output
20032009
most citedImproved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics

1.4k citations

Showing 2006 · astro-phShow all

13 papers · 2 filters

astro-ph200655 cited

The Energy-dependent X-ray Timing Characteristics of the Narrow Line Seyfert 1 Mkn 766

A. Markowitz, I. E. Papadakis, P. Arevalo +3

We present the energy-dependent power spectral density (PSD) and cross-spectral properties of Mkn 766, obtained from combining data obtained during an XMM-Newton observation spanni…

astro-ph200645 cited

An Evolutionary Model For Submillimeter Galaxies

Sukanya Chakrabarti, Yeshe Fenner, Lars Hernquist +2

[abridged]We calculate multi-wavelength spectral energy distributions (SEDs) (spanning optical to millimeter wavelengths) from simulations of major galaxy mergers with black hole f…

astro-ph2006109 cited

A Chandra Search for Coronal X Rays from the Cool White Dwarf GD 356

Martin C. Weisskopf, Kinwah Wu, Virginia Trimble +4

We report observations with the Chandra X-ray Observatory of the single, cool, magnetic white dwarf GD 356. For consistent comparison with other X-ray observations of single white…

astro-ph20065 cited

A New Nearby Candidate Star Cluster in Ophiuchus at d = 170 pc

Eric E. Mamajek

The recent discoveries of nearby star clusters and associations within a few hundred pc of the Sun, as well as the order of magnitude difference in the formation rates of the embed…

astro-ph20061 cited

Probing Cool and Warm Infrared Galaxies using Photometric and Structural Measures

Nurur Rahman, George Helou, Joseph M. Mazzarella

We have analyzed a sample of nearby cool and warm infrared (IR) galaxies using photometric and structural parameters. The set of measures include far-infrared color ($C = \log_{10}…

astro-ph200655 cited

Ellipsoidal Variability and Long Secondary Periods in MACHO Red Giant Stars

A. Derekas, L. L. Kiss, T. R. Bedding +3

We present a period-luminosity-amplitude analysis of 5899 red giant and binary stars in the Large Magellanic Cloud, using publicly available observations of the MACHO project. For…