activity
19982019
most citedOn the Origin of Intrinsic Narrow Absorption Lines in z<1 QSOs

91 citations · 209 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019★ 21 cited

Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures

Mason Ng, Nikole M. Nielsen, Glenn G. Kacprzak +4

We probe the high-ionization circumgalactic medium by examining absorber kinematics, absorber-galaxy kinematics, and average absorption profiles of 31 OVI absorbers from the "Multi…

astro-ph.GA2015★ 9 cited

A Comprehensive HST BVI Catalogue Of Star Clusters In Five Hickson Compact Groups Of Galaxies

K. Fedotov, S. C. Gallagher, P. R. Durrell +5

We present a photometric catalogue of star cluster candidates in Hickson compact groups (HCGs) 7, 31, 42, 59, and 92, based on observations with the Advanced Camera for Surveys and…

astro-ph2008★ 28 cited

Exploratory Study of the X-Ray Properties of Quasars With Intrinsic Narrow Absorption Lines

Toru Misawa, Michael Eracleous, George Chartas +1

We have used archival Chandra and XMM-Newton observations of quasars hosting intrinsic narrow UV absorption lines (intrinsic NALs) to carry out an exploratory survey of their X-ray…

astro-ph2001★ 19 cited

Variable UV Absorption in the Spectrum of MRC 2251-178

Rajib Ganguly, Jane C. Charlton, Michael Eracleous

We present an ultraviolet spectrum of MRC 2251-178 taken with HST/STIS-G230L. The observation is part of a snap shot program of QSOs to systematically search for intrinsic absorpti…

astro-ph2000★ 91 cited

On the Origin of Intrinsic Narrow Absorption Lines in z<1 QSOs

Rajib Ganguly, Nicholas A. Bond, Jane C. Charlton +3

We present a statistical analysis of the associated, high ionization narrow absorption line (NAL) systems in a sample of 59 QSOs defined from the HST QSO Absorption Line Key Projec…

astro-ph1998★ 41 cited

The Multiple Phases of Interstellar and Halo Gas in a Possible Group of Galaxies at z~1

Christopher W. Churchill, Jane C. Charlton

We used HIRES/Keck profiles (R=6 km/s) of MgII and FeII in combination with FOS/HST spectra (R=230 km/s) to place constraints on the physical conditions (metallicities, ionization…