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20002026
most citedThe Chandra Source Catalog

567 citations · 3.5k across the 87 of their papers we have counts for

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Showing 2003Show all

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astro-ph2003★ 17 cited

An Error Analysis of the Geometric Baade-Wesselink Method

Massimo Marengo, Margarita Karovska, Dimitar D. Sasselov +1

We derive an analytic solution for the minimization problem in the geometric Baade-Wesselink method. This solution allows deriving the distance and mean radius of a pulsating star…

astro-ph2003★ 9 cited

Spatially Resolved Circumnuclear Dust in Centaurus A

Margarita Karovska, Massimo Marengo, Martin Elvis +6

In this paper we present results from our exploratory mid-IR study of Centaurus A circumnuclear environment using high-angular resolution imaging at the Magellan 6.5m telescope wit…

astro-ph2003★ 27 cited

Molecular Hydrogen Emission Lines in Far Ultraviolet Spectroscopic Explorer Observations of Mira B

Brian E. Wood, Margarita Karovska

We present new Far Ultraviolet Spectroscopic Explorer (FUSE) observations of Mira A's wind-accreting companion star, Mira B. We find that the strongest lines in the FUSE spectrum a…

astro-ph2003★ 81 cited

Chandra Multi-wavelength Project (ChaMP). II. First Results of X-ray Source Properties

D. -W. Kim, B. J. Wilkes, P. J. Green +15

We present the first results of ChaMP X-ray source properties obtained from the initial sample of 62 observations. The data have been uniformly reduced and analyzed with techniques…

astro-ph2003★ 121 cited

Chandra Multi-wavelength Project (ChaMP). I. First X-ray Source Catalog

D. -W. Kim, R. A. Cameron, J. J. Drake +16

The Chandra Multi-wavelength Project (ChaMP) is a wide-area (~14 deg^2) survey of serendipitous Chandra X-ray sources, aiming to establish fair statistical samples covering a wide…

astro-ph2003★ 37 cited

Theoretical Limb Darkening for Classical Cepheids: II. Corrections for the Geometric Baade-Wesselink Method

Massimo Marengo, Margarita Karovska, Dimitar D. Sasselov +2

The geometric Baade-Wesselink method is one of the most promising techniques for obtaining a better calibration of the Cepheid period-luminosity relation by means of interferometri…