activity
19972020
most citedThe Origin of Fe II Emission in AGN

146 citations · 435 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020★ 29 cited

Hubble Space Telescope Observations of [O~III] Emission in Nearby QSO2s: Physical Properties of the Ionised Outflows

Anna Trindade Falcao, S. B. Kraemer, T. C. Fischer +14

We use Hubble Space Telescope (HST)/ Space Telescope Imaging Spectrograph (STIS) long-slit G430M and G750M spectra to analyse the extended [O~III] 5007A emission in a sample of twe…

astro-ph.GA2018★ 107 cited

Hubble Space Telescope Observations of Extended [O III] λ5007 Emission in Nearby QSO2s: New Constraints On AGN / Host Galaxy Interaction

Travis C. Fischer, S. B. Kraemer, H. R. Schmitt +15

We present a Hubble Space Telescope (HST) survey of extended [O III] λ5007 emission for a sample of 12 nearby (z < 0.12), luminous Type 2 quasars (QSO2s), which we use to measure t…

astro-ph.CO2012★ 45 cited

The Surprising Absence of Absorption in the Far-Ultraviolet Spectrum of Mrk 231

S. Veilleux, M. Trippe, F. Hamann +11

Mrk 231, the nearest (z = 0.0422) quasar, hosts both a galactic-scale wind and a nuclear-scale iron low-ionization broad absorption line (FeLoBAL) outflow. We recently obtained a f…

astro-ph2004★ 59 cited

A Change in the Physical State of Carinae?

K. Davidson, J. C. Martin, R. M. Humphreys +8

During Car's spectroscopic event in mid-2003, the stellar wind's bright H and H emission lines temporarily had a distinctive shape unlike that reported on any previous oc…

astro-ph2004★ 146 cited

The Origin of Fe II Emission in AGN

J. A. Baldwin, G. J. Ferland, K. T. Korista +2

We used a very large set of models of broad emission line (BEL) clouds in AGN to investigate the formation of the observed Fe II emission lines. We show that photoionized BEL cloud…

astro-ph2004★ 48 cited

Implications of Quasar Black Hole Masses at High Redshifts

Matthias Dietrich, Fred Hamann

We investigated a sample of 15 luminous high-redshift quasars (3.3 < z < 5.1) to measure the mass of their super-massive black holes (SMBH) and compare, for the first time, results…