical and X-ray properties of RX J1117.4+0743 ([VMF 98] 097)

E. R. Carrasco, E. S. Cypriano, G. B. Lima Neto +4

We present a multiwavelength study of the poor cluster RX J1117.4+0743 ([VMF 98] 097) at z=0.485, based on GMOS/Gemini South g', r' photometry and spectroscopy, and XMM-Newton obse…

astro-ph200772 cited

The Mid-Infrared Emission of M87

E. S. Perlman, R. E. Mason, Christopher Packham +6

We discuss Subaru and Spitzer Space Telescope imaging and spectroscopy of M87 in the mid-infrared from 5-35 um. These observations allow us to investigate mid-IR emission mechanism…