activity
20002014
most citedChandra Multiwavelength Project X-ray Point Source Catalog

153 citations · 380 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2014★ 22 cited

Constraints on the outer radius of the broad emission line region of active galactic nuclei

Hermine Landt, Martin J. Ward, Martin Elvis +1

Here we present observational evidence that the broad emission line region (BELR) of active galactic nuclei (AGN) generally has an outer boundary. This was already clear for source…

astro-ph.CO2013★ 47 cited

A near-infrared relationship for estimating black hole masses in active galactic nuclei

Hermine Landt, Martin J. Ward, Bradley M. Peterson +4

Black hole masses for samples of active galactic nuclei (AGN) are currently estimated from single-epoch optical spectra using scaling relations anchored in reverberation mapping re…

astro-ph.CO2011★ 89 cited

The near-infrared broad emission line region of active galactic nuclei. II. The one-micron continuum

Hermine Landt, Martin Elvis, Martin J. Ward +3

We use quasi-simultaneous near-infrared (near-IR) and optical spectroscopy from four observing runs to study the continuum around 1 micron in 23 well-known broad-emission line acti…

astro-ph2006★ 153 cited

Chandra Multiwavelength Project X-ray Point Source Catalog

Minsun Kim, Dong-Woo Kim, Belinda J. Wilkes +13

We present the Chandra Multiwavelength Project (ChaMP) X-ray point source catalog with ~6,800 X-ray sources detected in 149 Chandra observations covering \~10 deg^2. The full ChaMP…

astro-ph2006★ 9 cited

Chandra X-Ray Observatory Observations of Neutron Stars: An Overview

M. C. Weisskopf, M. Karovska, G. G. Pavlov +2

We present a brief review of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for obs…

astro-ph2002

Calibrating the Cepheid Period-Luminosity relation with the VLTI

M. Marengo, M. Karovska, D. Sasselov +3

The VLTI is the ideal instrument for measuring the distances of nearby Cepheids with the Baade-Wesselink method, allowing an accurate recalibration of the Cepheid Period-Luminosity…